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class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2023.168449">10.1016/j.nima.2023.168449 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Machine Learning based tool for CMS RPC currents quality monitoring </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Shumka%2C+E">E. Shumka</a>, <a href="/search/physics?searchtype=author&amp;query=Samalan%2C+A">A. Samalan</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Sawy%2C+M+E">M. El Sawy</a>, <a href="/search/physics?searchtype=author&amp;query=Alves%2C+G+A">G. A. Alves</a>, <a href="/search/physics?searchtype=author&amp;query=Marujo%2C+F">F. Marujo</a>, <a href="/search/physics?searchtype=author&amp;query=Coelho%2C+E+A">E. A. Coelho</a>, <a href="/search/physics?searchtype=author&amp;query=Da+Costa%2C+E+M">E. M. Da Costa</a>, <a href="/search/physics?searchtype=author&amp;query=Nogima%2C+H">H. Nogima</a>, <a href="/search/physics?searchtype=author&amp;query=Santoro%2C+A">A. Santoro</a>, <a href="/search/physics?searchtype=author&amp;query=De+Souza%2C+S+F">S. Fonseca De Souza</a>, <a href="/search/physics?searchtype=author&amp;query=Damiao%2C+D+D+J">D. De Jesus Damiao</a>, <a href="/search/physics?searchtype=author&amp;query=Thiel%2C+M">M. Thiel</a>, <a href="/search/physics?searchtype=author&amp;query=Amarilo%2C+K+M">K. Mota Amarilo</a>, <a href="/search/physics?searchtype=author&amp;query=Filho%2C+M+B+F">M. Barroso Ferreira Filho</a>, <a href="/search/physics?searchtype=author&amp;query=Aleksandrov%2C+A">A. Aleksandrov</a>, <a href="/search/physics?searchtype=author&amp;query=Hadjiiska%2C+R">R. Hadjiiska</a>, <a href="/search/physics?searchtype=author&amp;query=Iaydjiev%2C+P">P. Iaydjiev</a>, <a href="/search/physics?searchtype=author&amp;query=Rodozov%2C+M">M. Rodozov</a>, <a href="/search/physics?searchtype=author&amp;query=Shopova%2C+M">M. Shopova</a>, <a href="/search/physics?searchtype=author&amp;query=Soultanov%2C+G">G. Soultanov</a>, <a href="/search/physics?searchtype=author&amp;query=Dimitrov%2C+A">A. Dimitrov</a>, <a href="/search/physics?searchtype=author&amp;query=Litov%2C+L">L. Litov</a>, <a href="/search/physics?searchtype=author&amp;query=Pavlov%2C+B">B. Pavlov</a>, <a href="/search/physics?searchtype=author&amp;query=Petkov%2C+P">P. Petkov</a> , et al. (83 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2302.02764v1-abstract-short" style="display: inline;"> The muon system of the CERN Compact Muon Solenoid (CMS) experiment includes more than a thousand Resistive Plate Chambers (RPC). They are gaseous detectors operated in the hostile environment of the CMS underground cavern on the Large Hadron Collider where pp luminosities of up to $2\times 10^{34}$ $\text{cm}^{-2}\text{s}^{-1}$ are routinely achieved. The CMS RPC system performance is constantly m&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.02764v1-abstract-full').style.display = 'inline'; document.getElementById('2302.02764v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2302.02764v1-abstract-full" style="display: none;"> The muon system of the CERN Compact Muon Solenoid (CMS) experiment includes more than a thousand Resistive Plate Chambers (RPC). They are gaseous detectors operated in the hostile environment of the CMS underground cavern on the Large Hadron Collider where pp luminosities of up to $2\times 10^{34}$ $\text{cm}^{-2}\text{s}^{-1}$ are routinely achieved. The CMS RPC system performance is constantly monitored and the detector is regularly maintained to ensure stable operation. The main monitorable characteristics are dark current, efficiency for muon detection, noise rate etc. Herein we describe an automated tool for CMS RPC current monitoring which uses Machine Learning techniques. We further elaborate on the dedicated generalized linear model proposed already and add autoencoder models for self-consistent predictions as well as hybrid models to allow for RPC current predictions in a distant future. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.02764v1-abstract-full').style.display = 'none'; document.getElementById('2302.02764v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 February, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2211.16591">arXiv:2211.16591</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2211.16591">pdf</a>, <a href="https://arxiv.org/format/2211.16591">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2023.168271">10.1016/j.nima.2023.168271 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> RPC based tracking system at CERN GIF++ facility </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Amarilo%2C+K+M">K. Mota Amarilo</a>, <a href="/search/physics?searchtype=author&amp;query=Samalan%2C+A">A. Samalan</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Sawy%2C+M+E">M. El Sawy</a>, <a href="/search/physics?searchtype=author&amp;query=Alves%2C+G+A">G. A. Alves</a>, <a href="/search/physics?searchtype=author&amp;query=Marujo%2C+F">F. Marujo</a>, <a href="/search/physics?searchtype=author&amp;query=Coelho%2C+E+A">E. A. Coelho</a>, <a href="/search/physics?searchtype=author&amp;query=Da+Costa%2C+E+M">E. M. Da Costa</a>, <a href="/search/physics?searchtype=author&amp;query=Nogima%2C+H">H. Nogima</a>, <a href="/search/physics?searchtype=author&amp;query=Santoro%2C+A">A. Santoro</a>, <a href="/search/physics?searchtype=author&amp;query=De+Souza%2C+S+F">S. Fonseca De Souza</a>, <a href="/search/physics?searchtype=author&amp;query=Damiao%2C+D+D+J">D. De Jesus Damiao</a>, <a href="/search/physics?searchtype=author&amp;query=Thiel%2C+M">M. Thiel</a>, <a href="/search/physics?searchtype=author&amp;query=Filho%2C+M+B+F">M. Barroso Ferreira Filho</a>, <a href="/search/physics?searchtype=author&amp;query=Aleksandrov%2C+A">A. Aleksandrov</a>, <a href="/search/physics?searchtype=author&amp;query=Hadjiiska%2C+R">R. Hadjiiska</a>, <a href="/search/physics?searchtype=author&amp;query=Iaydjiev%2C+P">P. Iaydjiev</a>, <a href="/search/physics?searchtype=author&amp;query=Rodozov%2C+M">M. Rodozov</a>, <a href="/search/physics?searchtype=author&amp;query=Shopova%2C+M">M. Shopova</a>, <a href="/search/physics?searchtype=author&amp;query=Soultanov%2C+G">G. Soultanov</a>, <a href="/search/physics?searchtype=author&amp;query=Dimitrov%2C+A">A. Dimitrov</a>, <a href="/search/physics?searchtype=author&amp;query=Litov%2C+L">L. Litov</a>, <a href="/search/physics?searchtype=author&amp;query=Pavlov%2C+B">B. Pavlov</a>, <a href="/search/physics?searchtype=author&amp;query=Petkov%2C+P">P. Petkov</a>, <a href="/search/physics?searchtype=author&amp;query=Petrov%2C+A">A. Petrov</a> , et al. (83 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2211.16591v1-abstract-short" style="display: inline;"> With the HL-LHC upgrade of the LHC machine, an increase of the instantaneous luminosity by a factor of five is expected and the current detection systems need to be validated for such working conditions to ensure stable data taking. At the CERN Gamma Irradiation Facility (GIF++) many muon detectors undergo such studies, but the high gamma background can pose a challenge to the muon trigger system&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2211.16591v1-abstract-full').style.display = 'inline'; document.getElementById('2211.16591v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2211.16591v1-abstract-full" style="display: none;"> With the HL-LHC upgrade of the LHC machine, an increase of the instantaneous luminosity by a factor of five is expected and the current detection systems need to be validated for such working conditions to ensure stable data taking. At the CERN Gamma Irradiation Facility (GIF++) many muon detectors undergo such studies, but the high gamma background can pose a challenge to the muon trigger system which is exposed to many fake hits from the gamma background. A tracking system using RPCs is implemented to clean the fake hits, taking profit of the high muon efficiency of these chambers. This work will present the tracking system configuration, used detector analysis algorithm and results. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2211.16591v1-abstract-full').style.display = 'none'; document.getElementById('2211.16591v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 November, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages, 9 figures. Contribution to XVI Workshop on Resistive Plate Chambers and Related Detectors (RPC2022), September 26-30 2022. Submitted to Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2207.06291">arXiv:2207.06291</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2207.06291">pdf</a>, <a href="https://arxiv.org/format/2207.06291">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/18/03/P03035">10.1088/1748-0221/18/03/P03035 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Description and stability of a RPC-based calorimeter in electromagnetic and hadronic shower environments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Boumediene%2C+D">D. Boumediene</a>, <a href="/search/physics?searchtype=author&amp;query=Francais%2C+V">V. Francais</a>, <a href="/search/physics?searchtype=author&amp;query=Apostolakis%2C+J">J. Apostolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Folger%2C+G">G. Folger</a>, <a href="/search/physics?searchtype=author&amp;query=Ribon%2C+A">A. Ribon</a>, <a href="/search/physics?searchtype=author&amp;query=Sicking%2C+E">E. Sicking</a>, <a href="/search/physics?searchtype=author&amp;query=Goto%2C+K">K. Goto</a>, <a href="/search/physics?searchtype=author&amp;query=Kawagoe%2C+K">K. Kawagoe</a>, <a href="/search/physics?searchtype=author&amp;query=Kuhara%2C+M">M. Kuhara</a>, <a href="/search/physics?searchtype=author&amp;query=Suehara%2C+T">T. Suehara</a>, <a href="/search/physics?searchtype=author&amp;query=Yoshioka%2C+T">T. Yoshioka</a>, <a href="/search/physics?searchtype=author&amp;query=Pingault%2C+A">A. Pingault</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Garillot%2C+G">G. Garillot</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Kurca%2C+T">T. Kurca</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Liu%2C+B">B. Liu</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+B">B. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Mirabito%2C+L">L. Mirabito</a>, <a href="/search/physics?searchtype=author&amp;query=Alamillo%2C+E+C">E. Calvo Alamillo</a>, <a href="/search/physics?searchtype=author&amp;query=Carrillo%2C+C">C. Carrillo</a>, <a href="/search/physics?searchtype=author&amp;query=Fouz%2C+M+C">M. C. Fouz</a>, <a href="/search/physics?searchtype=author&amp;query=Cabrera%2C+H+G">H. Garcia Cabrera</a>, <a href="/search/physics?searchtype=author&amp;query=Marin%2C+J">J. Marin</a> , et al. (14 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2207.06291v2-abstract-short" style="display: inline;"> The CALICE Semi-Digital Hadron Calorimeter technological prototype completed in 2011 is a sampling calorimeter using Glass Resistive Plate Chamber (GRPC) detectors as the active medium. This technology is one of the two options proposed for the hadron calorimeter of the International Large Detector for the International Linear Collider. The prototype was exposed in 2015 to beams of muons, electron&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2207.06291v2-abstract-full').style.display = 'inline'; document.getElementById('2207.06291v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2207.06291v2-abstract-full" style="display: none;"> The CALICE Semi-Digital Hadron Calorimeter technological prototype completed in 2011 is a sampling calorimeter using Glass Resistive Plate Chamber (GRPC) detectors as the active medium. This technology is one of the two options proposed for the hadron calorimeter of the International Large Detector for the International Linear Collider. The prototype was exposed in 2015 to beams of muons, electrons, and pions of different energies at the CERN Super Proton Synchrotron. The use of this technology for future experiments requires a reliable simulation of its response that can predict its performance. GEANT4 combined with a digitization algorithm was used to simulate the prototype. It describes the full path of the signal: showering, gas avalanches, charge induction, and hit triggering. The simulation was tuned using muon tracks and electromagnetic showers for accounting for detector inhomogeneity and tested on hadronic showers collected in the test beam. This publication describes developments of the digitization algorithm. It is used to predict the stability of the detector performance against various changes in the data-taking conditions, including temperature, pressure, magnetic field, GRPC width variations, and gas mixture variations. These predictions are confronted with test beam data and provide an attempt to explain the detector properties. The data-taking conditions such as temperature and potential detector inhomogeneities affect energy density measurements but have a small impact on detector efficiency. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2207.06291v2-abstract-full').style.display = 'none'; document.getElementById('2207.06291v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 March, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 July, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Version published in JINST</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CALICE-PUB-2022-02 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> 2023 JINST 18 P03035 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2203.07286">arXiv:2203.07286</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2203.07286">pdf</a>, <a href="https://arxiv.org/format/2203.07286">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Precision timing for collider-experiment-based calorimetry </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Chekanov%2C+S+V">S. V. Chekanov</a>, <a href="/search/physics?searchtype=author&amp;query=Simon%2C+F">F. Simon</a>, <a href="/search/physics?searchtype=author&amp;query=Boudry%2C+V">V. Boudry</a>, <a href="/search/physics?searchtype=author&amp;query=Chung%2C+W">W. Chung</a>, <a href="/search/physics?searchtype=author&amp;query=Gorham%2C+P+W">P. W. Gorham</a>, <a href="/search/physics?searchtype=author&amp;query=Nguyen%2C+M">M. Nguyen</a>, <a href="/search/physics?searchtype=author&amp;query=Tully%2C+C+G">C. G. Tully</a>, <a href="/search/physics?searchtype=author&amp;query=Eno%2C+S+C">S. C. Eno</a>, <a href="/search/physics?searchtype=author&amp;query=Lai%2C+Y">Y. Lai</a>, <a href="/search/physics?searchtype=author&amp;query=Kotwal%2C+A+V">A. V. Kotwal</a>, <a href="/search/physics?searchtype=author&amp;query=Ko%2C+S">S. Ko</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+S">S. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+J+S+H">J. S. H. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Lucchini%2C+M+T">M. T. Lucchini</a>, <a href="/search/physics?searchtype=author&amp;query=Prechelt%2C+R">R. Prechelt</a>, <a href="/search/physics?searchtype=author&amp;query=Yoo%2C+H">H. Yoo</a>, <a href="/search/physics?searchtype=author&amp;query=Yeh%2C+C+-">C. -H Yeh</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+S+-">S. -S. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Varner%2C+G+S">G. S. Varner</a>, <a href="/search/physics?searchtype=author&amp;query=Zhu%2C+R">R. Zhu</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2203.07286v1-abstract-short" style="display: inline;"> In this White Paper for the 2021 Snowmass process, we discuss aspects of precision timing within electromagnetic and hadronic calorimeter systems for high-energy physics collider experiments. Areas of applications include particle identification, event and object reconstruction, and pileup mitigation. Two different system options are considered, namely cell-level timing capabilities covering the f&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.07286v1-abstract-full').style.display = 'inline'; document.getElementById('2203.07286v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2203.07286v1-abstract-full" style="display: none;"> In this White Paper for the 2021 Snowmass process, we discuss aspects of precision timing within electromagnetic and hadronic calorimeter systems for high-energy physics collider experiments. Areas of applications include particle identification, event and object reconstruction, and pileup mitigation. Two different system options are considered, namely cell-level timing capabilities covering the full detector volume, and dedicated timing layers integrated in calorimeter systems. A selection of technologies for the different approaches is also discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.07286v1-abstract-full').style.display = 'none'; document.getElementById('2203.07286v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 March, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">22 pages, 9 figures, Editors: S. V. Chekanov, F. Simon. Submitted to the Proceedings of the US Community Study on the Future of Particle Physics (Snowmass 2021)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> ANL-HEP-173859, MPP-2022-28 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2202.09684">arXiv:2202.09684</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2202.09684">pdf</a>, <a href="https://arxiv.org/format/2202.09684">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> Energy reconstruction of hadronic showers at the CERN PS and SPS using the Semi-Digital Hadronic Calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Liu%2C+B">B. Liu</a>, <a href="/search/physics?searchtype=author&amp;query=Boumediene%2C+D">D. Boumediene</a>, <a href="/search/physics?searchtype=author&amp;query=Baek%2C+Y+W">Y. W. Baek</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+D">D-W. