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26TH INTERNATIONAL CONFERENCE ON COMPUTING IN HIGH ENERGY & NUCLEAR PHYSICS (CHEP2023)

US/Eastern
Norfolk Waterside Marriott

Norfolk Waterside Marriott

235 East Main Street Norfolk, VA 23510
Boehnlein, Amber (JLAB) , Heyes, Graham (Jefferson Lab) , Sawatzky, Brad (Jefferson Lab)
Description

Thank you all for a very successful CHEP 2023 in Norfolk!  It was a pleasure to have you all here. Proceedings are in progress and recordings of most plenary sessions are available.

We look forward to seeing you all at CHEP 2024 in Krakow, Poland (Oct 19--25, 2024).


The CHEP conferences address the computing, networking and software issues for the world’s leading data‐intensive science experiments that currently analyze hundreds of petabytes of data using worldwide computing resources. The Conference provides a unique opportunity for computing experts across Particle and Nuclear Physics to come together to learn from each other and typically attracts over 500 participants. The event features plenary sessions, parallel sessions, and poster presentations; it publishes peer-reviewed proceedings.

You can find additional information through the Conference Website and the links on the right sidebar.

Special Notes

CHEP 2023 Proceedings are under development and will be published through the EPJ Web of Conferences in the new year.  If you gave a presentation at CHEP 2023, please watch your email and/or review the article submission process under Proceedings for instructions.

WLCG/HSF Pre-conference Workshop

A WLCG/HSF pre-conference workshop will be held on the prior weekend (May 6, 7).  If that is of interest, please check the appropriate box during Registration.

Conference Secretariat
    • 8:00 AM 9:00 AM
      Registration
    • 9:00 AM 10:30 AM
      Plenary Session: Welcome / Highlighted Keynotes Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Convener: Dodge, Gail (Olde Dominion University)
      • 9:00 AM
        Welcome and Introduction to CHEP23 30m
        Speakers: Boehnlein, Amber (JLAB) , Dodge, Gail (Old Dominion University) , Henderson, Stuart (Jefferson Lab) , Scott, Bobby (United States Congressman)
      • 9:30 AM
        Keynote: Evolutions and Revolutions in Computing: Science at the Frontier 30m

        The world is full of computing devices that calculate, monitor, analyze, and control processes. The underlying technical advances within computing hardware have been further enhanced by tremendous algorithmic advances across the spectrum of the sciences. The quest -- ever present in humans -- to push the frontiers of knowledge and understanding requires continuing advances in the development and use of computation, with an increasing emphasis on the analysis of complex data originating from experiments and observations. How this move toward data intensive computing affects our underlying processes in the sciences remains to be fully appreciated. In this talk, I will briefly describe how we arrived at this point, and also give a prospective toward the end of the talk.

        Speaker: Dean, David (TJNAF)
    • 10:30 AM 11:00 AM
      AM Break 30m Hampton Roads Ballroom (3rd floor)

      Hampton Roads Ballroom (3rd floor)

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
    • 11:00 AM 12:30 PM
      Track 1 - Data and Metadata Organization, Management and Access: Storage Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Barisits, Martin (CERN) , Lassnig, Mario (CERN)
      • 11:00 AM
        dCache: storage system for data intensive science 15m

        The dCache project provides open-source software deployed internationally to satisfy
        ever more demanding storage requirements. Its multifaceted approach provides an integrated
        way of supporting different use-cases with the same storage, from high throughput data
        ingest, data sharing over wide area networks, efficient access from HPC clusters and long
        term data persistence on a tertiary storage. Though it was originally developed for the
        HEP experiments, today it is used by various scientific communities, including astrophysics,
        biomed, life science, which have their specific requirements. With this contribution we
        would like to highlight the recent developments in the dCache regarding integration with
        CERN Tape Archive (CTA), advanced metadata handling, bulk API for QoS transitions, RESTAPI
        to control interaction with tape system and the future development directions.

        Speaker: Mr Litvintsev, Dmitry (Fermilab)
      • 11:15 AM
        Erasure Coding Xrootd Object Store 15m

        XRootD implemented a client-side erasure coding (EC) algorithm utilizing the Intel Intelligent Storage Acceleration Library. At SLAC, a prototype of XRootD EC storage was set up for evaluation. The architecture and configuration of the prototype is almost identical to that of a traditional non-EC XRootD storage behind a firewall: a backend XRootD storage cluster in its simplest form, and an internet facing XRootD proxy that handles EC and spreads the data stripes of a file/object across several backend nodes. This prototype supports all functions used on a WLCG storage system: HTTP(s) and XRootD protocols, Third Party Copy, X509/VOMS/Token, etc. The cross-node EC architecture brings significant advantages in both performance and resilience: e.g. parallel data access, tolerance of downtime and hardware failure. This paper will describe the prototype’s architecture and its design choices, the performance in high concurrent throughputs and file/object operations, failure modes and their handling, data recovery methods, and administration. This paper also describes the work that explores the HTTP protocol feature in XRootD to support data access via industry standard Boto3 S3 client library.

        Speaker: Yang, Wei (SLAC National Accelerator Laboratory)
      • 11:30 AM
        POSIX access to remote storage with OpenID Connect AuthN/AuthZ 15m

        INFN-CNAF is one of the Worldwide LHC Computing Grid (WLCG) Tier-1 data centers, providing support in terms of computing, networking, storage resources and services also to a wide variety of scientific collaborations, ranging from physics to bioinformatics and industrial engineering.
        Recently, several collaborations working with our data center have developed computing and data management workflows that require access to S3 storage services and the integration with POSIX capabilities.
        To accomplish this requirement in distributed environments, where computing and storage resources are located at geographically distant physical sites, the possibility to locally mount a file system from a remote site to directly perform operations on files and directories becomes crucial.
        Nevertheless, the access to the data must be regulated by standard, federated authentication and authorization mechanisms, such as OpenID Connect (OIDC), which is already adopted as AuthN/AuthZ mechanism within WLCG and the European Open Science Cloud (EOSC).
        Starting from such principles, we evaluated the possibility to regulate data access by integrating JSON Web Token (JWT) authentication, provided by INDIGO-IAM as Identity Provider (IdP), with solutions based on S3 (for object storage) and HTTP (for hierarchical storage) protocols.
        In particular, in regard to S3 data exposition, we integrated MinIO and CEPH RADOS Gateway with s3fs-fuse, providing the needed custom libraries to mount an S3 bucket via FUSE by preserving the native object format for files. Both solutions support Secure Token Service (STS), providing a client with temporary credentials to perform a given operation on a storage resource by checking the value of a JWT claim associated with the request.
        Native MinIO STS does not support IAM JWT profile, thus we delegated STS service to Hashicorp Vault in the case of MinIO.
        RADOS Gateway is an object storage interface for Ceph. It provides a RESTful S3-compatible API and a feature for integration with OIDC IdP. Access tokens produced for OIDC clients can be used by the STS implemented within RADOS Gateway for authorizing specific S3 operations.
        On the other hand, HTTP data access has been managed by using Rclone and WebDAV protocol, to mount a storage area via INDIGO-IAM token authentication. In this case the storage area is exposed via HTTP by using the StoRM-WebDAV application, but the solution is general enough to be used with other HTTP data management servers (e.g. Apache, NGINX).
        In such respect, a comparison between the performances yielded by S3 and WebDAV protocols has been carried out within the same Red Hat OpenShift environment, in order to better understand which solution is most suitable for each of the use cases of interest.

        Speaker: Dr Fornari, Federico (INFN-CNAF)
      • 11:45 AM
        Enabling Storage Business Continuity and Disaster Recovery with Ceph distributed storage 15m

        The Storage Group in the CERN IT Department operates several Ceph storage clusters with an overall capacity exceeding 100 PB. Ceph is a crucial component of the infrastructure delivering IT services to all the users of the Organization as it provides: i) Block storage for the OpenStack infrastructure, ii) CephFS used as persistent storage by containers (OpenShift and Kubernetes) and as shared filesystems by HPC clusters, and iii) S3 object storage for cloud-native applications, monitoring, and software distribution across the WLCG.

        The Ceph infrastructure at CERN has been rationalized and restructured to offer storage solutions for high(er) availability and Disaster Recovery / Business Continuity. In this contribution, we give an overview of how we transitioned from a single RBD zone to multiple ones enabling Storage Availability zones and how RBD mirroring functionalities available in Ceph upstream have been hardened. Also, we illustrate future plans for storage BC/DR including backups via restic to S3 and Tape, replication of objects across multiple storage zones, and the instantiation of clusters spanning different computing centres.

        Speaker: Bocchi, Enrico (CERN)
      • 12:00 PM
        ECHO: optimising object store data access for Run-3 and the evolution towards HL-LHC 15m

        Data access at the UK Tier-1 facility at RAL is provided through its ECHO storage, serving the requirements for the WLGC and increasing numbers of other HEP and astronomy related communities.
        ECHO is a Ceph-backed erasure-coded object store, currently providing in excess of 40PB of usable space, with frontend access to data provided via XRootD or gridFTP, using the libradosstriper library of Ceph.
        The storage must service the needs of: high-throughput compute, with staged and direct file access passing through an XCache on each workernode; data access to compute running at storageless satellite sites; and, managed inter-site data transfers using the recently adopted HTTPS protocol (via WebDav), which includes multi-hop data transfers to and from RAL’s newly commissioned CTA tape endpoint.
        A review of the experiences of providing data access via an object store within these data workflows is presented, including the details of the improvements necessary for the transition to WebDav, used for most inter-site data movements, and enhancements for direct-IO file access, where the development and optimisation of buffering and range coalescence strategies is explored.
        In addition to serving the requirements of LHC Run-3, preparations for Run-4 and for large astronomy experiments is underway. One example is with ROOT-based data formats, where the evolution from a TTree to RNTuple data structure provides an opportunity for storage providers to benchmark and optimise against this new format. A comparison of the current performance between data formats within ECHO is presented and the details of potential improvements presented.

        Speaker: Walder, James (RAL, STFC, UKRI)
      • 12:15 PM
        EOS Software Evolution Enabling LHC Run-3 15m

        EOS has been the main storage system at CERN for more than a decade, continuously improving in order to meet the ever evolving requirements of the LHC experiments and the whole physics user community. In order to satisfy the demands of LHC Run-3, in terms of storage performance and tradeoff between cost and capacity, EOS was enhanced with a set of new functionalities and features that we will detail in this paper.

        First of all, we describe the use of erasure coded layouts in a large-scale deployment which enables an efficient use of available storage capacity, while at the same time providing end-users with better throughput when accessing their data. This new operating model implies more coupling between the machines in a cluster, which in turn leads to the next set of EOS improvements that we discuss, targeting I/O traffic shaping, better I/O scheduling policies and tagged traffic prioritization. Increasing the size of the EOS clusters to cope with experiment demands, means stringent constraints on the data integrity and durability that we addressed by a re-designed consistency check engine. Another focus area of EOS development was to minimize the operational load by making the internal operational procedures (draining, balancing or conversions) more robust and efficient, to allow managing easily multiple clusters and avoid possible scaling issues.

        All these improvements available in the EOS 5 release series, are coupled with the new XRootD 5 framework which brings additional security features like TLS support and optimizations for large data transfers like page read and page write functionalities. Last but not least, the area of authentication/authorization methods has seen important developments by adding support for different types of bearer tokens that we will describe along with EOS specific token extensions. We conclude by highlighting potential areas of the EOS architecture that might require further developments or re-design in order to cope with the ever-increasing demands of our end-users.

        Speaker: Mr Caffy, Cedric (CERN)
    • 11:00 AM 12:30 PM
      Track 2 - Online Computing: DAQ Frameworks Marriott Ballroom V-VI

      Marriott Ballroom V-VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Antel, Claire (Universite de Geneve (CH)) , Pantaleo, Felice (CERN)
      • 11:00 AM
        One year of LHCb triggerless DAQ: achievements and lessons learned. 15m

        The LHCb experiment is one of the four large experiments on the LHC at CERN. This forward spectrometer is designed to investigate differences between matter and antimatter by studying beauty and charm Physics. The detector and the entire DAQ chain have been upgraded, to profit from the higher luminosity delivered by the particle accelerator during Run3. The new DAQ system introduces a substantially different model for reading-out the detector data, which has not been used in systems of similar scale up to now. We designed a system capable of performing read-out, event-building and online reconstruction of the full event-rate produced by the LHC, without incurring the inefficiencies that a low-level hardware trigger would introduce. This design paradigm requires a DAQ system capable of ingesting an aggregated throughput of ~32 Tb/s, this poses significant technical challenges which have been solved by using both off-the-shelf solutions - like InfiniBand HDR - and customly developed FPGA-based electronics.
        In this contribution, we will: provide an overview on the final system design, with a special focus on the event-building infrastructure; present quantitative measurements taken during the commissioning of the system; discuss the resiliency of the system concerning latency and fault tolerance; and provide feedback on the first year of operations of the system.

        Speaker: Pisani, Flavio (CERN)
      • 11:15 AM
        The new ALICE Data Acquisition system (O2/FLP) for LHC Run 3 15m

        ALICE (A Large Ion Collider Experiment) has undertaken a major upgrade during the LHC Long Shutdown 2. The increase in the detector data rates led to a hundredfold increase in the input raw data, up to 3.5 TB/s. To cope with it, a new common Online and Offline computing system, called O2, has been developed and put in production.

        The O2/FLP system, successor of the ALICE DAQ system, implements the critical functions of detector readout, data quality control and operational services running in the CR1 data centre at the experimental site. Data from the 15 ALICE subdetectors are read out via 8000 optical links by 500 custom PCIe cards hosted in 200 nodes. It addresses novel challenges such as the continuous readout of the TPC detector while keeping compatibility with legacy detector front-end electronics.

        This paper discusses the final architecture and design of the O2/FLP system and provides an overview of all its components, both hardware and software. It presents the selection process for the FLP nodes, the different commissioning steps and the main accomplishments so far. It will conclude with the challenges that lie ahead and how they will be addressed.

        Speaker: Barroso, Vasco (CERN)
      • 11:30 AM
        Operational experience with the new ATLAS HLT framework for LHC Run 3 15m

        Athena is the software framework used in the ATLAS experiment throughout the data processing path, from the software trigger system through offline event reconstruction to physics analysis. For Run 3 data taking (which started in 2022) the framework has been reimplemented into a multi-threaded framework. In addition to having to be remodelled to work in this new framework, the ATLAS High Level Trigger (HLT) system has also been updated to rely on common solutions between online and offline software to a greater extent than in Run 2 (data taking between 2015-2018). We present the now operational new HLT system, reporting on how the system was tested, commissioned and optimised. In addition, we show developments that have been made in tools that are used to monitor and configure the HLT, some of which are designed from scratch for Run 3.

        Speaker: Poreba, Aleksandra (CERN)
      • 11:45 AM
        INDRA-ASTRA 15m

        The INDRA-ASTRA project is part of the ongoing R&D on streaming readout and AI/ML at Jefferson Lab. In the interdisciplinary project, nuclear physicists and data scientists work towards a prototype for an autonomous, responsive detector system as a first step towards a fully autonomous experiment. In our presentation, we will present our method for autonomous calibration of DIS experiments using baseline calibrations and autonomous change detection via the multiscale method. We will demonstrate how the versatile multiscale method we have developed can be used to increase reliability of data and find and fix issues in near real time. We will show test results from a prototype detector and the running, large-scale SBS experiment at Jefferson Lab.

        Speaker: Mr Fang, Ronglong
      • 12:00 PM
        ATLAS Trigger and Data Acquisition Upgrades for the High Luminosity LHC 15m

        The ATLAS experiment at CERN is constructing upgraded system
        for the "High Luminosity LHC", with collisions due to start in
        2029. In order to deliver an order of magnitude more data than
        previous LHC runs, 14 TeV protons will collide with an instantaneous
        luminosity of up to 7.5 x 10e34 cm^-2s^-1, resulting in much higher pileup and
        data rates than the current experiment was designed to handle. While
        this is essential to realise the physics programme, it presents a huge
        challenge for the detector, trigger, data acquisition and computing.
        The detector upgrades themselves also present new requirements and
        opportunities for the trigger and data acquisition system.

        The design of the TDAQ upgrade comprises: a hardware-based low-latency
        real-time Trigger operating at 40 MHz, Data Acquisition which combines
        custom readout with commodity hardware and networking to deal with
        4.6 TB/s input, and an Event Filter running at 1 MHz which combines
        offline-like algorithms on a large commodity compute service
        with the potential to be augmented by commercial accelerators .
        Commodity servers and networks are used as far as possible, with
        custom ATCA boards, high speed links and powerful FPGAs deployed
        in the low-latency parts of the system. Offline-style clustering and
        jet-finding in FPGAs, and accelerated track reconstruction are
        designed to combat pileup in the Trigger and Event Filter
        respectively.

        This contribution will report recent progress on the design, technology and
        construction of the system. The physics motivation and expected
        performance will be shown for key physics processes.

        Speaker: Negri, Andrea (CERN)
      • 12:15 PM
        From hyperons to hypernuclei online 15m

        The fast algorithms for data reconstruction and analysis of the FLES (First Level Event Selection) package of the CBM (FAIR/GSI) experiment were successfully adapted to work on the High Level Trigger (HLT) of the STAR (BNL) experiment online. For this purpose, a so-called express data stream was created on the HLT, which enabled full processing and analysis of the experimental data in real time.

        With this express data processing, including online calibration, reconstruction of tracks and short-lived particles, as well as search and analysis of hyperons and hypernuclei, approximately 30% of all the data collected in 2019-2021 within the Beam Energy Scan (BES-II) program at energies down to 3 GeV has been processed on the free resources of the HLT computer farm.

        A block diagram of the express data processing and analysis will be presented, particular features of the online calibration and application of the reconstruction algorithms, work under pile-up conditions at low collision energies in the fixed-target mode, and results of the real-time search for hyperons and hypernuclei up to $^5_\Lambda$He with 11.6$\cdot\sigma$ at HLT will be presented and discussed. The high quality of the express data enabled preliminary analysis results in several physics measurements.

        Speaker: Prof. Kisel, Ivan (Goethe University Frankfurt am Main)
    • 11:00 AM 12:30 PM
      Track 3 - Offline Computing: Reconstruction Hampton Roads Ballroom VI

      Hampton Roads Ballroom VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Bandieramonte, Marilena (University of Pittsburgh) , Dr Srpimanobhas, Norraphat (Chulalongkorn University)
      • 11:00 AM
        Machine learning for ambiguity resolution in ACTS 15m

        The reconstruction of particle trajectories is a key challenge of particle physics experiments, as it directly impacts particle identification and physics performances while also representing one of the main CPU consumers of many high energy physics experiments. As the luminosity of particle collider increases, this reconstruction will become more challenging and resource intensive. New algorithms are thus needed to address these challenges efficiently. One potential step of track reconstruction is the ambiguity resolution. In this step, performed at the end of the tracking chain, we select which tracks candidates should to be kept and which ones need to be discarded. In the ATLAS experiment, for example, this is achieved by identifying fakes tracks, removing duplicates and determining via a Neural Network which hits should be shared by multiple tracks. The speed of this algorithm is directly driven by the number of track candidates, which can be reduced at the cost of some physics performance. Since this problem is fundamentally an issue of comparison and classification, we propose to use a machine learning based approach to the Ambiguity Resolution itself. Using a nearest neighbour search, we can efficiently determine which candidates belong to the same truth particle. Afterward, we can apply a Neural Network (NN) to compare those tracks and determine which ones are the duplicate and which one should be kept. Finally, another NN is applied to all the remaining candidates to identify which ones are fakes and remove those. This approach is implemented within A Common Tracking Software (ACTS) framework and tested on the Open Data Detector (ODD) a realistic virtual detector, similar to a future ATLAS one, to fully evaluate the potential of this approach.

        Speaker: Allaire, Corentin (IJCLab)
      • 11:15 AM
        Generalizing mkFit and its Application to HL-LHC 15m

        MkFit is an implementation of the Kalman filter-based track reconstruction algorithm that exploits both thread- and data-level parallelism. In the past few years the project transitioned from the R&D phase to deployment in the Run-3 offline workflow of the CMS experiment. The CMS tracking performs a series of iterations, targeting reconstruction of tracks of increasing difficulty after removing hits associated to tracks found in previous iterations. MkFit has been adopted for several of the tracking iterations, which contribute to the majority of reconstructed tracks. When tested in the standard conditions for production jobs, speedups in track pattern recognition are on average of the order of 3.5x for the iterations where it is used (3-7x depending on the iteration). Multiple factors contribute to the observed speedups, including vectorization and a lightweight geometry description, as well as improved memory management and single precision. Efficient vectorization is achieved with both the icc and the gcc (default in CMSSW) compilers and relies on a dedicated library for small matrix operations, Matriplex, which has recently been released in a public repository. While the mkFit geometry description already featured levels of abstraction from the actual Phase-1 CMS tracker, several components of the implementations were still tied to that specific geometry. We have further generalized the geometry description and the configuration of the run-time parameters, in order to enable support for the Phase-2 upgraded tracker geometry for the HL-LHC and potentially other detector configurations. The implementation strategy and preliminary results with the HL-LHC geometry will be presented. Speedups in track building from mkFit imply that track fitting becomes a comparably time consuming step of the tracking chain. Prospects for an mkFit implementation of the track fit will also be discussed.

        Speaker: Tadel, Matevz (UCSD)
      • 11:30 AM
        traccc - a close to single-source track reconstruction demonstrator for CPU and GPU 15m

        Despite recent advances in optimising the track reconstruction problem for high particle multiplicities in high energy physics experiments, it remains one of the most demanding reconstruction steps in regards to complexity and computing ressources. Several attemps have been made in the past to deploy suitable algorithms for track reconstruction on hardware accelerators, often by tailoring the algorithmic strategy to the hardware design. This led in certain cases to algorithmic compromises, and often came along with simplified descriptions of detector geometry, input data and magnetic field.
        The traccc project is an R&D initiative of the ACTS common track reconstruction; it aims to provide a complete track reconstruction chain for both CPU and GPU architectures. Emphasis has been put on sharing as much common source code as possible while trying to avoid algorithmic and physics performance compromises. Within traccc, dedicated components have been developed that are usable on standard CPU and GPU architectures: an astraction layer for linear algebra operations that allows to customize the mathematical backend (algebra-plugin), a host and device memory management system (vecmem), a generic vector field library (covfie) for the magneic field description, and a geometry and propagation library (detray). They serve as building blocks of a fully developed track reconstruction demonstrator based on clustering (connected component labelling), space point formation, track seeding and combinatorial track finding.
        We present the concepts and implementation of the traccc demonstrator and classify the physics and computational performance on selected hardware using the Open Data Detector in an scenario minicking the HL-LHC run condition. In addition, we give insight in our attempts to use different native language and portability solutions for GPUs, and summarize our main findings during the development of the entire traccc project.

        Speaker: Krasznahorkay, Attila (CERN)
      • 11:45 AM
        GPU-based algorithms for primary vertex reconstruction at CMS 15m

        The high luminosity expected from the LHC during the Run 3 and, especially, the HL-LHC of data taking introduces significant challenges in the CMS event reconstruction chain. The additional computational resources needed to treat this increased quantity of data surpass the expected increase in processing power for the next years. In order to fit the projected resource envelope, CMS is re-inventing its online and offline reconstruction algorithms, with their execution on CPU+GPU platforms in mind. Track clustering and primary vertex reconstruction accounts today about 10% of the reconstruction chain at 200 pileup and involves similar computations over hundreds to thousands of reconstructed tracks. This makes it a natural candidate for the development of a GPU-based algorithm that parallelizes it dividing the work in blocks. In this contribution we discuss the physics performance as well as the runtime performance of a new vertex clustering algorithm CMS developed for heterogeneous plarforms. We'll show that the physics results achieved are better than the current CMS vertexing algorithm in production, that the algorithm is up to 8 times faster on CPU and runs as well on GPUs. We will also discuss the plans for using this algorithm in production in Run 3 and for extending it to make use of timing information provided by the CMS Phase-2 MIP Timing Detector (MTD).

        Speaker: Erice Cid, Carlos Francisco (Boston University (US))
      • 12:00 PM
        The Exa.TrkX Project 15m

        Building on the pioneering work of the HEP.TrkX project [1], Exa.TrkX developed geometric learning tracking pipelines that include metric learning and graph networks. These end-to-end pipelines capture the relationships between spacepoint measurements belonging to a particle track. We tested the pipelines on simulated data from HL-LHC tracking detectors [2,5], Liquid Argon TPCs for neutrino experiments [3,8], and the straw tube tracker of the PANDA experiment[4]. The HL-LHC pipeline provides state-of-the-art tracking performance (Fig. 2), scales linearly with spacepoint density (Fig. 1), and has been optimized to run end-to-end on GP-GPUs, achieving a 20x speed-up with respect to the baseline implementation [6,9].
        The Exa.TrkX geometric learning approach also has shown promise in less traditional tracking applications, like large-radius tracking for new physics searches at the LHC [7].
        Exa.TrkX also contributed to developing and optimizing common data formats for ML training and inference targeting both neutrino detectors and LHC trackers.

        When applied to LArTPC neutrino experiments, the Exa.TrkX message-passing graph neural network classifies nodes, defined as the charge measurements or hits, according to the underlying particle type that produced them (Fig 3). Thanks to special 3D edges, our network can connect nodes within and across wire planes and achieve 94% accuracy with 96% consistency across wire planes [8].
        From the very beginning, the Exa.TrkX project has functioned as a collaboration open beyond its three original institutions (CalTech, FNAL, and LBNL). We released the code associated with every publication and produced tutorials and quickstart examples to test our pipeline.
        Eight US universities and six international institutions have contributed significantly to our research program and publications. The collaboration currently includes members of the ATLAS, CMS, DUNE, and PANDA experiments. Members of the FNAL muon g-2 experiment and CERN MUonE projects have tested the Exa.TrkX pipeline on their datasets.

        Exa.TrkX profits from multi-year partnerships with related research projects, namely the ACTS common tracking software, the ECP ExaLearn project, the NSF A3D3 institute, and the Fast ML Lab. More recently, as our pipeline matured and became applicable to more complex datasets, we started a partnership with HPE Lab, which uses our pipeline as a benchmark for its hyperparameter optimization and common metadata framework. NVIDIA (through the NERSC NESAP program) is evaluating the Exa.TrkX pipeline as an advanced use case for their R&D in Graph neural networks optimization.
        At this stage of the project, a necessary focus of the Exa.TrkX team is on consolidation and dissemination of the results obtained so far. We are re-engineering the LHC pipeline to improve its modularity and usability across experiment frameworks. We aim to integrate our pipelines with online and offline reconstruction chains of neutrino and collider detectors and release a repository of production-quality HEP pattern recognition models that can be readily composed into an experiment-specific pipeline.
        We are investigating heterogeneous graph networks to improve our pipelines' physics performance and make our models more easily generalizable [11]. Heterogeneity allows mixing and matching information from multiple detector geometries and types (strips vs. pixels, calorimeters vs. trackers vs. timing detectors, etc.).
        We have demonstrated that it is possible to recover “difficult” tracks (e.g., tracks with a missing spacepoint) by using hierarchical graph networks [10]. Next, we need to scale these models to more challenging datasets, including full HL-LHC simulations.
        We are also investigating how to parallelize our pipeline across multiple GPUs. Data parallelism for graph networks is an active research area in geometric learning. The unique setting of our problem, with large graphs that change structure with every event, makes parallelizing the inference step particularly challenging.
        A future research project's ultimate goal would be to combine these four R&D threads into a generic pipeline for HEP pattern recognition that operates on heterogeneous data at different scales, from raw data to particles.

        [1 ]Farrell, S., Calafiura, P., et al. . Novel deep learning methods for track reconstruction. (2018). arXiv. https://doi.org/10.48550/arXiv.1810.06111

        [2] Ju, X., Murnane, D., et al. Performance of a geometric deep learning pipeline for HL-LHC particle tracking. Eur. Phys. J. C 81, 876 (2021). https://doi.org/10.1140/epjc/s10052-021-09675-8

        [3] Hewes, J., Aurisano, A., et al. Graph Neural Network for Object Reconstruction in Liquid Argon Time Projection Chambers. EPJ Web of Conferences 251, 03054 (2021).
        https://doi.org/10.1051/epjconf/202125103054

        [4] Akram, A., & Ju, X. Track Reconstruction using Geometric Deep Learning in the Straw Tube Tracker (STT) at the PANDA Experiment. (2022) arXiv. https://doi.org/10.48550/arXiv.2208.12178

        [5] Caillou, S., Calafiura, P. et al. ATLAS ITk Track Reconstruction with a GNN-based pipeline. (2022). ATL-ITK-PROC-2022-006. https://cds.cern.ch/record/2815578

        [6] Lazar, A., Ju, X., et al. Accelerating the Inference of the Exa.TrkX Pipeline. (2022). arXiv. https://doi.org/10.48550/arXiv.2202.06929

        [7] Wang, C., Ju, X., et al. Reconstruction of Large Radius Tracks with the Exa.TrkX pipeline. (2022). arXiv. https://doi.org/10.48550/arXiv.2203.08800

        [8] Gumpula, K., et al., Graph Neural Network for Three Dimensional Object Reconstruction in Liquid Argon Time Projection Chambers. (2022). Presented at the Connecting the Dots 2022 workshop.
        https://indico.cern.ch/event/1103637/contributions/4821839

        [9] Acharya, N., Liu, E., Lucas, A., Lazar, A. Optimizing the Exa.TrkX Inference Pipeline for Manycore CPUs. (2022). Presented at the Connecting the Dots 2022 workshop. https://indico.cern.ch/event/1103637/contributions/4821918

        [10] Liu, R., Murnane, D., et al. Hierarchical Graph Neural Networks for Particle Reconstruction. (2022). Presented at the ACAT 2022 conference. https://indico.cern.ch/event/1106990/contributions/4996236/

        [11] Murnane, D., Caillou, S.,. Heterogeneous GNN for tracking. (2022). Presented at the Princeton Mini-workshop on Graph Neural Networks for Tracking. https://indico.cern.ch/event/1128328/contributions/4900744

        Speaker: Calafiura, Paolo (LBNL)
      • 12:15 PM
        Faster simulated track reconstruction in the ATLAS Fast Chain 15m

        The production of simulated datasets for use by physics analyses consumes a large fraction of ATLAS computing resources, a problem that will only get worse as increases in the instantaneous luminosity provided by the LHC lead to more collisions per bunch crossing (pile-up). One of the more resource-intensive steps in the Monte Carlo production is reconstructing the tracks in the ATLAS Inner Detector (ID), which takes up about 60% of the total detector reconstruction time [1]. This talk discusses a novel technique called track overlay, which substantially speeds up the ID reconstruction. In track overlay the pile-up ID tracks are reconstructed ahead of time and overlaid onto the ID tracks from the simulated hard-scatter event. We present our implementation of this track overlay approach as part of the ATLAS Fast Chain simulation, as well as a method for deciding in which cases it is possible to use track overlay in the reconstruction of simulated data without performance degradation.

        [1] ATL-PHYS-PUB-2021-012 (60% refers to Run3, mu=50, including large-radius tracking, p11)

        Speaker: Dr Leight, William (University of Massachusetts, Amherst)
    • 11:00 AM 12:30 PM
      Track 4 - Distributed Computing: Analysis Workflows, Modeling and Optimisation Marriott Ballroom II-III

      Marriott Ballroom II-III

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Barreiro Megino, Fernando (Unive) , Joshi, Rohini (SKAO)
      • 11:00 AM
        Distributed Machine Learning with PanDA and iDDS in LHC ATLAS 15m

        Machine learning has become one of the important tools for High Energy Physics analysis. As the size of the dataset increases at the Large Hadron Collider (LHC), and at the same time the search spaces become bigger and bigger in order to exploit the physics potentials, more and more computing resources are required for processing these machine learning tasks. In addition, complex advanced machine learning workflows are developed in which one task may depend on the results of previous tasks. How to make use of vast distributed CPUs/GPUs in WLCG for these big complex machine learning tasks has become a popular area. In this presentation, we will present our efforts on distributed machine learning in PanDA and iDDS (intelligent Data Delivery Service). We will at first address the difficulties to run machine learning tasks on distributed WLCG resources. Then we will present our implementation with DAG (Directed Acyclic Graph) and sliced parameters in iDDS to distribute machine learning tasks to distributed computing resources to execute them in parallel through PanDA. Next we will demonstrate some use cases we have implemented, such as Hyperparameter Optimization, Monte Carlo Toy confidence limits calculation and Active Learning. Finally we will describe some directions to perform in the future.

        Speaker: Weber, Christian (Brookhaven National Laboratory)
      • 11:15 AM
        ATLAS data analysis using a parallelized workflow on distributed cloud-based services with GPUs 15m

        We present a new implementation of simulation-based inference using data collected by the ATLAS experiment at the LHC. The method relies on large ensembles of deep neural networks to approximate the exact likelihood. Additional neural networks are introduced to model systematic uncertainties in the measurement. Training of the large number of deep neural networks is automated using a parallelized workflow with distributed computing infrastructure integrated with cloud-based services. We will show an example workflow using the ATLAS PanDA framework integrated with GPU infrastructure from Google Cloud Platform. Numerical analysis of the neural networks is optimized with JAX and JIT. The novel machine-learning method and cloud-based parallel workflow can be used to improve the sensitivity of several other analyses of LHC data.

        Speaker: Sandesara, Jay (University of Massachusetts, Amherst)
      • 11:30 AM
        Modelling Distributed Heterogeneous Computing Infrastructures for HEP Applications 15m

        Predicting the performance of various infrastructure design options in complex federated infrastructures with computing sites distributed over a wide area that support a plethora of users and workflows, such as the Worldwide LHC Computing Grid (WLCG), is not trivial. Due to the complexity and size of these infrastructures, it is not feasible to deploy experimental test-beds at large scales merely for the purpose of comparing and evaluating alternate designs.

        An alternative is to simulate the behaviours of these systems based on realistic simulation models. This approach has been used successfully in the past to identify efficient and practical infrastructure designs for High Energy Physics (HEP). A prominent example is the Monarc simulation framework, which was used to study the initial structure of the WLCG. However, new simulation capabilities are needed to simulate large-scale heterogeneous infrastructures with complex networks as well as application behaviours that include various data access and caching patterns.

        In this context, a modern tool to simulate high energy physics workloads that execute on distributed computing infrastructures based on the SimGrid and WRENCH simulation frameworks is outlined. Studies of its accuracy and scalability are presented using HEP as a case-study.

        Speaker: Mr Horzela, Maximilian (Karlsruhe Institute of Technology)
      • 11:45 AM
        Digital Twin Engine Infrastructure in the interTwin Project 15m

        InterTwin is an EU-funded project that started on the 1st of September 2022. The project will work with domain experts from different scientific domains in building a technology to support digital twins within scientific research. Digital twins are models for predicting the behaviour and evolution of real-world systems and applications.

        InterTwin will focus on employing machine-learning techniques to create and train models that are able to quickly and accurately reflect their physical counterparts in a broad range of scientific domains. The project will develop, deploy and “road harden” a blueprint for supporting digital twins on federated resources. For that purpose, it will support a diverse set of science use-cases, in the domains of radio telescopes (Meerkat), particle physics (CERN/LHC and Lattice-QCD), gravitational waves (Virgo), as well as climate research and environment monitoring (e.g. prediction of flooding and other extreme weather due to climate change). The ultimate goal is to provide a flexible infrastructure that can accommodate the needs of many additional scientific fields.

        In the talk, we will present an overview of the interTwin project along with the corresponding Digital Twin Engine (DTE) architecture for federating the different, heterogeneous resources available to the scientific use-cases (storage, HPC, HTC, quantum) when training and exploitation of digital twins within the different scientific domains. The challenges faced when designing the architecture will be described, along with the solutions being developed to address them. interTwin is required to be interoperable with other infrastructures, including EuroHPC-based Destination Earth Initiative (DestinE) and an infrastructure for accessing Copernicus satellite data, C-SCALE. We will also present our strategy for making DTE available within the European Open Science Cloud (EOSC). The details of all such interoperability will also be presented.

        Speaker: Fuhrmann, Patrick (DESY)
      • 12:00 PM
        IceCube SkyDriver - A SaaS Solution for Event Reconstruction using the Skymap Scanner 15m

        The IceCube Neutrino Observatory is a cubic kilometer neutrino telescope located at the geographic South Pole. To accurately and promptly reconstruct the arrival direction of candidate neutrino events for Multi-Messenger Astrophysics use cases, IceCube employs Skymap Scanner workflows managed by the SkyDriver service. The Skymap Scanner performs maximum-likelihood tests on individual pixels generated from the Hierarchical Equal Area isoLatitude Pixelation (HEALPix) algorithm. Each test is computationally independent, which allows for massive parallelization. This workload is distributed using the Event Workflow Management System (EWMS)—a message-based workflow management system designed to scale to trillions of pixels per day. SkyDriver orchestrates multiple distinct Skymap Scanner workflows behind a REST interface, providing an easy-to-use reconstruction service for real-time candidate, cataloged, and simulated events. Here, we outline the SkyDriver service technique and the initial development of EWMS.

        Speaker: Evans, Ric (IceCube, University of Wisconsin-Madison)
      • 12:15 PM
        Analysis Grand Challenge benchmarking tests on selected sites 15m

        A fast turn-around time and ease of use are important factors for systems supporting the analysis of large HEP data samples. We study and compare multiple technical approaches.
        This presentation will be about setting up and benchmarking the Analysis Grand Challenge (AGC) [1] using CMS Open Data. The AGC is an effort to provide a realistic physics analysis with the intent of showcasing the functionality, scalability and feature-completeness of the Scikit-HEP Python ecosystem.
        I will present the results of setting up the necessary software environment for the AGC and benchmarking the analysis' runtime on various computing clusters: the institute SLURM cluster at my home institute, LMU Munich, a SLURM cluster at LRZ (WLCG Tier-2 site) and the analysis facility Vispa [2], operated by RWTH Aachen.
        Each site provides slightly different software environments and modes of operation which poses interesting challenges on the flexibility of a setup like that intended for the AGC.
        Comparing these benchmarks to each other also provides insights about different storage and caching systems. At LRZ and LMU we have regular Grid storage (HDD) as well as and SSD-based XCache server and on Vispa a sophisticated per-node caching system is used.

        [1] https://github.com/iris-hep/analysis-grand-challenge
        [2] https://vispa.physik.rwth-aachen.de/

        Speaker: Koch, David (LMU)
    • 11:00 AM 12:30 PM
      Track 5 - Sustainable and Collaborative Software Engineering: Sustainable Languages and Architectures Chesapeake Meeting Room

      Chesapeake Meeting Room

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Sailer, Andre (CERN) , Sexton, Elizabeth (FNAL)
      • 11:00 AM
        Is Julia ready to be adopted by HEP? 15m

        The Julia programming language was created 10 years ago and is now a mature and stable language with a large ecosystem including more than 8,000 third-party packages. It was designed for scientific programming to be a high-level and dynamic language as Python is, while achieving runtime performances comparable to C/C++ or even faster. With this, we ask ourselves if the Julia language and its ecosystem is ready now for its adoption by the High Energy Physics community. We will report on a number of investigations and studies of the Julia language that have been done for various representative HEP applications, ranging from computing intensive initial data processing of experimental data and simulation, to final interactive data analysis and plotting. Aspects of collaborative code development of large software within a HEP experiment has also been investigated: scalability with large development teams, continuous integration and code test, code reuse, language interoperability to enable a adiabatic migration of packages and tools, software installation and distribution, training of the community, benefit from development from industry and academia from other fields.

        Speaker: Gál, Tamás (Erlangen Centre for Astroparticle Physics)
      • 11:15 AM
        Polyglot Jet Finding 15m

        The evaluation of new computing languages for a large community, like HEP, involves comparison of many aspects of the languages' behaviour, ecosystem and interactions with other languages. In this paper we compare a number of languages using a common, yet non-trivial, HEP algorithm: the tiled $N^2$ clustering algorithm used for jet finding. We compare specifically the algorithm implemented in Python, using numpy, Julia and Rust, with respect to the reference implementation in C++, from Fastjet. As well as the speed of the implementation we describe the ergonomics of the language for the coder, as well as the efforts required to achieve the best performance, which can directly impact on code readability and sustainability.

        Speaker: Stewart, Graeme (CERN)
      • 11:30 AM
        The ATLAS experiment software on ARM 15m

        With an increased dataset obtained during the Run-3 of the LHC at CERN and the even larger expected increase of the dataset by more than one order of magnitude for the HL-LHC, the ATLAS experiment is reaching the limits of the current data processing model in terms of traditional CPU resources based on x86_64 architectures and an extensive program for software upgrades towards the HL-LHC has been set up. The ARM architecture is becoming a competitive and energy efficient alternative. Some surveys indicate its increased presence in HPCs and commercial clouds, and some WLCG sites have expressed their interest. Chip makers are also developing their next generation solutions on ARM architectures, sometimes combining ARM and GPU processors in the same chip. Therefore it is important that the Athena software embraces the change and is able to successfully exploit this architecture.

        We report on the successful port of the ATLAS experiment offline and online software framework Athena to ARM and the successful physics validation of simulation workflows. For this we have set up an ATLAS Grid site using ARM compatible middleware and containers on Amazon Web Services (AWS) ARM resources. The ARM version of Athena is fully integrated in the regular software build system and distributed like default software releases. In addition, the workflows have been integrated into the HepScore benchmark suite which is the planned WLCG wide replacement of the HepSpec06 benchmark used for Grid site pledges. In the overall porting process we have used resources on AWS, Google Cloud Platform (GCP) and CERN. A performance comparison of different architectures and resources will be discussed.

        Speaker: Elmsheuser, Johannes (Brookhaven National Laboratory)
      • 11:45 AM
        Multilanguage Frameworks 15m

        High Energy Physics software has been a victim of the necessity to choose one implementation language as no really usable multi-language environment existed. Even a co-existence of two languages in the same framework (typically C++ and Python) imposes a heavy burden on the system. The role of different languages was generally limited to well encapsulated domains (like Web applications, databases, graphics), with very limited connection to the central framework.

        The new development in the domain of the compilers and run-time environments has enabled ways for creating really multilanguage frameworks, with seamless, user-friendly and high-performance inter-operation of many languages, which traditionally live in disconnected domains (like C-based languages vs JVM languages or Web languages).

        Various possibilities and strategies for creation of the true multi-language frameworks will be discussed, emphasizing their advantages and possible road blocks.

        A prototype of massively multilanguage application will be presented, using very wide spectrum of languages working together (C++, Python, JVM languages, JavaScript,...). Each language will be used in the domain where it offers a strong comparative advantage (speed, user-friendliness, availability of third-party libraries and tools, graphical and web capabilities).

        The performance gain from the modern multi-language environments will be also demonstrated, as well as gains in the overall memory footprint.

        Possibilities of converting existing HEP frameworks into multilanguage environments will be discussed in concrete examples and demonstrations.

        A real life example of widely multilanguage environment will be demonstrated on the case of the multi-language access to the data storage of the LSST telescope Fink project.

        Speaker: Hrivnac, Julius (IJCLab)
      • 12:00 PM
        User-Centered Design for the Electron-Ion Collider 15m

        Software and computing are an integral part of our research. According to the survey for the “Future Trends in Nuclear Physics Computing” workshop in September 2020, students and postdocs spent 80% of their time on the software and computing aspects of your research. For the Electron-Ion Collider, we are looking for ways to make software (and computing) "easier" to use. All scientists of all levels worldwide should be empowered to participate in Electron-Ion Collider simulations and analyses actively.

        In this presentation, we will summarize our work on user-centered design for the Electron-Ion Collider. We have collected information on the community's specific software tools and practices on an annual basis. We have also organized focus group discussions with the broader community and developed user archetypes based on the feedback from the focus groups. The user archetypes represent a common class of users and provide input to software developers as to which users they are writing software for and help with structuring documentation.

        Speaker: Diefenthaler, Markus (Jefferson Lab)
      • 12:15 PM
        Train to Sustain 15m

        The HSF/IRIS-HEP Software Training group provides software training skills to new researchers in High Energy Physics (HEP) and related communities. These skills are essential to produce high-quality and sustainable software needed to do the research. Given the thousands of users in the community, sustainability, though challenging, is the centerpiece of its approach. The training modules are open source and collaborative. Different tools and platforms, like GitHub, enable technical continuity, collaboration and nurture the sense to develop software that is reproducible and reusable. This contribution describes these efforts.

        Speaker: Malik, Sudhir (University of Puerto Rico Mayaguez)
    • 11:00 AM 12:30 PM
      Track 6 - Physics Analysis Tools: Statistical Inference and Fitting Hampton Roads Ballroom VIII

      Hampton Roads Ballroom VIII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Hageboeck, Stephan (CERN) , Held, Alexander (University of Wisconsin–Madison)
      • 11:00 AM
        RooFit's new heterogeneous computing backend 15m

        RooFit is a library for building and fitting statistical models that is part of ROOT. It is used in most experiments in particle physics, in particular, the LHC experiments. Recently, the backend that evaluates the RooFit likelihood functions was rewritten to support performant computations of model components on different hardware. This new backend is referred to as the "batch mode". So far, it supports GPUs with CUDA and also the vectorizing instructions on the CPU. With ROOT 6.28, the new batch mode is feature-complete and speeds up all use cases targeted by RooFit, even on a single CPU thread. The GPU backend further reduces the likelihood evaluation time, particularly for unbinned fits to large datasets. The speedup is most significant when all likelihood components support GPU evaluation. Still, if this is not the case, the backend will optimally distribute the computation on the CPU and GPU to guarantee a speedup.

        RooFit is a very extensible library with a vast user interface to inject behavior changes at almost every point of the likelihood calculation, which the new heterogeneous computation backend must handle. This presentation discusses our approach and lessons learned when facing this challenge. The highlight of this contribution is showcasing the performance improvements for benchmark examples, fits from the RooFit tutorials, and real-world fit examples from LHC experiments. We will also elaborate on how users can implement GPU support for their custom probability density functions and explain the current limitations and future developments.

        Speaker: Rembser, Jonas (CERN)
      • 11:15 AM
        Making Likelihood Calculations Fast: Automatic Differentiation Applied to RooFit 15m

        With the growing datasets of current and next-generation High-Energy and Nuclear Physics (HEP/NP) experiments, statistical analysis has become more computationally demanding. These increasing demands elicit improvements and modernizations in existing statistical analysis software. One way to address these issues is to improve parameter estimation performance and numeric stability using automatic differentiation (AD). AD's computational efficiency and accuracy is superior to the preexisting numerical differentiation techniques and offers significant performance gains when calculating the derivatives of functions with a large number of inputs, making it particularly appealing for statistical models with many parameters. For such models, many HEP/NP experiments use RooFit, a toolkit for statistical modeling and fitting that is part of ROOT.

        In this talk, we report on the effort to support the AD of RooFit likelihood functions. Our approach is to extend RooFit with a tool that generates overhead-free C++ code for a full likelihood function built from RooFit functional models. Gradients are then generated using Clad, a compiler-based source-code-transformation AD tool, using this C++ code. We present our results from applying AD to the entire minimization pipeline and profile likelihood calculations of several RooFit and HistFactory models at the LHC-experiment scale. We show significant reductions in calculation time and memory usage for the minimization of such likelihood functions. We also elaborate on this approach's current limitations and explain our plans for the future.

        This contribution combines R&D expertise from computer science applied at scale for HEP/NP analysis: we demonstrate that source-transformation-based AD can be incorporated into complex, domain-specific codes such as RooFit to give substantial performance and scientific capability improvements.

        Speaker: Singh, Garima (Princeton University (US)/CERN)
      • 11:30 AM
        Build-a-Fit: RooFit configurable parallelization and fine-grained benchmarking tools for order of magnitude speedups in your fits 15m

        RooFit is a toolkit for statistical modeling and fitting, presented first at CHEP2003, and together with RooStats is used for measurements and statistical tests by most experiments in particle physics, particularly the LHC experiments.

        As the LHC program progresses, physics analyses become more ambitious and computationally more demanding, with fits of hundreds of data samples to joint models with over a thousand parameters no longer an exception. While such complex fits can be robustly performed in RooFit, they may take many hours on a single CPU, significantly impeding the ability of physicists to interactively understand, develop and improve them. Here were present recent RooFit developments to address this, focusing on significant improvements of wall-time performance of complex fits.

        A complete rewrite of the internal back-end of the RooFit likelihood calculation code in ROOT 6.28 now allows to massively parallelize RooFit likelihood fits in two ways. Gradients that are normally serially calculated inside MINUIT, and which dominate the total fit time, are now calculated in a parallel way inside RooFit. Furthermore, calculations of the likelihood in serial phases of the minimizer (initialization and gradient descent steps) are also internally parallelized. No modification of any user code is required to take advantage of these features.

        A key to achieving good scalability for these parallel calculations is close to perfect load balancing over the workers, which is complicated by the fact that for realistic complex fit models the calculations to parallelize cannot be split in components of equal or even comparable size. As part of this update, instruments have been added to RooFit for extensive performance monitoring that allow the user to understand the effect of algorithmic choices in task scheduling and mitigate performance bottlenecks.

        We will show that that with a new dynamic scheduling strategy and a strategic choice of ordering derivative calculations excellent scalability can be achieved, resulting in an order-of-magnitude wall-time speedups for complex realistic LHC fits such as the ATLAS Run-2 combined Higgs interpretation.

        Speaker: Wolffs, Zef (Nikhef)
      • 11:45 AM
        New developments in Minuit2 15m

        Minuit is a program implementing a function minimisation algorithm written at CERN more than 50 years ago. It is still used by almost all statistical analysis in High Energy Physics to find optimal likelihood and best parameter values. A new version, Minuit2, has been re-implemented the original algorithm in C++ a few years ago and it is provided as a ROOT library or a standalone C++ module. It is also available as a Python package, IMinuit.
        This new version has been recently improved by adding some new features. These include support for external gradients and hessian, allowing the use of Automatic Differentiation techniques or parallel computation of the gradients and the addition of new minimisation algorithms such as BFGS and Fumili. We will present an overview of the new implementation showing the new added features and we will as well present a comparison with other existing minimisation packages, available in C++ or in the Python scientific ecosystem.

        Speaker: Moneta, Lorenzo (CERN)
      • 12:00 PM
        Bayesian methodologies in particle physics with pyhf 15m

        Collider physics analyses have historically favored Frequentist statistical methodologies, with some exceptions of Bayesian inference in LHC analyses through use of the Bayesian Analysis Toolkit (BAT). We demonstrate work towards an approach for performing Bayesian inference for LHC physics analyses that builds upon the existing APIs and model building technology of the pyhf and PyMC Python libraries and leverages pyhf’s automatic differentiation and hardware acceleration through its JAX computational backend. This approach presents a path toward unified APIs in pyhf that allow for users to choose a Frequentist or Bayesian approach towards statistical inference, leveraging their respective strengths as needed, without having to transition between using multiple libraries or fall back to using pyhf with BAT through the Julia programming language PyCall package. Examples of Markov chain Monte Carlo implementations using Metropolis-Hastings and Hamiltonian Monte Carlo are presented.

        Speaker: Horstmann, Malin (TU Munich / Max Planck Institute for Physics)
      • 12:15 PM
        A multidimensional, event-by-event, statistical weighting procedure for signal to background separation 15m

        Many current analyses in nuclear and particle physics are in search for signals that are encompassed by irreducible background events. These background events, entirely surrounding a signal of interest, would lead to inaccurate results when extracting physical observables from the data, due to the inability to reduce the signal to background ratio using any type of selection criteria. By looking at a data set in multiple dimensions, the phase space of a desired reaction can be characterized by a set of coordinates, where a subset of these coordinates (known as reference coordinates) contains a distinguishable distribution where the signal and background can easily be determined. The approach then uses the space defined by the non-reference coordinates, to determine the k-nearest neighbors of an event, where these events can then be fit on the reference coordinates of these k-nearest neighbors (using an unbinned maximum likelihood fit, etc.). From the fit, a quality factor can be defined for each event in the data set that states the probability that it originates from the actual signal of interest. The unique aspect of this procedure requires no a priori information of the signal or background distributions within the phase space in the desired reaction. This and many other useful properties for this statistical weighting procedure makes this method more advantageous in certain analyses than other methods. A detailed overview of this procedure will be shown along with examples using Monte Carlo and GlueX data.

        Speaker: Baldwin, Zachary (Carnegie Mellon University)
    • 11:00 AM 12:30 PM
      Track 7 - Facilities and Virtualization: Dynamic Provisioning and Anything-As-A-Service Marriott Ballroom IV

      Marriott Ballroom IV

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Kishimoto, Tomoe (KEK) , Weitzel, Derek (University of Nebraska-Lincoln)
      • 11:00 AM
        Securing an Open and Trustworthy Ecosystem for Research Infrastructure and Applications (SOTERIA) 15m

        Managing a secure software environment is essential to a trustworthy cyberinfrastructure. Software supply chain attacks may be a top concern for IT departments, but they are also an aspect of scientific computing. The threat to scientific reputation caused by problematic software can be just as dangerous as an environment contaminated with malware. The issue of managing environments affects any individual researcher performing computational research but is more acute for multi-institution scientific collaborations, such as high energy physics experiments, as they often preside over complex software stacks and must manage software environments across many distributed computing resources. We discuss a new project, Securing an Open and Trustworthy Ecosystem for Research Infrastructure and Applications (SOTERIA), to provide the HEP community with a container registry service and provide additional capabilities to assist with vulnerability assessment, authorship and provenance, and distribution. This service is currently being used to deliver containers for a wide range of the OSG Fabric of Services, the Coffea-Casa analysis facility, and the Analysis Facility at the University of Chicago; we discuss both the functionality it currently provides and the operational experiences of running a critical service for scientific cyberinfrastructure.

        Speaker: Bockelman, Brian (Morgridge Institute for Research)
      • 11:15 AM
        Modular toolsets for integrating HPC clusters in experiment control systems 15m

        New particle/nuclear physics experiments require a massive amount of computing power that is only achieved by using high performance clusters directly connected to the data acquisition systems and integrated into the online systems of the experiments. However, integrating an HPC cluster into the online system of an experiment means: Managing and synchronizing thousands of processes that handle the huge throughput. In this work, modular components that can be used to build and integrate such a HPC cluster in the experiment control systems (ECS) will be introduced.

        The Online Device Control library (ODC) [1] in combination with the Dynamic Deployment System (DDS) [2, 3] and FairMQ [4] message queuing library offers a sustainable solution for integrating HPC cluster controls into an ECS.

        DDS as part of the ALFA framework [5] is a toolset that automates and significantly simplifies a dynamic deployment of user-defined processes and their dependencies on any resource management system (RMS) using a given process graph (topology). Where ODC is the tool to control and communicate with a topology of FairMQ processes using DDS. ODC is designed to act as a broker between a high level experiment control system and a low level task management system e.g.: DDS.

        In this presentation the architecture of both DDS and ODC will be discussed, as well as the design decisions taken based on the experience gained of using these tools on production by the ALICE experiment at CERN to deploy and control thousands of processes (tasks) on the Event Processing Nodes cluster (EPN) during Run3 as a part of the ALICE O2 software ecosystem [6].

        References:
        1. FairRootGroup, “ODC git repository”, Last accessed 14th of November 2022: https://github.com/FairRootGroup/ODC
        2. FairRootGroup, “DDS home site”, Last accessed 14th of November 2022: http://dds.gsi.de
        3. FairRootGroup, “DDS source code repository”, Last accessed 14th of November 2022: https://github.com/FairRootGroup/DDS
        4. FairMQ, “FairMQ git repository”, Last accessed 14th of November 2022: https://github.com/FairRootGroup/FairMQ
        5.https://indico.gsi.de/event/2715/contributions/11355/attachments/8580/10508/ALFA_Fias.pdf
        5. ALICE Technical Design Report (2nd of June 2015), Last accessed 14th of November: https://cds.cern.ch/record/2011297/files/ALICE-TDR-019.pdf

        Speaker: Dr Al-Turany, Mohammad (GSI)
      • 11:30 AM
        Federated Heterogenous Compute and Storage Infrastructure for the PUNCH4NFDI Consortium 15m

        PUNCH4NFDI, funded by the Germany Research Foundation initially for five years, is a diverse consortium of particle, astro-, astroparticle, hadron and nuclear physics embedded in the National Research Data Infrastructure initiative.

        In order to provide seamless and federated access to the huge variaty of compute and storage systems provided by the participating communities covering their very diverse needs, the Compute4PUNCH and Storage4PUNCH concepts have been developed. Both concepts comprise state-of-the-art technolgies such as a token-based AAI for standardised access to compute and storage resources. The community supplied heterogenous HPC, HTC and Cloud compute resources are dynamically and transparently integrated into one federated HTCondor based overlay batch system using the COBaLD/TARDIS resource meta-scheduler. Traditional login nodes and a JupyterHub provide entry points into the entire landscape of available compute resources, while container technologies and the CERN Virtual Machine File System (CVMFS) ensure a scalable provisioning of community specific software environments. In Storage4PUNCH, community supplied storage systems mainly based on dCache or XRootD technology are being federated in a common infrastructure employing methods that are well established in the wider HEP community. Furthermore existig technologies for caching as well as metadata handling are being evaluated with the aim for a deeper integration. The combined Compute4PUNCH and Storage4PUNCH environment will allow a large variety of researchers to carry out resource-demanding analysis tasks.

        In this contribution we will present the Compute4PUNCH and Storage4PUNCH concepts, the current status of the developments as well as first experiences with scientific applications being executed on the available prototypes.

        Speaker: Dr Giffels, Manuel (Karlsruher Institut für Technologie (KIT))
      • 11:45 AM
        Progress on cloud native solution of Machine Learning as Service for HEP 15m

        Nowadays Machine Learning (ML) techniques are successfully used in many areas of High-Energy Physics (HEP) and will play a significant role also in the upcoming High-Luminosity LHC upgrade foreseen at CERN, when a huge amount of data will be produced by LHC and collected by the experiments, facing challenges at the exascale. To favor the usage of ML in HEP analyses, it would be useful to have a service allowing to perform the entire ML pipeline (in terms of reading the data, processing data, training a ML model, and serving predictions) directly using ROOT files of arbitrary size from local or remote distributed data sources. The MLaaS4HEP solution we have already proposed aims to provide such kind of service and to be HEP experiment agnostic. Recently new features have been introduced, such as the possibility to provide pre-processing operations, defining new branches, and applying cuts. To provide users with a real service and to integrate it into the INFN Cloud, we started working on MLaaS4HEP cloudification. This would allow to use cloud resources and to work in a distributed environment. In this work, we provide updates on this topic and discuss a working prototype of the service running on INFN Cloud. It includes an OAuth2 proxy server as authentication/authorization layer, a MLaaS4HEP server, an XRootD proxy server for enabling access to remote ROOT data, and the TensorFlow as a Service (TFaaS) service in charge of the inference phase. With this architecture a HEP user can submit ML pipelines, after being authenticated and authorized, using local or remote ROOT files simply using HTTP calls.

        Speaker: Giommi, Luca (INFN Bologna)
      • 12:00 PM
        Demand-driven provisioning of Kubernetes-like resource in OSG 15m

        The OSG-operated Open Science Pool is an HTCondor-based virtual cluster that aggregates resources from compute clusters provided by several organizations. A user can submit batch jobs to the OSG-maintained scheduler, and they will eventually run on a combination of supported compute clusters without any further user action. Most of the resources are not owned by, or even dedicated to OSG, so demand-based dynamic provisioning is important for maximizing usage without incurring excessive waste.
        OSG has long relied on GlideinWMS for most of its resource provisioning needs, but is limited to resources that provide a Grid-compliant Compute Entrypoint. To work around this limitation, the OSG software team had developed a pilot container that resource providers could use to directly contribute to the OSPool. The problem of that approach is that it is not demand-driven, relegating it to backfill scenarios only.
        To address this limitation, a demand-driven direct provisioner of Kubernetes resources has been developed and successfully used on the PRP. The setup still relies on the OSG-maintained backfill container images, it just automates the provisioning matchmaking and successive requests. That provisioner has also been recently extended to support Lancium, a green computing cloud provider with a Kubernetes-like proprietary interface. The provisioner logic had been intentionally kept very simple, making this extension a low cost project.
        Both PRP and Lancium resources have been provisioned exclusively using this mechanism for almost a year with great results.

        Speakers: Andrijauskas, Fabio , Schultz, David (IceCube, University of Wisconsin-Madison)
    • 11:00 AM 12:30 PM
      Track 8 - Collaboration, Reinterpretation, Outreach and Education: Tailored Collaboration and Training Initiatives Marriott Ballroom I

      Marriott Ballroom I

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Hernandez Villanueva, Michel (DESY) , Lange, Clemens (Paul Scherrer Institut)
      • 11:00 AM
        Involving the new generations in Fermilab endeavours 15m

        Since 1984 the Italian groups of the Istituto Nazionale di Fisica Nucleare (INFN) and Italian Universities, collaborating with the
        DOE laboratory of Fermilab (US) have been running a two-month summer training program for Italian university students. While
        in the first year the program involved only four physics students of the University of Pisa, in the following years it was extended
        to engineering students. This extension was very successful and the engineering students have been since then extremely well
        accepted by the Fermilab Technical, Accelerator and Scientific Computing Division groups. Over the many years of its existence,
        this program has proven to be the most effective way to engage new students in Fermilab endeavours. Many students have
        extended their collaboration with Fermilab with their Master Thesis and PhD.
        Since 2004 the program has been supported in part by DOE in the frame of an exchange agreement with INFN. Over its almost
        40 years of history, the program has grown in scope and size and has involved more than 550 Italian students from more than
        20 Italian Universities, A number of Institutes of Research, including ASI and INAF in Italy, and the ISSNAF Foundation in the
        US, have provided additional financial support. Since the program does not exclude appropriately selected non-italian students,
        a handful of students of European and non-European Universities were also accepted in the years.
        Each intern is supervised by a Fermilab Mentor responsible for performing the training program. Training programs spanned
        from Tevatron, CMS, Muon (g-2), Mu2e and Short Baseline Neutrino Experiments and DUNE design and experimental data
        analysis, development of particle detectors (silicon trackers, calorimeters, drift chambers, neutrino and dark matter detectors),
        design of electronic and accelerator components, development of infrastructures and software for tera-data handling, research
        on superconductive elements and on accelerating cavities, theory of particle accelerators
        Since 2010, within an extended program supported by the Italian Space Agency and the Italian National Institute of Astrophysics,
        a total of 30 students in physics, astrophysics and engineering have been hosted for two months in summer at US space
        science Research Institutes and laboratories.
        In 2015 the University of Pisa included these programs within its own educational programs. Accordingly, Summer School
        students are enrolled at the University of Pisa for the duration of the internship and are identified and ensured as such. At the
        end of the internship the students are required to write summary reports on their achievements. After positive evaluation by a
        University Examining Board, interns are acknowledged 6 ECTS credits for their Diploma Supplement.
        Information on student recruiting methods, on training programs of recent years and on final student's evaluation process at
        Fermilab and at the University of Pisa will be given in the presentation.
        In the ears 2020 and 2021 the Program has been canceled due to the persisting effects of the sanitary emergency which
        prevented researchers and students to travel to the United States. In 2022 the Program was successfully restarted and allowed
        a cohort of 21 students in physics and engineering to be trained for nine weeks at Fermilab. In the talk we will provide a detailed descriptions of the program, which can be easily taken as a model that can be easily adopted by interested Laboratories.

        Speaker: Mambelli, Marco (Fermilab)
      • 11:15 AM
        DUNE Computing Tutorials 15m

        Providing computing training to the next generation of physicists is the
        principal driver for a biannual multi-day workshop hosted by the DUNE
        Computing Consortium. Materials are cast in the Software Carpentries
        templates, and to date topics have included storage space, data
        management, LArSoft, grid job submission and monitoring. Moreover,
        experts provide extended breakout sessions to demonstrate the
        intricacies of the unique software used in HEP analysis. Each workshop
        session uses live documents for real time correspondence, and are
        captured on Zoom; afterwards, videos are embedded on the corresponding
        webpages for review. As a GitHub repository, shared editing of the
        learning modules is straightforward, and provides a trusted framework to
        extend to other training topics in the future. An overview of the
        machinery will be provided, post workshop statistics will be discussed,
        with lessons learned will be the focus of this presentation.

        Speaker: DeMuth, David (Valley City State University)
      • 11:30 AM
        A customized web application for XENON collaboration member management 15m

        The common form of inter-institute particle physics experiment collaborations generates unique needs for member management including paper authorship, shift assignments, subscription to mailing lists and access to 3rd party applications such as Github and Slack. For smaller collaborations, typically no facility for centralized member management is available and these needs are usually manually handled by long-term members in smaller collaborations but the management becomes tedious as collaborations grow. To automate many of these tasks for the expanding XENON collaboration, we developed the XENONnT User Management Website, a web application that stores and updates data related to the collaboration members through the use of NodeJs and MongoDB. The application allows for the scheduling of shifts for members to coordinate between institutes. User manipulation of 3rd party applications are implemented using REST API integration. The XENONnT User Management Website is open source and is a show case of quick implementation of utility application using the web framework.

        Speaker: Liang, Shixiao (Rice University)
      • 11:45 AM
        Training and on-boarding initiatives in HEP 15m

        We will discuss the training and on-boarding initiatives currently adopted by a range of High Energy Physics (HEP) experiments. On-boarding refers to the process by which new members of a collaboration gain the knowledge and skills needed to become effective members. Fast and efficient on-boarding is increasingly important for HEP experiments as physics analyses and, as a consequence, the related software becomes ever more complex with growing datasets. The HEP Software Foundation (HSF) held a meeting series in Summer 2022 where 6 LHC and non-LHC experiments showcased their initiatives. Here we summarise and analyse these initiatives and attempt to determine a set of best practices for current and future experiments.

        Speaker: Reinsvold Hall, Allison (US Naval Academy)
      • 12:00 PM
        Building International Research Software Collaborations in Physics 15m

        Building successful multi-national collaborations is challenging. The scientific communities in a range of physical sciences have been learning how to build collaborations that build upon regional capabilities and interests over decades, iteratively with each new generation of large scientific facilities required to advance their scientific knowledge. Much of this effort has naturally focused on collaborations for the construction of hardware and instrumentation. Software has however also become a critical element to design and maximize the physics discovery potential of large data intensive science projects. To fully realize their discovery potential a new generation of software algorithms and approaches is required. Building these research software collaborations is challenging and inherently international, matching the international nature of the experimental undertakings themselves. Initiatives such as the HEP Software Foundation have been instrumental in establishing international research software collaborations in high-energy physics, in particular between European and North American researchers.

        This talk is about a new initiative, HSF-India, aiming to implement new and impactful research software collaborations between India, Europe and the U.S. The experimental scope of this project is relatively broad, aiming to bring together researchers across facilities with common problems in research. The research and development scope is on three primary topics: analysis software and integrated facilities for analysis; simulation techniques including generators and Artificial Intelligence based approaches; and enabling open science. By exploiting national capabilities and strengths, an immediate mutual benefit of the international collaboration will be a training network that enables early-career researchers to pursue impactful research software initiatives in ways that advance their careers in experimental data-intensive science. In this presentation, we will describe the scope of this initiative, its mechanisms for fostering new collaborations, and ways for interested research groups to get involved. We will also discuss thoughts towards broadening our initiative to foster more general collaborations in research software projects between Asian researchers and European/North American researchers who are already jointly pursuing “team-science” endeavors in research software for high-energy, nuclear and astro-particle physics.

        Speaker: Lange, David (Princeton University)
      • 12:15 PM
        Support for experiments at INFN-T1 15m

        The Italian WLCG Tier-1 located in Bologna and managed by INFN-CNAF has a long tradition in supporting several research communities in the fields of High-Energy Physics, Astroparticle Physics, Gravitational Waves, Nuclear Physics and others, to which provides computing resources in the form of batch computing, both HPC, HTC and Cloud, and storage. Although the LHC experiments at CERN represent the main users of the Tier-1 resources, an increasing number of communities and experiments are also being supported in all of their computing activities. Due to this demanding user base, an efficient support system is needed in order to assure a smooth and appropriate exploitation of the computing infrastructure.
        In this framework, such a role is played by the Tier-1 User Support group, which acts as the entry point for services, support requests, and problem reports. The group makes use of multiple systems to meet the different needs and specificities of the supported experiments. Moreover, the group continuously maintains detailed knowledge base in the form of an on-line user guide and develops tools to advertise specific informations about the services available to the communities in a form that is easy to access and use.
        The communication channels are represented by ticketing systems and also by mailing lists used for a more direct communication, allowing to promptly notify maintenance interventions, downtimes and more in general all the new features and services provided by the center.
        In this talk, the ticketing systems, tools, platforms and services that User Support offers, and the internal organization of the department will be described. Future workflow plans in view of the DATACLOUD project, which will require an increasing effort, will also be presented.

        Speaker: Dr Pellegrino, Carmelo (INFN-CNAF)
    • 11:00 AM 12:30 PM
      Track 9 - Artificial Intelligence and Machine Learning: Applications 1 Hampton Roads VII

      Hampton Roads VII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Schaarschmidt, Jana (University of Washington (US)) , VALLECORSA, SOFIA (CERN)
      • 11:00 AM
        MLHad: Simulating Hadronization with Machine Learning 15m

        Hadronization is an important step in Monte Carlo event generators, where quarks and gluons are bound into physically observable hadrons. Today’s generators rely on finely-tuned empirical models, such as the Lund string model; while these models have been quite successful overall, there remain phenomenological areas where they do not match data well. In this talk, we present MLHad, a machine-learning-based alternative for generating hadronization chains, which we intend ultimately to be data-trainable. Latent-space vectors are encoded, trained to be distributed according to a user-defined distribution using the sliced-Wasserstein distance in the loss function, then decoded to simulate hadronization.

        We show that generated pion multiplicities and cumulative kinematic distributions match those generated using Pythia (arXiv:2203.04983). We also present our more-recent work using normalizing flows to generate non-pion hadrons and to propagate errors through the encoder and decoder. Finally, we present comparisons with empirical data.

        Speaker: Wilkinson, Michael (University of Cincinnati)
      • 11:15 AM
        SYMBA: Symbolic Computation of Squared Amplitudes in High Energy Physics with Machine Learning 15m

        The calculation of particle interaction squared amplitudes is a key step in the calculation of cross sections in high-energy physics. These lengthy calculations are currently done using domain-specific symbolic algebra tools, where the time required for the calculations grows rapidly with the number of final state particles involved. While machine learning has proven to be highly successful in numerical calculations in high-energy physics, analytical calculations using machine learning are still in their beginning. We developed a transformer-based sequence-to-sequence model inspired by natural language processing that is able to accurately predict squared amplitudes of QCD and QED processes, respectively, when trained on symbolic sequence pairs. The goal of this work is to significantly reduce the computational time and, more importantly, build a model that scales well with the number of final state particles. To the best of our knowledge, this model (SYMBA) is the first model that encapsulates a wide range of symbolic squared amplitude calculations and, therefore, represents a potentially significant advance in using symbolic machine learning techniques for practical scientific computations.

        Speaker: Mr Alnuqaydan, Abdulhakim (University of Kentucky)
      • 11:30 AM
        On Estimating Gradients of Discrete Stochastic Programs for Detector Design Optimization 15m

        The recent advances in Machine Learning and high-dimensional gradient-based optimization has led to increased interest in the question of whether we can use such methods to optimize the design of future detectors for high-level physics objectives. However this program faces a fundamental obstacle: The quality of a detector design must be judged on the physics inference it enables, but both simulation and reconstruction of events are to a large degree described by discrete and thus naively non-differentiable stochastic branching (e.g. particle showers, ) and clustering processes (e.g. jet algorithms). In this work we explore the use of gradient estimation techniques based on differentiable and probabilistic programming that provide sufficiently stable estimates such that they may be used in an optimization loop. We showcase the effectiveness of such methods in benchmark scenarios ranging from a few to many thousands of optimizable parameters and discuss current limitations and future directions.

        Speaker: Heinrich, Lukas (Technical University of Munich)
      • 11:45 AM
        Multi-Module based VAE to predict HVCM faults in the SNS accelerator 15m

        We present a Multi-Module framework based on Conditional Variational Autoencoder (CVAE) to detect anomalies in the High Voltage Converter Modulators (HVCMs) which have historically been a cause of major down time for the Spallation Neutron Source (SNS) facility. Previous studies using machine learning techniques were to predict faults ahead of time in the SNS accelerator using a Single Modulator. Using the proposed methodology, we can detect faults in the power signals coming from multiple HVCMs that vary in design specifications and operating conditions. By conditioning the model according to the given modulator system, we can capture different representations of the normal waveforms for multiple systems. Our experiments with the SNS experimental data show that the trained model generalizes well to detecting several fault types for different systems, which can be valuable to improve the HVCM reliability and SNS as a result. We also explore several neural network architectures in our CVAE model by visualizing their loss landscapes to study the stability and generalization of the developed models and assist in hyper-parameter optimization and model selection to produce well-performed predictions.

        Speaker: Mr Alanazi, Yasir (Jefferson Lab)
      • 12:00 PM
        Resilient Variational Autencoder for Unsupervised Anomaly Detection at the SLAC Linac Cohrerent Light Source 15m

        Significant advances in utilizing deep learning for anomaly detection have been made in recent years. However, these methods largely assume the existence of a normal training set (i.e., uncontaminated by anomalies), or even a completely labeled training set. In many complex engineering systems, such as particle accelerators, labels are sparse and expensive; in order to perform anomaly detection in these cases, we must drop these assumptions and utilize a completely unsupervised method. Moreover, only identifying the anomaly is insufficient: operators of these complex systems need additional localization information to identify the root cause of the anomaly and make an informed response. In this paper, we introduce the Resilient Variational Autoencoder (ResVAE), a deep generative model that is designed for anomaly detection, is resilient to anomalies in the training data, and yields feature-level anomaly attribution. During training, the ResVAE learns the anomaly probability for each sample as a whole and for each individual feature, and uses those probabilities to ignore anomalous examples in the training data. We apply our method to detecting anomalies in the accelerator status at the SLAC Linac Coherent Light Source (LCLS). Using shot-to-shot data from the beam position monitoring system, we identify and characterize several types of anomalies apparent in the accelerator, including many instances of known failures modes (e.g., beam loss) that are missed by current detection methods.

        Speaker: Humble, Ryan (Stanford University)
      • 12:15 PM
        Machine Learning for Etch-Pit Identification at MoEDAL 15m

        The MoEDAL experiment at CERN (https://home.cern/science/experiments/moedal-mapp) carries out searches for highly ionising exotic particles such as magnetic monopoles. One of the technologies deployed in this task is the Nuclear Track Detector (NTD). In the form of plastic films, these are passive detectors that are low cost and easy to handle. After exposure to the LHC collision environment in the LHCb cavern at point 8 on the LHC ring, they are etched and scanned under a microscope to potentially reveal the etch-pit signature of the passage of an exotic highly ionising particle. The scanning process takes place using microscopes and expert human inspection. With several 10s of metres squared of deployed plastic, and large backgrounds complicating the analysis, the process is highly time consuming.