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+S+C">S. C. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Min%2C+B+G">B. G. Min</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+S+W">S. W. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Deguchi%2C+Y">Y. Deguchi</a>, <a href="/search/physics?searchtype=author&amp;query=Kawagoe%2C+K">K. Kawagoe</a>, <a href="/search/physics?searchtype=author&amp;query=Miura%2C+Y">Y. Miura</a>, <a href="/search/physics?searchtype=author&amp;query=Mori%2C+R">R. Mori</a>, <a href="/search/physics?searchtype=author&amp;query=Sekiya%2C+I">I. Sekiya</a>, <a href="/search/physics?searchtype=author&amp;query=Suehara%2C+T">T. Suehara</a>, <a href="/search/physics?searchtype=author&amp;query=Yoshioka%2C+T">T. Yoshioka</a>, <a href="/search/physics?searchtype=author&amp;query=Caponetto%2C+L">L. Caponetto</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Garillot%2C+G">G. Garillot</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Ianigro%2C+J">J-C. Ianigro</a>, <a href="/search/physics?searchtype=author&amp;query=Kurca%2C+T">T. Kurca</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Liu%2C+B">B. Liu</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+B">B. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Lumb%2C+N">N. Lumb</a> , et al. (53 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2202.09684v1-abstract-short" style="display: inline;"> The CALICE Semi-Digital Hadronic CALorimeter (SDHCAL) is the first technological prototype in a family of high-granularity calorimeters developed by the CALICE Collaboration to equip the experiments of future lepton colliders. The SDHCAL is a sampling calorimeter using stainless steel for absorber and Glass Resistive Plate Chambers (GRPC) as a sensitive medium. The GRPC are read out by 1~cm&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.09684v1-abstract-full').style.display = 'inline'; document.getElementById('2202.09684v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2202.09684v1-abstract-full" style="display: none;"> The CALICE Semi-Digital Hadronic CALorimeter (SDHCAL) is the first technological prototype in a family of high-granularity calorimeters developed by the CALICE Collaboration to equip the experiments of future lepton colliders. The SDHCAL is a sampling calorimeter using stainless steel for absorber and Glass Resistive Plate Chambers (GRPC) as a sensitive medium. The GRPC are read out by 1~cm $\times$ 1~cm pickup pads combined to a multi-threshold electronics. The prototype was exposed to hadron beams in both the CERN PS and the SPS beamlines in 2015 allowing the test of the SDHCAL in a large energy range from 3~GeV to 80~GeV. After introducing the method used to select the hadrons of our data and reject the muon and electron contamination, we present the energy reconstruction approach that we apply to the data collected from both beamlines and we discuss the response linearity and the energy resolution of the SDHCAL. The results obtained in the two beamlines confirm the excellent SDHCAL performance observed with the data collected with the same prototype in the SPS beamline in 2012. They also show the stability of the SDHCAL in different beam conditions and different time periods. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.09684v1-abstract-full').style.display = 'none'; document.getElementById('2202.09684v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 February, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">21 pages,23 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CALICE-PUB-2022-001 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2109.14331">arXiv:2109.14331</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2109.14331">pdf</a>, <a href="https://arxiv.org/format/2109.14331">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/17/01/C01011">10.1088/1748-0221/17/01/C01011 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Upgrade of the CMS Resistive Plate Chambers for the High Luminosity LHC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Samalan%2C+A">A. Samalan</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Alves%2C+G+A">G. A. Alves</a>, <a href="/search/physics?searchtype=author&amp;query=Marujo%2C+F">F. Marujo</a>, <a href="/search/physics?searchtype=author&amp;query=De+Araujo%2C+F+T+D+S">F. Torres Da Silva De Araujo</a>, <a href="/search/physics?searchtype=author&amp;query=DaCosta%2C+E+M">E. M. DaCosta</a>, <a href="/search/physics?searchtype=author&amp;query=Damiao%2C+D+D+J">D. De Jesus Damiao</a>, <a href="/search/physics?searchtype=author&amp;query=Nogima%2C+H">H. Nogima</a>, <a href="/search/physics?searchtype=author&amp;query=Santoro%2C+A">A. Santoro</a>, <a href="/search/physics?searchtype=author&amp;query=De+Souza%2C+S+F">S. Fonseca De Souza</a>, <a href="/search/physics?searchtype=author&amp;query=Aleksandrov%2C+A">A. Aleksandrov</a>, <a href="/search/physics?searchtype=author&amp;query=Hadjiiska%2C+R">R. Hadjiiska</a>, <a href="/search/physics?searchtype=author&amp;query=Iaydjiev%2C+P">P. Iaydjiev</a>, <a href="/search/physics?searchtype=author&amp;query=Rodozov%2C+M">M. Rodozov</a>, <a href="/search/physics?searchtype=author&amp;query=Shopova%2C+M">M. Shopova</a>, <a href="/search/physics?searchtype=author&amp;query=Soultanov%2C+G">G. Soultanov</a>, <a href="/search/physics?searchtype=author&amp;query=Bonchev%2C+M">M. Bonchev</a>, <a href="/search/physics?searchtype=author&amp;query=Dimitrov%2C+A">A. Dimitrov</a>, <a href="/search/physics?searchtype=author&amp;query=Litov%2C+L">L. Litov</a>, <a href="/search/physics?searchtype=author&amp;query=Pavlov%2C+B">B. Pavlov</a>, <a href="/search/physics?searchtype=author&amp;query=Petkov%2C+P">P. Petkov</a>, <a href="/search/physics?searchtype=author&amp;query=Petrov%2C+A">A. Petrov</a>, <a href="/search/physics?searchtype=author&amp;query=Qian%2C+S+J">S. J. Qian</a>, <a href="/search/physics?searchtype=author&amp;query=Bernal%2C+C">C. Bernal</a>, <a href="/search/physics?searchtype=author&amp;query=Cabrera%2C+A">A. Cabrera</a> , et al. (86 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2109.14331v2-abstract-short" style="display: inline;"> During the upcoming High Luminosity phase of the Large Hadron Collider (HL-LHC), the integrated luminosity of the accelerator will increase to 3000 fb$^{-1}$. The expected experimental conditions in that period in terms of background rates, event pileup, and the probable aging of the current detectors present a challenge for all the existing experiments at the LHC, including the Compact Muon Solen&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2109.14331v2-abstract-full').style.display = 'inline'; document.getElementById('2109.14331v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2109.14331v2-abstract-full" style="display: none;"> During the upcoming High Luminosity phase of the Large Hadron Collider (HL-LHC), the integrated luminosity of the accelerator will increase to 3000 fb$^{-1}$. The expected experimental conditions in that period in terms of background rates, event pileup, and the probable aging of the current detectors present a challenge for all the existing experiments at the LHC, including the Compact Muon Solenoid (CMS) experiment. To ensure a highly performing muon system for this period, several upgrades of the Resistive Plate Chamber (RPC) system of the CMS are currently being implemented. These include the replacement of the readout system for the present system, and the installation of two new RPC stations with improved chamber and front-end electronics designs. The current overall status of this CMS RPC upgrade project is presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2109.14331v2-abstract-full').style.display = 'none'; document.getElementById('2109.14331v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 November, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 September, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2021. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2005.12769">arXiv:2005.12769</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2005.12769">pdf</a>, <a href="https://arxiv.org/format/2005.12769">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> CMS RPC Background -- Studies and Measurements </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Hadjiiska%2C+R">R. Hadjiiska</a>, <a href="/search/physics?searchtype=author&amp;query=Samalan%2C+A">A. Samalan</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Zaganidis%2C+N">N. Zaganidis</a>, <a href="/search/physics?searchtype=author&amp;query=Alves%2C+G+A">G. A. Alves</a>, <a href="/search/physics?searchtype=author&amp;query=Marujo%2C+F">F. Marujo</a>, <a href="/search/physics?searchtype=author&amp;query=De+Araujo%2C+F+T+D+S">F. Torres Da Silva De Araujo</a>, <a href="/search/physics?searchtype=author&amp;query=Da+Costa%2C+E+M">E. M. Da Costa</a>, <a href="/search/physics?searchtype=author&amp;query=Damiao%2C+D+D+J">D. De Jesus Damiao</a>, <a href="/search/physics?searchtype=author&amp;query=Nogima%2C+H">H. Nogima</a>, <a href="/search/physics?searchtype=author&amp;query=Santoro%2C+A">A. Santoro</a>, <a href="/search/physics?searchtype=author&amp;query=De+Souza%2C+S+F">S. Fonseca De Souza</a>, <a href="/search/physics?searchtype=author&amp;query=Aleksandrov%2C+A">A. Aleksandrov</a>, <a href="/search/physics?searchtype=author&amp;query=Iaydjiev%2C+P">P. Iaydjiev</a>, <a href="/search/physics?searchtype=author&amp;query=Rodozov%2C+M">M. Rodozov</a>, <a href="/search/physics?searchtype=author&amp;query=Shopova%2C+M">M. Shopova</a>, <a href="/search/physics?searchtype=author&amp;query=Sultanov%2C+G">G. Sultanov</a>, <a href="/search/physics?searchtype=author&amp;query=Bonchev%2C+M">M. Bonchev</a>, <a href="/search/physics?searchtype=author&amp;query=Dimitrov%2C+A">A. Dimitrov</a>, <a href="/search/physics?searchtype=author&amp;query=Litov%2C+L">L. Litov</a>, <a href="/search/physics?searchtype=author&amp;query=Pavlov%2C+B">B. Pavlov</a>, <a href="/search/physics?searchtype=author&amp;query=Petkov%2C+P">P. Petkov</a>, <a href="/search/physics?searchtype=author&amp;query=Petrov%2C+A">A. Petrov</a>, <a href="/search/physics?searchtype=author&amp;query=Qian%2C+S+J">S. J. Qian</a>, <a href="/search/physics?searchtype=author&amp;query=Bernal%2C+C">C. Bernal</a> , et al. (84 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2005.12769v2-abstract-short" style="display: inline;"> The expected radiation background in the CMS RPC system has been studied using the MC prediction with the CMS FLUKA simulation of the detector and the cavern. The MC geometry used in the analysis describes very accurately the present RPC system but still does not include the complete description of the RPC upgrade region with pseudorapidity $1.9 &lt; \lvert 畏\rvert &lt; 2.4$. Present results will be upd&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2005.12769v2-abstract-full').style.display = 'inline'; document.getElementById('2005.12769v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2005.12769v2-abstract-full" style="display: none;"> The expected radiation background in the CMS RPC system has been studied using the MC prediction with the CMS FLUKA simulation of the detector and the cavern. The MC geometry used in the analysis describes very accurately the present RPC system but still does not include the complete description of the RPC upgrade region with pseudorapidity $1.9 &lt; \lvert 畏\rvert &lt; 2.4$. Present results will be updated with the final geometry description, once it is available. The radiation background has been studied in terms of expected particle rates, absorbed dose and fluence. Two High Luminosity LHC (HL-LHC) scenarios have been investigated - after collecting $3000$ and $4000$ fb$^{-1}$. Estimations with safety factor of 3 have been considered, as well. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2005.12769v2-abstract-full').style.display = 'none'; document.getElementById('2005.12769v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 May, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, Conference proceeding for the 2020 Resistive Plate Chambers and Related Detectors. Minor revision of the report, the results remain unchanged. Three new plots are added and some details were explained better</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2004.02972">arXiv:2004.02972</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2004.02972">pdf</a>, <a href="https://arxiv.org/format/2004.02972">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/15/10/P10009">10.1088/1748-0221/15/10/P10009 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Particle Identification Using Boosted Decision Trees in the Semi-Digital Hadronic Calorimeter Prototype </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Boumediene%2C+D">D. Boumediene</a>, <a href="/search/physics?searchtype=author&amp;query=Pingault%2C+A">A. Pingault</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Bilki%2C+B">B. Bilki</a>, <a href="/search/physics?searchtype=author&amp;query=Northacker%2C+D">D. Northacker</a>, <a href="/search/physics?searchtype=author&amp;query=Onel%2C+Y">Y. Onel</a>, <a href="/search/physics?searchtype=author&amp;query=Cho%2C+G">G. Cho</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+D">D-W. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+S+C">S. C. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+W">W. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Vallecorsa%2C+S">S. Vallecorsa</a>, <a href="/search/physics?searchtype=author&amp;query=Deguchi%2C+Y">Y. Deguchi</a>, <a href="/search/physics?searchtype=author&amp;query=Kawagoe%2C+K">K. Kawagoe</a>, <a href="/search/physics?searchtype=author&amp;query=Miura%2C+Y">Y. Miura</a>, <a href="/search/physics?searchtype=author&amp;query=Mori%2C+R">R. Mori</a>, <a href="/search/physics?searchtype=author&amp;query=Sekiya%2C+I">I. Sekiya</a>, <a href="/search/physics?searchtype=author&amp;query=Suehara%2C+T">T. Suehara</a>, <a href="/search/physics?searchtype=author&amp;query=Yoshioka%2C+T">T. Yoshioka</a>, <a href="/search/physics?searchtype=author&amp;query=Caponetto%2C+L">L. Caponetto</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Garillot%2C+R+E+G">R. Ete G. Garillot</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Ianigro%2C+J">J-C. Ianigro</a>, <a href="/search/physics?searchtype=author&amp;query=Kurca%2C+T">T. Kurca</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a> , et al. (65 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2004.02972v1-abstract-short" style="display: inline;"> The CALICE Semi-Digital Hadronic CALorimeter (SDHCAL) prototype using Glass Resistive Plate Chambers as a sensitive medium is the first technological prototype of a family of high-granularity calorimeters developed by the CALICE collaboration to equip the experiments of future leptonic colliders. It was exposed to beams of hadrons, electrons and muons several times in the CERN PS and SPS beamlines&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2004.02972v1-abstract-full').style.display = 'inline'; document.getElementById('2004.02972v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2004.02972v1-abstract-full" style="display: none;"> The CALICE Semi-Digital Hadronic CALorimeter (SDHCAL) prototype using Glass Resistive Plate Chambers as a sensitive medium is the first technological prototype of a family of high-granularity calorimeters developed by the CALICE collaboration to equip the experiments of future leptonic colliders. It was exposed to beams of hadrons, electrons and muons several times in the CERN PS and SPS beamlines between 2012 and 2018. We present here a new method of particle identification within the SDHCAL using the Boosted Decision Trees (BDT) method applied to the data collected in 2015. The performance of the method is tested first with Geant4-based simulated events and then on the data collected by the SDHCAL in the energy range between 10 and 80~GeV with 10~GeV energy steps. The BDT method is then used to reject the electrons and muons that contaminate the SPS hadron beams. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2004.02972v1-abstract-full').style.display = 'none'; document.getElementById('2004.02972v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 April, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CALICE-PUB-2020-001 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2002.09678">arXiv:2002.09678</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2002.09678">pdf</a>, <a href="https://arxiv.org/format/2002.09678">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/15/05/C05016">10.1088/1748-0221/15/05/C05016 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> APRIL : a novel Algorithm for Particle Reconstruction at ILC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Li%2C+B">B. Li</a>, <a href="/search/physics?searchtype=author&amp;query=%C3%89t%C3%A9%2C+R">R. 脡t茅</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2002.09678v2-abstract-short" style="display: inline;"> The current developments for future electron-positron colliders are driven by the Particle Flow concept. In these developments, high granularity calorimeters play a central role. This presentation will focus on a new Particle Flow Algorithm (PFA) developed for high granularity calorimeters, and especially for the Semi-Digital Hadronic CALorimeter (SDHCAL) option of the International Large Detector&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2002.09678v2-abstract-full').style.display = 'inline'; document.getElementById('2002.09678v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2002.09678v2-abstract-full" style="display: none;"> The current developments for future electron-positron colliders are driven by the Particle Flow concept. In these developments, high granularity calorimeters play a central role. This presentation will focus on a new Particle Flow Algorithm (PFA) developed for high granularity calorimeters, and especially for the Semi-Digital Hadronic CALorimeter (SDHCAL) option of the International Large Detector (ILD) project. The first PFA for ILD was PandoraPFA. This new PFA (APRIL) is based on the PandoraPFA Software Development Kit, but implements a different clustering inspired from the ARBOR PFA approach. This proceeding will describe briefly the APRIL algorithm and discuss its performance against that of PandoraPFA. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2002.09678v2-abstract-full').style.display = 'none'; document.getElementById('2002.09678v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 March, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 22 February, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 5 figures, proceeding for third conference on Calorimetry for the High Energy Frontier (CHEF), November 25-29, 2019, Kyushu University, Fukuoka, Japan</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1807.05680">arXiv:1807.05680</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1807.05680">pdf</a>, <a href="https://arxiv.org/format/1807.05680">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/14/10/C10037">10.1088/1748-0221/14/10/C10037 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> High Rate RPC detector for LHC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Lagarde%2C+F">F. Lagarde</a>, <a href="/search/physics?searchtype=author&amp;query=Fagot%2C+A">A. Fagot</a>, <a href="/search/physics?searchtype=author&amp;query=Gul%2C+M">M. Gul</a>, <a href="/search/physics?searchtype=author&amp;query=Roskas%2C+C">C. Roskas</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Zaganidis%2C+N">N. Zaganidis</a>, <a href="/search/physics?searchtype=author&amp;query=De+Souza%2C+S+F">S. Fonseca De Souza</a>, <a href="/search/physics?searchtype=author&amp;query=Santoro%2C+A">A. Santoro</a>, <a href="/search/physics?searchtype=author&amp;query=De+Araujo%2C+F+T+D+S">F. Torres Da Silva De Araujo</a>, <a href="/search/physics?searchtype=author&amp;query=Aleksandrov%2C+A">A. Aleksandrov</a>, <a href="/search/physics?searchtype=author&amp;query=Hadjiiska%2C+R">R. Hadjiiska</a>, <a href="/search/physics?searchtype=author&amp;query=Iaydjiev%2C+P">P. Iaydjiev</a>, <a href="/search/physics?searchtype=author&amp;query=Rodozov%2C+M">M. Rodozov</a>, <a href="/search/physics?searchtype=author&amp;query=Shopova%2C+M">M. Shopova</a>, <a href="/search/physics?searchtype=author&amp;query=Sultanov%2C+G">G. Sultanov</a>, <a href="/search/physics?searchtype=author&amp;query=Dimitrov%2C+A">A. Dimitrov</a>, <a href="/search/physics?searchtype=author&amp;query=Litov%2C+L">L. Litov</a>, <a href="/search/physics?searchtype=author&amp;query=Pavlov%2C+B">B. Pavlov</a>, <a href="/search/physics?searchtype=author&amp;query=Petkov%2C+P">P. Petkov</a>, <a href="/search/physics?searchtype=author&amp;query=Petrov%2C+A">A. Petrov</a>, <a href="/search/physics?searchtype=author&amp;query=Qian%2C+S+J">S. J. Qian</a>, <a href="/search/physics?searchtype=author&amp;query=Han%2C+D">D. Han</a>, <a href="/search/physics?searchtype=author&amp;query=Yi%2C+W">W. Yi</a>, <a href="/search/physics?searchtype=author&amp;query=Avila%2C+C">C. Avila</a>, <a href="/search/physics?searchtype=author&amp;query=Cabrera%2C+A">A. Cabrera</a> , et al. (77 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1807.05680v1-abstract-short" style="display: inline;"> The High Luminosity LHC (HL-LHC) phase is designed to increase by an order of magnitude the amount of data to be collected by the LHC experiments. The foreseen gradual increase of the instantaneous luminosity of up to more than twice its nominal value of $10\times10^{34}\ {\rm cm}^{-1}{\rm s}^{-2}$ during Phase I and Phase II of the LHC running, presents special challenges for the experiments. The&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.05680v1-abstract-full').style.display = 'inline'; document.getElementById('1807.05680v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.05680v1-abstract-full" style="display: none;"> The High Luminosity LHC (HL-LHC) phase is designed to increase by an order of magnitude the amount of data to be collected by the LHC experiments. The foreseen gradual increase of the instantaneous luminosity of up to more than twice its nominal value of $10\times10^{34}\ {\rm cm}^{-1}{\rm s}^{-2}$ during Phase I and Phase II of the LHC running, presents special challenges for the experiments. The region with high pseudo rapidity ($畏$) region of the forward muon spectrometer ($2.4 &gt; |畏| &gt; 1.9$) is not equipped with RPC stations. The increase of the expected particles rate up to 2 kHz cm$^{-1}$ ( including a safety factor 3 ) motivates the installation of RPC chambers to guarantee redundancy with the CSC chambers already present. The current CMS RPC technology cannot sustain the expected background level. A new generation of Glass-RPC (GRPC) using low-resistivity glass was proposed to equip the two most far away of the four high $畏$ muon stations of CMS. In their single-gap version they can stand rates of few kHz cm$^{-1}$. Their time precision of about 1 ns can allow to reduce the noise contribution leading to an improvement of the trigger rate. The proposed design for large size chambers is examined and some preliminary results obtained during beam tests at Gamma Irradiation Facility (GIF++) and Super Proton Synchrotron (SPS) at CERN are shown. They were performed to validate the capability of such detectors to support high irradiation environment with limited consequence on their efficiency. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.05680v1-abstract-full').style.display = 'none'; document.getElementById('1807.05680v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1606.04291">arXiv:1606.04291</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1606.04291">pdf</a>, <a href="https://arxiv.org/format/1606.04291">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/11/09/C09017">10.1088/1748-0221/11/09/C09017 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> R&amp;D towards the CMS RPC Phase-2 upgrade </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Fagot%2C+A">A. Fagot</a>, <a href="/search/physics?searchtype=author&amp;query=Cimmino%2C+A">A. Cimmino</a>, <a href="/search/physics?searchtype=author&amp;query=Crucy%2C+S">S. Crucy</a>, <a href="/search/physics?searchtype=author&amp;query=Gul%2C+M">M. Gul</a>, <a href="/search/physics?searchtype=author&amp;query=Rios%2C+A+A+O">A. A. O. Rios</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Zaganidis%2C+N">N. Zaganidis</a>, <a href="/search/physics?searchtype=author&amp;query=Aly%2C+S">S. Aly</a>, <a href="/search/physics?searchtype=author&amp;query=Assran%2C+Y">Y. Assran</a>, <a href="/search/physics?searchtype=author&amp;query=Radi%2C+A">A. Radi</a>, <a href="/search/physics?searchtype=author&amp;query=Sayed%2C+A">A. Sayed</a>, <a href="/search/physics?searchtype=author&amp;query=Singh%2C+G">G. Singh</a>, <a href="/search/physics?searchtype=author&amp;query=Abbrescia%2C+M">M. Abbrescia</a>, <a href="/search/physics?searchtype=author&amp;query=Iaselli%2C+G">G. Iaselli</a>, <a href="/search/physics?searchtype=author&amp;query=Maggi%2C+M">M. Maggi</a>, <a href="/search/physics?searchtype=author&amp;query=Pugliese%2C+G">G. Pugliese</a>, <a