        We have studied the use of AI to identify etch-pits in scanned images of NTDs. A specially prepared stack of NTD plastic films – where one layer has been exposed to the harsh LHC environment and the others have not – is placed in a heavy ion beam to simulate the passage of particles such as magnetic monopoles. The plastic is then etched and optically scanned. The images are used to prepare training and evaluation data sets for three different approaches: a deconvolution-convolution algorithm with machine learning based thresholding, a convolutional neural network, trained as a classifier and then used in a fully convolutional mode, and a convolutional neural network making use of a U-Net based technique.

        We present an overview of MoEDAL and our study, the evaluation of the methods, and the prospects for further uses of AI in this area.

        Speaker: Hays, Jonathan (Queen Mary University of London)
    • 11:00 AM 12:30 PM
      Track X - Exascale Science, Heterogeneous Computing and Accelerators, and Quantum Computing: Exascale Computing Marriott Ballroom VII

      Marriott Ballroom VII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Campos, Isabel (CSIC) , Timm, Steven (Fermi National Accelerator Laboratory)
      • 11:00 AM
        Application of performance portability solutions for GPUs and many-core CPUs to track reconstruction kernels 15m

        Next generation High-Energy Physics (HEP) experiments are presented with significant computational challenges, both in terms of data volume and processing power. Using compute accelerators, such as GPUs, is one of the promising ways to provide the necessary computational power to meet the challenge. The current programming models for compute accelerators often involve using architecture-specific programming languages promoted by the hardware vendors and hence limit the set of platforms that the code can run on. Developing software with platform restrictions is especially unfeasible for HEP communities as it takes significant effort to convert typical HEP algorithms into ones that are efficient for compute accelerators. Multiple performance portability solutions have recently emerged and provide an alternative path for using compute accelerators, which allow the code to be executed on hardware from different vendors.
        We apply several portability solutions, such as Kokkos, SYCL, std::execution::par and Alpaka, on two mini-apps extracted from the mkFit project: p2z and p2r. These apps include basic kernels for a Kalman filter track fit, such as propagation and update of track parameters, for detectors at a fixed z or fixed r position, respectively. The two mini-apps explore different memory layout formats.

        We report on the development experience with different portability solutions, as well as their performance on GPUs and many-core CPUs, measured as the throughput of the kernels from different GPU and CPU vendors such as NVIDIA, AMD and Intel.

        Speaker: Kwok, Ka Hei Martin (Fermilab)
      • 11:15 AM
        INFN and the evolution of distributed scientific computing in Italy 15m

        INFN has been running for more than 20 years a distributed infrastructure (the Tier-1 at Bologna-CNAF and 9 Tier-2 centers) which currently offers about 140000 CPU cores, 120 PB of enterprise-level disk space and 100 PB of tape storage, serving more than 40 international scientific collaborations.
        This Grid-based infrastructure was augmented in 2019 with the INFN Cloud: a production quality multi-site federated Cloud infrastructure, composed by a core backbone, and which is able to integrate other INFN sites and public or private Clouds as well. The INFN Cloud provides a customizable and extensible portfolio offering computing and storage services spanning the IaaS, PaaS and SaaS layers, with dedicated solutions to serve special purposes, such as ISO-certified regions for the handling of sensitive data.
        INFN is now revising and expanding its infrastructure to tackle the challenges expected in the next 10 years of scientific computing adopting a “cloud-first” approach, through which all the INFN data centers will be federated via the INFN Cloud middleware and integrated with key HPC centers, such as the pre-exascale Leonardo machine at CINECA.
        In such a process, which involves both the infrastructures and the higher level services, initiatives and projects such as the "Italian National Centre on HPC, Big Data and Quantum Computing" (funded in the context of the Italian "National Recovery and Resilience Plan") and the Bologna Technopole are precious opportunities that will be exploited to offer advanced resources and services to Universities, research institutions and industry.
        In this paper we describe how INFN is evolving its computing infrastructure, with the ambition to create and operate a national vendor-neutral, open, scalable and flexible "data lake" able to serve much more than just INFN users and experiments.

        Speaker: Fanzago, Federica
      • 11:30 AM
        Outlines in hardware and software for new generations of exascale interconnects 15m

        RED-SEA (https://redsea-project.eu/) is a European project funded in the framework of the H2020-JTI-EuroHPC-2019-1 call that started in April 2021. The goal of the project is to evaluate the architectural design of the main elements of the interconnection networks for the next generation of HPC systems supporting hundreds of thousands of computing nodes enabling the Exa-scale for HPC, HPDA and AI applications, and to provide preliminary prototypes.

        The main technological feature is the BXI network, originally designed and produced by ATOS (France). The plan is to integrate in the next release of the network – BXI3 – the architectural solutions and novel IPs developed within the framework of the RED-SEA project.

        The consortium is composed of 11 well-established research teams across Europe, with extensive experience in interconnects, including network design, deployment and evaluation.

        Within RED-SEA INFN is adopting a hardware/software co-design approach to design APEnetX, a scalable interconnect prototyped on latest generation Xilinx FPGAs, adding innovative components for the improvement of the performance and resiliency of the interconnect. APEnetX is an FPGA-based, PCIe Gen3/4 network interface card equipped with RDMA capabilities being the endpoint of a direct multidimensional toroidal network and suitable to be integrated in the BXI environment. APEnetX design will be benchmarked on project testbeds using real scientific applications like NEST, a spiking neural network simulator.

        In this presentation we introduce the main scientific and technological motivations at the basis of the project, focusing on the current status of the development.

        Speaker: Dr Martinelli, Michele (INFN)
      • 11:45 AM
        ICSC: The Italian National Research Centre on HPC, Big Data and Quantum Computing 15m

        ICSC is one of the five Italian National Centres created in the framework of the Next Generation EU funding by the European Commission. The aim of ICSC, designed and approved through 2022 and eventually started in September 2022, is to create the national digital infrastructure for research and innovation, leveraging exixting HPC, HTC and Big Data infrastructures evolving towards a cloud datalake model. It will be accessible by the scientific and industrial communities through flexible and uniform cloud web interfaces, and will be relying on a high-level support team; as such, it will form a globally attractive ecosystem based on strategic public-private partnerships to fully exploit top level digital infrastructure for scientific and technical computing and promote the development of new computing technologies.

        The ICSC IT infrastructure is built upon existing scientific digital infrastructures provided by the major national players: GARR, the Italian NREN, provides the network infrastructure, whose capacity will be upgraded to multiples of Tbps; CINECA hosts Leonardo, one of the world largest HPC systems, with a power of over 250 Pflops, that will be further increased and complemented with a quantum computer; INFN contributes with its distributed Big Data cloud infrastructure, built in the last decades to respond to the needs of the High Energy Physics community.

        On top of the IT infrastructure, several thematic activities will be funded and will focus on the development of tools and applications in several research domains. Of particular relevance to this audience are the activities on "Fundamental Research and Space Economy" and "Astrophysics and Cosmos Observations", strictily aligned with the INFN and HEP core activities. Finally two technological research activities will foster research on "Future HPC and Big Data" and "Quantum Computing".

        In this contribution, the organisation of the National Centre and its relevance for the HEP community will be presented.

        Speaker: Grandi, Claudio (INFN Bologna)
      • 12:00 PM
        Performance Portability with Compiler Directives for Lattice QCD in the Exascale Era 15m

        The upcoming exascale computers in the United States and elsewhere will have diverse node architectures, with or without compute accelerators, making it a challenge to maintain a code base that is performance portable across different systems. As part of the US Exascale Computing Project (ECP), the USQCD collaboration has embarked on a collaborative effort to prepare the lattice QCD software suites for exascale, with a particular focus on achieving performance portability across diverse exascale architectures.

        In this presentation, I will focus on efforts to use compiler directives, OpenMP and OpenACC, to port the Grid C++ lattice QCD library to AMD/Intel/NVIDIA GPUs and multi/many-core CPUs. Performance comparisons with architecture-native implementations in HIP, SYCL and CUDA will be given. I will also discuss the problems encountered and pros and cons of using compiler directives for performance portability.

        Speaker: Lin, Meifeng (Brookhaven National Laboratory)
      • 12:15 PM
        Opticks : GPU Optical Photon Simulation using NVIDIA OptiX 7 and NVIDIA CUDA 15m

        Opticks is an open source project that accelerates optical photon simulation by
        integrating NVIDIA GPU ray tracing, accessed via the NVIDIA OptiX 7 API, with
        Geant4 toolkit based simulations. A single NVIDIA Turing architecture GPU has
        been measured to provide optical photon simulation speedup factors exceeding
        1500 times single threaded Geant4 with a full JUNO analytic GPU geometry
        automatically translated from the Geant4 geometry. Optical physics processes of
        scattering, absorption, scintillator reemission and boundary processes are
        implemented in CUDA based on Geant4. Wavelength-dependent material and surface
        properties as well as inverse cumulative distribution functions for reemission
        are interleaved into GPU textures providing fast interpolated property lookup
        or wavelength generation.

        In this work we describe the near complete re-implementation of geometry and
        optical simulation required to adopt the entirely new NVIDIA OptiX 7 API, with
        the implementation now directly CUDA based with OptiX usage restricted to
        providing intersects. The new Opticks features a modular many small header
        design that provides fine grained testing both on GPU and CPU as well as
        substantial code reductions from CPU/GPU sharing. Enhanced modularity has
        enabled CSG tree generalization to support "list-nodes", similar to
        G4MultiUnion, that improve performance for complex CSG solids. Recent addition
        of support for interference effects in boundaries with multiple thin layers,
        such as anti-reflection coatings and photocathodes, using CUDA compatible
        transfer matrix method (TMM) calculations of reflectance, transmittance and
        absorptance is also reported.

        Speaker: Dr Lin, Tao (IHEP)
    • 12:30 PM 2:00 PM
      Lunch on Own 1h 30m
    • 2:00 PM 3:30 PM
      Track 1 - Data and Metadata Organization, Management and Access: Networks Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Davila, Diego (University of California, San Diego) , Lassnig, Mario (CERN)
      • 2:00 PM
        Automated Network Services for Exascale Data Movement 15m

        The Large Hadron Collider (LHC) experiments distribute data by leveraging a diverse array of National Research and Education Networks (NRENs), where experiment data management systems treat networks as a “blackbox” resource. After the High Luminosity upgrade, the Compact Muon Solenoid (CMS) experiment alone will produce roughly 0.5 exabytes of data per year. NREN Networks are a critical part of the success of CMS and other LHC experiments. However, during data movement, NRENs are unaware of data priorities, importance, or need for quality of service, and this poses a challenge for operators to coordinate the movement of data and have predictable data flows across multi-domain networks. The overarching goal of SENSE (The Software-defined network for End-to-end Networked Science at Exascale) is to enable National Labs and universities to request and provision end-to-end intelligent network services for their application workflows leveraging SDN (Software-Defined Networking) capabilities. This work aims to allow LHC Experiments and Rucio, the data management software used by CMS Experiment, to allocate and prioritize certain data transfers over the wide area network. In this paper, we will present the current progress of the integration of SENSE, Multi-domain end-to-end SDN Orchestration with QoS (Quality of Service) capabilities, with Rucio, the data management software used by CMS Experiment.

        Speaker: Balcas, Justas (California Institute of Technology)
      • 2:15 PM
        A Named Data Networking Based Fast Open Storage System plugin for XRootD 15m

        We present an NDN-based Open Storage System (OSS) plugin for XRootD instrumented with an accelerated packet forwarder, built for data access in the CMS and other experiments at the LHC, together with its current status, performance as compared to other tools and applications, and plans for ongoing developments.

        Named Data Networking (NDN) is a leading Future Internet Architecture where data in the network is accessed directly by its name rather than the location of the data containers (hosts). NDN enables the joint design of multipath forwarding and caching to achieve superior latency and failover performance. The Caltech team, together with Northeastern University, UCLA, Tennessee Tech and other collaborators from the NDN for Data Intensive Science Experiments (N-DISE) project, has implemented (1) a small C++ NDN library (NDNc) to bridge the existing NDN libraries with the new high-throughput NDN-DPDK forwarder developed by NIST, (2) a corresponding NDN naming scheme for accessing datasets in the network, (3) two basic classes of entities for transferring data in NDN: consumer and producer, and (4) an NDN-based OSS plugin for XRootD.

        The XRootD plugin offers implementation for all filesystem related calls (e.g., open, read, close) and it embeds the NDN consumer that translates these calls to NDN Interest packets using well-established naming conventions. For example, the Interest for a read operation for the third segment from a file at /path/to/foo location on disk has the corresponding name /ndnc/ft/path/to/foo/v=1/seg=3. Once Interest packets are assembled, they are passed to a proxy entity which forwards them to the local interface. The proxy provides reliable data fetching by handling timeouts and retransmissions, and can adopt different congestion control algorithms (e.g., fixed window size, or congestion-aware AIMD). The local interface implements a memif shared memory packet interface, providing high-performance packet transmission to and from the local NDN-DPDK forwarder. NDN Interest packets find nearest copies of requested data on the NDN network, from either in-network caches or data producers. Alongside this plugin, a corresponding producer has been implemented, which can communicate with multiple file systems (CEPH, HDFS); upon receiving Interest packets, the producer responds with data packets that encapsulate byte ranges at proper offsets from an existing file indicated by the segment numbers of received Interest packets.

        In this paper we present the architecture of the NDNc library, the consumer application and the NDN-based XRootD plugin. We will also present the throughput performance of the plugin over a continental-scale wide area network testbed, in comparison with other tools and applications used for accessing data at the CMS experiment.

        Speaker: Shannigrahi, Susmit (Tennessee Tech University)
      • 2:30 PM
        ALTO/TCN: Toward an Architecture of Efficient and Flexible Data Transport Control for Data-Intensive Sciences using Deep Infrastructure Visibility 15m

        There is increasing demand for the efficiency and flexibility of data transport systems supporting data-intensive sciences. With growing data volume, it is essential that the transport system of a data-intensive science project fully utilize all available transport resources (e.g., network bandwidth); to achieve statistical multiplexing gain, there is an increasing trend that multiple projects share the same transport infrastructure, but the wide deployment of a shared infrastructure requires flexible resource control. In this talk, we first conduct a rigorous analysis of existing data transport systems and show that considering the infrastructures as a black box can limit efficiency and flexibility. We then introduce ALTO/TCN, a new architecture that introduces deep infrastructure visibility to achieve efficient, flexible data transport. We will provide additional details on 3 key components to realize the architecture: (1) how to achieve infrastructure visibility in multi-domain networks, using the Internet Engineering Task Force (IETF) Application-Layer Traffic Optimization (ALTO) protocol and the openalto.org visibility orchestrator; (2) how to integrate visibility into transport scheduling optimization, with zero-orde/first-order gradient and time-multiplexing control, using FTS integration as an example; and (3) how to integrate visibility into data selection orchestration, with general distances as a visibility abstraction, using Rucio integration as an example. We will report evaluation results and implementation lessons. We conclude with planning for the next steps, in particular, how the project complements existing related efforts in HEP, such as application awareness (e.g., packet marking) and adaptive networking resource allocation (e.g., NOTED/SENSE/AutoGOLE).

        Speaker: Yang, Ryan (Choate Rosemary Hall)
      • 2:45 PM
        A study case of Content Delivery Network solutions for the CMS experiment 15m

        In 2029 the LHC will start the High-Luminosity LHC (HL-LHC) program, with a boost in the integrated luminosity resulting in an unprecedented amount of experimental and simulated data samples to be transferred, processed and stored in disk and tape systems across the Worldwide LHC Computing Grid (WLCG). Content delivery network (CDN) solutions are being explored with the purposes of improving the performance of the compute tasks reading input data via the Wide Area Network (WAN), and also to provide a mechanism for cost-effective deployment of lightweight storages supporting traditional or opportunistic compute resources. In this contribution we study the benefits of applying cache solutions for the CMS experiment, in particular the configuration and deployment of xCache serving data to two Spanish WLCG sites supporting CMS: the Tier-1 site at PIC and the Tier-2 site at CIEMAT. The deployment and configuration of the system and the developed monitoring tools will be shown, as well as data popularity studies in relation to the optimization of the cache configuration, the effects on CPU efficiency improvements for analysis tasks, and the cost benefits and impact of including this solution in the region.

        Speaker: Dengra, Carlos (CIEMAT/PIC)
      • 3:00 PM
        Identifying and Understanding Scientific Network Flows 15m

        The High-Energy Physics (HEP) and Worldwide LHC Computing Grid (WLCG) communities have faced significant challenges in understanding their global network flows across the world’s research and education (R&E) networks. When critical links, such as transatlantic or transpacific connections, experience high traffic or saturation, it is very challenging to clearly identify which collaborations are generating the traffic and what activity that traffic represents. Without knowing the owner and the purpose of the traffic, we are unable to alert them or mitigate the issue. In general, the HEP and WLCG communities found they have insufficient visibility into which experiments are creating the flows and their purpose. Having such visibility also allows new understanding of scientific workflows and their associated resource use, and allows organizations and network providers to demonstrate the value of their participation

        The Research Networking Technical Working Group was formed in the spring of 2020, partially in response to this challenge. The first of its three working areas concerns network visibility; specifically, the use of packet marking or flow marking to identify the owner and associated activity of network traffic. The SciTags initiative was created to push this into production, not just for HEP/WLCG, but for any global users of R&E networks.

        We will describe the status of the work to date, including the evolving architecture and tools, as well as our plans to get this capability into production before the next WLCG Network Data Challenge in early 2024.

        Speaker: McKee, Shawn (University of Michigan Physics)
      • 3:15 PM
        Managing multi-instrument data streams in secure environments 15m

        The capture and curation of all primary instrument data is a potentially valuable source of added insight into experiments or diagnostics in laboratory experiments. The data can, when properly curated, enable analysis beyond the current practice that uses just a subset of the as-measured data. Complete curated data can also be input for machine learning and other data exploration tools. Conveniently storing and accessing instrument data requires that the instruments are connected to databases and users through a networking infrastructure. This infrastructure needs to accommodate a wide array of instruments which can range from single laboratory mounted probes for environment monitoring to computers managing multiple instruments. These resources may also include mobile devices on which researchers record instrument and experiment state related notes. These varied data sources bring with them the challenges of different communications capabilities and protocols as well as the primary data typically being produced in proprietary formats. These challenges are further compounded when the instruments need to operate in secure environments such as required in national laboratories.

        We will discuss the SmartLab, an ongoing effort to set up a system for instrument and simulation data curation at NASA Langley Research Center. We will outline the challenges faced in managing the data sources required for ongoing research activities and the solutions that are being considered and implemented to address those challenges.

        Speaker: Dr Sauti, Godfrey (NASA)
    • 2:00 PM 3:30 PM
      Track 2 - Online Computing: Online Reconstruction Marriott Ballroom V-VI

      Marriott Ballroom V-VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Pantaleo, Felice (CERN) , Shahoyan, Ruben (CERN)
      • 2:00 PM
        Cluster reconstruction in the HGCAL at the Level 1 trigger 15m

        The CMS collaboration has chosen a novel high granularity calorimeter (HGCAL) for the endcap regions as part of its planned upgrade for the high luminosity LHC. The calorimeter will have fine segmentation in both the transverse and longitudinal directions and will be the first such calorimeter specifically optimised for particle flow reconstruction to operate at a colliding-beam experiment. The calorimeter data will be part of the Level 1 trigger of the CMS experiment and, together with tracking information that will also be available, will allow particle-flow techniques to be used as part of this trigger. The trigger has tight constraints on latency and rate, and will need to be implemented in hardware. The high granularity results in around six million readout channels in total, reduced to one million that are used at 40 MHz as part of the Level 1 trigger, presenting a significant challenge in terms of data manipulation and processing for the trigger system; the trigger data volumes will be an order of magnitude above those currently handled at CMS. In addition, the high luminosity will result in an average of 140 (or more) interactions per bunch crossing that give a huge background rate in the forward region and these will need to be efficiently rejected by the trigger algorithms. Furthermore, reconstruction of the particle clusters to be used for particle flow in events with high hit rates is also a complex computational problem for the trigger. The status of the cluster reconstruction algorithms developed to tackle these major challenges, as well as the associated trigger architecture, will be presented.

        Speaker: Alves, Bruno (LLR, École Polytechnique, Paris)
      • 2:15 PM
        Level-3 trigger for CLAS12 with Artificial Intelligence 15m

        Fast, efficient and accurate triggers are a critical requirement for modern high energy physics experiments given the increasingly large quantities of data that they produce. The CEBAF Large Acceptance Spectrometer (CLAS12) employs a highly efficient Level 3 electron trigger to filter the amount of data recorded by requiring at least one electron in each event, at the cost of a low purity in electron identification. However, machine learning algorithms are increasingly employed for classification tasks such as particle identification due to their high accuracy and fast processing times. In this article we show how a convolutional neural network could be deployed as a Level 3 electron trigger at CLAS12. We demonstrate that the AI trigger would achieve a significant data reduction compared to the traditional trigger, whilst preserving a 99.5% electron identification efficiency. The AI trigger purity also improves relative to the traditional trigger with increased luminosity, as the AI trigger can achieve a reduction in recorded data with respect to the traditional trigger that increases at a rate of 0.32% per nA whilst keeping a stable efficiency above 99.5%.

        Speaker: Mr Tyson, Richard (Glasgow University)
      • 2:30 PM
        Impact of the high-level trigger for detecting long-lived particles at LHCb 15m

        Long-lived particles (LLPs) are very challenging to search for with current detectors and computing requirements, due to their very displaced vertices. This study evaluates the ability of the trigger algorithms used in the Large Hadron Collider beauty (LHCb) experiment to detect long-lived particles and attempts to adapt them to enhance the sensitivity of this experiment to undiscovered long-lived particles. One of the challenges in the track reconstruction is to deal with the large amount of combinatorics of hits. A dedicated algorithm has been developed to cope with the large data output. When fully implemented, this algorithm would greatly increase the available statistics for any long-lived particle search in the forward region, for the Standard Model of particle physics and beyond.

        Speaker: Prof. Vilasís-Cardona, Xavier (La Salle URL)
      • 2:45 PM
        Reconstructing jets in the Phase-2 upgrade of the CMS Level-1 Trigger with a seeded cone algorithm 15m

        The Phase-2 Upgrade of the CMS Level-1 Trigger will reconstruct particles using the Particle Flow algorithm, connecting information from the tracker, muon, and calorimeter detectors, and enabling fine-grained reconstruction of high level physics objects like jets. We have developed a jet reconstruction algorithm using a cone centred on an energetic seed from these Particle Flow candidates. The implementation is designed to find up to 16 jets in each Xilinx Ultrascale+ FPGA, with a latency of less than 1 μs, and event throughput of 6.7 MHz to fit within the L1T system constraints. Pipelined processing enables reconstruction of jet collections with different cone sizes for little additional resource cost. The design of the algorithm also provides a platform for additional computation using the jet constituents, such as jet tagging using neural networks. In this talk we will describe the implementation, its jet reconstruction performance, computational metrics, and the developments towards jet tagging.

        Speaker: Summers, Sioni (CERN)
      • 3:00 PM
        The Particle Flow Algorithm in the Phase II Upgrade of the CMS Level-1 Trigger. 15m

        The CMS experiment has greatly benefited from the utilization of the particle-flow (PF) algorithm for the offline reconstruction of the data. The Phase II upgrade of the CMS detector for the High Luminosity upgrade of the LHC (HL-LHC) includes the introduction of tracking in the Level-1 trigger, thus offering the possibility of developing a simplified PF algorithm in the Level-1 trigger. We present the logic of the algorithm, along with its inputs and its firmware implementation. We show that this implementation is capable of operating under the limited timing and processing resources available in the Level-1 trigger environment. The expected performance and physics implications of such an algorithm are shown using Monte Carlo samples with hιgh pile-up, simulating the harsh conditions of the HL-LHC. New calorimeter features allow for better performance under high pileup (PU) to be achieved, provided that careful tuning and selection of the prompt clusters has been made. Additionally, advanced pile-up techniques are needed to preserve the physics performance in the high-intensity environment. We present a method that combines all information yielding PF candidates and performs Pile-Up Per Particle Identification (PUPPI) capable of running in the low latency level-1 trigger environment. Demonstration of the algorithm on dedicated hardware relying on ATCA platform is presented

        Speaker: Summers, Sioni (CERN)
      • 3:15 PM
        Online tagging and triggering with deep learning AI for next generation particle imaging detector 15m

        The current and future programs for accelerator-based neutrino imaging detectors feature the use of Liquid Argon Time Projection Chambers (LArTPC) as the fundamental detection technology. These detectors combine high-resolution imaging and precision calorimetry to enable the study of neutrino interactions with unparalleled capabilities. However, the volume of data from LArTPCs will exceed 25 Petabytes each year for DUNE (Deep Underground Neutrino Experiment) and event reconstruction techniques are complex, requiring significant computational resources. These aspects of LArTPC data make utilization of real-time event triggering and event filtering algorithms that can distinguish signal from background important, but still challenging to accomplish with reasonable efficiency especially for low energy neutrino interactions. At Fermilab, we are developing a machine-learning-based trigger and filtering algorithm for the lab's flagship experiment DUNE, to extend the sensitivity of the detector, particularly for low energy neutrinos that do not come from an accelerator beam. Building off of recent research in machine learning to improve artificial intelligence, this new trigger algorithm will employ software to optimize data collection, pre-processing, and to make a final event selection decision. Development and testing of the trigger decision system will leverage data from MicroBooNE, ProtoDUNE, and Short Baseline Neutrino (SBN) LArTPC detectors, and will also provide benefits to the physics programs of those experiments.
        This talk will focus on application of a Convolutional Neural Network (CNN) to MicroBooNE data and will study performance metrices such as memory usage and latency. We will also discuss progress towards applying a Semantic Segmentation with Sparse Convolutional Network (SparseCNN) on the same data and compare the performance of the two algorithms.

        Speaker: Bhattacharya, Meghna (Fermilab)
    • 2:00 PM 3:30 PM
      Track 3 - Offline Computing: Physics performance (part I) Hampton Roads Ballroom VI

      Hampton Roads Ballroom VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Dr Srpimanobhas, Norraphat (Chulalongkorn University) , Yang, Tingjun (Fermilab)
      • 2:00 PM
        Investigating mixed-precision for AGATA pulse-shape analysis 15m

        The AGATA project (1) aims at building a 4pi gamma-ray spectrometer consisting of 180 germanium crystals, each crystal being divided into 36 segments. Each gamma ray produces an electrical signal within several neighbouring segments, which is compared with a data base of reference signals, enabling to locate the interaction. This step is called Pulse-Shape Analysis (PSA).

        In the execution chain leading to the PSA, we observe successive data conversions : the original 14 bits integers given by the electronics are finally converted to 32-bit floats. This made us wonder about the real numerical accuracy of the results, and investigate the use of shorter floats, with the hope to speedup the computation, and also reduce a major cache-miss problem previously identified with the Perf (2) tool.

        Our proposed talk would first report about the numerical validation of the C++ PSA code, thanks to the Discrete Stochastic Arithmetic implemented in the CADNA library (3). After the code being properly instrumented, CADNA performs each computation three times with a random rounding mode. This allows, for each operation, to evaluate the number of exact significant digits using a Student test with 95% confidence threshold.

        In a second step, we will report our successes and challenges while refactoring the code so to mix different numerical formats, using high precision only when necessary, and taking benefit of hardware speedup elsewhere. Such mixed-precision appears as a promising option for high performance computation in the next years, provided we use tools such as CADNA so to keep control of the accuracy of the computed results.

        (1) https://www.agata.org/about
        (2) https://perf.wiki.kernel.org/index.php/Main_Page
        (3) http://cadna.lip6.fr

        Speaker: Molina, Roméo (IJCLab)
      • 2:15 PM
        Kiwaku, a C++20 library for multidimensional arrays, applied to ACTS tracking 15m

        Track reconstruction, also known as tracking, is a vital part of the HEP event reconstruction process, and one of the largest consumers of computing resources. The upcoming HL-LHC upgrade will exacerbate the need for efficient software able to make good use of the underlying heterogeneous hardware. However, this evolution should not imply the production of code unintelligible to most of its maintainers, hence the need to provide good usability to both end users and developers.

        C++ has been a language of choice for efficient scientific computing tasks. The Generative Programming paradigm [CZAR98], which relies on heavy type based template meta-programming, provides a powerful solution for supporting multiple execution contexts[MASL16]. Yet, the templates are usually blamed for binary bloat, high code complexity and unreadable error messages.

        In this presentation, we will discuss recent developments made to the C++ language, helping to define a new process for constructing libraries both efficient and easy to use, using a streamlined Generative Programming process:
        • easier code selection at compile time using “if constexpr”
        • better error reporting using “Concepts”, i.e. compile-time type constraints
        • easier meta-programming with Non-Type Template Parameters

        We will then introduce Kiwaku[KWK22], a new multidimensional arrays library taking advantage of the most recent C++ usability improvements, yet providing portable performance on various execution contexts (CPU, GPU). We will finally discuss a few proofs of concept, based on use-cases borrowed from the ACTS toolkit[ACTS22]: magnetic field computation, clustering and seeding.

        References:

        [ACTS22] Ai, X., Allaire, C., Calace, N. et al. A Common Tracking Software Project. Comput Softw Big Sci 6, 8 (2022). https://doi.org/10.1007/s41781-021-00078-8

        [CZAR98] Krzysztof Czarnecki, Ulrich W. Eisenecker, Robert Glück, David Vandevoorde, Todd L. Veldhuizen: "Generative Programming and Active Libraries". Generic Programming 1998: 25-39

        [KWK22] Kiwaku main repository - https://github.com/jfalcou/kiwaku/

        [MASL16] Ian Masliah, Marc Baboulin, Joel Falcou: "Meta-programming and Multi-stage Programming for GPGPUs". 2016 IEEE 10th International Symposium on Embedded Multicore/Many-core Systems-on-Chip (MCSOC)

        Speaker: Mr Joube, Sylvain (IJCLab - LISN, Universit Paris-Saclay, CNRS/IN2P3)
      • 2:30 PM
        A physical dimensions aware evaluator for High Energy Physics applications 15m

        The LHCb software stack is developed in C++ and uses the Gaudi framework for event processing and DD4hep for the detector description. Numerical computations are done either directly in the C++ code or by an evaluator used to process the expressions embedded in the XML describing the detector geometry.
        The current system relies on conventions for the physical units used (identical as what is used in the Geant4 simulation framework) and it is up to the developers to ensure that the correct factors are applied to the values entered. Physical units are not primary entities in the framework, it is therefore not possible to check the dimensional consistency of the computation performed. In this paper we investigate the possibilities to add physical units and dimensions to the existing evaluator or to replace it by a more suitable system, and how this would integrate with the possible tools to express units in C++ code (such as boost::units).

        Speaker: Clemencic, Marco (CERN EP-LBC)
      • 2:45 PM
        Physics Performance of the ATLAS GNN4ITk Track Reconstruction Chain 15m

        Applying graph-based techniques, and graph neural networks (GNNs) in particular, has been shown to be a promising solution to the high-occupancy track reconstruction problems posed by the upcoming HL-LHC era. Simulations of this environment present noisy, heterogeneous and ambiguous data, which previous GNN-based algorithms for ATLAS ITk track reconstruction could not handle natively. We present a range of upgrades to the so-called GNN4ITk pipeline that allow detector regions to be handled heterogeneously, ambiguous and shared nodes to be reconstructed more rigorously, and tracks-of-interest to be treated with more importance in training. With these improvements, we are able to present for the first time apples-to-apples comparisons with existing reconstruction algorithms on a range of physics metrics, including reconstruction efficiency across particle type and pileup condition, jet reconstruction performance in dense environments, displaced tracking, and track parameter resolutions. We also demonstrate that our results are robust to misalignment of ITk modules, showing the GNN4ITk approach to perform well under changing experimental conditions. By integrating this solution with the offline ATLAS Athena framework, we also explore a range of reconstruction chain configurations, for example by using the GNN4ITk pipeline to build regions-of-interest while using traditional techniques for track cleaning and fitting.

        Speaker: Ju, Xiangyang (Lawrence Berkeley National Laboratory)
      • 3:00 PM
        Calibration Data Flow and Performance at Belle II 15m

        The Belle II experiment has been accumulating data since 2019 at the SuperKEKB $e^+e^-$ accelerator in Tsukuba, Japan. The accelerator operates at the $\Upsilon(4S)$ resonance and is an excellent laboratory for precision flavor measurements and dark sector searches. The accumulated data are promptly reconstructed and calibrated at a dedicated calibration center in an automated process based on a directed acyclic graph to resolve dependencies in the calibration using selected prescaled data skims. After calibration, the raw data are reconstructed on the GRID and provided in an analysis-oriented format (mDST) on the GRID for the collaboration.
        In this talk we will present the calibration data flow from raw data to mDST production. We will discuss the physical principles behind the calibrations and how we tune the calibration data samples accordingly. We will show performance metrics which underpin the importance of the data calibration for our precision physics results.

        Speaker: Prim, Markus
      • 3:15 PM
        EIC Software Overview 15m

        Development of the EIC project detector "ePIC" is now well underway and this includes the "single software stack" used for simulation and reconstruction. The stack combines several non-experiment-specific packages including ACTS, DD4hep, JANA2, and PODIO. The software stack aims to be forward looking in the era of AI/ML and heterogeneous hardware. A formal decision making process was implemented to choose the components that involved everyone in the collaboration that was interested. This talk will present an overview of the software stack currently used for development of the ePIC detector and on which we expect to execute the experiment.

        Speaker: Lawrence, David (Jefferson Lab)
    • 2:00 PM 3:30 PM
      Track 3+9 Crossover: Simulation Chesapeake Meeting Room

      Chesapeake Meeting Room

      Norfolk Waterside Marriott

      235 East Main Street, Norfolk, VA, 23510
      Conveners: Bandieramonte, Marilena (University of Pittsburgh) , VALLECORSA, SOFIA (CERN)
      • 2:00 PM
        Development of particle flow algorithms based on Neural Network techniques for the IDEA calorimeter at future colliders 15m

        IDEA (Innovative Detector for an Electron-positron Accelerator) is an innovative general-purpose detector concept, designed to study electron-positron collisions at future e$^+$e$^-$ circular colliders (FCC-ee and CEPC).
        The detector will be equipped with a dual read-out calorimeter able to measure separately the hadronic component and the electromagnetic component of the showers initiated by the impinging hadrons.

        Particle flow algorithms (PFAs) have become the paradigm of detector design for the high energy frontier and this talk discusses a project to build a Particle Flow algorithm for the IDEA detector using Machine Learning (ML) techniques. Machine Learning is used for particle reconstruction and identification profiting of the high granularity of the fiber-based dual-readout calorimeter. Neural Networks (NN) are built for electron, pions, neutral kaons, muons reconstruction and identification inside the calorimeter and for the jet reconstruction. The performances of the algorithm using several NN architectures will be shown, with particular attention to the layer setup and the activation function choices. The performances will be evaluated on the resolution function of the reconstructed particles and of the reconstructed jet. The algorithm will be trained using both parallel CPUs and GPU, and the time performances and the memory usage of the two approaches will be systematically compared.
        Finally, the aim of the project is to develop the NN algorithm inside the Pandora PFA framework.

        Speaker: DOnofrio, Adelina (INFN-Roma Tre)
      • 2:15 PM
        PARSIFAL: parametrized simulation of triple-GEM and micro-RWELL response to a charged particle 15m

        PARSIFAL (PARametrized SImulation) is a software tool that can reproduce the complete response of both triple-GEM and micro-RWELL based trackers. It takes into account the involved physical processes by their simple parametrization and thus in a very fast way. Existing software as GARFIELD++ are robust and reliable, but very CPU time consuming. The implementation of PARSIFAL was driven by the necessity to reduce the processing time, without losing the precision of a full simulation. A series of parameters, that can be extracted from the GARFIELD++ simulation, are set as input to PARSIFAL, which then runs independently from GARFIELD++. PARSIFAL can simulate samples with high statistics much faster, taking into account the various steps (ionization, diffusion, multiplication, signal induction and electronics) from the simple sampling from parameterized distributions. In the case of the micro-RWELL MPGD, the effect of the high resistivity layer on the charge spread on the anode was introduced, following M.S. Dixit and A. Rankin treatment.
        PARSIFAL was used to simulate triple-GEM chambers and the results were tuned to match experimental data from testbeams. In this case the adopted electronics was APV-25 readout by SRS system, which has been simulated in the code. The same procedure was later applied to micro-RWELL chambers, readout this time by the TIGER ASIC and the GEMROC system. This new electronics was added to PARSIFAL code and a tuning of the simulated-to-real data was performed. A presentation of the full code will be given in this contribution, setting the focus on the latest implementations and on a first comparison with experimental data from micro-RWELL.