href="/search/physics?searchtype=author&amp;query=Verwilligen%2C+P">P. Verwilligen</a>, <a href="/search/physics?searchtype=author&amp;query=Van+Doninck%2C+W">W. Van Doninck</a>, <a href="/search/physics?searchtype=author&amp;query=Colafranceschi%2C+S">S. Colafranceschi</a>, <a href="/search/physics?searchtype=author&amp;query=Sharma%2C+A">A. Sharma</a>, <a href="/search/physics?searchtype=author&amp;query=Benussi%2C+L">L. Benussi</a>, <a href="/search/physics?searchtype=author&amp;query=Bianco%2C+S">S. Bianco</a>, <a href="/search/physics?searchtype=author&amp;query=Piccolo%2C+D">D. Piccolo</a>, <a href="/search/physics?searchtype=author&amp;query=Primavera%2C+F">F. Primavera</a>, <a href="/search/physics?searchtype=author&amp;query=Bhatnagar%2C+V">V. Bhatnagar</a> , et al. (71 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1606.04291v1-abstract-short" style="display: inline;"> The high pseudo-rapidity region of the CMS muon system is covered by Cathode Strip Chambers (CSC) only and lacks redundant coverage despite the fact that it is a challenging region for muons in terms of backgrounds and momentum resolution. In order to maintain good efficiency for the muon trigger in this region additional RPCs are planned to be installed in the two outermost stations at low angle&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.04291v1-abstract-full').style.display = 'inline'; document.getElementById('1606.04291v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1606.04291v1-abstract-full" style="display: none;"> The high pseudo-rapidity region of the CMS muon system is covered by Cathode Strip Chambers (CSC) only and lacks redundant coverage despite the fact that it is a challenging region for muons in terms of backgrounds and momentum resolution. In order to maintain good efficiency for the muon trigger in this region additional RPCs are planned to be installed in the two outermost stations at low angle named RE3/1 and RE4/1. These stations will use RPCs with finer granularity and good timing resolution to mitigate background effects and to increase the redundancy of the system. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.04291v1-abstract-full').style.display = 'none'; document.getElementById('1606.04291v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 June, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">13th Workshop on Resistive Plate Chambers and related detectors, 22-26 February 2016, Ghent University, Belgium</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1606.01398">arXiv:1606.01398</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1606.01398">pdf</a>, <a href="https://arxiv.org/format/1606.01398">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/11/09/C09006">10.1088/1748-0221/11/09/C09006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> High rate, fast timing Glass RPC for the high 畏 CMS muon detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Lagarde%2C+F">F. Lagarde</a>, <a href="/search/physics?searchtype=author&amp;query=Gouzevitch%2C+M">M. Gouzevitch</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Buridon%2C+V">V. Buridon</a>, <a href="/search/physics?searchtype=author&amp;query=Chen%2C+X">X. Chen</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Eynard%2C+A">A. Eynard</a>, <a href="/search/physics?searchtype=author&amp;query=Germani%2C+L">L. Germani</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Mathez%2C+H">H. Mathez</a>, <a href="/search/physics?searchtype=author&amp;query=Mirabito%2C+L">L. Mirabito</a>, <a href="/search/physics?searchtype=author&amp;query=Petrukhin%2C+A">A. Petrukhin</a>, <a href="/search/physics?searchtype=author&amp;query=Steen%2C+A">A. Steen</a>, <a href="/search/physics?searchtype=author&amp;query=Tromeuraa%2C+W">W. Tromeuraa</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+Y">Y. Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Gongab%2C+A">A. Gongab</a>, <a href="/search/physics?searchtype=author&amp;query=Moreau%2C+N">N. Moreau</a>, <a href="/search/physics?searchtype=author&amp;query=de+la+Taille%2C+C">C. de la Taille</a>, <a href="/search/physics?searchtype=author&amp;query=Dulucqac%2C+F">F. Dulucqac</a>, <a href="/search/physics?searchtype=author&amp;query=Cimmino%2C+A">A. Cimmino</a>, <a href="/search/physics?searchtype=author&amp;query=Crucy%2C+S">S. Crucy</a>, <a href="/search/physics?searchtype=author&amp;query=Fagot%2C+A">A. Fagot</a>, <a href="/search/physics?searchtype=author&amp;query=Gul%2C+M">M. Gul</a>, <a href="/search/physics?searchtype=author&amp;query=Rios%2C+A+A+O">A. A. O. Rios</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a> , et al. (86 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1606.01398v2-abstract-short" style="display: inline;"> The HL-LHC phase is designed to increase by an order of magnitude the amount of data to be collected by the LHC experiments. To achieve this goal in a reasonable time scale the instantaneous luminosity would also increase by an order of magnitude up to $6.10^{34} cm^{-2} s^{-1}$ . The region of the forward muon spectrometer ($|畏| &gt; 1.6$) is not equipped with RPC stations. The increase of the expec&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.01398v2-abstract-full').style.display = 'inline'; document.getElementById('1606.01398v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1606.01398v2-abstract-full" style="display: none;"> The HL-LHC phase is designed to increase by an order of magnitude the amount of data to be collected by the LHC experiments. To achieve this goal in a reasonable time scale the instantaneous luminosity would also increase by an order of magnitude up to $6.10^{34} cm^{-2} s^{-1}$ . The region of the forward muon spectrometer ($|畏| &gt; 1.6$) is not equipped with RPC stations. The increase of the expected particles rate up to $2 kHz/cm^{2}$ (including a safety factor 3) motivates the installation of RPC chambers to guarantee redundancy with the CSC chambers already present. The actual RPC technology of CMS cannot sustain the expected background level. The new technology that will be chosen should have a high rate capability and provides a good spatial and timing resolution. A new generation of Glass-RPC (GRPC) using low-resistivity (LR) glass is proposed to equip at least the two most far away of the four high $畏$ muon stations of CMS. First the design of small size prototypes and studies of their performance in high-rate particles flux is presented. Then the proposed designs for large size chambers and their fast-timing electronic readout are examined and preliminary results are provided. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.01398v2-abstract-full').style.display = 'none'; document.getElementById('1606.01398v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 June, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">14 pages, 11 figures, Conference proceeding for the 2016 Resistive Plate Chambers and Related Detectors</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1606.00993">arXiv:1606.00993</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1606.00993">pdf</a>, <a href="https://arxiv.org/format/1606.00993">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2016.05.073">10.1016/j.nima.2016.05.073 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> High rate, fast timing Glass RPC for the high $畏$ CMS muon detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Gouzevitch%2C+M">Maxime Gouzevitch</a>, <a href="/search/physics?searchtype=author&amp;query=Lagarde%2C+F">Fran莽ois Lagarde</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">Imad Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Buridon%2C+V">Victor Buridon</a>, <a href="/search/physics?searchtype=author&amp;query=Chen%2C+X">Xiushan Chen</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">Christophe Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Eynard%2C+A">Alexis Eynard</a>, <a href="/search/physics?searchtype=author&amp;query=Germani%2C+L">Lionel Germani</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">Gerald Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Mathez%2C+H">Herv茅 Mathez</a>, <a href="/search/physics?searchtype=author&amp;query=Mirabito%2C+L">Laurent Mirabito</a>, <a href="/search/physics?searchtype=author&amp;query=Petrukhin%2C+A">Alexei Petrukhin</a>, <a href="/search/physics?searchtype=author&amp;query=Steen%2C+A">Arnaud Steen</a>, <a href="/search/physics?searchtype=author&amp;query=Tromeur%2C+W">William Tromeur</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+Y">Yi Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+F">Fuyue Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Moreau%2C+N">Nathalie