        Speaker: Farinelli, Riccardo (INFN Ferrara)
      • 2:30 PM
        The AtlFast3, the ATLAS fast simulation tool in Run3 15m

        AtlFast3 is the new, high-precision fast simulation in ATLAS that was deployed by the collaboration to replace AtlFastII, the fast simulation tool that was successfully used for most of Run2. AtlFast3 combines a parametrization-based Fast Calorimeter Simulation and a new machine-learning-based Fast Calorimeter Simulation based on Generative Adversarial Networks (GANs). The new fast simulation can reproduce the Geant4 inputs with higher accuracy than the old AtlFast2. In particular, the simulation of jets of particles reconstructed with large radii and the detailed description of their substructure are significantly improved in AtlFast3. Results will be presented on the performance of the new AtlFast3 that will be deployed for the simulation of the majority of events in Run3; these changes are crucial for achieving the precision needed by analyses that will need to rely mainly on fast simulation.

        Speaker: Dr Faucci Giannelli, Michele (INFN Roma Tor Vergata)
      • 2:45 PM
        Simulation and Reconstruction of Photoelectric X-ray Polarimetry on LPD 15m

        The Large Field Low-energy X-ray Polarization Detector (LPD) is a gas photoelectric effect polarization detector designed for the detailed study of X-ray temporary sources in high-energy astrophysics. Previous studies have shown that the polarization degree of gamma ray bursts (GRBs) is generally low or unpolarized. Considering the spatial background and other interferences, We need high modulation algorithms to observe low polarization GRB. For this purpose, moment analysis, graph theory, neural network algorithms are studied for the reconstruction of photoelectron emission angle. Combined with experimental and simulation data, the reconstruction performance of different algorithms at various energy and incident angles is evaluated.

        Moment analysis algorithm finds out the large angle scattering point of photoelectron and remove the zone. Photoelectron track after cutting can be reconstructed. However, on the one hand, when track length is large, the performance of moment analysis algorithm becomes worse. On the other hand, for short cases, the track information loss caused by cutting is more serious, and the performance of moment analysis algorithm will also be degraded. In order to address these problems, graph theory algorithm and neural network are studied. Graph theory algorithm improves the reconstruction performance by precisely positioning the photoelectric action point through the trunk endpoint, which is more effective for longer tracks. Training samples of neural network algorithm are from the simulation platform built based on Geant4 in which photoelectric interaction, ionization diffusion, signal digitization and other processes on the detector are simulated as real as possible. Two typical neural networks, CNN and GNN, are studied. The results show that both neural networks predict high modulation and stability in designed energy range. In order to carefully evaluate the performance of the algorithm, the simulation should be as close to the real situation as possible.

        Speaker: Dr Yi, Difan (University of Chinese Academy of Sciences)
      • 3:00 PM
        The LHCb ultra-fast simulation option, Lamarr: design and validation 15m

        Detailed detector simulation is the major consumer of CPU resources at LHCb, having used more than 80% of the total computing budget during Run 2 of the Large Hadron Collider at CERN. As data is collected by the upgraded LHCb detector during Run 3 of the LHC, larger requests for simulated data samples are necessary, and will far exceed the pledged resources of the experiment, even with existing fast simulation options. An evolution of technologies and techniques to produce simulated samples is mandatory to meet the upcoming needs of analysis to interpret signal versus background and measure efficiencies. In this context, we propose Lamarr, a Gaudi-based framework designed to offer to LHCb the fastest solution for simulations.
        Lamarr consists of a pipeline of modules parametrizing both the detector response and the reconstruction algorithms of the LHCb experiment. Most of the parameterizations are made of Deep Generative Models and Gradient Boosted Decision Trees trained on simulated samples or alternatively, where possible, on real data. Embedding Lamarr in the general LHCb Gauss Simulation framework allows combining its execution with any of the available generators in a seamless way.
        Lamarr has been validated by comparing key reconstructed quantities with Detailed Simulation. Good agreement of the simulated distributions is obtained with two-order-of-magnitude speed-up of the simulation phase.

        Speaker: Barbetti, Matteo (INFN Firenze)
      • 3:15 PM
        Generative Models for Fast Simulation of Electromagnetic and Hadronic Showers in Highly Granular Calorimeters 15m

        Modern high energy physics experiments fundamentally rely on accurate simulation- both to characterise detectors and to connect observed signals to underlying theory. Traditional simulation tools are reliant upon Monte Carlo methods which, while powerful, consume significant computational resources. These computing pressures are projected to become a major bottleneck at the high luminosity stage of the LHC and for future colliders. Deep generative models hold promise to potentially offer significant reductions in compute times, while maintaining a high degree of physical fidelity.

        This contribution provides an overview of a growing body of work focused on simulating showers in highly granular calorimeters, which is making significant strides towards realising fast simulation tools based on deep generative models. Progress on the simulation of both electromagnetic and hadronic showers, as well further steps to address challenges faced when broadening the scope of these simulators, will be reported. A particular focus will be placed on the high degree of physical fidelity achieved, as well as the performance after interfacing with reconstruction algorithms.

        Speaker: Mr Gaede, Frank (DESY)
    • 2:00 PM 3:30 PM
      Track 4 - Distributed Computing: Computing Strategies and Evolution Marriott Ballroom II-III

      Marriott Ballroom II-III

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Barreiro Megino, Fernando (Unive) , Miyake, Hideki (KEK/IPNS)
      • 2:00 PM
        JUNO distributed computing system 15m

        The Jiangmen Underground Neutrino Observatory (JUNO) is a multipurpose neutrino experiment and the determination of the neutrino mass hierarchy is its primary physics goal. JUNO is going to take data in 2024 with 2PB raw data each year and use distributed computing infrastructure for simulation, reconstruction and analysis tasks. The JUNO distributed computing system has been built up based on DIRAC since 2018. The official Monte Carlo production has started to run in the system and PBs of massive MC data has been shared among JUNO data centers through this system since last year. In this paper, an overview of the JUNO distributed computing system will be presented, including workload management system, data management system and calibration data access system. Also the progress of adapting the system to the token-based AAI and WebDAV TPC will be reported. The paper will also describe the preparations for the coming data-taking, and how we will arrange JUNO data processing activities in this platform for data-taking.

        Speaker: Zhang, Xiaomei (Institute of High Energy Physics)
      • 2:15 PM
        Computing Challenges for the Einstein Telescope project 15m

        The discovery of gravitational waves, first observed in September 2015 following the merger of a binary black hole system, has already revolutionised our understanding of the Universe. This was further enhanced in August 2017, when the coalescence of a binary neutron star system was observed both with gravitational waves and a variety of electromagnetic counterparts; this joint observation marked the beginning of gravitational multi-messenger astronomy. The Einstein Telescope, a proposed next-generation ground-based gravitational-wave observatory, will dramatically increase the sensitivity to sources: the number of observations of gravitational waves is expected to increase from roughly 100 per year to roughly 100’000 per year, and signals may be visible for hours at a time, given the low frequency cutoff of the planned instrument. This increase in the number of observed events, and the duration with which they are observed, is hugely beneficial to the scientific goals of the community, but poses a number of significant computing challenges. Moreover, the currently used computing algorithms do not scale to this new environment, both in terms of the amount of resources required and the speed with which each signal must be characterised.

        This contribution will discuss the Einstein Telescope's computing challenges, and the activities that are underway to prepare for them. Available computing resources and technologies will greatly evolve in the years ahead, and those working to develop the Einstein Telescope data analysis algorithms will need to take this into account. The availability of huge parallel HPC systems and ubiquitous Cloud computing will also be important to factor into the initial development of the experiment's computing model; the design of the model will also, for the first time, include the environmental impact as one of the optimisation metrics.

        Speaker: Pardi, Silvio (INFN)
      • 2:30 PM
        The Ligo-Virgo-KAGRA Computing Infrastructure for Gravitational-wave Research 15m

        The LIGO, VIRGO and KAGRA Gravitational-wave (GW) observatories are getting ready for their fourth observational period, O4, scheduled to begin in March 2023, with improved sensitivities and thus higher event rates.
        GW-related computing has both large commonalities with HEP computing, particularly in the domain of offline data processing and analysis, and important differences, for example in the fact that the amount of raw data doesn’t grow much with the instrument sensitivity, or the need to timely generate and distribute “event candidate alerts” to EM and neutrino observatories, thus making gravitational multi-messenger astronomy possible.

        Data from the interferometers are exchanged between collaborations both for low-latency and offline processing; in recent years, the three collaborations designed and built a common distributed computing infrastructure to prepare for a growing computing demand, and to reduce the maintenance burden of legacy custom-made tools, by increasingly adopting tools and architectures originally developed in the context of HEP computing. So for example HTCondor is used for workflow management, Rucio for many data management needs, CVMFS for code and data distribution, and more.

        We will present GW computing use cases and report about the architecture of the computing infrastructure as will be used during O4, as well as some planned upgrades for the subsequent observing run O5.

        Speaker: Legger, Federica (INFN Torino)
      • 2:45 PM
        The U.S. CMS HL-LHC R&D Strategic Plan 15m

        The HL-LHC run is anticipated to start at the end of this decade and will pose a significant challenge for the scale of the HEP software and computing infrastructure. The mission of the U.S. CMS Software & Computing Operations Program is to develop and operate the software and computing resources necessary to process CMS data expeditiously and to enable U.S. physicists to fully participate in the physics of CMS. We have developed a strategic plan to prioritize R&D efforts to reach this goal for the HL-LHC. This plan includes four grand challenges: modernizing physics software and improving algorithms, building infrastructure for exabyte-scale datasets, transforming the scientific data analysis process and transitioning from R&D to operations. We are involved in a variety of R&D projects that fall within these grand challenges. In this talk, we will introduce our four grand challenges and outline the R&D program of the U.S. CMS Software & Computing Operations Program.

        Speaker: Gutsche, Oliver (Fermi National Accelerator Laboratory)
      • 3:00 PM
        R&D in ATLAS Distributed Computing towards HL-LHC 15m

        The computing challenges at HL-LHC require fundamental changes to the distributed computing models that have served experiments well throughout LHC. ATLAS planning for HL-LHC computing started back in 2020 with a Conceptual Design Report outlining various challenges to explore. This was followed in 2022 by a roadmap defining concrete milestones and associated effort required. Today, ATLAS is proceeding further with a set of "demonstrators" with focussed R&D in specific topics described in the roadmap. The demonstrators cover areas such as optimised tape writing and access, data recreation on-demand and the use of commercial clouds. This paper presents an overview of the demonstrators, detailing the plans, timelines and expected impact of the work.

        Speaker: South, David
      • 3:15 PM
        Future Data-Intensive Experiment Computing Models: Lessons learned from the recent evolution of the ATLAS Computing Model 15m

        In this talk, we discuss the evolution of the computing model of the ATLAS experiment at the LHC. After LHC Run 1, it became obvious that the available computing resources at the WLCG were fully used. The processing queue could reach millions of jobs during peak loads, for example before major scientific conferences and during large scale data processing. The unprecedented performance of the LHC during Run 2 and subsequent large data volumes required more computing power than the WLCG consortium pledged. In addition to unpledged/opportunistic resources available through the grid, the integration of resources such as supercomputers and cloud computing with the ATLAS distributed computing model has led to significant changes in both the workload management system and the data management system, thereby changing the computing model as a whole. The implementation of the data carousel model and data on-demand, cloud and HPC integration, and other innovations expanded the physics capabilities of experiments in the field of high energy physics and made it possible to implement bursty data simulation and processing. In the past few years ATLAS, and many other High Energy (HEP) or Nuclear Physics (NP) and Astroparticle experiments, evaluated commercial clouds as an additional part of their computing resources. In this talk, we will briefly describe the ATLAS-Google and ATLAS-Amazon projects and how they were fully integrated with the ATLAS computing model. We will try to answer a fundamental question about the future computing model for experiments with large data volumes and distributed computing resources by considering three possible options:
        - HEP/NP experiments will continue to own and use pledged resources
        - HEP/NP experiments will buy resources from commercial providers
        - HEP/NP experiments will own core resources and buy additional resources from commercial providers.

        Speaker: Klimentov, Alexei (Brookhaven National Laboratory)
    • 2:00 PM 3:30 PM
      Track 6 - Physics Analysis Tools: I/O and Data Formats Hampton Roads Ballroom VIII

      Hampton Roads Ballroom VIII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Hageboeck, Stephan (CERN) , Heddle, Dave (CNU)
      • 2:00 PM
        DUNE HDF5 Experience 15m

        The Deep Underground Neutrino Experiment (DUNE) has historically represented data using a combination of custom data formats and those based on ROOT I/O. Recently, DUNE has begun using the Hierarchical Data Format (HDF5) for some of its data storage applications. HDF5 provides high-performance, low-overhead I/O in DUNE’s data acquisition (DAQ) environment. DUNE will use HDF5 to record raw data from the ProtoDUNE Horizontal Drift (HD), ProtoDUNE Vertical Drift (VD) and ICEBERG detectors, and the HD and VD coldbox test stands. Dedicated I/O modules have been developed to read the HDF5 data from these detectors into the offline framework for reconstruction directly and via XRootD. HDF5 is also very commonly used on High Performance Computers (HPCs) and is well-suited for use in AI/ML applications. The DUNE software stack contains modules that export data from an offline job in HDF5 format, so that they can be processed by external AI/ML software. The collaboration is also developing strategies to incorporate HDF5 in the detector simulation chains.

        Speaker: Dr Chowdhury, Barnali
      • 2:15 PM
        Schema-Evolution and the TTree within HDF5 15m

        ROOT's TTree data structure has been highly successful and useful for HEP; nevertheless, alternative file formats now exist which may offer broader software tool support and more-stable in-memory interfacing. We present a data serialization library that produces a similar data structure within the HDF5 data format; supporting C++ standard collections, user-defined data types, and schema evolution of those types. This HDF5-based serialization shows improved performance compared to a similar ROOT-based serialization library when embedded into an event processing framework for a HEP experiment and opens the door to using other software that struggled to interface with the ROOT format.

        Speaker: Eichlersmith, Tom (University of Minnesota)
      • 2:30 PM
        ROOT’s RNTuple I/O Subsystem: The Path to Production 15m

        The RNTuple I/O subsystem is ROOT's future event data file format and access API. It is driven by the expected data volume increase at upcoming HEP experiments, e.g. at the HL-LHC, and recent opportunities in the storage hardware and software landscape such as NVMe drives and distributed object stores. RNTuple is a redesign of the TTree binary format and API and has shown to deliver substantially faster data throughput and better data compression both compared to TTree and to industry standard formats. In order to let HENP computing workflows benefit from RNTuple's superior performance, however, the I/O stack needs to connect efficiently to the rest of the ecosystem, from grid storage to (distributed) analysis frameworks to (multithreaded) experiment frameworks for reconstruction and ntuple derivation. With the RNTuple binary format arriving at version 1.0, we present RNTuple's feature set, integration efforts, and its performance impact on the time-to-solution. We show the latest performance figures of RDataFrame analysis code of realistic complexity, comparing RNTuple and TTree as data sources. We discuss RNTuple's approach to functionality critical to the HENP I/O (such as multithreaded writes, fast data merging, schema evolution) and we provide an outlook on the road to its use in production.

        Speaker: Blomer, Jakob (CERN)
      • 2:45 PM
        Integration of RNTuple in ATLAS Athena 15m

        After using ROOT TTree for over two decades and storing more than an exabyte of compressed data, advances in technology have motivated a complete redesign, RNTuple, that breaks backward-compatibility to take better advantage of these storage options. The RNTuple I/O subsystem has been designed to address performance bottlenecks and shortcomings of ROOT's current state of the art TTree I/O subsystem. Specifically, it comes with an updated, more compact binary data format, that can be stored both in ROOT files and natively in object stores, on performance engineering for modern storage hardware (e.g. high-throughput low-latency NVMe SSDs), and robust and easy to use interfaces.
        RNTuple is scheduled to become production grade in 2024; recently it became mature enough to start exploring the integration into experiments' software. In particular, in this contribution we analyze the challenges and discuss their solutions on the way to supporting the ATLAS Analysis Event Data Model (based on xAOD data format) in Athena, part of the software stack for the ATLAS experiment.

        Speaker: Mrs De Geus, Florine (University of Amsterdam)
      • 3:00 PM
        Improving ROOT I/O Performance for Analysis 15m

        Analysis performance has a significant impact on the productivity of physicists. The vast majority of analyses use ROOT (https://root.cern). For a few years now, ROOT has offered an analysis interface called RDataFrame which helps getting the best performance for analyses, ideally making them I/O limited, i.e. with their performance limited by the throughput of reading the input data.

        The CERN IT department has recently noted (https://doi.org/10.5281/zenodo.6337728) that for the analysis activities (that they heuristically identified as such) there was no apparent performance CPU nor I/O bottleneck as seen from their point of view. We will report on our investigation in collaboration with USCMS and the CERN IT department to understand better where the inefficiencies that gave rise to this situation come from and the improvements that were made in ROOT to significantly reduce those inefficiencies. We will also describe additional logging and tagging facilities introduced to help distinguish the type of workload and help correlate the information gathered on the server side with the activities carried out by the users’ analysis.

        Speaker: Canal, Philippe
      • 3:15 PM
        Boosting RDataFrame performance with transparent bulk event processing 15m

        RDataFrame is ROOT's high-level interface for Python and C++ data analysis. Since it first became available, RDataFrame adoption has grown steadily and it is now poised to be a major component of analysis software pipelines for LHC Run 3 and beyond. Thanks to its design inspired by declarative programming principles, RDataFrame enables the development of high-performance, highly parallel analyses without requiring expert knowledge of multi-threading and I/O: user logic is expressed in terms of self-contained, small computation kernels tied together via a high-level API. This design completely decouples analysis logic from its actual execution, and opens several interesting avenues for workflow optimization. In particular, in this work we explore the benefits of moving internal data processing from an event-by-event to a bulk-by-bulk loop: it dramatically reduces framework's performance overheads; in collaboration with the I/O layer it improves data access patterns; it exposes information that optimizing compilers might use to auto-vectorize the invocation of user-defined computations; finally, while existing user-facing interfaces remain unaffected, it becomes possible to additionally offer interfaces that explicitly expose bulks of events, useful e.g. for the injection of GPU kernels into the analysis workflow. Design challenges useful to inform future R&D will be presented, as well as an investigation of the relevant time-memory tradeoffs backed by novel performance benchmarks.

        Speaker: Guiraud, Enrico (EP-SFT, CERN)
    • 2:00 PM 3:30 PM
      Track 7 - Facilities and Virtualization: Analysis Facilities Marriott Ballroom IV

      Marriott Ballroom IV

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Kishimoto, Tomoe (KEK) , Weitzel, Derek (University of Nebraska-Lincoln)
      • 2:00 PM
        Experience deploying an analysis facility for the Rubin Observatory’s Legacy Survey of Space and Time (LSST) data 15m

        The Vera C. Rubin observatory is preparing for the execution of the most ambitious astronomical survey ever attempted, the Legacy Survey of Space and Time (LSST). Currently, in its final phase of construction in the Andes mountains in Chile and due to start operations in late 2024 for 10 years, its 8.4-meter telescope will nightly scan the southern sky and collect images of the entire visible sky every 4 nights using a 3.2 Gigapixel camera, the largest imaging device ever built for astronomy. Automated detection and classification of celestial objects will be performed by sophisticated algorithms on high-resolution images to progressively produce an astronomical catalog eventually composed of 20 billion galaxies and 17 billion stars and their associated physical properties.

        In this contribution, we will briefly present the infrastructure deployed at the French Rubin data facility (operated by the IN2P3 computing center) to deploy the Rubin Science Platform, a set of web-based services to provide effective and convenient access to LSST data for scientific analysis.

        We will describe the main services of the platform, the components that provide those services and our deployment model as well as some feedback collected by end users. We will also present the Kubernetes-based infrastructure we are experimenting with for hosting LSST astronomical catalog, a multi-petabyte relational database developed for the specific needs of the project.

        Speaker: Mainetti, Gabriele (CC-IN2P3/CNRS)
      • 2:15 PM
        The Spanish CMS Analysis Facility at CIEMAT 15m

        The increasingly larger data volumes that the LHC experiments will accumulate in the coming years, especially in the High-Luminosity LHC era, call for a paradigm shift in the way experimental datasets are accessed and analyzed. The current model, based on data reduction on the Grid infrastructure, followed by interactive data analysis of manageable size samples on the physicists’ individual computers, will be superseded by the adoption of Analysis Facilities. This rapidly evolving concept is converging to include dedicated hardware infrastructures and computing services optimized for the effective analysis of large HEP data samples. This contribution will describe the actual implementation of this new analysis facility model at the CIEMAT institute, in Spain, to support the local CMS experiment community. Our presentation will report on the deployment of dedicated highly-performant hardware, the operation of data staging and caching services, that ensure prompt and efficient access to CMS physics analysis datasets, and the integration and optimization of a custom analysis framework, based on ROOT's RDataFrame and CMS NanoAOD format. Finally, performance results obtained by benchmarking the deployed infrastructure and software against a full CMS reference analysis workflow will be presented.

        Speakers: Dr Delgado Peris, Antonio (CIEMAT - PIC) , Dr Pérez-Calero Yzquierdo, Antonio (CIEMAT - PIC)
      • 2:30 PM
        The Creation and Evolution of the US ATLAS Shared Analysis Facilities 15m

        Prior to the start of the LHC Run 3, the US ATLAS Software and Computing operations program established three shared Tier 3 Analysis Facilities (AFs). The newest AF was established at the University of Chicago in the past year, joining the existing AFs at Brookhaven National Lab and SLAC National Accelerator Lab. In this paper, we will describe both the common and unique aspects of these three AFs, and the resulting distributed facility from the user’s perspective, including how we monitor and measure the AFs. The common elements include enabling easy access via Federated ID, file sharing via EOS, provisioning of similar Jupyter environments using common Jupyter kernels and containerization, and efforts to centralize documentation and user support channels. The unique components we will cover are driven in turn by the requirements, expertise and resources at each individual site. Finally, we will highlight how the US AFs are collaborating with other ATLAS and LHC wide (IRIS-HEP and HSF) user analysis support activities, evaluating tools like ServiceX and new file formats such as DAOD PHYSLITE.

        Speaker: Rind, Ofer (Brookhaven National Laboratory)
      • 2:45 PM
        Toward Ten-Minute Turnaround in CMS Data Analysis: The View from Notre Dame 15m

        Effective analysis computing requires rapid turnaround times in order to enable frequent iteration, adjustment, and exploration, leading to discovery. An informal goal of reducing 10TB of experimental data in about ten minutes using campus-scale computing infrastructure is an achievable goal, just considering raw hardware capability. However, compared to production computing, which seeks to maximize throughput at a massive scale over the timescale of weeks and months, analysis computing requires different optimizations in terms of startup latency, data locality, scalability limits, and long-tail behavior. At Notre Dame, we have developed substantial experience with running scalable analysis codes on campus infrastructure on a daily basis. Using the TopEFT application, based on the Coffea data analysis framework and the Work Queue distributed executor, we reliably process 2TB of data, 375 CPU-hours analysis codes to completion in about one hour on hundreds of nodes, albeit with a high variability due to competing system loads. The python environment needed in the compute nodes is setup and cached on the fly if needed (300MB as tarball sent to worker nodes, 1GB unpacked). In this talk, we present our analysis of the performance limits of the current system, taking into account software dependencies, data access, result generation, and fault tolerance. We present our plans for attacking the ten minute goal through a combination of hardware evolution, improved storage management, and application scheduling.

        Speaker: Lawrence, John (University of Notre Dame)
      • 3:00 PM
        Data handling of CYGNO experiment using INFN-Cloud solution 15m

        The INFN Cloud project was launched at the beginning of 2020, aiming to build a distributed Cloud infrastructure and provide advanced services for the INFN scientific communities. A Platform as a Service (PaaS) was created inside INFN Cloud that allows the experiments to develop and access resources as a Software as a Service (SaaS), and CYGNO is the beta-tester of this system. The aim of the CYGNO experiment is to realize a large gaseous Time Projection Chamber based on the optical readout of the photons produced in the avalanche multiplication of ionization electrons in a GEM stack. To this extent, CYGNO exploits the progress in commercial scientific Active Pixel Sensors based on Scientific CMOS for Dark Matter search and Solar Neutrino studies. CYGNO, like many other astroparticle experiments, requires a computing model to acquire, store, simulate and analyze data typically far from High Energy Physics (HEP) experiments. Indeed, astroparticle experiments are typically characterized by the fact to be less demanding from computing resources with respect to HEP one but have to deal with unique and unrepeatable data, sometimes collected in extreme conditions, with extensive use of templates and Montecarlo, and are often re-calibrated and reconstructed many times for a given data sets. Moreover, the varieties and the scale of computing models and requirements are extremely large. In this scenario, the Cloud infrastructure with standardized and optimized services offered to the scientific community could be a useful solution able to match the requirements of many small/medium size experiments. In this work, we will present the CYGNO computing model based on the INFN cloud infrastructure where the experiment software, easily extendible to similar experiments to similar applications on other similar experiments, provides tools as a service to store, archive, analyze, and simulate data.

        Speaker: Dr Mazzitelli, Giovanni (Laboratori Nazionali di Frascati)
      • 3:15 PM
        I/O performance studies of analysis workloads on production and dedicated resources at CERN 15m

        The recent evolutions of the analysis frameworks and physics data formats of the LHC experiments provide the opportunity of using central analysis facilities with a strong focus on interactivity and short turnaround times, to complement the more common distributed analysis on the Grid. In order to plan for such facilities, it is essential to know in detail the performance of the combination of a given analysis framework, of a specific analysis and of the installed computing and storage resources. This contribution describes performance studies performed at CERN, using the EOS disk-based storage, either directly or through an XCache instance, from both batch resources and high-performance compute nodes which could be used to build an analysis facility. A variety of benchmarks, both synthetic and based on real-world physics analyses and their corresponding input datasets, are utilized. In particular, the RNTuple format from the ROOT project is put to the test and compared to the latest version of the TTree format, and the impact of caches is assessed. In addition, we assessed the difference in performance between the use of storage system specific protocols, like XRootd, and FUSE. The results of this study are intended to be a valuable input in the design of analysis facilities, at CERN and elsewhere.

        Speaker: Sciabà, Andrea (CERN)
    • 2:00 PM 3:30 PM
      Track 8 - Collaboration, Reinterpretation, Outreach and Education: Open Science Project Reports Marriott Ballroom I

      Marriott Ballroom I

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Hernandez Villanueva, Michel (DESY) , Lange, Clemens (Paul Scherrer Institut)
      • 2:00 PM
        Machine Learning for Columnar High Energy Physics Analysis 15m

        Machine learning (ML) has become an integral component of high energy physics data analyses and is likely to continue to grow in prevalence. Physicists are incorporating ML into many aspects of analysis, from using boosted decision trees to classify particle jets to using unsupervised learning to search for physics beyond the Standard Model. Since ML methods have become so widespread in analysis and these analyses need to be scaled up for HL-LHC data, neatly integrating ML training and inference into scalable analysis workflows will improve the user experience of analysis in the HL-LHC era.

        We present the integration of ML training and inference into the IRIS-HEP Analysis Grand Challenge (AGC) pipeline to provide an example of how this integration can look like in a realistic analysis environment. We also utilize Open Data to ensure the project’s reach to the broader community. Different approaches for performing ML inference at analysis facilities are investigated and compared, including performing inference through external servers. Since ML techniques are applied for many different types of tasks in physics analyses, we showcase options for ML integration that can be applied to various inference needs.

        Speaker: Kauffman, Elliott (Princeton University)
      • 2:15 PM
        ML_INFN project: status report and future perspectives 15m

        The ML_INFN initiative (“Machine Learning at INFN”) is an effort to foster Machine Learning activities at the Italian National Institute for Nuclear Physics (INFN).

        In recent years, AI inspired activities have flourished bottom-up in many efforts in Physics, both at the experimental and theoretical level.

        Many researchers have procured desktop-level devices, with consumer oriented GPUs, and have trained themselves in a variety of ways, from webinars, books, tutorials.

        ML_INFN aims to help and systematize such effort, in multiple ways: by offering state-of-the art hardware for Machine Learning, leveraging on the INFN-Cloud provisioning solutions and thus sharing more efficiently GPU-like resources and leveling the access to such resources to all INFN researchers, and by organizing and curating Knowledge Bases with production grade examples from successful activities already in production.

        Moreover, training events have been organized for beginners, based on existing INFN ML research and focussed on flattening the learning curve.

        In this contribution we will update the status of the project reporting in particular on the development of tools to take advantage of High-Performance computing resources provisioned by CINECA for interactive and batch support to machine learning activities and on the organization of the first in-person advanced-level training event, with a GPU-equipped cloud-based envioronment provided to each participant.

        Speaker: Giommi, Luca (INFN Bologna)
      • 2:30 PM
        ScienceMesh: pan-European collaboration fabric for Science 15m

        Over the last few years, Cloud Sync&Share platforms have become go-to services for collaboration in scientific, academic and research environments, providing users with coherent and simple ways to access their data assets. Collaboration within those platforms, between local users on local applications, has been demonstrated in various settings, with visible improvements in the research production process. However, extending this paradigm beyond the borders of local and regional services has shown to be a challenge.

        The EU-funded CS3MESH4EOSC Project aims to address that problem, by providing a bridge between local data and applications, and remote users, in what can be described as a "mesh" of interconnected services. The ScienceMesh, a pan-European federated network of interoperable services, is the main outcome of this Project.

        We will present the architecture of the ScienceMesh and how it can be leveraged to extend local functionalities to remote users in other institutions, extending HEP beyond national frontiers and boosting cross-disciplinary research. We will then explain its technical foundations, from the APIs and protocols used in its design to the workflows which underlie its operations. We will also discuss the challenges faced during the implementation of the project, especially the integration with the two major open-source Sync&Share products on the market (ownCloud and Nextcloud). We will finish by explaining how we plan to extend the ScienceMesh to other areas and geographies.

        Speaker: Gonzalez, Hugo (CERN)
      • 2:45 PM
        10 years of Zenodo – growing the world’s largest general-purpose scholarly repository 15m

        Zenodo has over the past 10 years grown from a proof of concept to being the world's largest general-purpose research repository, cementing CERN’s image as a pioneer and leader in Open Science. We will review key challenges faced over the past 10 years and how we overcame them, from getting off the ground, over building trust to securing funding.

        Growing Zenodo was an enriching and learning experience on how CERN technology can be put at the service of everyone across all research disciplines. We will show how Zenodo helped shape Open Science as we know it and became an essential component of the future European and global Open Science infrastructure.

        After 10 successful years, we are getting ready for the next decade. Zenodo is going through a transformation that will make CERN technology even more reachable and useful to the world-wide research community. We will show a glimpse of what’s coming and look ahead to key challenges such as governance, data publishing ethics and how Zenodo can help continue to grow and support the adoption of open science practices, not only within physics but also across the globe’s research communities.

        Speaker: Nielsen, Lars Holm (CERN)
      • 3:00 PM
        The ALICE Glance Service Work system 15m

        The "A Large Ion Collider Experiment" (ALICE), one of the four large experiments at the European Organization for Nuclear Research (CERN), is responsible for studying the physics of strongly interacting matter and the quark-gluon plasma.
        In order to ensure the full success of ALICE operation and data taking during the Large Hadron Collider Runs 3 and 4, a list of tasks identified as Service Work is established and maintained, which concerns detector maintenance, operation, calibration, quality control, data processing and outreach, as well as coordination and managerial roles in ALICE.
        The ALICE Glance Service Work system is a tool developed in a cooperation between the Federal University of Rio de Janeiro and the ALICE Collaboration that serves as the link between the user interaction and thousands of database entries. In this poster we describe the development process of this system and its functionalities that ranges from planning the entire year of work for hundred of tasks to individually assigning these tasks to members of the collaboration.
        The system is divided into two distinct environments that communicates to generate a service. The first is a REST API written in modern PHP with its source code composed of bounded contexts following the Domain Driven Design paradigm, making the code very adaptable to different interfaces, be it a HTTP controller, in our case the Slim framework or a CLI command. The second is a responsive and clean web page made with the Vue.js framework, responsible to communicate with the user and to provide them with the means to make the requests to the API.
        Our database versioning is managed by the PHP Doctrine library, making it easy to semi-automatic deploy our development changes to production.

        Speaker: De Souza Pereira, Jomar Junior (Universidade Federal do Rio De Janeiro, COPPE/EE/IF, Brazil)
      • 3:15 PM
        Software Citation in HEP: Current State and Recommendations for the Future 15m

        In November 2022, the HEP Software Foundation (HSF) and the Institute for Research and Innovation for Software in High-Energy Physics (IRIS-HEP) organized a workshop on the topic of “Software Citation and Recognition in HEP”. The goal of the workshop was to bring together different types of stakeholders whose roles relate to software citation and the associated credit it provides, in order to engage the community in a discussion of: 1) the ways in which HEP experiments handle citation of software; 2) recognition for software efforts that enable physics results disseminated to the public; and 3) how the scholarly publishing ecosystem supports these activities. We heard from the publication board leadership of ATLAS, CMS, and LHCb in order to understand the current practice of these experiments; various open source community organizations (ROOT, Scikit-HEP, MCnet) discussed how they prefer their software to be cited; talks from publishers (Elsevier, JOSS) recognized the issue and showed an openness to following the wishes of the community; and discussions with tool providers (INSPIRE, Zenodo) covered new standards and tools for citation. The workshop made a number of tensions clear, for example between citations being used for credit and for reproducibility, and between supporting the immediate (and possibly contradictory) desires of software producers that lead to credit in today's culture and actions that might positively change the culture to better recognize the work of these developers. This talk will present highlights from the workshop as well as findings and recommendations documented in the workshop report.

        Speaker: Feickert, Matthew (University of Wisconsin-Madison)
    • 2:00 PM 3:30 PM
      Track 9 - Artificial Intelligence and Machine Learning: Applications 2 Hampton Roads VII

      Hampton Roads VII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Dal Pra, Stefano (INFN-CNAF) , Wenzel, Sandro (CERN)
      • 2:00 PM
        Deep Learning for Amplitude Analysis in Spectroscopy 15m

        Abstract

        We present results on Deep Learning applied to Amplitude and Partial Wave Analysis (PWA) for spectroscopic analyses. Experiments in spectroscopy often aim to observe strongly-interacting, short-lived particles that decay to multi-particle final states. These particle decays have angular distributions that our deep learning model has been trained to identify. Working with TensorFlow and Keras libraries we have developed several neural network architectures that will be presented. One architecture that will be highlighted is our “Hybrid” Autoencoder (AE) architecture that has the best performance by far as it is able to resolve ambiguities. This AE is an unsupervised regressor that constrains the latent space variables to represent physically relevant quantities such as production amplitudes. As the training needs to be performed in a large amount of simulated data, a novel on-the-fly generation techniques is also used. Results of performed mass-independent and mass-dependent amplitude analyses using this technique will be presented.

        Speaker: Dr Phelps, William (Christopher Newport University and Jefferson Lab)
      • 2:15 PM
        Machine learning based compression for scientific data 15m

        One common issue in vastly different fields of research and industry is the ever-increasing need for more data storage. With experiments taking more complex data at higher rates, the data recorded is quickly outgrowing the storage capabilities. This issue is very prominent in LHC experiments such as ATLAS where in five years the resources needed are expected to be many times larger than the storage available (assuming a flat budget model and current technology trends) [1]. Since the data formats used are already highly compressed, storage constraints could require more drastic measures such as lossy compression, where some data accuracy is lost during the compression process.

        In our work, following from a number of undergraduate projects [2,3,4,5,6,7], we have developed an interdisciplinary open-source tool for machine learning-based lossy compression. The tool utilizes an autoencoder neural network, which is trained to compress and decompress data based on correlations between the different variables in the dataset. The process is lossy, meaning that the original data values and distributions cannot be reconstructed precisely. However, for certain variables and observables where the precision loss is tolerable, the high compression ratio allows for more data to be stored yielding greater statistical power.

        [1] - https://cerncourier.com/a/time-to-adapt-for-big-data/
        [2] - http://lup.lub.lu.se/student-papers/record/9049610
        [3] - http://lup.lub.lu.se/student-papers/record/9012882
        [4] - http://lup.lub.lu.se/student-papers/record/9004751
        [5] - http://lup.lub.lu.se/student-papers/record/9075881
        [6] - https://zenodo.org/record/5482611#.Y3Yysy2l3Jz
        [7] - https://zenodo.org/record/4012511#.Y3Yyny2l3Jz

        Speakers: Gallén, Axel (Lund University (SE)) , Ekman, Alexander (Lund University (SE))
      • 2:30 PM
        Pion/Kaon Identification at STCF DTOF Based on Classical/Quantum Convolutional Neural Network 15m

        The Super Tau Charm Facility (STCF) proposed in China is a new-generation electron–positron collider with center-of-mass energies covering 2-7 GeV. In STCF, the discrimination of high momentum hadrons is a challenging and critical task for various physics studies. In recent years, machine learning methods have gradually become one of the mainstream methods in the PID field of high energy physics experiments, with the advantage of big data processing.
        In this work, targeting at the pion/kaon identification problem at STCF, we have developed a convolutional neural network (CNN) in the endcap PID system, which is a time-of-flight detector based on detection of internally reflected Cherenkov light (DTOF). By combining the hit position and arrival time of each Cherenkov photon at multi-anode microchannel plate photomultipliers, a two dimensional pixel map is constructed as the CNN input. The preliminary results show that the CNN model has a promising performance against the pion/kaon identification problem. In addition, based on the traditional CNN, a quantum convolution neural network (QCNN) is developed as well, as a proof-of-concept work exploring possible quantum advantages provided by quantum machine learning methods.

        Speaker: Li, Teng
      • 2:45 PM
        Particle identification with machine learning in ALICE Run 3 15m

        The main focus of the ALICE experiment, quark-gluon plasma measurements, requires
        accurate particle identification (PID). The ALICE detectors allow identifying particles over a broad momentum interval ranging from about 100 MeV/c up to 20 GeV/c.

        However, hand-crafted selections and the Bayesian method do not perform well in the
        regions where the particle signals overlap. Moreover, an ML model can explore more
        detector information. During LHC Run 2, preliminary studies with Random Forests obtained much higher efficiencies and purities for selected particles than standard techniques.

        For Run 3, we investigate Domain Adaptation Neural Networks that account for the
        discrepancies between the Monte Carlo simulations and the experimental data. Preliminary studies show that domain adaptation improves particle classification. Moreover, the solution is extended with Feature Set Embedding to give the network more flexibility to train on data with various sets of detector signals.

        PID ML is already integrated with the ALICE Run 3 Analysis Framework. Preliminary results for the PID of selected particle species, including real-world analyzes, will be discussed as well as the possible optimizations.

        Speaker: Kabus, Maja (CERN / Warsaw University of Technology)
      • 3:00 PM
        Flashsim: a ML based simulation for analysis datatiers 15m

        Analyses in HEP experiments often rely on large MC simulated datasets. These datasets are usually produced with full-simulation approaches based on Geant4 or exploiting parametric “fast” simulations introducing approximations and reducing the computational cost. With our work we created a prototype version of a new “fast” simulation that we named “flashsim” targeting analysis level data tiers (such as CMS NanoAOD). Such a simulation software is based on Machine Learning, in particular exploiting the Normalizing Flows generative model. We will present the physics results achieved with this prototype, currently simulating only a few physics objects collections, in terms of: 1) accuracy of object properties, 2) correlations among paris of observables, 3) comparisons of analysis level derived quantities and discriminators between full-simulation and flash-simulation of the very same events. The speed up obtained with such an approach is of several orders of magnitude, so that when using flashsim the simulation bottleneck is represented by the “generator” (e.g. Pythia) step. We further investigated upsampling techniques, reusing the same “generated event” passing it multiple times through the detector simulation, in order to understand the increase in statistical precision that could be ultimately achieved. The results achieved with the current prototype show a higher physics accuracy and a lower computing cost compared to other fast simulation approaches such as CMS standard fastsim and Delphes based simulations.

        Speaker: Vaselli, Francesco (Scuola Normale Superiore & INFN Pisa)
      • 3:15 PM
        FastCaloGAN: a fast simulation of the ATLAS Calorimeter with GANs 15m

        AtlFast3 is the new ATLAS fast simulation that exploits a wide range of ML techniques to achieve high-precision fast simulation. The latest version of the AtlFast3 used in Run3 deploys FastCaloGANV2 which consists of 500 Generative Adversarial Networks used to simulate the showers of all particles in the ATLAS calorimeter system. The Muon Punch Through tool has also been completely rewritten using deep NN for the classification of events. An additional deep network is used to predict and correct the longitudinal position of the hits in the calorimeter layer based on the energy deposited by each shower in the calorimeter layers. These tools have been instrumental in improving the performance of AtlFast3.

        Speaker: Giannelli, Michele Faucci (INFN Roma Tor Vergata and Universita' di Roma Tor Vergata)
    • 2:00 PM 3:30 PM
      Track X - Exascale Science, Heterogeneous Computing and Accelerators, and Quantum Computing: Simulaton on Heterogeneous Architectures Marriott Ballroom VII

      Marriott Ballroom VII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Aaij, Roel (Nikhef National institute for subatomic physics (NL)) , Timm, Steven (Fermi National Accelerator Laboratory)
      • 2:00 PM
        CaTS: Integration of Geant4 and Opticks 15m

        CaTS is a Geant4 advanced example that is part of Geant4[1] since version 11.0. It demonstrates the use of Opticks[2] to offload the simulation of optical photons to GPUs. Opticks interfaces with the Geant4 toolkit to collect all the necessary information to generate and trace optical photons, re-implements the optical physics processes to be run on the GPU, and automatically translates the Geant4 geometry into a GPU appropriate format. To trace the photons Opticks
        uses NVIDIA® OptiX7™ [3]. In this presentation we shall describe CaTS and the work performed to integrate Opticks with Geant4 using the tasking mechanism and the work to include CaTS in the software framework used by liquid Argon TPC neutrino experiments. We shall demonstrate that the generation and tracing of optical photons represents an ideal application to be offloaded to GPUs, fully utilizing the high degree of available parallelism. In a typical liquid Argon TPC simulation, a speedup of several hundred times compared to single threaded Geant4 is observed.

        [1]https://geant4.web.cern.ch/
        [2]https://doi.org/10.1051/epjconf/202125103009
        [3]https://developer.nvidia.com/rtx/ray-tracing/optix

        Keywords: Simulation of optical photons, GPUs.

        Speaker: Wenzel, Hans (Fermilab)
      • 2:15 PM
        Madgraph5_aMC@NLO on GPUs and vector CPUs: experience with the first alpha release 15m

        Madgraph5_aMC@NLO is one of the workhorses for Monte Carlo event generation in the LHC experiments and an important consumer of compute resources. The software has been reengineered to maintain the overall look-and-feel of the user interface while achieving very large overall speedups. The computationally intensive part (the calculation of "matrix elements") is offloaded to new implementations optimized for GPUs and for vector CPUs, using event-level data parallelism. In this contribution, we will report on the first experience with the alpha release of the software supporting leading-order QCD processes. The achieved performance speedups and the potential for further improvements will be discussed in detail.

        Speaker: Hageboeck, Stephan
      • 2:30 PM
        Acceleration beyond lowest order event generation 15m

        An important area of HEP studies at the LHC currently concerns the need for more extensive and precise comparison data. Important tools in this realm are event reweighting and the evaluation of more precise next-to-leading order (NLO) physics processes via Monte Carlo (MC) event generators, especially in the context of the upcoming High Luminosity LHC phase. Current event generators need to improve their throughput for these studies. MadGraph5_aMC@NLO (MGaMC) is an event generator being used heavily by LHC experiments which has been accelerated considerably with a GPU and vector CPU port, but as of yet only for leading order processes. In this contribution, a prototype for event reweighting using the accelerated MGaMC software package, as well as plans for the implementation of NLO calculations, will be presented.

        Speaker: Wettersten, Zenny (CERN)
      • 2:45 PM
        Parallelization of Air Shower Simulation with IceCube 15m

        The IceCube Neutrino Observatory is a cubic kilometer neutrino telescope
        located at the Geographic South Pole. For every observed neutrino event,
        there are over 10^6 background events caused by cosmic-ray air shower
        muons. In order to properly separate signal from background, it is
        necessary to produce Monte Carlo simulations of these air showers.
        Although to-date, IceCube has produced large quantities of background
        simulation, these studies remain statistics limited. The most
        significant impediment to producing more simulation is complicated
        computing requirements: the first stage of the simulation, air shower
        and muon propagation, needs to be run on CPUs while the second stage,
        photon propagation, can only be performed efficiently on GPUs.
        Processing both of these stages on the same node will result in an
        underutilized GPU but using different nodes will encounter bandwidth
        bottlenecks. Furthermore, due to the power-law energy spectrum of cosmic
        rays, the memory footprint of the detector response often exceeded the
        limit in unpredictable ways. In this talk, I will present new
        client/server code which parallelizes the first stage onto multiple CPUs
        on the same node and then passes it on to the GPU for photon
        propagation. This results in GPU utilization of greater than 90% as well
        as more predictable memory usage and an overall factor of 20 improvement
        in speed over previous techniques.

        Speaker: Dr Meagher, Kevin (University of Wisconsin–Madison)
      • 3:00 PM
        Celeritas: EM physics on GPUs and a path to full-featured accelerated detector simulation 15m

        Celeritas is a new Monte Carlo detector simulation code designed for computationally intensive applications (specifically, HL-LHC simulation) on high-performance heterogeneous architectures. In the past two years Celeritas has advanced from prototyping a simple, GPU-based, single-physics-model infinite medium to implementing a full set of electromagnetic physics processes in complex geometries. The latest release of Celeritas has incorporated full VecGeom device-based navigation, an event loop in the presence of magnetic fields, and detector hit scoring. The new Acceleritas library provides a scheduler to offload electromagnetic physics to the GPU within a Geant4 driven simulation, enabling integration of Celeritas into HEP experimental frameworks such as CMSSW. Finally, we are collaborating with the AdePT team to design a suite of benchmarks to verify the correctness and evaluate the performance of GPU-enabled detector simulations. We present an overview of these new capabilities in Celeritas and show the performance results on both standalone and Geant4-integrated detector simulation benchmarks on both Nvidia and AMD GPU-based architectures.

        Speaker: Johnson, Seth (Oak Ridge National Laboratory)
    • 3:30 PM 4:00 PM
      PM Break 30m Hampton Roads Ballroom (3rd floor)

      Hampton Roads Ballroom (3rd floor)

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
    • 4:00 PM 6:00 PM
      Plenary Session: "Challenges in AI/ML" & "Opportunities in ESCAPE" Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Convener: Girone, Maria (CERN)
      • 4:00 PM
        Radically different futures for HEP enabled by AI/ML 30m

        Instead of focusing on the concrete challenges of incremental changes to HEP driven by AI/ML, it is perhaps a useful exercise to think through more radical, speculative changes. What might be enabled if we embraced a dramatically different approach? What would we lose? How would those changes impact the computational, organizational, and epistemological nature of the field?

        Speaker: Cranmer, Kyle (University of Wisconsin-Madison)
      • 4:30 PM
        AI and Beyond: New Techniques for Simulation and Design in HEP 30m

        Simulation is a critical component of high energy physics research, with a corresponding computing footprint. Generative AI has emerged as a promising complement to intensive full simulation with relatively high accuracy compared to existing classical fast simulation alternatives. Such algorithms are naturally suited to acceleration on coprocessors, potentially running fast enough to match the high data volumes at next-generation experiments. Numerous techniques are currently being explored, each with its own advantages and challenges. Looking beyond the next generation, foundational building blocks of AI such as automatic differentiation and gradient descent are now being incorporated into fully differentiable programming. This new paradigm will provide revolutionary tools for designing and optimizing future experiments.

        Speaker: Pedro, Kevin (Fermilab)
      • 5:00 PM
        The ESCAPE Dark Matter Science Project in the European Science Cloud 30m

        A Dark Matter Science Project is being developed in the context of the ESCAPE project as a collaboration between scientists in European Research Infrastructures and experiments seeking to explain the nature of dark matter (such as HL-LHC, KM3NeT, CTA, DarkSide).
        The goal of this ESCAPE Science Project is to highlight the synergies between different dark matter communities and experiments, by producing new scientific results as well as by making the necessary data and software tools fully available.
        As part of this Science Project, we use experimental data and software algorithms from selected direct detection, indirect detection, and particle collider experiments involved in ESCAPE as prototypes for end-to-end analysis pipelines on a Virtual Research Environment that is being prepared as one of the building blocks of the European Open Science Cloud (EOSC).
        This contribution focuses on the implementation of the workflows on the Virtual Research Environment using ESCAPE tools (such as the Data Lake and REANA), and on the prospects for data management, data analysis and computing in the EOSC-Future project.

        Speaker: Little, Jared (LAPP/CNRS)
      • 5:30 PM
        The ESCAPE Collaboration - long term perspective 30m

        The EU-funded ESCAPE project has brought together the ESFRI and other world class Research Infrastructures in High Energy and Nuclear Physics, Astro-Particle Physics, and Astronomy.  In the 3 years of the project many synergistic and collaborative aspects have been highlighted and explored,  from pure technical collaboration on common solutions for data management, AAI, and workflows, through development of new tools, such as AI/ML, and in education and training, for example in the area of Research Software.  In addition, the project has shown that the communities have a lot in common, and can act as a single voice towards the funding agencies, the EC, and other key developments such as the European Open Science Cloud.   ESCAPE is one of five such "cluster" projects, and the communities involved have found that the cluster concept is extremely useful in structuring the overall scientific community, and with many cross-domain commonalities are very important in acting together towards various political and funding bodies.  Consequently we consider forming a long-term ESCAPE collaboration, that would exist independently of specific project funding, that can maintain the synergistic aspects of the ESCAPE scientific communities, while bringing new ones into the forum, and coordinate the interaction of those communities with the broader scientific and funding landscape.  This talk will justify such a collaboration, outline some of its goals, and discuss the possible forms that it can take.

        Speaker: Lamanna, Giovanni (CNRS-LAPP)
    • 6:30 PM 7:30 PM
      Reception 1h Hampton Roads Ballroom & Foyer (3rd floor)

      Hampton Roads Ballroom & Foyer (3rd floor)

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
    • 8:00 AM 9:00 AM
      Registration
    • 9:00 AM 10:30 AM
      Plenary Session: Computing Infrastructure & Future Directions Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Convener: LAURET, Jerome (Brookhaven Science Associates)
      • 9:00 AM
        The Virtual Research Environment: towards a comprehensive analysis platform 30m

        One of the objectives of the EOSC (European Open Science Cloud) Future Project is to integrate diverse analysis workflows from Cosmology, Astrophysics and High Energy Physics in a common framework. The project’s development relies on the implementation of the Virtual Research Environment (VRE), a prototype platform supporting the goals of Dark Matter and Extreme Universe Science Projects in the respect of FAIR data policies. It makes use of a common AAI system, and exposes the experiments’ data (ATLAS, Fermi-LAT, CTA, Darkside, Km3Net, Virgo, LOFAR) in a reliable distributed storage infrastructure for multi-science: the Data Lake. The entry point of such a platform is a jupyterhub instance deployed on top of a scalable Kubernetes infrastructure, providing an interactive graphical interface for researchers to access, analyse and share data. The data access and browsability is enabled through API calls to the high level data management and storage orchestration software (Rucio). In this contribution we will provide an overview of the VRE and present our recent work to improve its usability and functionality. The improvements include a software repository plug-in enabling researchers to directly select computational environments from Docker images and the integration of a re-analysis platform (Reana) supporting various distributed computing backends. The final goal of the VRE project, bringing together data and software access, workflow reproducibility and enhanced user interface, is to facilitate scientific collaboration, ultimately accelerating research in various fields.

        Speaker: Gazzarrini, Elena (CERN)
      • 9:30 AM
        Evolution of ESnet - A Changing Landscape in Scientific Networking 30m

        The Energy Sciences Network (ESnet) is the high performance network of the US Department of Energy Office of Science. Over its 36-year span, ESnet has evolved to meet the requirements of ever changing scientific workflows. This presentation will provide a brief history of ESnet's generational changes and highlight the capabilities of its current generation network ESnet6. This presentation will also provide a glimpse into a future ESnet(7) and the requirements driving its design.

        Speaker: Guok, Chin (ESnet)
      • 10:00 AM
        Coffea-Casa: Building composable analysis facilities for the HL-LHC 30m

        The large data volumes expected from the High Luminosity LHC (HL-LHC) present challenges to existing paradigms and facilities for end-user data analysis. Modern cyberinfrastructure tools provide a diverse set of services that can be composed into a system that provides physicists with powerful tools that give them straightforward access to large computing resources, with low barriers to entry. The coffea-casa analysis facility provides an environment for end users enabling the execution of increasingly complex analyses such as those demonstrated by the Analysis Grand Challenge (AGC) and capturing the features that physicists will need for the HL-LHC.
        We describe the development progress of the coffea-casa facility featuring its modularity while demonstrating the ability to port and customize the facility software stack to other locations. The facility also facilitates the support of different backends to other batch systems while staying Kubernetes-native.
        We present evolved architecture of the facility, such as the integration of advanced data delivery services (e.g. ServiceX) and making data caching services (e.g. XCache) available to end users of the facility.
        We also highlight the composability of modern cyberinfrastructure tools. To enable machine learning pipelines at coffee-casa analysis facilities, a set of industry ML solutions adopted for HEP columnar analysis were integrated on top of existing facility services. These services also feature transparent access for user workflows to GPUs available at a facility via inference servers while using Kubernetes as enabling technology.

        Speaker: Shadura, Oksana (University Nebraska-Lincoln (US))
    • 10:30 AM 11:00 AM
      AM Break 30m Hampton Roads Ballroom (3rd floor)

      Hampton Roads Ballroom (3rd floor)

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
    • 11:00 AM 12:30 PM
      Track 1 - Data and Metadata Organization, Management and Access: Clouds & Caches Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Barisits, Martin (CERN) , Kirby, Michael (FNAL)
      • 11:00 AM
        Xrootd S3 Gateway for WLCG Storage 15m

        The Xrootd S3 Gateway is a universal high performance proxy service that can be used to access S3 portals using existing HEP credentials (e.g. JSON Web Tokens and x509). This eliminates one of the biggest roadblocks to using public cloud storage resources. This paper describes how the S3 Gateway leverages existing HEP software (e.g. Davix and XRootD) to provide a familiar scalable service that works with public (i.e. AWS, GCS, etc) and private (i.e. CEPH, MinIO, etc.) S3 portal available to the HEP community, and to seamlessly integrate them into the WLCG storage and data transfer ecosystem. The test was conducted at an ATLAS site and ATLAS installation in GCP and AWS.

        Speaker: Yang, Wei (SLAC National Accelerator Laboratory)
      • 11:15 AM
        Predicting Resource Usage Trends with Southern California Petabyte Scale Cache 15m

        There has been a significant increase in data volume from various large scientific projects, including the Large Hadron Collider (LHC) experiment. The High Energy Physics (HEP) community requires increased data volume on the network, as the community expects to produce almost thirty times annual data volume between 2018 and 2028 [1]. To mitigate the repetitive data access issue and network overloading, regional data caching mechanism [2], [3], or in-network cache has been deployed in Southern California for the US CMS, and its effectiveness has been studied [4], [5]. With the number of redundant data transfers over the wide-area network decreasing, the caching approach improves overall application performance as well as network traffic savings.

        In this work, we examined the trends in data volume and data throughput performance from the Southern California Petabyte Scale Cache (SoCal Repo) [6], which includes 24 federated caching nodes with approximately 2.5PB of total storage. From the trends, we also determined how much a machine learning model can predict the network access patterns for the regional data cache. The fluctuation in the daily cache utilization, as shown in Figure 1, is high, and it is challenging to build a learning model to follow the trends.

        Figure 1: Daily proportion of cache hits volume and cache misses volume from July 2021 to June 2022, with 8.02 million data access records for 8.2PB of traffic volume for cache misses and 4.5PB of traffic volume for cache hits. 35.4% of the total traffic has been saved from the cache.

        The daily and hourly study also modeled the cache utilization and data throughput performance, with 80% of the training data and 20% of the testing data. Figure 2 shows the samples of our hourly study results. The root-mean-square error (RMSE) is measured and compared to the standard deviation of the input data values to provide a reference to determine how large the errors of predictions are. The relative error, ratio of testing RMSE and standard deviation, is less than 0.5, indicating the predictions are pretty accurate.


        Figure 2 (a): Hourly volume of cache misses; training set RMSE=0.16, testing set RMSE=0.40, std.dev=1.42

        Figure 2 (b): Hourly throughput of cache misses; training set RMSE=25.90, testing set RMSE=18.93, std.dev=121.36

        The study results can be used to optimize the cache utilization, network resources, and application workflow performance, and become the base for exploring characteristics of other data lakes as well as examining longer term network requirements for the data caches.

        Full PDF of the extended abstract is available online: https://sdm.lbl.gov/students/chep23/CHEP23_xcache_ext_abstract.pdf

        References
        [1] B. Brown, E. Dart, G. Rai, L. Rotman, and J. Zurawski, “Nuclear physics network requirements review report,” Energy Sciences Network, University of California, Publication Management System Report LBNL- 2001281, 2020. [Online]. Available: https://www.es.net/assets/Uploads/ 20200505- NP.pdf
        [2] X. Espinal, S. Jezequel, M. Schulz, A. Sciaba`, I. Vukotic, and F. Wuerthwein, “The quest to solve the hl-lhc data access puzzle,” EPJ Web of Conferences, vol. 245, p. 04027, 2020. [Online]. Available: https://doi.org/10.1051/epjconf/202024504027
        [3] E. Fajardo, D. Weitzel, M. Rynge, M. Zvada, J. Hicks, M. Selmeci, B. Lin, P. Paschos, B. Bockelman, A. Hanushevsky, F. Wu ̈rthwein, and I. Sfiligoi, “Creating a content delivery network for general science on the internet backbone using XCaches,” EPJ Web of Conferences, vol. 245, p. 04041, 2020. [Online]. Available: https://doi.org/10.1051/epjconf/202024504041
        [4] E. Copps, H. Zhang, A. Sim, K. Wu, I. Monga, C. Guok, F. Wurthwein, D. Davila, and E. Fajardo, “Analyzing scientific data sharing patterns with in-network data caching,” in 4th ACM International Workshop on System and Network Telemetry and Analysis (SNTA 2021), ACM. ACM, 2021.
        [5] R. Han, A. Sim, K. Wu, I. Monga, C. Guok, F. Wurthwein, D. Davila, J. Balcas, and H. Newman, “Access trends of in-network cache for scientific data,” in 5th ACM International Workshop on System and Network Telemetry and Analysis (SNTA 2022), ACM. ACM, 2022.
        [6] E. Fajardo, A. Tadel, M. Tadel, B. Steer, T. Martin, and F. Wu ̈rthwein, “A federated xrootd cache,” Journal of Physics: Conference Series, vol. 1085, p. 032025, 2018.

        Speaker: Sim, Alex (Lawrence Berkeley National Laboratory)
      • 11:30 AM
        Storing LHC Data in Amazon S3 and Intel DAOS through RNTuple 15m

        Current and future distributed HENP data analysis infrastructures rely increasingly on object stores in addition to regular remote file systems. Such file-less storage systems are popular as a means to escape the inherent scalability limits of the POSIX file system API. Cloud storage is already dominated by S3-like object stores, and HPC sites are starting to take advantage of object stores for the next generation of supercomputers. In light of this, ROOT's new I/O subsystem RNTuple has been engineered to support object stores alongside (distributed) file systems as first class citizens, while also addressing performance bottlenecks and interface shortcomings of its predecessor, TTree I/O.
        In this contribution, we describe the improvements around RNTuple’s support for object stores, expounding on the challenges and insights toward efficient storage and high-throughput data transfers. Specifically, we introduce RNTuple’s native backend for the Amazon S3 cloud storage and present the latest developments in our Intel DAOS backend, demonstrating RNTuple’s integration with next-generation HPC sites.
        Through experimental evaluations, we compare the two backends in single node and distributed end-to-end analyses using ROOT’s RDataFrame, proving Amazon S3 and Intel DAOS as viable HENP storage providers.

        Speaker: Ms Lazzari Miotto, Giovanna (UFRGS (BR))
      • 11:45 AM
        Understanding Data Access Patterns for dCache System 15m

        At Brookhaven National Lab, the dCache storage management system is used as a disk cache for large high-energy physics (HEP) datasets primarily from the ATLAS experiment[1]. Storage space on dCache is considerably smaller than the full ATLAS data collection. Therefore, a policy is needed to determine what data files to keep in the cache and what files to evict. A good policy is to keep frequently needed files in the future. In this work, we use the current and past file access information to predict the number of file accesses in the next day. The analysis tasks from the ATLAS experiment often access a predefined dataset as a group. Therefore, this study predicts how many times a dataset will be accessed in the future rather than each individual file.
        HEP collaborations like ATLAS generate files in groups known as datasets and each of these groups (datasets) is produced by a task (such as an physical exepriement and a simulation) with a Task ID, or TID. The dCache system operators are considering policies specified in TIDs rather than individual files. For example, if a dataset (with a specific TID) is expected to be very popular in the next few days, it might make sense to ping all files of the dataset in disk.
        To investigate how datasets tend to be accessed, we first performed K-means clustering on 9 months’ worth of dCache operational logs. Figure 1 shows the results of clustering the datasets according to their present and next day access counts. The cluster corresponding to datasets with less than 10^4 accesses is extremely large, whereas the clusters corresponding to higher numbers of accesses are small. This indicates that the majority of datasets are accessed relatively few times, and that there is also a small number of highly popular datasets. Pinging the small group of very popular datasets in dCache would achieve our goal of a popularity-based cache policy.

        Figure 1: K-means clustering with k=4. A small number of datasets are accessed much more frequently than others and their access counts might be predictable.

        The neural network was trained using a dataset containing information for 9 months’ worth of dCache transactions. We process the raw dCache logs into daily access statistics with the next day’s access count as the target variable for learning. The neural network was built using PyTorch; it uses 2 dense layers, the Tanh activation function, and the ADAM optimizer.

        Figure 2: Predicted vs. actual access counts in the next day. The 100 most popular datasets sorted according to their actual access counts.

        Figure 2 shows the predicted access values vs the actual access values for the 100 most popular datasets. The most popular dataset is accessed much more than the second most popular dataset, while the access counts of the next ten most popular datasets follow a power law with the exponent of -0.57, and an RMSE of 5.7 × 10^5. The access counts of many commonly accessed datasets follow the same power law show in Figure 2 for the majority of the top 100 popular datasets. This power law has an exponent of -0.47, and an RMSE of 2.0 × 10^6. This corroborates the pattern shown in Figure 1, where there is a small group of highly popular datasets, and their accesses are more predictable. Since the most popular few datasets are accessed much more frequently than others, pinging them in the disk cache could simplify the cache replacement decisions without sacrificing the overall disk cache effectiveness.
        In summary, our results show that the popularity of the most popular datasets are predictable. It is therefore possible to ping these datasets in dCache, yielding a more effective cache policy. Future work will develop, simulate, and benchmark cache policies based off of the method presented here.

        The PDF version of the extended abstract is available on https://sdm.lbl.gov/students/chep23/CHEP23_dCache_ext_abstract.pdf

        Speaker: Wu, Kesheng (Lawrence Berkeley National Laboratory)
      • 12:00 PM
        A Ceph S3 Object Data Store for HEP 15m

        In this talk, we present a novel data format design that obviates the need for data tiers by storing individual event data products in column objects. The objects are stored and retrieved through Ceph S3 technology, and a companion metadata system handles tracking of the object lifecycle. Performance benchmarks of data storage and retrieval will be presented, along with scaling tests of the data and metadata system.

        Speaker: Smith, Nick (Fermilab)
      • 12:15 PM
        Extending Rucio with modern cloud storage support: Experiences from ATLAS, SKA and ESCAPE 15m

        Rucio is a software framework that provides scientific collaborations with the ability to organise, manage and access large volumes of data using customisable policies. The data can be spread across globally distributed locations and across heterogeneous data centres, uniting different storage and network technologies as a single federated entity. Rucio offers advanced features such as distributed data recovery or adaptive replication, and is highly scalable, modular, and extensible. Rucio has been originally developed to meet the requirements of the high-energy physics experiment ATLAS, and is being continuously extended to support LHC experiments and other diverse scientific communities. In recent years several R&D projects in these communities have started to evaluate the integration of both private and commercially-provided cloud storage systems. As they are using Rucio, new functionality has been developed to make the integration as seamless as possible. In addition the underlying systems, FTS and GFAL/Davix, have been extended for these use cases. In this contribution we detail the technical aspects of this work. In particular the challenges when building a generic interface to self-hosted cloud storage such as MinIO or CEPH S3 Gateway, to established providers such as Google Cloud Storage and Amazon Simple Storage Service, as well as upcoming decentralised clouds such as SEAL. We will highlight aspects such as authentication and authorisation, direct and remote access, throughput and cost estimation, and give experiences on daily operations.

        Speaker: Lassnig, Mario (CERN)
    • 11:00 AM 12:30 PM
      Track 2 - Online Computing: DQ, Monitoring & Control Marriott Ballroom V-VI

      Marriott Ballroom V-VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Antel, Claire (Universite de Geneve (CH)) , Shahoyan, Ruben (CERN)
      • 11:00 AM
        The Run-3 ATLAS jet trigger 15m

        The ATLAS jet trigger is instrumental in selecting events both for Standard Model measurements and Beyond the Standard Model physics searches. Non-standard triggering strategies, such as saving only a small fraction of trigger objects for each event, avoids bandwidth limitations and increases sensitivity to low-mass and low-momentum objects. These events are used by Trigger Level Analyses, which can reach regions of parameter space that would otherwise be inaccessible. To this end, the calibration of trigger-level jets is imperative both to ensure good trigger performance across the ATLAS physics programme and to provide well-measured jets for Trigger Level Analysis. This contribution presents an introduction to the ATLAS jet trigger for Run-3 of the LHC and discusses the performance of the trigger jet calibration. These studies will allow us to commission a Run-3 trigger jet calibration that provides excellent performance across a broad jet transverse momentum range as low as 25 GeV.

        Speaker: Amerl, Maximilian
      • 11:15 AM
        LHCb Online Monitoring 15m

        The LHCb experiment started taking data with an upgraded detector in the Run 3 of the LHC, reading at 30 MHz full detector data with a software-only trigger system. In this context, live data monitoring is crucial to ensure that the quality of the recorded data is optimal. Data from the experiment control system, as well as raw detector data and the output of the software trigger, is used as input to the monitoring system. Plots of important quantities are delivered to the so called data manager shifter, present permanently in the control room. In addition, the same system is used to evaluate the quality of the data for future physics analyses. The presentation will describe the tools involved in the online monitoring: the infrastructure, the data processing, the plot visualisation applications and the various reporting tools available for experts to diagnose and follow problems arising during data taking.

        Speaker: Matev, Rosen
      • 11:30 AM
        First year of experience with the new operational monitoring tool for data taking in CMS during Run 3 15m

        The CMS Online Monitoring System (OMS) aggregates and integrates different sources of information into a central place and allows users to view, compare and correlate information. It displays real-time and historical information.
        The tool is heavily used by run coordinators, trigger experts and shift crews, to achieve optimal trigger and efficient data taking. It provides aggregated information for many use cases including data certification.
        OMS is the successor of WBM, the Web Based Monitoring which was in use during Run 1 and Run 2 of the LHC.
        WBM started as a small tool and grew substantially over the years so that maintenance became challenging. OMS was developed from scratch following several design ideas: to strictly separate the presentation layer from the data aggregation layer; to use a well-defined standard for the communication between presentation layer and aggregation layer; and to employ widely used frameworks from outside the HEP community.

        A report on our experience of the operation of OMS for the first year of data taking of Run 3 in 2022 is presented.

        Speaker: Mr Petrucci, Andrea (University of California, San Diego, San Diego, California, USA)
      • 11:45 AM
        Computer Vision for Data Quality Monitoring with Hydra 15m

        Hydra is a system which utilizes computer vision to monitor data quality in near real time. Currently, it is deployed in all of Jefferson Lab’s experimental halls and lightens the load on shift takers by autonomously monitoring diagnostic plots in near real time. Hydra is constructed from “off-the-shelf” technologies and is backed up by a full MySQL database. To aid with both labeling and monitoring of Hydra’s inference, web apps have been developed, lowering the barrier to entry. Hydra connects with the EPICS alarm system and includes full history recording. This has enabled it to spot issues that were missed by shift takers. When issues are spotted a natural first question is “Why does Hydra think there is a problem?”. To answer this question Hydra uses gradCAM to highlight regions of an image which are most important in inference classification. This provides a level of interpretability/trustworthiness; essential for any operational system in science. This talk will describe the Hydra system, the technologies employed as well as in situ results. The sociological hurdles in deploying such a system will also be discussed.

        Speaker: Jeske, Torri (JLAB)
      • 12:00 PM
        The ALICE Data Quality Control 15m

        ALICE (A Large Ion Collider Experiment) has undertaken a major upgrade during the Long Shutdown 2. The increase in the detector data rates, and in particular the continuous readout of the TPC, led to a hundredfold increase in the input raw data, up to 3.5 TB/s. To cope with it, a new common Online and Offline computing system, called O2, has been developed and put in production.

        The online Data Quality Monitoring (DQM) and the offline Quality Assurance (QA) are critical aspects of the data acquisition and reconstruction software chains. The former intends to provide shifters with precise and complete information to quickly identify and overcome problems while the latter aims at selecting good quality data for physics analyses. Both DQM and QA typically involve the gathering of data, its distributed analysis by user-defined algorithms, the merging of the resulting objects and their visualization.

        This paper discusses the final architecture and design of the QC, which runs synchronously to the data taking and asynchronously on the Worldwide LHC Computing Grid. Following the successful first year of data taking with beam, we will present our experience and the lessons we learned, before and after the LHC restart, when monitoring the data quality in a real-world and challenging environment. We will finally illustrate the wide range of usages people make of this system by presenting a few, carefully picked, use cases.

        Speaker: Konopka, Piotr (CERN)
      • 12:15 PM
        AI Driven Experiment Calibration and Control 15m

        One critical step on the path from data taking to physics analysis is calibration. For many experiments this step is both time consuming and computationally expensive. The AI Experimental Calibration and Control project seeks to address these issues, starting first with the GlueX Central Drift Chamber (CDC). We demonstrate the ability of a Gaussian Process to estimate the gain correction factor (GCF) of the GlueX CDC accurately, and also the uncertainty of this estimate. Using the estimated GCF, the developed system infers a new high voltage (HV) setting that stabilizes the GCF in the face of changing environmental conditions. This happens in near real time during data taking and produces data which are already approximately gain-calibrated, eliminating the cost of performing those calibrations which vary by up to 30% with fixed HV. We also demonstrate an implementation of an uncertainty aware system which exploits a key feature of a Gaussian process.

        Speaker: Britton, Thomas (JLab)
    • 11:00 AM 12:30 PM
      Track 3 - Offline Computing: Physics performance (part 2) Hampton Roads Ballroom VI

      Hampton Roads Ballroom VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Dr Srpimanobhas, Norraphat (Chulalongkorn University) , Yang, Tingjun (Fermilab)
      • 11:00 AM
        Algorithms: Framework- and Experiment-independent algorithms at EPIC 15m

        The EPIC collaboration at the Electron-Ion Collider recently laid the groundwork for its software infrastructure. Large parts of the software ecosystem for EPIC mirror the setup from the Key4hep project, for example DD4hep for geometry description, and EDM4hep/PODIO for the data model. However, other parts of the EPIC software ecosystem diverge from Key4hep, for example for the event processing framework (JANA2 for EPIC versus Gaudi for Key4hep). The algorithms initiative by the EPIC collaboration tries to foster cross-community collaboration and algorithm-sharing by providing a framework- and experiment-independent approach to digitization and reconstruction algorithms. In this talk we will focus on the design choices behind Algorithms and showcase real-world integration of algorithms with both JANA2 and Gaudi.

        Speaker: Joosten, Sylvester (Argonne National Laboratory)
      • 11:15 AM
        Performance of track reconstruction at STCF using ACTS 15m

        The reconstruction of charged particles’ trajectories is one of the most complex and CPU-consuming event processing chains in high energy physics (HEP) experiments. Meanwhile, the precision of track reconstruction has direct and significant impact on vertex reconstruction, physics flavour tagging and particle identfication, and eventually on physics precision, in particular for HEP experiments at the precison frontier, such as the Super τ-Charm facility (STCF).

        With an electron-positron collider operating at center-of-mass-energy 2∼7 GeV and a peak luminosity above 0.5 × 10^35 cm^−2 s^−1, the STCF physics program will provide an unique platform for in-depth studies of hadron structure and non-perturbative strong interaction, as well as probing physics beyond the Standard Model at the τ-Charm sector suceeding the present Being Electron-Positron Collider II (BEPCII). To fulfill the physics targets and to further maximize the physics potential at the STCF, the charged particles with momentum down to 50 MeV must be detected and reconstructed, and an excellent momentum and angular resolution of the charged particles must be achieved. Therefore, development of a highly-performant and maintenable tracking software is very curcial for the design, construction and operation of STCF.

        Based on the tracking experience at LHC, the project, A Common Tracking Software (ACTS), aims to provide an open-source experiment-independent and framework-independent software designed for modern computing architectures. It provides a set of high-level performant track reconstruction tools which are agnostic to the details of the detection technologies and magnetic field configuration, and tested for strict thread-safety to support multi-threaded event processing. ACTS has been used as a tracking toolkit at experiments such as ATLAS, sPHENIX, ALICE etc. and has shown very promising tracking performance in terms of both physics performance and time performance. However, its applications so far are mainly focusing on silicon-based tracking systems and are often less concerned with charged tracks with momentum below a few hundreds of MeV.

        In this talk, I will report on development of the STCF track reconstrcon software based on the detection information from a Silicon (or uRWELL)-based Inner Tracker and a Main Drift Chamber using the Kalman Filter based track finding and fitting algorithms of ACTS. This is the first application of ACTS for a drift chamber and shows very promising performance. Therefore, the efforts on tuning its performance, in particular for charged tracks with low momentum down to 50 MeV, will be highlighted.

        Speaker: Li, Teng (Shandong University)
      • 11:30 AM
        Flexible, robust and minimal-overhead Event Data Model for track reconstruction in ACTS 15m

        ACTS is an experiment independent toolkit for track reconstruction, which is designed from the ground up for thread-safety and high performance. It is built to accommodate different experiment deployment scenarios, and also serves as community platform for research and development of new approaches and algorithms.

        The Event Data Model (EDM) is a critical piece of the tracking library that is visible to clients. Until this point, ACTS was mostly focused on an internal EDM, targeting data interchange betweens various components in the toolkit.
        This contribution reports on a new and improved client EDM for ACTS. For an experiment-agnostic toolkit like ACTS, this requires strong abstractions of potentially experiment-specific details, including event context data like sensor alignments, and tracking inputs like measurements. By applying similar abstraction strategies, the presented EDM can be an expressive, low-overhead abstraction over experiment-specific backends, and seamlessly integrates into an experiment framework and IO model.

        The presented EDM includes the ACTS track class, the main data type which tracking clients interact with. It is designed to be interfaced with different IO backends, and also flexible enough to support dynamic information required by various track fitters. At the same time, careful design ensures it can seamlessly serve as a key data object in experiment reconstruction data flows.

        In this contribution, the interaction of this centerpiece of the example workflows in ACTS with the standalone ROOT IO, as well as the integration with the EDM4hep package will be shown, and key performance characteristics discussed.

        Speaker: Dr Gessinger, Paul (CERN)
      • 11:45 AM
        Multithreading ATLAS offline software: a retrospective 15m

        For Run 3, ATLAS redesigned its offline software, Athena, so that the
        main workflows run completely multithreaded. The resulting substantial
        reduction in the overall memory requirements allows for better use
        of machines with many cores. This talk will discuss the performance
        achieved by the multithreaded reconstruction as well as the process
        of migrating the large ATLAS code base and tools and techniques
        that were useful in debugging threading-related problems.

        Speaker: Snyder, Scott (Brookhaven National Laboratory)
      • 12:00 PM
        Machine Learning Tools for the CMS Tracker Data Quality Monitoring and Certification 15m

        During the long shutdown between LHC Run 2 and 3, a reprocessing of 2017 and 2018 CMS data with higher granularity data quality monitoring (DQM) harvesting was done. The time granularity of DQM histograms in this dataset is increased by 3 orders of magnitude. In anticipation of deploying this higher granularity DQM harvesting in the ongoing Run 3 data taking, this dataset is used to study the application of Machine Learning (ML) techniques to data certification with the goal of developing tools for online monitoring and offline certification. In this talk, we will discuss the challenges and present some of the results, illustrating the tools developed for CMS Tracker Data Quality Monitoring and Certification. Studies consider both the use case of anomaly detection in the context of reprocessing campaigns, when all the data is available, and in the context of continuous data taking, when conditions are constantly changing and models need to be trained on data previously collected with similar conditions. Data augmentation is pursued, including information from the CMS Online Monitoring System (luminosity, pile-up, LHC fill, run and trigger), from the CMS Run Registry (sub-detector certification flags), from the CMS conditions database (calibrations). The status of the web application integrating data sources and facilitating development, testing and benchmarking of ML models will be presented using a few test cases.

        Speaker: Benelli, Gabriele (Brown University)
    • 11:00 AM 12:30 PM
      Track 4 - Distributed Computing: Infrastructure and Services Marriott Ballroom II-III

      Marriott Ballroom II-III

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Barreiro Megino, Fernando (Unive) , Ellis, Katy (STFC-RAL)
      • 11:00 AM
        Tools and Services for Collaborations: On-Boarding to the OSG Fabric of Services 15m

        We present a collection of tools and processes that facilitate onboarding a new science collaboration onto the OSG Fabric of Services. Such collaborations typically rely on computational workflows for simulations and analysis that are ideal for executing on OSG's distributed High Throughput Computing environment (dHTC). The produced output can be accumulated and aggregated at available ephemeral storage for inspection and then distribution to other facilities for long-term storage and further analysis. This work focuses on matching workflow requirements to tools and services that provide job management, automation (Pegasus WMS), and delivery of collaboration-specific software and input data to Execution Points (EP) using the Open Science Data Federation (OSDF) or Rucio. We describe best-supported practices to transfer data products to remote facilities at runtime or after the job completion. We emphasize the importance of early planning that meets the goals of the typically long life cycle of HEP experiments and advocate for an engagement model where the collaboration eventually becomes self-reliant in workload and data management.

        Speaker: Paschos, Pascal (University of Chicago)
      • 11:15 AM
        Managing the OSG Fabric of Services the GitOps Way 15m

        There is no lack of approaches for managing the deployment of distributed services – in the last 15 years of running distributed infrastructure, the OSG Consortium has seen many of them. One persistent problem has been each physical site has its style of configuration management and service operations, leading to a partitioning of the staff knowledge and inflexibility in migrating services between sites.

        Recently, the team has been migrating the OSG Fabric of Services to be deployed via Kubernetes which provides a common service orchestration fabric across all sites. However, this leaves open a question - how does the team interact with Kubernetes? To coordinate this new style of deployment among geographically distributed clusters and team members, the team has adopted "GitOps", an operational model that uses Git version control repositories to drive service updates. Git-driven operations provides all the benefits of version control such as recording the who, what, when, and why of any given change. But, more powerfully, automated agents synchronize the current state of the Git repository with the current state of the Kubernetes clusters, streamlining the ability to redeploy services from scratch or transfer services between clusters. In this paper, we will describe the setup that enables GitOps deployments of central OSG services and the lessons learned along the way, including rebuilding a suite of services after a critical failure and our experiences with providing high-availability services across multiple Kubernetes clusters.

        Speaker: Bockelman, Brian (Morgridge Institute for Research)
      • 11:30 AM
        CernVM-FS at Extreme Scales 15m

        The CernVM File System (CVMFS) provides the software distribution backbone for High Energy and Nuclear Physics experiments and many other scientific communities in the form of a globally available shared software area. It has been designed for the software distribution problem of experiment software for LHC Runs 1 and 2. For LHC Run 3 and even more so for HL-LHC (Runs 4-6), the complexity of the experiment software stacks and their build pipelines is substantially larger. For instance, software is being distributed for several CPU architectures, often in the form of containers which includes base and operating system libraries, the number of external packages such as machine learning libraries has multiplied, and there is a shift from C++ to more Python-heavy software stacks that results in more and smaller files needing to be distributed. For CVMFS, the new software landscape means an order of magnitude increase of scale in key metrics such as number of files, number of system calls, and number of concurrent processes accessing the file system client. In this contribution, we report on the performance and reliability engineering on the file system client to sustain current and expected future software access load. Concretely, we show the impact of the newly designed file system cache management, including upstreamed improvements to the fuse kernel module itself, improved utilization of network links and caches (such as line optimization, prefetching, and proxy sharding), and operational improvements on network failure handling, error reporting, and integration with container runtimes. Overall, the new CVMFS client is designed to sustain applications with more than one million file lookups during startup, nodes with hundreds of cores, and thousands of concurrent processes accessing software from the file system client.

        Speaker: Promberger, Laura (CERN)
      • 11:45 AM
        AUDITOR: Accounting for opportunistic resources 15m

        The increasing computational demand in High Energy Physics (HEP) as well as increasing concerns about energy efficiency in high performance/throughput computing are driving forces in the search for more efficient ways to utilize available resources. Since avoiding idle resources is key in achieving high efficiency, an appropriate measure is sharing of idle resources of under-utilized sites with fully occupied sites. The software COBalD/TARDIS can automatically, transparently and dynamically (dis)integrate such resources in an opportunistic manner.
        Sharing resources however also requires accounting. In this work we introduce AUDITOR (AccoUnting DatahandlIng Toolbox for Opportunistic Resources), a flexible and extensible accounting system that is able to cover a wide range of use cases and infrastructure. AUDITOR gathers accounting data via so-called collectors which are designed to monitor batch systems, COBalD/TARDIS, cloud schedulers or other sources of information. The data is stored in a database and provided to so-called plugins, which take an action based on accounting records. An action could for instance be creating a bill or computing the CO2 footprint, adjusting parameters of a service (for instance priorities in a batch system) or forwarding accounting information to other accounting systems. Depending on the use case, a suitable collector and plugin are selected from a growing ecosystem of collectors and plugins. Libraries for interacting with AUDITOR are provided to facilitate the development of collectors and plugins by the community.
        This contribution gives insights into the design of AUDITOR and how it integrates into a number of different use cases.

        Speaker: Dr Boehler, Michael (Freiburg University)
      • 12:00 PM
        JIRIAF: JLAB Integrated Research Infrastructure Across Facilities 15m

        The JIRIAF project aims to combine geographically diverse computing facilities into an integrated science infrastructure. This project starts by dynamically evaluating temporarily unallocated or idled compute resources from multiple providers. These resources are integrated to handle additional workloads without affecting local running jobs. This paper describes our approach to launch best-effort batch tasks which exploit these underutilized resources. Our system measures the real-time behavior of jobs running on a machine and learns to distinguish typical performance from outliers. Unsupervised ML techniques are used to analyze hardware-level performance measures, followed by a real-time cross-correlation analysis to determine which applications cause performance degradation. We then ameliorate bad behavior by throttling these processes. We demonstrate that problematic performance interference can be detected and acted on, which makes it possible to continue to share resources between applications and simultaneously maintain high utilization levels in a computing cluster. For a case study, we relocate the CLAS12 data processing workflow to a remote data center, preventing file migration and temporal data persistency.

        Speaker: Gyurjyan, Vardan (Jefferson Lab)
      • 12:15 PM
        The Platform-as-a-Service paradigm meets ATLAS: developing an automated analysis workflow on the newly established INFN Cloud 15m

        The Worldwide LHC Computing Grid (WLCG) is a large-scale collaboration which gathers the computing resources of around 170 computing centres from more than 40 countries. The grid paradigm, unique to the realm of high energy physics, has successfully supported a broad variety of scientific achievements. To fulfil the requirements of new applications and to improve the long-term sustainability of the grid middleware, more versatile solutions are being investigated. Cloud computing is becoming increasingly popular among open-source and commercial players. The HEP community has also recognized the benefits of integrating cloud technologies into the legacy grid-based workflows. Since March 2021, INFN has entered the field of cloud computing establishing the INFN Cloud infrastructure. Large data centers of the INFN National Computing Center, connected to a nation-wide backbone maintained by the GARR Consortium, are gathered into a redundant and federated infrastructure. This cloud service supports scientific computing, software development and training, and serves as an extension of local computing and storage resources. Among available services, INFN Cloud administrators can create virtual machines, Docker-based deployments or Kubernetes clusters. These options allow the creation of customized environments, both for individual users and for scientific collaborations. This study investigates the feasibility of an automated, cloud-based data analysis workflow for the ATLAS experiment using INFN Cloud resources. The concept is designed as a Platform-as-a-Service (PaaS) solution, based on a Centos 7 Docker image. The customized image is responsible for the provisioning of CERN’s CVMFS and EOS shared filesystems, from which a standardized ATLAS environment can be loaded. The end user’s only responsibility is to provide a working application capable of retrieving and analysing data, and to export the results to a persistent storage. The analysis code can be sourced either from remote git repositories or from a local Docker bind mount. As a final step in the automation workflow, a Kubernetes cluster will be configured within the INFN Cloud infrastructure to allow dynamic resource allocation and the interoperability with batch systems, such as HTCondor, will be investigated.

        Speaker: Marcon, Caterina (INFN Milan (IT))
    • 11:00 AM 12:30 PM
      Track 5 - Sustainable and Collaborative Software Engineering: Sustainable CI and Build Infrastructure Chesapeake Meeting Room

      Chesapeake Meeting Room

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Rodrigues, Eduardo (University of Liverpool) , Sailer, Andre (CERN)
      • 11:00 AM
        Large scale dynamic web deployment for CERN, experience and outlook 15m

        CERN hosts more than 1200 websites essential for the mission of the Organization, internal and external collaboration and communicaiton as well as public outreach. The complexity and scale of CERN’s online presence is very diverse with some websites, like https://home.cern/

        , accommodating more than one million unique visitors in a day.

        However, regardless of their diversity, all websites are created using the Drupal content management system (CMS), and are self-hosted directly in the CERN Datacenter on a dedicated infrastructure that runs on Kubernetes

        . Workflows like provisioning, deleting, cloning, upgrading, and similar are fully automated and managed by a customised Kubernetes controller. By leveraging the custom controller, the infrastrucutre has proven highly reliant with minimal, manual intervention necessary. In order to further automate deployments and improve goverance, we run a customised version of Drupal called the CERN Drupal Distribution. Supported by end-to-end integration tests and automated browser simulation, our setup enables us to propagate security and feature updates seamlessly to all websites without any downtime.

        In this paper, we outline the architecture allowing us to build, test, and distribute updates to a large number of websites without any downtime. We further share our experiences and learnings from managing such a service at CERN with a lean team.

        Speaker: Rajula, Vineet Reddy
      • 11:15 AM
        Modern Software Development for JUNO offline software 15m

        The Jiangmen Underground Neutrino Observatory (JUNO), under construction in South China, primarily aims to determine the neutrino mass hierarchy and the precise measure oscillation parameters. The data-taking is expected to start in 2024 and plans to run for more than 20 years. The development of JUNO offline software (JUNOSW) started in 2012, and it is quite challenging to maintain the JUNOSW for such a long time. In the last ten years, tools such as Subversion, Trac, and CMT had been adopted for software development. However, there are some new requirements, such as how to reduce the building time for the whole project, how to deploy offline algorithms to an online environment, and how to improve the code quality with code review and continuous integration. To meet the further requirements of software development, modern development tools are evaluated for JUNOSW, such as Git, GitLab, CMake, Docker, and Kubernetes. This contribution will present the software development system based on these modern tools for JUNOSW and the functionalities we have achieved: CMake macros are developed to simplify the build instructions for users; CMake generator expressions are used to control the build flags for the online and offline environments; a tool named git-junoenv is developed to help users partially checkout and build the software; a script is used to build and deploy the software on the CVMFS server; a Docker image with CVMFS client installed is created for continuous integration; a GitLab agent is set up to manage GitLab runners in Kubernetes with all the configurations in a GitLab repository. In late 2022, the migration had been done.

        Speaker: Dr Lin, Tao (IHEP)
      • 11:30 AM
        Operational Intelligence in the ATLAS Continuous Integration System 15m

        The ATLAS Continuous Integration (CI) System is the major component of the ATLAS software development infrastructure, synchronizing efforts of several hundred software developers working around the world and around the clock. Powered by 700 fast processors, it is based on the ATLAS GitLab code management service and Jenkins CI server and performs daily up to 100 ATLAS software builds probing the code changes proposed in merge requests. The system uses Operational Intelligence methods to shorten development cycles and lower operating costs. The paper describes these methods, such as removal of redundant operations, compilation and testing parallelization, usage of the directed acyclic graph (DAG) approach in CI pipelines as well as reports achieved improvements.

        Speaker: Undrus, Alexander (BNL)
      • 11:45 AM
        Managing software build infrastructure at ALICE using Hashicorp Nomad 15m

        The ALICE experiment at CERN uses a cluster consisting of virtual and bare-metal machines to build and test proposed changes to the ALICE Online-Offline (O2) software in addition to building and publishing regular software releases.

        Nomad is a free and open-source job scheduler for containerised and non-containerised applications developed by Hashicorp. It is integrated into an ecosystem of related software, including Consul and Vault, providing a consistent interface to orchestration, monitoring and secret storage. At ALICE, it recently replaced Apache Mesos, Aurora and Marathon as the primary tool for managing our computing resources.

        First, we will describe the architecture of the build cluster at the ALICE experiment. After giving an overview of the advantages that Nomad gives us in managing our computing workload, and our reasons for switching away from the Mesos software stack, we will present concrete examples of improvements in monitoring and automatic configuration of web services that we are already benefiting from. Finally, we will discuss where we see opportunities for future work in integrating the ALICE build infrastructure more deeply with Nomad, in order to take advantage of its larger feature set compared to Mesos.

        Speaker: Wilken, Timo (CERN)
      • 12:00 PM
        Version control and DevOps platform for accelerator and experiments: experience and outlook 15m

        GitLab has been running at CERN since 2012. It is a self-service code hosting application based on Git that provides collaboration and code review features, becoming one of the key infrastructures at CERN. It is being widely used at CERN, with more than 17 000 active users, hosting more than 120 000 projects and triggering more than 5 000 jobs per hour.

        On its initial stage, a custom-made solution has been deployed that, aligned with the exponential increase of projects, workflows and continuous integrations, made the GitLab infrastructure hard and complex to scale and to maintain.

        The recent migration performed, adopting a new supported Cloud Hybrid infrastructure, has contributed CERN to line up the GitLab infrastructure with both industry standards and best practices, to make the new infrastructure much more robust and performant, obtaining notable benefits in the whole deployment process.

        This paper will address how this deployment process, on the road to success, has presented a series of challenges and pitfalls that have been faced during this complex migration process.

        Speaker: Posada Trobo, Ismael (CERN)
    • 11:00 AM 12:30 PM
      Track 6 - Physics Analysis Tools: Machine Learning in Analysis Hampton Roads Ballroom VIII

      Hampton Roads Ballroom VIII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Heddle, Dave (CNU) , Held, Alexander (University of Wisconsin–Madison)
      • 11:00 AM
        Binning high-dimensional classifier output for HEP analyses through a clustering algorithm 15m

        The usage of Deep Neural Networks (DNNs) as multi-classifiers is widespread in modern HEP analyses. In standard categorisation methods, the high-dimensional output of the DNN is often reduced to a one-dimensional distribution by exclusively passing the information about the highest class score to the statistical inference method. Correlations to other classes are hereby omitted.
        Moreover, in common statistical inference tools, the classification values need to be binned, which relies on the researcher's expertise and is often non-trivial. To overcome the challenge of binning multiple dimensions and preserving the correlations of the event-related classification information, we perform K-means clustering on the high-dimensional DNN output to create bins without marginalising any axes.
        We evaluate our method in the context of a simulated cross section measurement at the CMS experiment, showing an increased expected sensitivity over the standard binning approach.

        Speaker: Eich, Niclas (RWTH Aachen University)
      • 11:15 AM
        Deep generative models for generating Drell-Yan events in the ATLAS collaboration at the LHC 15m

        The search for the dimuon decay of the Standard Model (SM) Higgs boson looks for a tiny peak on top of a smoothly falling SM background in the dimuon invariant mass spectrum 𝑚(𝜇𝜇). Due to the very small signal-to-background ratio, which is at the level of 0.2% in the region 𝑚(𝜇𝜇) = 120–130 GeV for an inclusive selection, an accurate determination of the background is of paramount importance. The 𝑚(𝜇𝜇) background spectrum is parameterised by analytic functions that can describe this distribution at the per-mill level to avoid a significant bias in the extracted signal yields. The criteria used to select the background functions are based on the spurious signal, which measures the residual signal events obtained from signal-plus-background fits to background-only MC templates. Therefore, these MC templates have to be derived from events with very high statistics in order to reduce possible fluctuations. Computationally, it is extremely expensive, if not impossible, to generate the Drell-Yan 𝑍/𝛾∗ → 𝜇𝜇 background events with detailed simulation. Our study focuses on the use of generative models, trained on the existing fully simulated events of the ATLAS experiment in order to generate billions of events using GPUs for the spurious signal study, and to test the statistical independence of these events. This study presents an interesting alternative procedure in for the generation of events with high statistical power that could be used in the future by default in many analyses at the LHC.

        Speaker: Ju, Xiangyang (Lawrence Berkeley National Laboratory)
      • 11:30 AM
        Unbiased detection of data departures from expectations with machine learning 15m

        We present New Physics Learning Machine (NPLM), a machine learning-based strategy to detect data departures from a Reference model, with no prior bias on the source of discrepancy. The main idea behind the method is to approximate the optimal log-likelihood-ratio hypothesis test parametrising the data distribution with a universal approximating function, and solving its maximum-likelihood fit as a machine learning problem with a customised loss function [1]. The method returns a $p$-value that measures the compatibility of the data with the Reference model. The most interesting potential applications are model-independent New Physics searches, validation of new Monte Carlo event generators and data quality monitoring. Using efficient large-scale implementations of kernel methods as universal approximators [2], the NPLM algorithm can be deployed on a GPU-based data acquisition system and be exploited to explore online the readout of an experimental setup. This would allow to spot out detectors malfunctioning or, possibly, unexpected anomalous patters in the data. One crucial advantage of the NPLM algorithm over standard goodness-of-fit tests routinely used in many experiments is its capability of inspecting multiple variables at once, taking care of correlations in the process. It also identifies the most discrepant region of the phase-space and it reconstructs the multidimensional data distribution, allowing for further inspection and interpretation of the results.
        Finally, a way for dealing with systematic uncertainties affecting the knowledge of the Reference model has been developed in a neural network framework [3] and is under construction for kernel methods.

        Speaker: Grosso, Gaia (Universita e INFN, Padova (IT))
      • 11:45 AM
        Data driven background estimation in HEP using Generative Adversarial Networks 15m

        Data-driven methods are widely used to overcome shortcomings of Monte Carlo (MC) simulations (lack of statistics, mismodeling of processes, etc.) in experimental High Energy Physics. A precise description of background processes is crucial to reach the optimal sensitivity for a measurement. However, the selection of the control region used to describe the background process in a region of interest biases the distribution of some physics observables, rendering the use of such observables impossible in a physics analysis. Rather than discarding these events and/or observables, we propose a novel method to generate physics objects compatible with the region of interest and properly describing the correlations with the rest of the event properties. We use generative adversarial networks (GAN) for this task, as GAN are among the best performing generator models for various machine learning applications. The method is illustrated by generating a new misidentified photon for the $\mathrm{\gamma+Jets}$ background of the $\mathrm{H\rightarrow\gamma\gamma}$ analysis at the CERN LHC, thanks to CMS Open Data simulated samples. We demonstrate that the GAN is able to generate a coherent object within the region of interest and still correlated with the different properties of the rest of the event.

        Speaker: Lohezic, Victor (Irfu, CEA Saclay - Université Paris-Saclay)
      • 12:00 PM
        An Active Learning application in a dark matter search with ATLAS PanDA and iDDS 15m

        Many theories of Beyond Standard Model (BSM) physics feature multiple BSM particles. Generally, these theories live in higher dimensional phase spaces that are spanned by multiple independent BSM parameters such as BSM particle masses, widths, and coupling constants. Fully probing these phase spaces to extract comprehensive exclusion regions in the high dimensional space is challenging. Constraints on person-power and computational resources can limit analyses to focus only on one- or two-dimensional regions of the relevant parameter spaces. Nonetheless, fully comprehensive exclusion regions, even for complex theory phase spaces, are generally desirable to maximize the utility of such BSM searches.
        We are presenting an advanced analysis workflow composed of an integrated pipeline and active learning that enables such a comprehensive exclusion. The integrated pipeline automatically executes all steps of an analysis from event generation through to limit setting. Active learning is a technique to guide the sampling of the multi-dimensional phase space to find the exclusion contours in an iterative process: the sampled theory phase space points are selected such that the vicinity of the exclusion region is prioritized, reducing the sampling density in the less interesting areas. As a result, it allows searches over a larger space at the same precision, or reduces the resources required for the same search-space. We will present the implementation of the workflow with the Production and Distributed Analysis system (PanDA system) and intelligent Data Delivery Service (iDDS) in ATLAS, and showcase its abilities and utility in an extended search for a dark Z-boson using events with four-lepton final states.

        Speaker: Weber, Christian (Brookhaven National Laboratory)
      • 12:15 PM
        Deep Learning for Matrix Element Method 15m

        The matrix element method (MEM) is a powerful technique that can be used for the analysis of particle collider data utilizing an ab initio calculation of the approximate probability density function for a collision event to be due to a physics process of interest. The most serious difficulty with the ME method, which has limited its applicability to searches for beyond-the-SM physics and precision measurements at colliders, is that it is computationally expensive. Complex final states can take minutes per event or more to calculate the probability densities. ML methods can be used to speed up the numerical evaluation dramatically. In this work, we explore Deep Learning based solutions to approximate MEM calculations and compare their performance with respect to existing computational benchmarks.

        Speaker: Neubauer, Mark (University of Illinois)
    • 11:00 AM 12:30 PM
      Track 7 - Facilities and Virtualization: Computing Centre Infrastructure Marriott Ballroom IV

      Marriott Ballroom IV

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Weitzel, Derek (University of Nebraska-Lincoln) , Wiebalck, Arne (CERN)
      • 11:00 AM
        Finalizing Transition to the New Data Center at BNL 15m

        Computational science, data management and analysis have been key factors in the success of Brookhaven National Laboratory's scientific programs at the Relativistic Heavy Ion Collider (RHIC), the National Synchrotron Light Source (NSLS-II), the Center for Functional Nanomaterials (CFN), and in biological, atmospheric, and energy systems science, Lattice Quantum Chromodynamics (LQCD) and Materials Science, as well as our participation in international research collaborations, such as the ATLAS Experiment at Europe's Large Hadron Collider (LHC) at CERN (Switzerland) and the Belle II Experiment at KEK (Japan). The construction of a new data center is an acknowledgement of the increasing demand for computing and storage services at BNL in the near term and enable the Lab to address the needs of the future experiments at the High-Luminosity LHC at CERN and the Electron-Ion Collider (EIC) at BNL in the long term. The Computing Facility Revitalization (CFR) project is aimed at repurposing the former National Synchrotron Light Source (NSLS-I) building as the new data center for BNL. The construction of the new data center was finished in 2021Q3, and it was delivered for production in early FY2022 for all collaborations supported by the Scientific Data and Computing Center (SDCC), including: STAR, PHENIX and sPHENIX experiments at RHIC collider at BNL, the Belle II Experiment at KEK (Japan), and the Computational Science Initiative at BNL (CSI). The extension of the central network systems into the new data center and the migration of a significant portion of IT load and services from the existing data center to the new data center has been underway for the duration of the first year of operations. The deployment of four new IBM TS4500 tape libraries was carried out in FY2022 as well for BNL ATLAS Tier-1 Site and sPHENIX experiment at RHIC for which the first period of data taking is expected to be carried out later in FY2023. This presentation will highlight the key mechanical, electrical, and networking components of the new data center in its final configuration as used in production since 2021Q4. Also, we will overview the IT payload deployment operations performed so far in the new data and describe plans to complete the gradual IT equipment replacement and migration from the old data center into the new one to be completed by the end of FY2023 (Sep 30, 2023). We will also show the expected state of occupancy and infrastructure utilization for the new data center up to FY2027 and further upgrade steps for its infrastructure needed in that period.

        Speaker: Mr Zaytsev, Alexandr (Brookhaven National Laboratory (BNL))
      • 11:15 AM
        Measuring Carbon: Net-Zero and the IRISCAST Project 15m

        Moving towards Net-Zero requires robust information to enable good decision making at all levels: covering hardware procurement, workload management and operations, as well as higher level aspects encompassing grant funding processes and policy framework development.

        The IRISCAST project is a proof-of-concept study funded as part of the UKRI Net-Zero Scoping Project. We have performed an audit of carbon costs across a multi-site heterogenous infrastructure by collecting and analysing snapshots of actual usage across different facilities within the IRIS community (https://iris.ac.uk). This combines usage information with an analysis of the embodied costs and careful mapping and consideration of the underlying assumptions to produce an estimate of the overall carbon cost, the key elements that contribute to it, and the important metrics needed to measure it. We present our key findings, lessons learned, and recommendations.

        Speaker: Owen, Alex (Queen Mary University of London)
      • 11:30 AM
        The IT infrastructure of the LUX-ZEPLIN experiment at SURF 15m

        LUX-ZEPLIN (LZ) is a direct detection dark matter experiment currently operating at the Sanford Underground Research Facility (SURF) in Lead, South Dakota. The core component is a liquid xenon time projection chamber with an active mass of 7 tonnes.
        To meet the performance, availability, and security requirements for the LZ DAQ, Online, Slow Control and data transfer systems located at SURF, we have developed and implemented a standalone IT infrastructure. It consists of a fully redundant 10 Gigabit network spanning underground and surface locations with hybrid virtual/physical data centers in both places. We employ virtualization, redundant firewalls, central authentication and user management, a web portal, 2-factor authentication for all remote access, VPN, fine-grained authorization and role management via a central directory, SAML identity and service providers, central configuration management, logging, monitoring, multiple relational databases, and frequent on-site and offsite backups. We exclusively use Open Source tools to provide these services.
        Data is sent from SURF to the National Energy Sciences Computer Center (NERSC) in Berkeley, California which provides CPU and storage for reconstruction and analysis.
        The system has been running reliably since its installation at SURF in 2019. We currently manage about 100 physical and virtual servers and almost 300 user accounts with 10-20 users online at any time.
        This presentation will give an overview of the system and report on the operational experience.

        Speaker: Dr Luitz, Steffen (SLAC National Accelerator Laboratory)
      • 11:45 AM
        Estimating the environmental impact of a large Tier 2 15m

        Recent years have seen an increasing interest in the environmental impact, especially the carbon footprint, generated by the often large scale computing facilities used by the communities represented at CHEP. As this is a fairly new requirement, this information is not always readily available, especially at universities and similar institutions which do not necessarily see large scale computing provision as their core competency. Here we present the results of a survey of a large WLCG Tier 2 with respect to power usage and carbon footprint leveraging all sources of information available to us: Power usage data collected from built-in host level monitoring and external aggregates from the power distribution units at rack level; data sheets provided by the hardware manufacturers and the specifics of data centre that hosts our infrastructure.
        We show that it is possible to estimate the environmental impact without having to invest in dedicated monitoring equipment, but also discuss the limitations of this approach.

        Speaker: Whitehouse, Dan (Imperial College)
      • 12:00 PM
        Migrating the INFN-CNAF datacenter to the Bologna Tecnopolo - a status update 15m

        The INFN Tier1 data center is currently located in the premises of the Physics Department of the University of Bologna, where CNAF is also located. During 2023 it will be moved to the “Tecnopolo”, the new facility for research, innovation, and technological development in the same city area; the same location is also hosting Leonardo, the pre-exascale supercomputing machine managed by CINECA, co-financed as part of the EuroHPC Joint Undertaking, 4th ranked in the top500 November 2022 list.
        The construction of the new CNAF data center consists of two phases, corresponding to the computing requirements of LHC: Phase 1 involves an IT power of 3 MW, and Phase 2, starting from 2025, involves an IT power up to 10 MW.
        The new datacenter is designed to cope with the computing requirements of the data taking of the HL-LHC experiments, in the time spanning from 2026 to 2040 and will provide, at the same time, computing services for several other INFN experiments and projects, not only belonging to the HEP domain. The co-location with Leonardo opens wider possibilities to integrate HTC and HPC resources and the new CNAF datacenter will be tightly coupled with it, allowing access from a single entrypoint to resources located at CNAF and provided by the supercomputer. Data access from both infrastructures will be transparent to users.
        In this presentation we describe the new data center design, providing a status update on the migration, and we focus on the Leonardo integration showing the results of the preliminary tests to access it from the CNAF access points.

        Speaker: Dr Pellegrino, Carmelo (INFN-CNAF)
      • 12:15 PM
        Data Centre Refurbishment with the aim of Energy Saving and Achieving Carbon Net Zero 15m

        Queen Mary University of London (QMUL) as part of the refurbishment of one of its's data centres has installed water to water heat pumps to use the heat produced by the computing servers to provide heat for the university via a district heating system. This will enable us to reduce the use of high carbon intensity natural gas heating boilers, replacing them with electricity which has a lower carbon intensity due to the contribution from wind, solar, hydroelectric, nuclear, biomass sources of power sources.

        The QMUL GridPP cluster today provides 15PB of storage and over 20K jobs slots mainly devoted to the ATLAS experiment. The data centre that houses the QMUL GridPP cluster, was originally commissioned in 2004. By 2020 it was in significant need of refurbishment. The original design had a maximum power capacity of 200KW, no hot/cold aisle containment, down flow air conditioning units using refrigerant cooling and no raised floor or ceiling plenum.

        The main requirements of the refurbishment are: To significantly improve the energy efficiency and reduce the carbon usage of the University; Improve the availability and reliability of the power and cooling; Increase the capacity of the facility to provide for future expansion; Provide a long term home for the GridPP cluster to support the computing needs of the LHC and other new large science experiments (SKA/LSST) into the next decade.

        After taking into account the future requirements and likely funding allocation, floor space in the datacentre and the space available to house the cooling equipment the following design was chosen: A total power capacity of 390KW with redundant feeds to each rack; 39 racks with an average of 10KW of power per rack (flexable up to 20KW); An enclosed hot aisle design with in row cooling units using water cooling; water to water heat pumps connected to the universities district heating system

        An overview of the project, it's status and expected benefits in power and carbon saving are presented.

        Speaker: Traynor, Daniel (Queen Mary University of London)
    • 11:00 AM 12:30 PM
      Track 8 - Collaboration, Reinterpretation, Outreach and Education: Collaborative Infrastructure Marriott Ballroom I

      Marriott Ballroom I

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Gazzarrini, Elena (CERN) , Hernandez Villanueva, Michel (DESY)
      • 11:00 AM
        The SMARTHEP European Training Network 15m

        Synergies between MAchine learning, Real-Time analysis and Hybrid architectures for efficient Event Processing and decision making (SMARTHEP) is a European Training Network with the aim of training a new generation of Early Stage Researchers to advance real-time decision-making, effectively leading to data-collection and analysis becoming synonymous.

        SMARTHEP will bring together scientists from the four major LHC collaborations which have been driving the development of real-time analysis (RTA) and key specialists from computer science and industry. By solving concrete problems as a community, SMARTHEP will bring forward a more widespread use of RTA techniques, enabling future HEP discoveries and generating impact in industry.
        The students will contribute to European growth, leveraging their hands-on experience machine learning and accelerators towards concrete commercial deliverables in fields that can most profit from RTA, such as transport, manufacturing, and finance.

        This contribution presents the training and outreach plan for the network, as well as some of its early results, and is intended as an opportunity for further collaboration and feedback from the CHEP community.

        Speaker: Gooding, Jamie (Dortmund)
      • 11:15 AM
        ScienceBox 2.0: Evolving the demonstrator package for CERN storage and analysis services 15m

        In this contribution we describe the 2022 reboot of the ScienceBox project, the containerised SWAN/CERNBox/EOS demonstrator package for CERN storage and analysis services. We evolved the original implementation to make use of Helm charts across the entire dependency stack. Charts have become the de-facto standard for application distribution and deployment in managed clusters (e.g., Kubernetes, OpenShift), providing developers and operators with a rich ecosystem of tools to benefit from, as well as the handles to configure applications and rollout changes in a programmatic way.

        At the same time, we incorporated in ScienceBox the major architectural update to CERNBox, replacing the previous PHP backend with distributed microservices based on Reva. Besides enhancing our existing use cases, the new CERNBox implementation enables and streamlines interoperability with additional applications and sites deployed under the same technology.

        We present this update as a self-contained and easy-to-use package with minimal dependencies and with the same goals as the original ScienceBox: Provide a sandbox to evaluate the storage, sharing, and analysis services we run at CERN on external premises to non-CERN users. We believe there is not only a great value in releasing and contributing back to the open source projects that sustain these services, but also in describing the configuration and artifacts that make operating such complex software systems at scale possible.

        Speaker: Bocchi, Enrico (CERN)
      • 11:30 AM
        First results from the PUNCH4NFDI Consortium 15m

        In the frame of the German NFDI (National Research Data Infrastructure), by now 27 consortia across all domains of science have been setup in order to enhance the FAIR usage and re-usage of scientific data. The consortium PUNCH4NFDI, composed of the German particle, astroparticle, hadron&nuclear, and astrophysics communities, has been approved for initially 5 years of significant funding.

        On its way towards its still visionary science data platform – a biotope for the entire lifecycle of digital research products – PUNCH4NFDI has already made substantial achievements. To provide a federated infrastructure for the involved communities, prototypes of the Computer4PUNCH and Storage4PUNCH servers have been setup that employ established components and middleware from the WLCG community. Existing workflow execution engines are evaluated and adopted for an increasing number of usecases from the participating science disciplines. Work on overarching metadata schemata and related services is ongoing. Furthermore, a set of outreach and education & training activities is being devised, and the integration of the consortium and the disciplines represented by it into the greater German “National Research Data Infrastructure” is progressing, respecting European and international boundary conditions and efforts.

        This contribution lays out the plan of the consortium and presents what it could contribute to the joint effort of the international HEP community.

        Speaker: Schneide, Christiane (DESY)
      • 11:45 AM
        EOSC-CZ plans for physical sciences 15m

        Planned EOSC-CZ projects will significantly improve data management in many scientific fields in the Czech Republic. Several calls for projects are under preparation according to the implementation architecture document created in 2021. Emerging National data infrastructure will build basic infrastructure with significant storage capacity for long term archive of scientific data and their accessibility from computing resources. National metadata directory project covers findability and interoperability of data. National repository platform project will operate storage services and related services like authentication and authorization. The system will support already existing data repositories to avoid data duplication, but still to ensure unified access to data. Another project will cover education of researchers and specialists for data curation. About eight additional projects will cover different scientific fields.
        The prepared project for physical sciences will bring together small groups producing data on apparatuses in different laboratories with large projects from high energy physics. Many HEP projects are well advanced in ensuring FAIR principles in data management. Some of their data management tools can be used by small groups if sufficient support is available. We present several examples of differences in requirements on data volumes, their structure and description via metadata together with planned solution how to spread FAIR standards to all participating physics projects.

        Speaker: Chudoba, Jiri
      • 12:00 PM
        Facilitating the preservation of LHCb analyses 15m

        High Energy Physics experiments at the Large Hadron Collider generate petabytes of data that go though multiple transformation before final analysis and paper publication. Recording the provenance of these data is therefore crucial to maintain the quality of the final results. While the tools are in place within LHCb to keep this information for the common experiment-wide transforms, analysts have to implement solutions themselves for the steps dealing with ntuples. The gap between centralised and interactive processing can become problematic. In order to facilitate the task, ntuples extracted by LHCb analysts via so-called “Analysis Productions” are tracked in the experiment bookkeeping database and can be enriched with extra information about their meaning and intended use. This information can then be used to access the data more easily: a set of Python tools allow locating the files based on their metadata and integrating their processing within analysis workflows. The tools are designed with the intention of ensuring analysis code continues to be functional into the future and are robust against evolutions in how data is accessed. This paper presents the integration of these new tools within the LHCb codebase and demonstrates how they will be used in LHCb data processing and analysis.

        Speaker: Couturier, Benjamin (CERN)
      • 12:15 PM
        Scalable training on scalable infrastructures for programmable hardware 15m

        The increasingly pervasive and dominant role of machine learning (ML) and deep learning (DL) techniques in High Energy Physics is posing challenging requirements to effective computing infrastructures on which AI workflows are executed, as well as demanding requests in terms of training and upskilling new users and/or future developers of such technologies.

        In particular, a growth in the request for training opportunities to become proficient in exploiting programmable hardware capable of delivering low latencies and low energy consumption, like FPGAs, is observed. While training opportunities on generic ML/DL concepts is rich and quite wide in the coverage of sub-topics, a gap is observed in the delivery of hands-on tutorials on ML/DL on FPGAs that can scale to a relatively large number of attendants and that can give access to a relatively diverse set of ad-hoc hardware with different hardware specs.

        A pilot course on ML/DL on FPGAs - born from the collaboration of INFN-Bologna, the University of Bologna and INFN-CNAF - has been successful in paving the way for the creation of a line of work dedicated to maintaining and expanding an ad-hoc scalable toolkit for similar courses in the future. The practical sessions are based on virtual machines (for code development, no FPGAs), in-house cloud platforms (INFN-cloud infrastructure equipped with AMD/Xilinx Alveo FPGA), Amazon AWS instances for project deployment on FPGAs - all complemented by docker containers with the full environments for the DL frameworks used, as well as Jupyter Notebooks for interactive exercises. The current results and plans of work along the consolidation of such a toolkit will be presented and discussed.

        Finally, a software ecosystem called Bond Machine, capable of dynamically generate computer architectures that can be synthesised in FPGA, is being considered as a suitable alternative to teach FPGA programming without entering into the low-level details, thanks to the hardware abstraction it offers which can simplify the interaction with FPGAs.

        Speaker: Lorusso, Marco (University of Bologna)
    • 11:00 AM 12:30 PM
      Track 9 - Artificial Intelligence and Machine Learning: Reconstruction Hampton Roads VII

      Hampton Roads VII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Schaarschmidt, Jana (University of Washington (US)) , Wenzel, Sandro (CERN)
      • 11:00 AM
        A deep-learning reconstruction algorithm for cluster counting 15m

        Future e+e- colliders are crucial to extend the search for new phenomena possibly related to the open questions that the Standard Model presently does not explain. Among the major physics programs, the flavor physics program requires particle identification (PID) performances well beyond that of most detectors designed for the current generation. The cluster counting, which measures the number of primary ionizations (dN/dx) instead of the energy loss (dE/dx) along the particle trajectory in a gaseous detector, represents the most promising breakthrough in PID. The Poissonian nature of the dN/dx offers a more statistically significant way of ionization measurement, which makes the dN/dx potentially has a resolution two times better than the dE/dx. Drift chamber (DC) with cluster counting has been proposed as the future advanced detector candidates for Circular Electron Positron Collider (CEPC) and Future Circular Collider (FCC).

        Machine learning (ML) algorithms, which are designed to exploit large datasets to reduce complexity and find new features in data, are the state-of-the-art in PID. The reconstruction of dN/dx measurement needs to determine the number of peaks associated with the primary ionizations in the induced current waveform in a DC cell. The major challenges of the reconstruction are to detect peaks in the highly pileup and noisy situations, and to discriminate the peaks formed by the primary and secondary ionizations. Traditional method, such as taking derivatives, can hardly reach the required efficiency due to the inefficient use of the information. In this study, a two-step ML based algorithm is developed for the dN/dx reconstruction. The algorithm consists of an RNN-based peak finding model, and a CNN-based discrimination model. According to the simulated results, the performance of the ML algorithm surpasses the derivative algorithm in terms of detection efficiency and resolution. The algorithm is further demonstrated by analyzing the test beam data taken at CERN and preliminary results will be presented.

        Speaker: Dr Wu, Linghui (Institute of High Energy Physics)
      • 11:15 AM
        Scalable, End-to-End, Machine-Learning-Based Data Reconstruction Chain for Particle Imaging Detectors 15m

        Recent inroads in Computer Vision (CV), enabled by Machine Learning (ML), have motivated a new approach to the analysis of particle imaging detector data. Unlike previous efforts which tackled isolated CV tasks, this paper introduces an end-to-end, ML-based data reconstruction chain for Liquid Argon Time Projection Chambers (LArTPCs), the state-of-the-art in precision imaging at the intensity frontier of neutrino physics. The chain is a multi-task network cascade which combines voxel-level feature extraction using Sparse Convolutional Neural Networks and particle superstructure formation using Graph Neural Networks. Each individual algorithm incorporates physics-informed inductive biases, while their collective hierarchy enforces a causal relashionship between them. The output is a comprehensive description of an event that may be used for high-level physics inference. The chain is end-to-end optimizable, eliminating the need for time-intensive manual software adjustments. The ICARUS detector, part of the short baseline neutrino (SBN) program at Fermilab, is the largest LArTPC built and operated to date and is used to assess the performance of this reconstruction chain in a realistic setting.

        Speaker: Drielsma, Francois (SLAC)
      • 11:30 AM
        HyperTrack: neural combinatorics for high energy physics 15m

        I will introduce a new neural algorithm -- HyperTrack, designed for exponentially demanding combinatorial inverse problems of high energy physics final state reconstruction and high-level analysis at the LHC and beyond. Many of these problems can be formulated as clustering on a graph resulting in a hypergraph. The algorithm is based on a machine learned geometric-dynamical input graph constructor and a neural network operating on that graph. The neural model is built using a graph neural network and a set transformer, which are end-to-end optimized under a fusion loss function targeting simultaneously the graph node, edge and clustering objectives. The clustering procedure can be changed according to the problem complexity requirements, from a greedy diffusion like iteration to a more computationally demanding but powerful Monte Carlo search based. I will demonstrate the scalability and physics performance of this cutting-edge approach with simulations and discuss possible future directions towards a hybrid quantum computer algorithm.

        Speaker: Mieskolainen, Mikael (Imperial College London)
      • 11:45 AM
        Implicit Neural Representation as a Differentiable Surrogate for Photon Propagation in a Monolithic Neutrino Detector 15m

        Modern neutrino experiments employ hundreds to tens of thousands of photon detectors to detect scintillation photons produced from the energy deposition of charged particles. A traditional approach of modeling individual photon propagation as a look-up table requires high computational resources, and therefore it is not scalable for future experiments with multi-kiloton target volume.

        We propose a new approach using SIREN, an implicit neural representation with periodic activation functions, to model the look-up table as a 3D scene. It reproduces the acceptance map with high accuracy using orders of magnitude less number of parameters than the look-up table. As a continuous and differentiable parameterization, SIREN also represents a smooth gradient surface. As such, it allows downstream applications such as inverse problem-solving and gradient-based optimizations. We demonstrate a data-driven method to optimize the SIREN model and an application of reconstruction using data collected from the Deep Underground Neutrino Experiment's (DUNE) near detector prototype.

        Speaker: Tsang, Patrick (SLAC)
      • 12:00 PM
        Neutrino interaction vertex-finding in a DUNE far-detector using Pandora deep-learning 15m

        The Deep Underground Neutrino Experiment (DUNE) will operate four large-scale Liquid-Argon Time-Projection Chambers (LArTPCs) at the far site in South Dakota, producing high-resolution images of neutrino interactions.

        LArTPCs represent a step-change in neutrino interaction imaging and the resultant images can be highly detailed and complex. Extracting the maximum value from LArTPC hardware requires correspondingly sophisticated pattern-recognition software to interpret signals from the detectors as physically meaningful objects that form the inputs to physics analyses. A critical component is the identification of the neutrino interaction vertex, which is non-trivial due to the interaction occurring at any point within the detector volume. Subsequent reconstruction algorithms use this location to identify the individual primary particles and ensure they each result in a separate reconstructed particle.

        A new vertex-finding procedure presented in this talk integrates a U-Net performing hit-level classification into the multi-algorithm approach used by the Pandora pattern recognition framework to identify the neutrino interaction vertex. The machine learning solution is seamlessly integrated into a chain of traditional pattern-recognition algorithms incorporating knowledge of the detector, demonstrating that traditional and machine learning methods need not be mutually exclusive in leveraging the potential of machine learning for neutrino physics.

        Speaker: Chappell, Andrew (University of Warwick)
      • 12:15 PM
        Graph Neural Network for 3D Reconstruction in Liquid Argon Time Projection Chambers 15m

        The Exa.TrkX team has developed a Graph Neural Network (GNN) for reconstruction of liquid argon time projection chamber (LArTPC) data. We discuss the network architecture, a multi-head attention message passing network that classifies detector hits according to the particle type that produced them. By utilizing a heterogeneous graph structure with independent subgraphs for each 2D plane’s hits and for 3D space points, the model achieves a consistent description of the neutrino interaction across all planes.

        Performance results will be presented based on publicly available samples from MicroBooNE. These will include both physics performance metrics, achieving ~95% accuracy when integrated over all particle classes, and computational metrics for training on single or distributed GPU systems and for inference on CPU or GPU.

        We will discuss applications of the network for additional LArTPC reconstruction tasks, such as event classification, cosmic rejection and particle instance segmentation. Prospects for integration in the data processing chains of experiments will also be presented.

        Speaker: Hewes, V (University of Cincinnati)
    • 11:00 AM 12:30 PM
      Track X - Exascale Science, Heterogeneous Computing and Accelerators, and Quantum Computing: Software tools for Parallel Computing Marriott Ballroom VII

      Marriott Ballroom VII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Aaij, Roel (Nikhef National institute for subatomic physics (NL)) , Campos, Isabel (CSIC)
      • 11:00 AM
        Results from HEP-CCE 15m

        High energy physics is facing serious challenges in the coming decades due to the projected shortfall of CPU and storage resources compared to our anticipated budgets. In the past, HEP has not made extensive use of HPCs, however the U.S. has had a long term investment in HPCs and it is the platform of choice for many simulation workloads, and more recently, data processing for projects such as LIGO, the light sources, sky surveys, as well as for many AI and ML tasks. By mid to late decade, we expect on the order of 10 exaflops of peak power to be available in HPCs, and an order of magnitude more in the following decade. This is at least two orders of magnitude more than HEP requires, but it would be a significant challenge for HEP experiments to use, especially since most of the cycles will be provided by accelerators like GPUs. Can the HEP community leverage these resources to address our computational shortfalls?

        The High Energy Physics Center for Computational Excellence (HEP-CCE), a 3 year pilot project which started in 2020, was formed to investigate this challenge, and provide strategies for HEP experiments to make use of HPC and other massively parallel resources. HEP-CCE functions in close co-operation with the stakeholder experiments, and is split into 4 parts. The first is to investigate Portable Parallelization Strategies, to make use of the massive available parallelism in GPU enabled HPCs, and to engineer portable coding solutions that allow single source software to run on all architectures. The second is to tackle fine grained I/O and the related storage issues on HPCs, by enhancing the existing Darshan HPC I/O monitoring tool to handle HEP workflows and characterize those for ATLAS, CMS & DUNE, developing a I/O mimicking framework allowing scalability studies for different I/O implementations (including ROOT, HDF5) in regimes not yet accessible to HEP production jobs, using HDF5 via ROOT serialization with parallel I/O and investigating new data model with more performant I/O and offloading to GPU resources. The third looks at Event Generators, such as MadGraph and Sherpa, to convert them to run efficiently on GPUs. And the last is to understand how we can map our Complex Workflows onto HPC resources, which are very different from normal HPC workflows.

        In this submission we present the results of our 3 year investigations from all 4 domains and give an outlook on recommendations for current and future HEP experiments on how to best use the U.S. HPC environment.

        Speaker: Leggett, Charles (Lawrence Berkeley National Laboratory)
      • 11:15 AM
        Enabling INFN-T1 to support heterogeneous computing architectures 15m

        The INFN-CNAF Tier-1 located in Bologna (Italy) is a center of the WLCG e-Infrastructure providing computing power to the four major LHC collaborations and also supports the computing needs of about fifty more groups - also from non HEP research domains. The CNAF Tier1 center has been historically very active putting effort in the integration of computing resources, proposing and prototyping solutions both for extension through Cloud resources, public and private, and with remotely owned sites, as well as developing an integrated HTC+HPC system with the PRACE CINECA supercomputer center located 8Km far from the CNAF Tier-1 located in Bologna. In order to meet the requirements for the new Tecnopolo center, where the CNAF Tier-1 will be hosted, the resource integration activities keep progressing. In particular, this contribution will detail the challenges that have recently been addressed, providing opportunistic access to non standard CPU architectures, such as PowerPC and hardware accelerators (GPUs). We explain the strategy adopted to both transparently provision x86_64, ppc64le and nVidia V100 GPUs from the Marconi 100 HPC cluster managed by CINECA and to access data from the Tier1 storage system at CNAF. Finally we will discuss the results of the early experience.

        Speaker: Dr Dal Pra, Stefano (INFN-CNAF)
      • 11:30 AM
        Using parallel I/O libraries for managing HEP experimental data 15m

        The computing and storage requirements of the energy and intensity frontiers will grow significantly during the Run 4 & 5 and the HL-LHC era. Similarly, in the intensity frontier, with larger trigger readouts during supernovae explosions, the Deep Underground Neutrino Experiment (DUNE) will have unique computing challenges that could be addressed by the use of parallel and accelerated data-processing capabilities. Most of the requirements of the energy and intensity frontier experiments rely on increasing the role of high performance computing (HPC) in the HEP community. In this presentation, we will describe our ongoing efforts that are focused on using HPC resources for the next generation HEP experiments. The HEP-CCE (High Energy Physics-Center for Computational Excellence) IOS (Input/Output and Storage) group has been developing approaches to map HEP data to the HDF5 , an I/O library optimized for the HPC platforms to store the intermediate HEP data. The complex HEP data products are ROOT serialized before mapping into the HDF5 format. The mapping of the data products can be designed to optimize parallel I/O. Similarly, simpler data can be directly mapped into the HDF5, which can also be suitable for offloading into the GPUs directly. We will present our works on both complex and simple data model models.

        Speaker: Bashyal, Amit (Argonne National Lab)
      • 11:45 AM
        Fast, high-quality pseudo random number generators for heterogeneous computing 15m

        Random number generation is key to many applications in a wide variety of disciplines. Depending on the application, the quality of the random numbers from a particular generator can directly impact both computational performance and critically the outcome of the calculation.

        High-energy physics applications use Monte Carlo simulations and machine learning widely, which both require high-quality random numbers. In recent years, to meet increasing performance requirements, many high-energy physics workloads leverage GPU acceleration. While on a CPU, there exist a wide variety of generators with different performance and quality characteristics, the same cannot be stated for GPU and FPGA accelerators.

        On GPUs, the most common implementation is provided by cuRAND - an NVIDIA library that is not open source or peer reviewed by the scientific community. The highest-quality generator implemented in cuRAND is a version of the Mersenne Twister. Given the availability of better and faster random number generators, high-energy physics moved away from Mersenne Twister several years ago and nowadays MixMax is the standard generator in Geant4 via CLHEP.

        The MixMax original design supports parallel streams with a seeding algorithm that makes it especially suited for GPU and FPGA where extreme parallelism is a key factor. In this study we implement the MixMax generator on both architectures and analyze its suitability and applicability for accelerator implementations. We evaluated the results against “Mersenne Twister for a Graphic Processor” (MTGP32) on GPUs which resulted in 5, 13 and 14 times higher throughput when a 240, 17 and 8 sized vector space was used respectively. The MixMax generator coded in VHDL and implemented on Xilinx Ultrascale+ FPGAs, requires 50% fewer total LUTs compared to a 32-bit Mersenne Twister (MT-19337), or ~75% fewer LUTs per output bit.

        In summary, the state-of-the art MixMax pseudo random number generator has been implemented on GPU and FPGA platforms and the performance benchmarked.

        Speaker: Barbone, Marco (Imperial College London)
      • 12:00 PM
        XkitS:A computational storage framework for high energy physics based on EOS storage system 15m

        Large-scale high-energy physics experiments generate petabytes or even exabytes of scientific data, and high-performance data IO is required during their processing. However, computing and storage devices are often separated in large computing centers, and large-scale data transmission has become a bottleneck for some data-intensive computing tasks, such as data encoding and decoding, compression, sorting, etc. Data transfer can take up to 30% of the entire computing process. The more data is called in a compute task, the more obvious this cost becomes. One attractive solution to this problem is to offload some of the data processing to the storage layer. However, modifying legacy storage systems to support compute offloading is often tedious and requires an extensive understanding of the internals.
        Therefore, we have designed a new software framework XkitS for building computational storage systems by extending the existing storage system, EOS. The framework is deployed on EOS FTS storage servers and offloads computing tasks by calling the computing power (including CPU, FPGA, etc.) on FST. XkitS can embed multiple data processing methods into the storage layer, which can be implemented in scripting languages or evolved independently of the storage system in the form of containers. On the storage server side, XkitS implements an XRootD plugin that executes first when FTS receives a file access request. It calls the target program on the storage server by parsing the parameters of the command to open file. At this point, the input file is on the FTS storage server, and the output file is also written on it. At the end of the task execution, the file is automatically registered with the MGM metadata server. On the storage client side, XkitS is fully compatible with XRootD's API and EOS commands. Users can add tasks and parameters to be performed in the open option. XkitS processing is black-box for users, and they get the same results as they normally would, but jobs are processed faster and queues are avoided. At present, it has been tested and applied in the data processing of the Large High Altitude Air Shower Observatory (LHAASO), and the results show that the efficiency of data decoding is more than 5 times higher than the original method.

        Speaker: CHENG, Yaodong (IHEP, CAS)
      • 12:15 PM
        Evaluation of ARM CPUs for IceCube available through Google Kubernetes Engine 15m

        The IceCube experiment has substantial simulation needs and is in continuous search for the most cost-effective ways to satisfy them. The most CPU-intensive part relies on CORSIKA, a cosmic ray air shower simulation. Historically, IceCube relied exclusively on x86-based CPUs, like Intel Xeon and AMD EPYC, but recently server-class ARM-based CPUs are also becoming available, both on-prem and in the cloud.
        In this paper we present our experience in running a sample CORSIKA simulation on both ARM and x86 CPUs available through Google Kubernetes Engine (GKE). We used the production binaries for the x86 instances, but had to build the binaries for ARM instances from source code, which turned out to be mostly painless. Our benchmarks show that ARM-based CPUs in GKE are not only the most cost-effective but are also the fastest in absolute terms in all the tested configurations. While the advantage is not drastic, about 20% in cost-effectiveness and less than 10% in absolute terms, it is still large enough to warrant an investment in ARM support for IceCube.

        Speaker: Sfiligoi, Igor
    • 12:30 PM 2:00 PM
      Lunch on Own 1h 30m
    • 2:00 PM 3:30 PM
      Track 1 - Data and Metadata Organization, Management and Access: Tapes Norfolk Ballroom III-V

      Norfolk Ballroom III-V

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Davila, Diego (University of California, San Diego) , Lassnig, Mario (CERN)
      • 2:00 PM
        An HTTP REST API for Tape-backed Storage 15m

        The goal of the “HTTP REST API for Tape” project is to provide a simple, minimalistic and uniform interface to manage data transfers between Storage Endpoints (SEs) where the source file is on tape. The project is a collaboration between the developers of WLCG storage systems (EOS+CTA, dCache, StoRM) and data transfer clients (gfal2, FTS). For some years, HTTP has been growing in popularity as the preferred data transfer protocol between many WLCG SEs. However — unlike other protocols such as XRootD and SRM — HTTP does not include a method to stage files from tape to disk prior to transfer, forcing the use of workarounds such as hybrid protocols (different protocols used for the “stage” and “transfer” parts of the operation). The HTTP REST API offers a simple and consistent solution, by extending the HTTP protocol to include staging operations. It provides clients with a common and consistent API across different storage systems to manage and monitor the disk and tape residency of stored files. In this contribution, we present the history and motivation of the HTTP REST API project, the specification of version 1 of the API and implementation details in the various storage and data transfer systems. We also describe our experiences of its deployment and use for LHC Run-3 operations. We conclude with a discussion of possible future work.

        Speakers: Davis, Michael (CERN) , Mr Afonso, Joao (CERN)
      • 2:15 PM
        Challenging the economy of tape storage with the disk-based one 15m

        CDS (Custodial Disk Storage), a disk-based custodial storage powered by CERN EOS storage system, has been operating for the ALICE experiment at the KISTI Tier-1 Centre since November 2021. The CDS replaced existing tape storage operated for almost a decade, after its stable demonstration in the WLCG Tape Challenges in October 2021. We tried to challenge the economy of tape storage in the aspects of data protection and storage capacity by purchasing cheap off-the-shelf disk enclosures and applying four-parity mode of EOS RAIN (Redundant Array of Independent Nodes) layout. In order to get a brief picture of the TCO (Total Cost of Ownership) of the CDS comparing with tape storage, we tried to conduct an estimation of acquisition, operation and other costs on both tape and disk-based custodial storages. A detailed discussion will be presented including capital and operating expenses over time for the custodial storages such as initial purchases and their expansions (with some predictions on the CDS), spaces, installation, software and hardware licenses, maintenance and power consumption.

        Speaker: Ahn, Sang Un (KISTI)
      • 2:30 PM
        Updates to the ATLAS Data Carousel Project 15m

        The High Luminosity upgrade to the LHC (HL-LHC) is expected to deliver scientific data at the multi-exabyte scale. In order to address this unprecedented data storage challenge, the ATLAS experiment launched the Data Carousel project in 2018. Data Carousel is a tape-driven workflow whereby bulk production campaigns with input data resident on tape are executed by staging and promptly processing a sliding window to disk buffer such that only a small fraction of inputs are pinned on disk at any one time. Data Carousel is now in production for ATLAS in Run3. In this paper, we will provide updates on recent Data Carousel R&D projects, including data-on-demand and tape smart writing. Data-on-demand removes from disk data that has not been accessed for a predefined period, when users request them, they will be either staged from tape or recreated by following the original production steps. Tape smart writing employs intelligent algorithms for file placement on tape in order to retrieve data back more efficiently, which is our long term strategy to achieve optimal tape usage in Data Carousel.

        Speaker: Zhao, Xin (Brookhaven National Laboratory (US))
      • 2:45 PM
        Evolution of the CERN Backup system based on RESTIC and the CERN Tape Archive (CTA) 15m

        The CERN IT Department is responsible for ensuring the integrity and security of data stored in the IT Storage Services. General storage backends such as EOSHOME/PROJECT/MEDIA and CEPHFS are used to store data for a wide range of use cases for all stakeholders at CERN, including experiment project spaces and user home directories.

        In recent years a backup system, CBACK, was developed based on the open source backup program Restic. CBACK is currently used to backup all CERNBox data (about 18PB) stored on disks in the CERN Computing Centre to a disk based S3 service instance in the Prevessin Nethub.

        To significantly increase the reliability and security of the backups and reduce the storage costs, by limiting the amount of data on disk, we have added a tape storage backend to CBACK. Tape backup also offers a better protection against potential ransomware attacks. To achieve this we have created a transparent interface to the CERN Tape Archive (CTA) service.

        With this addition CBACK can reliably be extended to new use cases. CBACK has already been extended to backup CephFS Manila shares and in principle can be used to back up any local mountable file system, such as EOS, CephFS, NFS or DFS. Furthermore, CBACK can potentially serve as a replacement for certain use cases currently covered by IBM Spectrum Protect, including the backup of PCs belonging to individual users.

        In this presentation we will describe the architecture and implementation of CBACK with the new tape storage backend and a number of developments planned for the near future.

        Speaker: Dr Rademakers, Fons (CERN)
      • 3:00 PM
        The CERN Tape Archive Beyond CERN — an Open Source Data Archival System for HEP 15m

        The CERN Tape Archive (CTA) was conceived as the successor to CASTOR and as the tape back-end to EOS, designed for the archival storage of data from LHC Run-3 and other experimental programmes at CERN. In the wider WLCG, the tape software landscape is quite heterogenous, but we are now entering a period of consolidation. This has led to a number of sites in WLCG (and beyond) reevaluating their options and choosing CTA for their future tape archival storage needs. However, the original mandate for CTA created a number of design constraints which are not necessarily optimal for other sites beyond CERN Tier-0. In this contribution, we discuss how the CTA team has engaged with the wider HEP community and collaborated on changes to the software to allow it to be adopted more widely. In particular, we describe community contributions to CTA to allow it to be used as the tape backend for dCache, and to allow migrations from other tape systems such as Enstore. In addition, we discuss improvements to the building and packaging of CTA to remove CERN-specific dependencies and to facilitate easy distribition to other sites, and describe the schema upgrade procedure for the CTA Catalogue database. Finally, we present a roadmap for the community edition of CTA.

        Speaker: Davis, Michael (CERN)
    • 2:00 PM 3:30 PM
      Track 2 - Online Computing: Accelerated Computing & Artificial Intelligence Marriott Ballroom V-VI

      Marriott Ballroom V-VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Pantaleo, Felice (CERN) , Yamada, Satoru (KEK)
      • 2:00 PM
        Line Segment Tracking in the High-luminosity LHC 15m

        The Large Hadron Collider (LHC) will be upgraded to High-luminosity LHC, increasing the number of simultaneous proton-proton collisions (pile-up, PU) by several-folds. The harsher PU conditions lead to exponentially increasing combinatorics in charged-particle tracking, placing a large demand on the computing resources. The projection on required computing resources exceeds the computing budget with the current algorithms running on single-thread CPUs. Motivated by the rise of heterogeneous computing in high-performance computing centers, we present Line Segment Tracking (LST), a highly parallelizeable algorithm that can run efficiently on GPUs and has been integrated to the CMS experiment central software. The usage of Alpaka framework for the algorithm implementation allows better portability of the code to run on different types of commercial parallel processors allowing flexibility on which processors to purchase for the experiment in the future. To verify a similar computational performance with a native solution, the alpaka implementation is compared with a cuda one on a NVIDIA Tesla V100 GPU. The algorithm creates short track segments in parallel, and progressively form higher level objects by linking segments that are consistent with genuine physics track hypothesis. The computing and physics performance are on par with the latest, multi-CPU versions of existing CMS tracking algorithms.

        Speaker: Chang, Philip (University of Florida)
      • 2:15 PM
        Demonstration of track reconstruction with FPGAs on live data at LHCb 15m

        The LHCb experiment is currently taking data with a completely renewed DAQ system, capable for the first time of performing a full real-time reconstruction of all collision events occurring at LHC point 8.
        The Collaboration is now pursuing a further upgrade (LHCb "Upgrade-II"), to enable the experiment to retain the same capability at luminosities an order of magnitude larger than the maximum planned for the current Run 3. To this purpose, a vigorous R&D program is ongoing to boost the real-time processing capability of LHCb, needed to cope both with the luminosity increase and the adoption of correspondingly more granular and complex detectors.
        New heterogeneous computing solutions are being explored, with the aim of moving reconstruction and data reduction to the earliest possible stages of processing. In this talk we describe the results obtained from a realistic demonstrator for a high-throughput reconstruction of tracking detectors, operated parasitically on real LHCb data from Run 3 in a purposedly built testbed facility. This demonstrator is based on a extremely parallel, 'artificial retina' architecture, implemented in commercial, PCIe-hosted FPGA cards interconnected by fast optical links, and encompasses a sizable fraction of the LHCb VELO pixel detector. The implications of the results in view of potential applications in HEP are discussed.

        Speaker: Lazzari, Federico (Pisa University & INFN)
      • 2:30 PM
        Track reconstruction for the ATLAS Phase-II HLT using GNNs on FPGAs 15m

        The High-Luminosity LHC (HL-LHC) will provide an order of magnitude increase in integrated luminosity and enhance the discovery reach for new phenomena. The increased pile-up foreseen during the HL-LHC necessitates major upgrades to the ATLAS detector and trigger. The Phase-II trigger will consist of two levels, a hardware-based Level-0 trigger and an Event Filter (EF) with tracking capabilities. Within the Trigger and Data Acquisition group, a heterogeneous computing farm consisting of CPUs and potentially GPUs and/or FPGAs is under study, together with the use of modern machine learning algorithms such as Graph Neural Networks (GNNs).

        GNNs are a powerful class of geometric deep learning methods for modelling spatial dependencies via message passing over graphs. They are well-suited for track reconstruction tasks by learning on an expressive structured graph representation of hit data and considerable speedup over CPU-based execution is possible on FPGAs.

        The focus of this talk is a study of track reconstruction for the Phase-II EF system using GNNs on FPGAs. We explore each of the steps in a GNN-based EF tracking pipeline: graph construction, edge classification using an interaction network, and track reconstruction. Several methods and hardware platforms are under evaluation, studying resource utilisation and minimization of model size using quantization aware training, while simultaneously retaining high track reconstruction efficiency and low fake rates required for the EF tracking system.

        Speaker: Dittmeier, Sebastian (Heidelberg University)
      • 2:45 PM
        A vendor-unlocked ITS GPU reconstruction in ALICE 15m

        During the LHC Run 3, the significant upgrades on many detectors and a brand new reconstruction software allows the ALICE experiment to record Pb-Pb collisions at an interaction rate of 50 kHz in a trigger-less continuous readout mode.

        The key to process the 1TB/s peak data rate in ALICE is the usage of GPUs. There are two main data processing phases: the synchronous phase, where the TPC reconstruction uses most computing resources, and the asynchronous one, where more GPU resources are available.

        Other detectors are aiming at profiting from this computing potential to offload their reconstructions on graphics cards.

        In this talk, we illustrate how we successfully ported on GPU both the primary vertex finding and the track reconstruction of the silicon tracker of ALICE, the Inner Tracking System.

        We implemented, integrated, and natively supported the ITS code using automatic code generation on two different GPU brands with a single code base.

        The implementation details, performance, and how this technique can be easily used in other applications will be discussed.

        Speaker: Concas, Matteo (CERN)
      • 3:00 PM
        Preliminary Performance Study of an Alternative Calorimeter Clustering Solution for Allen in LHCb 15m

        The LHCb experiment has recently started a new period of data taking after a major upgrade in both software and hardware. One of the biggest challenges has been the migration of the first part of the trigger system (HLT1) into a parallel GPU architecture framework called Allen, which performs a partial reconstruction of most of the LHCb sub-detectors. In Allen, the reconstruction of the Electromagnetic Calorimeter (ECAL) sub-detector is used in many selection algorithms, but its efficiency is currently 10% lower than the full reconstruction performed in the second stage of the trigger. In this talk, we present a preliminary performance study of an alternative ECAL reconstruction algorithm implemented in Allen that complements the current algorithm to maximise the reconstruction efficiency and also minimise the impact on the throughput rate.

        Speaker: Valls Canudas, Núria (La Salle URL)
      • 3:15 PM
        Triggerless data acquisition pipeline for Machine Learning based statistical anomaly detection 15m

        The sensitivity of modern HEP experiments to New Physics (NP) is limited by the hardware-level triggers used to select data online, resulting in a bias in the data collected. The deployment of efficient data acquisition systems integrated with online processing pipelines is instrumental to increase the experiments' sensitivity to the discovery of any anomaly or possible signal of NP. In designing such systems the combination of heterogeneous processing elements, including FPGAs and GPUs, is foreseen to sustain the large throughput of raw data from the detectors.
        In this work, we present the first implementation of an end-to-end infrastructure that acquires continuously data from an experimental setup and processes it online looking for statistical anomalies using a Machine Learning (ML) technique. The infrastructure is deployed at the INFN Legnaro National Laboratory (LNL) and reads out data from a reduced-sized version of the drift tube muon detector of the CMS experiment at CERN. The data stream is first processed by an FPGA to cluster signals associated with the passage of a muon through the detector and produce candidate stubs. Candidate events are then reconstructed and all muon hits and the reconstructed muon stubs are analyzed online by an algorithm deployed on a GPU to perform unbiased data exploration and statistical anomaly detection. The New Physics Learning Machine (NPLM) technique is used to evaluate the compatibility between incoming batches of experimental data and a reference sample representing the normal behavior of the data. In the specific case of the LNL test stand, the NPLM algorithm uses as a reference sample a dataset gathered in nominal detector conditions; data deviations from the normal behavior, if detected, are characterized and then mapped to known sources of detector malfunctioning with some degree of confidence. Unexpected behaviors, that might signal the presence of New Physics, can be singled out if the observed discrepancy doesn't match any of the expected anomalies. The system is currently dealing with the limited throughput originated by the cosmic muon flux; nevertheless, all components of the readout chain are designed to scale up and be eventually employed in experiments at the LHC.
        In this contribution, we describe the technical implementation of the online processing pipeline and assess the performance of its most critical components.

        Speaker: Migliorini, Matteo (Padova University & INFN)
    • 2:00 PM 3:30 PM
      Track 3 - Offline Computing: Data preparation (part I) Hampton Roads Ballroom VI

      Hampton Roads Ballroom VI

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Bandieramonte, Marilena (University of Pittsburgh) , Dr Srpimanobhas, Norraphat (Chulalongkorn University)
      • 2:00 PM
        CMS Tier0 data processing during the detector commissioning in Run-3 15m

        The CMS Tier-0 service is responsible for the prompt processing and distribution of the data collected by the CMS Experiment. A number of upgrades were implemented during the long shutdown of the Large Hadron Collider, which improved the performance and reliability of the service. We report our experience of the data taking during Run-3 detector commissioning as well as performance of the system with respect to Run-2.

        Speaker: Amado, Jhonatan
      • 2:15 PM
        JUNO Offline Software for Data Processing and Analysis 15m

        (on behalf of the JUNO Collaboration)

        Jiangmen Underground Neutrino Observatory (JUNO), under construction in southern China, is a multi-purpose neutrino experiment designed to determine the neutrino mass hierarchy and precisely measure oscillation parameters. Equipped with a 20-kton liquid scintillator central detector viewed by 17,612 20-inch and 25,6000 3-inch photomultiplier tubes, JUNO could reach the unprecedented energy resolution of 3% at 1 MeV.

        JUNO is expected to start data taking in 2024 and plans to run for more than 20 years with about 2 petabytes of raw data each year. The large volume of data has brought a great challenge to the JUNO offline data processing and analysis.

        This contribution will comprehensively review the development of JUNO offline software (JUNOSW) which started in 2012 in order to support JUNO’s specific requirements, and will particularly highlight the following topics:

        1) Data processing framework which supports buffering and management of multiple events, event splitting and mixing, TBB-based multi-threading, and integration of machine learning etc.
        2)Unified detector geometry management to support multiple applications including simulation, calibration, reconstruction and detector visualization.
        3)ROOT based event data model charactering data representations at different processing stages and complicated relationships between them.
        4)Event index based correlation analysis to support selection of sparse physics events from the large volume of data.

        The JUNO data processing and analysis chain was completed and has been used by several rounds of Monte Carlo data challenge on both local computing clusters and the distributed computing infrastructure.

        Speaker: HUANG, Xingtao (Shandong University)
      • 2:30 PM
        Repurposing of the Run 2 CMS High Level Trigger Infrastructure as an Cloud Resource for Offline Computing 15m

        The former CMS Run 2 High Level Trigger (HLT) farm is one of the largest contributors to CMS compute resources, providing about 30k job slots for offline computing. The role of this farm has been evolving, from an opportunistic resource exploited during inter-fill periods in the LHC Run 2, to a nearly transparent extension of the CMS capacity at CERN during LS2 and into the LHC Run 3 started in 2022. This “permanent cloud” is located on-site at the LHC interaction point 5, where the CMS detector is installed. As a critical example, the execution of Tier 0 tasks, such as prompt detector data reconstruction, has been fully commissioned. This resource can therefore be used in combination with the dedicated Tier 0 capacity at CERN, in order to process and absorb peaks in the stream of data coming from the CMS detector, as well as contributing to the prompt reconstruction of a substantial fraction of the “parked data sample”, dedicated primarily to B physics studies. The initial deployment model for this resource, based on long-lived statically configured VMs, including HTCondor execution node services connected to the CMS Submission Infrastructure (SI), provided the required level of functionality to enable its exploitation for offline computing. However, this configuration presented certain limitations in its flexibility of use in comparison to pilot-based resource acquisition at the WLCG sites. For example, slot defragmentation techniques were required to enable matching of Tier 0 multicore jobs. Additionally, the configuration of fair-share quotas and priorities for the diverse CMS tasks could not be directly managed by the CMS SI team, in charge of enforcing the global CMS resource provisioning and exploitation policies. A new configuration of this permanent cloud has been proposed in order to solve these shortcomings. A vacuum-like model, based on GlideinWMS pilot jobs joining the CMS CERN HTCondor Pool has been prototyped and successfully tested and deployed. This contribution will describe this redeployment work on the permanent cloud for an enhanced support to CMS offline computing, comparing the former and new models’ respective functionalities, along with the commissioning effort for the new setup.

        Speaker: Mascheroni, Marco (University of California San Diego)
      • 2:45 PM
        Offline Data Processing Software for the Super Tau Charm Facility 15m

        The Super Tau Charm Facility (STCF) proposed in China is a new-generation electron–positron collider with center-of-mass energies covering 2-7 GeV and a peak luminosity of 5*10^34 cm^-2s^-1. The offline software of STCF (OSCAR) is developed to support the offline data processing, including detector simulation, reconstruction, calibration as well as physics analysis. To meet STCF’s specific requirements, OSCAR is designed and developed based on the SNiPER framework, a lightweight common software for HEP experiments. Besides the commonly used software such as Geant4 and ROOT, several state-of-art software and tools in the HEP community are incorporated as well, such as the Detector Description Toolkit (DD4hep), the plain-old-data I/O (Podio) and Intel Thread Building Blocks (TBB) etc.

        This contribution will present the overall design of OSCAR, and in particular, the following topics will be highlighted.
        1. The design of the Event Data Model based on Podio, and the implementation of the data management system, via the integration of Podio and SNiPER.
        2. The parallelized data processing based on SNiPER and TBB, and in particular, the design of GlobalStore based on the Podio EventStore to support concurrent data access and data I/O.
        3. The geometry management system based on DD4hep that provides consistent geometry for detector simulation, calibration, reconstruction and detector visualization.
        4. Automated software validation system that supports validation at multiple levels ranging from unit test to physical validation.

        Currently, OSCAR is fully functioning to facilitate the conceptual design of the STCF detector and the physics potential study. Meanwhile, OSCAR can also provide a potential solution for other lightweight HEP experiments as well.

        Speaker: Li, Teng (Shandong University)
      • 3:00 PM
        Status of DUNE Offline Computing 15m

        We summarize the status of Deep Underground Neutrino Experiment (DUNE) software and computing development. We describe plans for the computing infrastructure needed to acquire, catalog, reconstruct, simulate and analyze the data from the DUNE experiment and its prototypes in pursuit of the experiment's physics goals of precision measurements of neutrino oscillation parameters, detection of astrophysical neutrinos, measurement of neutrino interaction properties and searches for physics beyond the Standard Model. In contrast to traditional HEP computational problems, DUNE's Liquid Argon TPC data consist of simple but very large (many GB) data objects which share many characteristics with astrophysical images. We have successfully reconstructed and simulated data from 4% prototype detector runs at CERN. The data volume from the full DUNE detector, when it starts commissioning late in this decade will present memory management challenges in conventional processing but significant opportunities to use advances in machine learning and pattern recognition as a frontier user of High Performance Computing facilities capable of massively parallel processing. Our goal is to develop infrastructure resources that are flexible and accessible enough to support creative software solutions as HEP computing evolves.

        Speaker: Kirby, Michael (FNAL)
      • 3:15 PM
        DUNE Database Development 15m

        The Deep Underground Neutrino Experiment (DUNE) is a long-baseline experiment which aims to study neutrino oscillation and astroparticle physics. It will produce vast amounts of metadata, which describe the data coming from the read-out of the primary DUNE detectors. Various databases will make up the overall DB architecture for this metadata. ProtoDUNE at CERN is the largest existing prototype for DUNE and serves as a testing ground for - among other things - possible database solutions for DUNE.
        The subset of all metadata that is accessed during offline data reconstruction and analysis is referred to as ‘conditions data’ and it is stored in a dedicated database. As offline data reconstruction and analysis will be deployed on HTC and HPC resources, conditions data is expected to be accessed at very high rates. It is therefore crucial to store it in a granularity that matches the expected access patterns allowing for extensive caching. This requires a good understanding of the sources and use cases of conditions data. This contribution will briefly summarize the database architecture deployed at ProtoDUNE and explain the various sources of conditions data. We will present how the conditions data is retrieved from the run conditions and beam database; and how, together with the conditions data from the Detector Control System (Slow Controls) and those needed for the calibration of a LArTPC, are put in a format to match the expected access patterns.

        Speaker: Dr Vizcaya Hernandez, Ana Paula (Colorado State University)
    • 2:00 PM 3:30 PM
      Track 4 - Distributed Computing: Monitoring, Testing and Analytics Marriott Ballroom II-III

      Marriott Ballroom II-III

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Ellis, Katy (STFC-RAL) , Miyake, Hideki (KEK/IPNS)
      • 2:00 PM
        The CMS monitoring applications for LHC Run 3 15m

        Data taking at the Large Hadron Collider (LHC) at CERN restarted in 2022. The CMS experiment relies on a distributed computing infrastructure based on WLCG (Worldwide LHC Computing Grid) to support the LHC Run 3 physics program. The CMS computing infrastructure is highly heterogeneous and relies on a set of centrally provided services, such as distributed workload management and data management, and computing resources hosted at almost 150 sites worldwide. Smooth data taking and processing requires all computing subsystems to be fully operational, and available computing and storage resources need to be continuously monitored. During the long shutdown between LHC Run 2 and Run 3, the CMS monitoring infrastructure has undergone major changes to increase the coverage of monitored applications and services, while becoming more sustainable and easier to operate and maintain. The used technologies are based on open-source solutions, either provided by the CERN IT department through the MONIT infrastructure, or managed by the CMS monitoring team. Monitoring applications for distributed workload management, submission infrastructure based on HTCondor, distributed data management, facilities have been ported from mostly custom-built applications to use common data flow and visualization services. Data are mostly stored in no-SQL databases and storage technologies such as ElasticSearch, VictoriaMetrics, InfluxDB and HDFS, and accessed either via programmatic APIs, Apache Spark or Sqoop jobs, or visualized preferentially using Grafana. Most CMS monitoring applications are deployed on Kubernetes clusters to minimize maintenance operations. In this contribution we present the full stack of CMS monitoring services and show how we leveraged the use of common technologies to cover a variety of monitoring applications and cope with the computing challenges of LHC Run 3.

        Speaker: Legger, Federica (INFN Torino)
      • 2:15 PM
        BigPanDA monitoring system evolution in the ATLAS experiment 15m

        Monitoring services play a crucial role in the day-to-day operation of distributed computing systems. The ATLAS experiment at LHC uses the production and distributed analysis workload management system (PanDA WMS), which allows a million computational jobs to run daily at over 170 computing centers of the WLCG and other opportunistic resources, utilizing 600k cores simultaneously on average. The BigPanDAmon system is an essential part of the monitoring infrastructure for the ATLAS experiment that provides a wide range of views from the top-level summaries to a single computational job and its logs. Over the past few years of the PanDA WMS advancement in the ATLAS experiment several new components were developed, such as Harvester, iDDS, Data Carousel, and Global Shares. Due to its modular architecture, BigPanDAmon naturally grew into a platform where the relevant data from all PanDA WMS components and accompanying services are accumulated and displayed in the form of interactive charts and tables. Moreover the system has been adopted by other experiments beyond HEP. In this paper we describe the evolution of the BigPanDAmon system, the development of new modules, and the integration process into other experiments.

        Speaker: Klimentov, Alexei (Brookhaven National Laboratory)
      • 2:30 PM
        Site Sonar - A Flexible and Extensible Infrastructure Monitoring Tool for ALICE Grid 15m

        The ALICE experiment at the CERN Large Hadron Collider relies on a massive, distributed Computing Grid for its data processing. The ALICE Computing Grid is built by combining a large number of individual computing sites distributed globally. These Grid sites are maintained by different institutions across the world and contribute thousands of worker nodes possessing different capabilities and configurations. Developing software for Grid operations that works on all nodes while harnessing the maximum capabilities offered by any given Grid site is challenging without advance knowledge of what capabilities each site offers. Site Sonar is an architecture-independent Grid infrastructure monitoring framework developed by the ALICE Grid team to monitor the infrastructure capabilities and configurations of worker nodes at sites across the ALICE Grid without the need to contact local site administrators. Site Sonar is a highly flexible and extensible framework that offers infrastructure metric collection without local agent installations at Grid sites. This paper introduces the Site Sonar Grid infrastructure monitoring framework and reports significant findings acquired about the ALICE Computing Grid using Site Sonar.

        Speaker: Storetvedt, Maksim (CERN)
      • 2:45 PM
        Bringing the ATLAS HammerCloud setup to the next level with containerization 15m

        HammerCloud (HC) is a testing service and framework for continuous functional tests, on-demand large-scale stress tests, and performance benchmarks. It checks the computing resources and various components of distributed systems with realistic full-chain experiment workflows.

        The HammerCloud software was initially developed in Python 2. After support for Python 2 was discontinued in 2020, migration to Python 3 became vital in order to fulfill the latest security standards and to use the new CERN Single Sign-On, which requires Python 3.

        The current deployment setup based on RPMs allowed a stable deployment and secure maintenance over several years of operations for the ATLAS and CMS experiments. However, the current model is not flexible enough to support an agile and rapid development process. Therefore, we have decided to use a containerization solution, and switched to industry-standard technologies and processes. Having an "easy to spawn" instance of HC enables a more agile development cycle and easier deployment. With the help of such a containerized setup, CI/CD pipelines can be integrated into the automation process as an extra layer of verification.

        A quick onboarding process for new team members and communities is essential,
        as there is a lot of personnel rotation and a general lack of personpower. This is achieved with the container-based setup, as developers can now work locally with a quick turnaround without needing to set up a production-like environment first. These developments empower the whole community to bravely test and prototype new ideas and deliver new types of resources or workflows to our community.

        Speaker: Mr Rottler, Benjamin (Freiburg University)
      • 3:00 PM
        Operational Analytics Studies for ATLAS Distributed Computing: Data Popularity Forecast and Ranking of the WLCG Centers 15m

        Operational analytics is the direction of research related to the analysis of the current state of computing processes and the prediction of the future in order to anticipate imbalances and take timely measures to stabilize a complex system. There are two relevant areas in ATLAS Distributed Computing that are currently in the focus of studies: end-user physics analysis including the forecast of samples of data popularity among users, and ranking of WLCG centers for user analysis tasks. Studies in these areas are non-trivial and require detailed knowledge of all boundary conditions, which may be numerous in large-scale distributed computing infrastructures. Forecasts of data popularity are impossible without the categorization of user tasks by their types (data transformation or physics analysis), which do not always appear on the surface but may induce noise, which introduces significant distortions for predictive analysis. Ranking the WLCG resources is also a challenging task as it is necessary to find a balance between the workload of the resource, its performance, the waiting time for jobs on it, as well as the volume of jobs that it processes. This is especially difficult in a heterogeneous computing environment, where legacy resources are used along with modern high-performance machines. We will look at these areas of research in detail and discuss what tools and methods we use in our work, demonstrating the results that we already have. The difficulties we face and how we solve them will also be described.

        Speaker: Klimentov, Alexei (Brookhaven National Laboratory)
      • 3:15 PM
        Analysis and optimization of ALICE Run 3 multicore Grid jobs 15m

        For LHC Run3 the ALICE experiment software stack has been completely refactored, incorporating support for multicore job execution. The new multicore jobs spawn multiple processes and threads within the payload. Given that some of the deployed processes may be short-lived, accounting for their resource consumption presents a challenge. This article presents the newly developed methodology for payload execution monitoring, which correctly accounts for the resources used by all processes within the payload.

        We also present a black box analysis of the new multicore experiment software framework tracing the used resources and system function calls issued by MonteCarlo simulation jobs. Multiple sources of overhead in the processes and threads lifecycle have thus been identified. This paper describes the tracing techniques and what solutions were implemented to address them. The analysis and subsequent improvements of the code have positively impacted the resource consumption and the overall turnaround time of the payloads with a notable 35% reduction in execution time for a reference production job. We also introduce how this methodology will be used to further improve the efficiency of our experiment software and what other optimization venues are currently being pursued.

        Speaker: Bertran Ferrer, Marta (CERN)
    • 2:00 PM 3:30 PM
      Track 5 - Sustainable and Collaborative Software Engineering: Glance and Web based applications Chesapeake Meeting Room

      Chesapeake Meeting Room

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Eulisse, Giulio , Sexton, Elizabeth (FNAL)
      • 2:00 PM
        Iterative and incremental development of the ATLAS Publication Tracking system 15m

        The ATLAS experiment involves almost 6000 members from approximately 300 institutes spread all over the globe and more than 100 papers published every year. This dynamic environment brings some challenges such as how to ensure publication deadlines, communication between the groups involved, and the continuity of workflows. The solution found for those challenges was automation, which was achieved through the Glance project, more specifically through the Glance Analysis systems, developed to support the analysis and publications life cycle in 2010. Now, after twelve years, in order to satisfy the experiments’ most recent needs, the systems need code refactoring and database remodeling. The goal is to have only one system to accommodate all the analysis and publications workflows, the so-called ATLAS Publication Tracking system, an evolution of the current Analysis systems. This project includes a database remodeling that reflects the hierarchical relation between analyses and publications; a code base that supports non-linear workflows; the expansion of the current API so all the authorized ATLAS members can access ATLAS publication data programmatically; a service-oriented architecture for integration with external software, such as GitLab; the creation of an automatic test environment, which assures the quality of the systems on each update. The ATLAS Publication Tracking system is a long-term project being developed with an iterative and incremental approach, which ensures that the most valuable tools are implemented with priority while allowing a smooth transition between the old systems and the new one.

        Speaker: Cruz, Ana Clara Loureiro (Universidade Federal do Rio De Janeiro)
      • 2:15 PM
        Enhancing data consistency in ATLAS and CERN databases through automated synchronization 15m

        As the largest particle physics laboratory in the world, CERN has more than 17000 collaborators spread around the globe. ATLAS, one of CERN’s experiments, has around 6000 active members and 300 associate institutes, all of which must go through the standard registration and updating procedures within CERN’s HR (Foundation) database. Simultaneously, the ATLAS Glance project, among other functions, also has the same goal within the ATLAS context. At the time of its first development, no tools were available to allow Glance to write into the Foundation database, therefore the solution put into place was to duplicate data. This however proved to be inefficient as the databases grew over time. Information had to be constantly updated manually by the ATLAS Secretariat to keep members and institutes data (such as names, employment information and authorship status) coherent between databases. Today, equipped with new tools, the Glance system is about to change its relationship with Foundation: a sole source of truth for the data shall be determined, removing the duplication of information. This includes automating a series of internal processes so the ATLAS secretariat need not to manually intervene to keep both databases synchronized. For this, a workflow had to be developed so that the previous manual work could be successfully replaced considering the multitude of possible actions by the Secretariat. The remodeling of the current structure of the database, along with the refactoring of the code, shall also be required to establish an easy communication between the two systems. Finally, a number of tools developed on Foundation’s side (such as SQL procedures and APIs) have to be put in place to enable the writing and reading between databases.

        Speaker: Aleksandravicius, Gabriel de Aragão (Universidade Federal do Rio De Janeiro)
      • 2:30 PM
        Glance Search Interface 15m

        The LHCb experiment is one of the 4 LHC experiments at CERN. With more than 1500 members and tens of thousands of assets, the Collaboration requires systems that allow the extraction of data from many databases according to some very specific criteria. In LHCb there are 4 production web applications responsible for managing members and institutes, tracking assets and their current status, presenting radiological information of the cavern and supporting the management of cables. A common requirement shared across all these systems is to allow searching information based on logic sentences. Therefore, in order to avoid rework, the Glance Search Library was created with the goal to provide components for applications to deploy frontend search interfaces capable of generating standardized queries based on users' input, and backend utility functions that compile such queries into a SQL clause. The Glance Search Library is split into 2 smaller libraries maintained in different GitLab repositories. The first one only contains Vue components and JavaScript modules and, in LHCb, it is included as a dependency of the SPAs. The second is a PHP Object-Oriented library, mainly used by REST APIs that are required to expose large amounts of data stored in their relational databases. This separation provides greater flexibility and more agile deployments. It also enables lighter applications with no graphical interface to build command line tools solely on top of the backend classes and predefined queries, for example.

        Speaker: Ferreira Brito Filho, Carlos Henrique
      • 2:45 PM
        The migration to a standardized architecture for developing systems on the Glance project 15m

        The Glance project is responsible for over 20 systems across three CERN experiments: ALICE, ATLAS and LHCb. Students, engineers, physicists and technicians have been using systems designed and managed by Glance on a daily basis for over 20 years. In order to produce quality products continuously, considering internal stakeholder's ever-evolving requests, there is the need of standardization. The adoption of such a standard had to take into account not only future developments but also legacy systems of the three experiments. These systems were built as a monolith, which, as they scaled, became difficult to maintain due to its lack of documentation and use of technologies that were becoming obsolete. Migrating them to a new architecture would mean speeding up the development process, avoiding rework and integrating CERN systems widely. Since a lot of the core functionalities of the systems are shared between them, both on the frontend and on the backend, the architecture had to assure modularity and reusability. In this architecture, the principles behind Hexagonal Architecture are followed and the systems’ codebase is split into two applications: a JavaScript client and a REST backend server. The open-source framework Vue.js was chosen for the frontend. Its versatility, approachability and extended documentation made it the ideal tool for creating components that are reused throughout Glance applications. The backend uses PHP libraries created by the team to expose information through REST APIs both internally, allowing easier integration between the systems, and externally, introducing to users outside Glance information managed by the team.

        Speaker: Ferreira Brito Filho, Carlos Henrique (UFRJ)
      • 3:00 PM
        Security Models for ALICE Online Web-Based Applications 15m

        The recent major upgrade of the ALICE Experiment at CERN’s Large Hadron Collider has been coupled with the development of a new Online-Offline computing system capable of interacting with a sustained input throughput of 3.5TB/s. To facilitate the control of the experiment, new web applications have been developed and deployed to be used 24 hours a day, 365 days a year in the control room and remotely by the subsystem experts and on-call support staff.
        Over the past years, an exponential increase in number of exploits on applications vulnerabilities has been observed. This includes but it is not limited to malicious user input, DDoS, SQL Injection and Cross-Site Scripting attacks. Thus, the ALICE interfaces are being built using modern web technologies and a common library developed in-house which provides the core functionalities and building blocks for preventing vulnerabilities. This approach ensures a consolidated and secure environment towards maintaining data integrity and a straightforward non-malicious control of the experiment. This work showcases the tools and practices applied to enhance the application-level security and privacy needed for the experiment to be controlled and observed remotely. A report is also presented of incidents encountered during the first year of ALICE Run 3 operation.

        Speaker: Raduta, George (CERN)
      • 3:15 PM
        Building a highly modular user-oriented notification system 15m

        CERN, as many large organizations, relies on multiple communication means for different use-cases and teams.
        Email and mailing lists are the most popular ones, but more modern communications systems gain traction such as Mattermost and Push notifications.
        On one end of the spectrum we have communication teams writing individual emails to users on a daily basis, which may be small targets, or in the order of thousands. On the other end, there are many automated tools and scripts which generate thousands of notifications daily, mostly in the form of emails.

        As a consequence of the large amount of notifications received every day, for the users receiving them, it is challenging to control and keep track of where, how and when some information was received.
        At the same time for those sending and maintaining the tools that deliver notifications, it is difficult to choose which targets to adopt (email, Mattermost, etc). Additionally it is difficult to please all users and take into account their preferences. Ultimately, across all those responsible for sending information, a lot of effort is spent on maintaining similar scripts and tools.

        The CERN Notifications system aims at consolidating communication by providing a central place where notifications are created, maintained and distributed.
        It allows to save efforts and costs by avoiding multiple parallel implementations of communication systems and their maintenance and details such as retry and failure mechanism, version updates, etc.
        CERN Notifications allows not only optimising the flow for the multiple people and teams which are responsible for sending, but also empowers the target users by respecting their preferences: how, where and when they receive their notifications.
        The system was designed to allow those who send information to focus on the the content and relevance of the communication without knowing the technical details of the many frameworks available to distribute information.

        This paper describes the design and architecture of the CERN Notifications system and its components, how it was designed with a flexible and highly modular architecture which allows adding further device targets with little effort. Furthermore, it presents implementation details and the decisions behind those. And last but not least it describes the features that empower users to choose how to consume information send to them.

        Speaker: Antunes, Carina
    • 2:00 PM 3:30 PM
      Track 6 - Physics Analysis Tools: Reconstruction and Amplitude Fitting Hampton Roads Ballroom VIII

      Hampton Roads Ballroom VIII

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Heddle, Dave (CNU) , Skidmore, Nicole (University of Manchester)
      • 2:00 PM
        A Kinematic Kalman Filter Track Reconstruction Algorithm for the Mu2e Experiment 15m

        The primary physics goal of the Mu2e experiment requires reconstructing an isolated 105 MeV electron with better than 500 KeV/c momentum resolution. Mu2e uses a low-mass straw tube tracker, and a CsI crystal calorimeter, to reconstruct tracks.
        In this paper, we present the design and performance of a track reconstruction algorithm optimized for Mu2e’s unusual requirements. The algorithm is based on the KinKal kinematic Kalman filter track fit package. KinKal supports multiple track parameterizations, including one optimized for looping tracks, such as Mu2e signal tracks, and others optimized for straight or slightly-curved tracks, such as the high-momentum (P>1 GeV/c) cosmic ray muons used to calibrate and align the Mu2e detectors. All KinKal track parameterizations include the track origin time, to correctly model correlations arising from measurements that couple time and space, such as the straw drift time or the calorimeter cluster time. KinKal employs magnetic field inhomogeneity and material effect correction algorithms with 10-4 fractional precision. The Mu2e fit uses Artificial Neural Net functions to discriminate background hits from signal hits, and to resolve the straw tube hit left-right ambiguity, while iterating the extended Kalman filter. The efficiency, accuracy, and precision of the Mu2e track reconstruction, as tested on detailed simulations of Mu2e data, will be presented.

        Speaker: Brown, David (LBL)
      • 2:15 PM
        MEDUSA, A MULTITHREAD 4-BODY DECAY FITTING AND SIMULATION SOFTWARE 15m

        Among the biggest computational challenges for High Energy Physics (HEP) experiments there are the increasingly larger datasets that are being collected, which often require correspondingly complex data analyses. In particular, the PDFs used for modeling the experimental data can have hundreds of free parameters. The optimization of such models involves a significant computational effort and a considerable amount of time, of the order of days, before reaching a result.

        Medusa is a C++ application designed to perform physics data analyses of generic 4-body decays deploying massively parallel platforms (multicore CPUs and GPUs) on Linux systems. It relies on Hydra, a header-only library that provides a high-level and user-friendly interface for common algorithms used in HEP, abstracting away the complexities associated with the implementation of code for different massively parallel architectures.

        Medusa has been tested through the measurement of the CP-violating phase phi_s in b-hadron decays exploiting the data collected by the LHCb experiment. By deploying such technologies as CUDA, TBB and OpenMP, Medusa accelerates the optimization of the full model, running over 500000 events, by factors 74 (multicore CPU) and 370 (GPU) in comparison with a non-parallelized program.

        Speaker: Dr Ricci, Alessandro Maria (University of Pisa and INFN Pisa)
      • 2:30 PM
        Event Generator Tuning Incorporating MC Systematic Uncertainty 15m

        To accurately describe data, tuning the parameters of MC event Generators is essential. At first, experts performed tunings manually based on their sense of physics and goodness of fit. The software, Professor, made tuning more objective by employing polynomial surrogate functions to model the relationship between generator parameters and experimental observables (inner-loop optimization), then optimizing an objective function to obtain generator parameters (outer-loop optimization). Finally, Apprentice, a purely python-based tool, was developed to leverage High-Performance Computing and introduced rational approximation as an alternative surrogate function. However, none of these tuning methods includes MC systematic uncertainties. More importantly, the estimated uncertainties of tuned parameters are unreliable because the objective distribution does not match a chi-squared distribution, and one has to manually set a cutoff threshold on the objective function using educated guesses. In this work, we integrate the MC systematic uncertainties into the inner-loop optimization and outer-loop optimization. With our new method, we find that the objective function nicely follows the chi-square distribution; thus, the uncertainty of the tuned generator parameters is better quantified.

        Speaker: Ju, Xiangyang (Lawrence Berkeley National Laboratory)
      • 3:00 PM
        `epic-analysis`: Common Physics Analysis Software for the EIC 15m

        Performing a physics analysis of data from simulations of a high energy experiment requires the application of several common procedures, from obtaining and reading the data to producing detailed plots for interpretation. Implementing common procedures in a general analysis framework allows the analyzer to focus on the unique parts of their analysis. Over the past few years, EIC simulations have been performed using differing frameworks and data models; we thus developed epic-analysis, a common analysis framework to support all of them, allowing for comparison studies and cross checks while the design of the EIC continues to evolve. The reconstruction of kinematic variables is fundamental to several physics channels, including inclusive, semi-inclusive, and jet physics. epic-analysis includes many different kinematics reconstruction methods, ranging from using the scattered electron to machine learning methods, each of which produce the same set of kinematic variables needed for physics analysis. Since the number of variables is large, a multi-dimensionally binned analysis is also often employed. We thus developed adage, a novel graph-based data structure that not only associates data to their bins, but also stores and can execute user-specified algorithms on any lower dimensional subsets. This approach allows the analyzer to write analysis algorithms that are fully independent of the binning strategy, expediting the exploration of the high dimensional phase space. Finally, as part of the EPIC software stack, epic-analysis continuous integration tests can be triggered by upstream changes in the simulation or reconstruction. For example, this automation allows for the physics impact on a detector design change to be quickly assessed, completing the full feedback loop for EIC detector design.

        Speaker: Dilks, Christopher (Duke University)
      • 3:15 PM
        Laurelin: A ROOT I/O implementation for Apache Spark 15m

        Apache Spark is a distributed computing framework which can process very large datasets using large clusters of servers. Laurelin is a Java-based implementation of ROOT I/O which allows Spark to read and write ROOT files from common HEP storage systems without a dependency on the C++ implementation of ROOT. We discuss improvements due to the migration to an Arrow-based in-memory representation as well as detail the performance difference for analyses over data stored in either ROOT or the Parquet format.

        Speaker: Melo, Andrew (Vanderbilt University)
    • 2:00 PM 3:30 PM
      Track 7 - Facilities and Virtualization: Computing Centre Infrastructure and Cloud Marriott Ballroom IV

      Marriott Ballroom IV

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Weitzel, Derek (University of Nebraska-Lincoln) , Wiebalck, Arne (CERN)
      • 2:00 PM
        HEPscore: a new benchmark for WLCG compute resources 15m

        HEPscore is a CPU benchmark, based on HEP applications, that the HEPiX Working Group is proposing as a replacement of the HEPSpec06 benchmark (HS06), which is currently used by the WLCG for procurement, computing resource requests and pledges, accounting and performance studies. At the CHEP 2019 conference, we presented the reasons for building a benchmark for the HEP community that is based on HEP applications instead of standard industrial benchmarks. In this contribution we describe the mix of HEP workloads selected to build HEPscore. We present the results of the 2022 campaign of measurements that studied the performance of eleven HEP applications on more than 70 unique computer systems on multiple WLCG sites. We provide an update on the current status of a HEPScore candidate and its deployment plans for 2023. We also discuss how HEPscore can be used to assess the power efficiency of different CPU architectures.

        Speaker: Dr Sobie, Randall (University of Victoria)
      • 2:15 PM
        Using CRIU for checkpointing batch jobs 15m

        Creating new materials, discovering new drugs, and simulating systems are essential processes for research and innovation, and require substantial computational power. While many applications can be split into many smaller independent tasks, some cannot and may take hours or weeks to run to completion. To better manage those longer-running jobs, it would be desirable to stop them at any arbitrary point in time and later continue their computation on another compute resource; this is usually referred to as checkpointing. While some applications can manage checkpointing in a programmatic way, it would be preferable if the batch scheduling system could do that independently. In this paper, we evaluate the feasibility of using CRIU (Checkpoint Restore in Userspace), an open-source tool available for the GNU/Linux environment, with an emphasis on the OSG’s OSPool HTCondor setup. CRIU allows for checkpointing of the process state into a disk image, and is able to seamlessly deal with both open files and established network connections. Furthermore, it can be used for checkpointing of both traditional Linux processes and containerized workloads. The functionality seems adequate for many scenarios supported in the OSPool. although there are some limitations that prevent it from being usable in all circumstances.

        Speaker: Andrijauskas, Fabio
      • 2:30 PM
        Preparing for a new Data Center: Automated Management of a 10’000 node bare-metal fleet in CERN IT 15m

        CERN IT has consolidated all life-cycle management of its physical server fleet on the Ironic bare-metal API. From the initial registration upon the first boot, over the inventory checking, the burn-in and the benchmarking for acceptance, the provisioning to the end users and the repairs during its service, up to the retirement at the end of the servers’ life, all stages can be managed within this framework. In this presentation we will follow a server throughout its life in the CERN data center, and explain how this enables us to handle a fleet of 10’000 nodes in an automated and efficient way and to prepare for the new data centre which is currently being built. We will add the top challenges we faced when moving to this system, like the transparent adoption of already in-production nodes or after-the-fact inventory updates, and eventually round things up with our “GRUBsetta stone”, a collection of boot errors and what they really mean.

        Speaker: Dr Wiebalck, Arne (CERN)
      • 2:45 PM
        A grid site reimagined: building a fully cloud-native ATLAS T2 on Kubernetes 15m

        The University of Victoria (UVic) operates an Infrastructure-as-a-Service science cloud for Canadian researchers, and a WLCG T2 grid site for the ATLAS experiment at CERN. At first, these were two distinctly separate systems, but over time we have taken steps to migrate the T2 grid services to the cloud. This process has been significantly facilitated by basing our approach on Kubernetes, a versatile, robust, and very widely-adopted automation platform for orchestrating and managing containerized applications. Previous work exploited the batch capabilities of Kubernetes to run the computing jobs of the UVic ATLAS T2, and replace the conventional grid Computing Elements, by interfacing with the Harvester workload management system of the ATLAS experiment. However, the required functionality of a T2 site encompasses more than just batch computing. Likewise, the capabilities of Kubernetes extend far beyond running batch jobs, and include for example scheduling recurring tasks and hosting long-running externally-accessible services in a resilient way. We are now undertaking the more complex and challenging endeavour of adapting and migrating all remaining functions of the T2 site - such as APEL accounting and Squid caching proxies, but in particular the grid Storage Element - to cloud-native deployments on Kubernetes. We aim to enable fully comprehensive deployment of a complete ATLAS T2 site on a Kubernetes cluster via Helm charts, which will benefit the community by providing a streamlined and replicable way to install and configure an ATLAS site. We also describe our experience running a high-performance self-managed Kubernetes ATLAS T2 cluster at the scale of 8,000 CPU cores for the last 2 years, and compare with the conventional setup of grid services.

        Speaker: Taylor, Ryan Paul (University of Victoria)
      • 3:00 PM
        Accelerating science: the usage of commercial clouds in ATLAS distributed computing 15m

        The ATLAS experiment at CERN is one of the largest scientific machines built to date and will have ever growing computing needs as the Large Hadron Collider collects an increasingly larger volume of data over the next 20 years. ATLAS is conducting R&D projects on Amazon and Google clouds as complementary resources for distributed computing, focusing on some of the key features of commercial clouds: lightweight operation, elasticity and availability of multiple chip architectures.

        The proof of concept phases have concluded with the cloud-native, vendor-agnostic integration with the experiment’s data and workload management frameworks. Google has been used to evaluate elastic batch computing, ramping up ephemeral clusters of up to O(100k) cores to process tasks requiring quick turnaround. Amazon cloud has been exploited for the successful physics validation of the Athena simulation software on ARM processors.
        We have also set up an interactive facility for physics analysis allowing end-users to spin up private, on-demand clusters for parallel computing with up to 4000 cores, or run GPU enabled notebooks and jobs for machine learning applications.

        The success of the proof of concept phases has led to the extension of the Google cloud project, where ATLAS will study the total cost of ownership of a production cloud site during 15 months with 10k cores on average, fully integrated with distributed grid computing resources and continue the R&D projects.

        Speaker: Megino, Fernando Harald Barreiro (The University of Texas at Arlington)
      • 3:15 PM
        Financial Case Study on the Use of Cloud Resources in HEP Computing 15m

        An all-inclusive analysis of costs for on-premises and public cloud-based solutions to handle the bulk of HEP computing requirements shows that dedicated on-premises deployments are still the most cost-effective. Since the advent of public cloud services, the HEP community has engaged in multiple proofs of concept to study the technical viability of using cloud resources; however, the financial viability of using cloud resources for HEP computing and storage is of greater importance. We present the results of a study comparing the cost of providing computing resources ina public cloud and a comprehensive estimate for the cost of an on-premises solution for HEP computing. Like previous studies, the fundamental conclusion is that for the bulk of HEP computing needs, on premises is significantly more cost effective than public clouds.

        Speakers: Misawa, Shigeki (Brookhaven National Laboratory) , LAURET, Jerome (Brookhaven Science Associates)
    • 2:00 PM 3:30 PM
      Track 8 - Collaboration, Reinterpretation, Outreach and Education: Open Data and Open Science Marriott Ballroom I

      Marriott Ballroom I

      Norfolk Waterside Marriott

      235 East Main Street Norfolk, VA 23510
      Conveners: Gazzarrini, Elena (CERN) , Lange, Clemens (Paul Scherrer Institut)
      • 2:00 PM
        MicroBooNE Public Data Sets: a Collaborative Tool for LArTPC Software Development 15m

        Among liquid argon time projection chamber (LArTPC) experiments MicroBooNE is the one that continually took physics data for the longest time (2015-2021), and represents the state of the art for reconstruction and analysis with this detector. Recently published analyses include oscillation physics results, searches for anomalies and other BSM signatures, and cross section measurements. LArTPC detectors are being used in current experiments such as ICARUS and SBND, and being planned for future experiments such as DUNE.

        MicroBooNE has recently released to the public two of its data sets, with the goal of enabling collaborative software developments with other LArTPC experiments and with AI or computing experts. These datasets simulate neutrino interactions on top of off-beam data, which include cosmic ray background and noise. The datasets are released in two formats: the native artroot format used internally by the collaboration and familiar to other LArTPC experts, and the HDF5 format which contains reduced and simplified content and is suitable for usage by the broader community.

        This contribution presents the open data sets, discusses their motivation, the technical implementation, and the extensive documentation - all inspired by FAIR principles. Finally, opportunities for collaborations are discussed.

        Speaker: Cerati, Giuseppe (Fermilab)
      • 2:15 PM
        ATLAS Open Data: developing education and outreach resources from research data 15m

        The ATLAS Open Data project aims to deliver open-access resources for education and outreach in High Energy Physics using real data recorded by the ATLAS detector. The Open Data release so far has resulted in the release of a substantial amount of data from 8 TeV and 13 TeV collisions in an easily-accessible format and supported by dedicated software and documentation to allow its fruitful use by users at a range of experience levels. To maximise the value of the data, software, and documentation resources provided ATLAS has developed initiatives and promotes stakeholder engagement in the creation of these materials through on-site and remote training schemes such as high-school work experience and summer schools programs, university projects and PhDs qualification tasks. We present examples of how multiple training programs inside and outside CERN have helped and continue to help development the ATLAS Open Data project, lessons learnt, impacts, and future goals.

        Speaker: Krasznahorkay, Attila (CERN)
      • 2:30 PM
        BaBar’s Experience with the Preservation of Data and Analysis Capabilities 15m

        The BaBar experiment collected electron-positron collisions at the SLAC National Accelerator Laboratory from 1999-2008. Although data taking has stopped 15 years ago, the collaboration is still actively doing data analyses, publishing results, and giving presentations at international conferences. Special considerations were needed to do analyses using a computing environment that was developed more than a decade ago. A framework is required that preserves the data, data access, and the capability of doing analyses using a well defined and preserved environment. Also, BaBar’s support by SLAC National Accelerator Laboratory, the place where the experiment took place, ended at the beginning of 2021. Fortunately, the HEP Research Computing group at the University of Victoria (UVic), Canada, offered to be the new home for the main BaBar computing infrastructure, GridKa offered to host all data for access by analyses running at UVic, and CERN and IN2P3 offered to store a backup of all data. In this talk, we will present what was done at BaBar to preserve the data and analysis capabilities and needed to move the whole computing infrastructure, including collaboration tools and data files, away from the SLAC National Accelerator Laboratory. It will be shown how BaBar preserved the ability to continue to do data analyses and also have a working collaboration tools infrastructure. The talk will detail what was needed to move the different bits of an experiment’s computing infrastructure to a new home, access the data from a different location, and how to move to more modern systems where older infrastructure could not be used anymore. The talk will be focused on BaBar’s experience with such a big change in its infrastructure and what was learned from it, which may be useful to other experiments which are interested in long term analysis support and data preservation in general.

        Speaker: Ebert, Marcus (University of Victoria)
      • 2:45 PM
        Automatising open data publishing workflows: experience with CMS open data curation 15m

        In this paper we discuss the CMS open data publishing workflows, summarising experience with eight releases of CMS open data on the CERN Open Data portal since its initial launch in 2014. We present the recent enhancements of data curation procedures, including (i) mining information about collision and simulated datasets with accompanying generation parameters and processing configuration files, (ii) building an API service covering information related to luminosity, run number ranges and other contextual dataset information, as well as (iii) configuring the CERN Open Data storage area as a Rucio endpoint that manages over four petabytes of released CMS open data and serves as a WLCG Tier 3 site to simplify data transfers. Finally, we discuss the latest CMS content released as open data (completed Run 1 data, first samples from Run 2 data) and the associated runnable analysis examples demonstrating its use in containerised data analysis workflows. We conclude by a short list of lessons learnt as well as general recommendations to facilitate upcoming releases of Run 2 data.

        Speaker: Dr Simko, Tibor (CERN)
      • 3:00 PM
        An Ntuple production service for accessing LHCb Open Data: the Ntuple Wizard 15m

        Making the large datasets collected at the LHC accessible to the public is a considerable challenge given the complexity and volume of data. Yet to harness the full scientific potential of the facility, it is essential to enable meaningful access to the data by the broadest physics community possible. Here we present an application, the LHCb Ntuple Wizard, which lev