Moreau</a>, <a href="/search/physics?searchtype=author&amp;query=de+la+Taille%2C+C">Christophe de la Taille</a>, <a href="/search/physics?searchtype=author&amp;query=Dulucq%2C+F">Fr茅deric Dulucq</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1606.00993v1-abstract-short" style="display: inline;"> The HL-LHC phase is designed to increase by an order of magnitude the amount of data to be collected by the LHC experiments. To achieve this goal in a reasonable time scale the instantaneous luminosity would also increase by an order of magnitude up to $6 \cdot 10^{34}$ cm$^{-2}$s$^{-1}$. The region of the forward muon spectrometer ($|畏| &gt; 1.6$) is not equipped with RPC stations. The increase of t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.00993v1-abstract-full').style.display = 'inline'; document.getElementById('1606.00993v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1606.00993v1-abstract-full" style="display: none;"> The HL-LHC phase is designed to increase by an order of magnitude the amount of data to be collected by the LHC experiments. To achieve this goal in a reasonable time scale the instantaneous luminosity would also increase by an order of magnitude up to $6 \cdot 10^{34}$ cm$^{-2}$s$^{-1}$. The region of the forward muon spectrometer ($|畏| &gt; 1.6$) is not equipped with RPC stations. The increase of the expected particles rate up to 2 kHz/cm$^2$ ( including a safety factor 3 ) motivates the installation of RPC chambers to guarantee redundancy with the CSC chambers already present. The actual RPC technology of CMS cannot sustain the expected background level. A new generation Glass-RPC (GRPC) using low resistivity glass (LR) is proposed to equip at least the two most far away of the four high eta muon stations of CMS. The design of small size prototypes and the studies of their performances under high rate particles flux is presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.00993v1-abstract-full').style.display = 'none'; document.getElementById('1606.00993v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 June, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">5 pages, 5 figures, proceeding for the conference VCI 2016</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Instruments &amp; Methods in Physics Research A (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1605.06798">arXiv:1605.06798</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1605.06798">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Performance of Resistive Plate Chambers installed during the first long shutdown of the CMS experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Shopova%2C+M">M. Shopova</a>, <a href="/search/physics?searchtype=author&amp;query=Aleksandrov%2C+A">A. Aleksandrov</a>, <a href="/search/physics?searchtype=author&amp;query=Hadjiiska%2C+R">R. Hadjiiska</a>, <a href="/search/physics?searchtype=author&amp;query=Iaydjiev%2C+P">P. Iaydjiev</a>, <a href="/search/physics?searchtype=author&amp;query=Sultanov%2C+G">G. Sultanov</a>, <a href="/search/physics?searchtype=author&amp;query=Rodozov%2C+M">M. Rodozov</a>, <a href="/search/physics?searchtype=author&amp;query=Stoykova%2C+S">S. Stoykova</a>, <a href="/search/physics?searchtype=author&amp;query=Assran%2C+Y">Y. Assran</a>, <a href="/search/physics?searchtype=author&amp;query=Sayed%2C+A">A. Sayed</a>, <a href="/search/physics?searchtype=author&amp;query=Radi%2C+A">A. Radi</a>, <a href="/search/physics?searchtype=author&amp;query=Aly%2C+S">S. Aly</a>, <a href="/search/physics?searchtype=author&amp;query=Singh%2C+G">G. Singh</a>, <a href="/search/physics?searchtype=author&amp;query=Abbrescia%2C+M">M. Abbrescia</a>, <a href="/search/physics?searchtype=author&amp;query=Iaselli%2C+G">G. Iaselli</a>, <a href="/search/physics?searchtype=author&amp;query=Maggi%2C+M">M. Maggi</a>, <a href="/search/physics?searchtype=author&amp;query=Pugliese%2C+G">G. Pugliese</a>, <a href="/search/physics?searchtype=author&amp;query=Verwilligen%2C+P">P. Verwilligen</a>, <a href="/search/physics?searchtype=author&amp;query=Van+Doninck%2C+W">W. Van Doninck</a>, <a href="/search/physics?searchtype=author&amp;query=Colafranceschi%2C+S">S. Colafranceschi</a>, <a href="/search/physics?searchtype=author&amp;query=Sharma%2C+A">A. Sharma</a>, <a href="/search/physics?searchtype=author&amp;query=Benussi%2C+L">L. Benussi</a>, <a href="/search/physics?searchtype=author&amp;query=Bianco%2C+S">S. Bianco</a>, <a href="/search/physics?searchtype=author&amp;query=Piccolo%2C+D">D. Piccolo</a>, <a href="/search/physics?searchtype=author&amp;query=Primavera%2C+F">F. Primavera</a>, <a href="/search/physics?searchtype=author&amp;query=Cimmino%2C+A">A. Cimmino</a> , et al. (71 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1605.06798v1-abstract-short" style="display: inline;"> The CMS experiment, located at the CERN Large Hadron Collider, has a redundant muon system composed by three different detector technologies: Cathode Strip Chambers (in the forward regions), Drift Tubes (in the central region) and Resistive Plate Chambers (both its central and forward regions). All three are used for muon reconstruction and triggering. During the first long shutdown (LS1) of the L&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1605.06798v1-abstract-full').style.display = 'inline'; document.getElementById('1605.06798v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1605.06798v1-abstract-full" style="display: none;"> The CMS experiment, located at the CERN Large Hadron Collider, has a redundant muon system composed by three different detector technologies: Cathode Strip Chambers (in the forward regions), Drift Tubes (in the central region) and Resistive Plate Chambers (both its central and forward regions). All three are used for muon reconstruction and triggering. During the first long shutdown (LS1) of the LHC (2013-2014) the CMS muon system has been upgraded with 144 newly installed RPCs on the forth forward stations. The new chambers ensure and enhance the muon trigger efficiency in the high luminosity conditions of the LHC Run2. The chambers have been successfully installed and commissioned. The system has been run successfully and experimental data has been collected and analyzed. The performance results of the newly installed RPCs will be presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1605.06798v1-abstract-full').style.display = 'none'; document.getElementById('1605.06798v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 May, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">5 pages, 6 figures, proceeding to The XIII workshop on Resistive Plate Chambers and Related Detectors (RPC2016)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CMS CR-2016/090 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1605.00440">arXiv:1605.00440</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1605.00440">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Radiation Tests of Real-Sized Prototype RPCs for the Future CMS RPC Upscope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Lee%2C+K+S">K. S. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Choi%2C+S">S. Choi</a>, <a href="/search/physics?searchtype=author&amp;query=Hong%2C+B+S">B. S. Hong</a>, <a href="/search/physics?searchtype=author&amp;query=Jo%2C+M">M. Jo</a>, <a href="/search/physics?searchtype=author&amp;query=Kang%2C+J+W">J. W. Kang</a>, <a href="/search/physics?searchtype=author&amp;query=Kang%2C+M">M. Kang</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+H">H. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+K">K. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Parka%2C+S+K">S. K. Parka</a>, <a href="/search/physics?searchtype=author&amp;query=Cimmino%2C+A">A. Cimmino</a>, <a href="/search/physics?searchtype=author&amp;query=Crucy%2C+S">S. Crucy</a>, <a href="/search/physics?searchtype=author&amp;query=Fagot%2C+A">A. Fagot</a>, <a href="/search/physics?searchtype=author&amp;query=Gul%2C+M">M. Gul</a>, <a href="/search/physics?searchtype=author&amp;query=Rios%2C+A+A+O">A. A. O. Rios</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Zaganidis%2C+N">N. Zaganidis</a>, <a href="/search/physics?searchtype=author&amp;query=Ali%2C+S">S. Ali</a>, <a href="/search/physics?searchtype=author&amp;query=Assran%2C+Y">Y. Assran</a>, <a href="/search/physics?searchtype=author&amp;query=Radi%2C+A">A. Radi</a>, <a href="/search/physics?searchtype=author&amp;query=Sayed%2C+A">A. Sayed</a>, <a href="/search/physics?searchtype=author&amp;query=Singh%2C+G">G. Singh</a>, <a href="/search/physics?searchtype=author&amp;query=Abbrescia%2C+M">M. Abbrescia</a>, <a href="/search/physics?searchtype=author&amp;query=Iaselli%2C+G">G. Iaselli</a>, <a href="/search/physics?searchtype=author&amp;query=Maggi%2C+M">M. Maggi</a>, <a href="/search/physics?searchtype=author&amp;query=Pugliese%2C+G">G. Pugliese</a> , et al. (71 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1605.00440v2-abstract-short" style="display: inline;"> We report on a systematic study of double-gap and four-gap phenolic resistive plate chambers (RPCs) for future high-畏 RPC triggers in the CMS. In the present study, we constructed real-sized double-gap and four-gap RPCs with gap thicknesses of 1.6 and 0.8 mm, respectively, with 2-mm-thick phenolic high-pressure-laminated (HPL) plates. We examined the prototype RPCs for cosmic rays and 100 GeV muon&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1605.00440v2-abstract-full').style.display = 'inline'; document.getElementById('1605.00440v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1605.00440v2-abstract-full" style="display: none;"> We report on a systematic study of double-gap and four-gap phenolic resistive plate chambers (RPCs) for future high-畏 RPC triggers in the CMS. In the present study, we constructed real-sized double-gap and four-gap RPCs with gap thicknesses of 1.6 and 0.8 mm, respectively, with 2-mm-thick phenolic high-pressure-laminated (HPL) plates. We examined the prototype RPCs for cosmic rays and 100 GeV muons provided by the SPS H4 beam line at CERN. We applied maximum gamma rates of 1.5 kHz cm-2 provided by 137Cs sources at Korea University and the GIF++ irradiation facility installed at the SPS H4 beam line to examine the rate capabilities of the prototype RPCs. In contrast to the case of the four-gap RPCs, we found the relatively high threshold was conducive to effectively suppressing the rapid increase of strip cluster sizes of muon hits with high voltage, especially when measuring the narrow-pitch strips. The gamma-induced currents drawn in the four-gap RPC were about one-fourth of those drawn in the double-gap RPC. The rate capabilities of both RPC types, proven through the present testing using gamma-ray sources, far exceeded the maximum rate expected in the new high-畏 endcap RPCs planned for future phase-II LHC runs. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1605.00440v2-abstract-full').style.display = 'none'; document.getElementById('1605.00440v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 May, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 2 May, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Conference proceeding for the 2016 Resistive Plate Chambers and Related Detectors 8 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1604.04550">arXiv:1604.04550</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1604.04550">pdf</a>, <a href="https://arxiv.org/format/1604.04550">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/11/06/P06014">10.1088/1748-0221/11/06/P06014 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Resistive Plate Chamber Digitization in a Hadronic Shower Environment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Deng%2C+Z">Z. Deng</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+Y">Y. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+Y">Y. Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Yue%2C+Q">Q. Yue</a>, <a href="/search/physics?searchtype=author&amp;query=Yang%2C+Z">Z. Yang</a>, <a href="/search/physics?searchtype=author&amp;query=Apostolakis%2C+J">J. Apostolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Folger%2C+G">G. Folger</a>, <a href="/search/physics?searchtype=author&amp;query=Grefe%2C+C">C. Grefe</a>, <a href="/search/physics?searchtype=author&amp;query=Ivantchenko%2C+V">V. Ivantchenko</a>, <a href="/search/physics?searchtype=author&amp;query=Ribon%2C+A">A. Ribon</a>, <a href="/search/physics?searchtype=author&amp;query=Uzhinskiy%2C+V">V. Uzhinskiy</a>, <a href="/search/physics?searchtype=author&amp;query=Boumediene%2C+D">D. Boumediene</a>, <a href="/search/physics?searchtype=author&amp;query=Carloganu%2C+C">C. Carloganu</a>, <a href="/search/physics?searchtype=author&amp;query=Fran%C3%A7ais%2C+V">V. Fran莽ais</a>, <a href="/search/physics?searchtype=author&amp;query=Cho%2C+G">G. Cho</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+D">D-W. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+S+C">S. C. Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+W">W. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Vallecorsa%2C+S">S. Vallecorsa</a>, <a href="/search/physics?searchtype=author&amp;query=Cauwenbergh%2C+S">S. Cauwenbergh</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a>, <a href="/search/physics?searchtype=author&amp;query=Pingault%2C+A">A. Pingault</a>, <a href="/search/physics?searchtype=author&amp;query=Zaganidis%2C+N">N. Zaganidis</a>, <a href="/search/physics?searchtype=author&amp;query=Brianne%2C+E">E. Brianne</a>, <a href="/search/physics?searchtype=author&amp;query=Ebrahimi%2C+A">A. Ebrahimi</a> , et al. (103 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1604.04550v1-abstract-short" style="display: inline;"> The CALICE Semi-Digital Hadron Calorimeter (SDHCAL) technological prototype is a sampling calorimeter using Glass Resistive Plate Chamber detectors with a three-threshold readout as the active medium. This technology is one of the two options proposed for the hadron calorimeter of the International Large Detector for the International Linear Collider. The prototype was exposed to beams of muons, e&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.04550v1-abstract-full').style.display = 'inline'; document.getElementById('1604.04550v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1604.04550v1-abstract-full" style="display: none;"> The CALICE Semi-Digital Hadron Calorimeter (SDHCAL) technological prototype is a sampling calorimeter using Glass Resistive Plate Chamber detectors with a three-threshold readout as the active medium. This technology is one of the two options proposed for the hadron calorimeter of the International Large Detector for the International Linear Collider. The prototype was exposed to beams of muons, electrons and pions of different energies at the CERN Super Proton Synchrotron. To be able to study the performance of such a calorimeter in future experiments it is important to ensure reliable simulation of its response. In this paper we present our prototype simulation performed with GEANT4 and the digitization procedure achieved with an algorithm called SimDigital. A detailed description of this algorithm is given and the methods to determinate its parameters using muon tracks and electromagnetic showers are explained. The comparison with hadronic shower data shows a good agreement up to 50 GeV. Discrepancies are observed at higher energies. The reasons for these differences are investigated. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.04550v1-abstract-full').style.display = 'none'; document.getElementById('1604.04550v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 April, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1602.08578">arXiv:1602.08578</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1602.08578">pdf</a>, <a href="https://arxiv.org/format/1602.08578">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/11/06/P06013">10.1088/1748-0221/11/06/P06013 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Hadron shower decomposition in the highly granular CALICE analogue hadron calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=The+CALICE+Collaboration"> The CALICE Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Price%2C+T">T. Price</a>, <a href="/search/physics?searchtype=author&amp;query=Watson%2C+N+K">N. K. Watson</a>, <a href="/search/physics?searchtype=author&amp;query=Marshall%2C+J+S">J. S. Marshall</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a>, <a href="/search/physics?searchtype=author&amp;query=Khoulaki%2C+Y">Y. Khoulaki</a>, <a href="/search/physics?searchtype=author&amp;query=Apostolakis%2C+J">J. Apostolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Dotti%2C+A">A. Dotti</a>, <a href="/search/physics?searchtype=author&amp;query=Folger%2C+G">G. Folger</a>, <a href="/search/physics?searchtype=author&amp;query=Ivantchenko%2C+V">V. Ivantchenko</a>, <a href="/search/physics?searchtype=author&amp;query=Ribon%2C+A">A. Ribon</a>, <a href="/search/physics?searchtype=author&amp;query=Uzhinskiy%2C+V">V. Uzhinskiy</a>, <a href="/search/physics?searchtype=author&amp;query=Hostachy%2C+J+-">J. -Y. Hostachy</a>, <a href="/search/physics?searchtype=author&amp;query=Morin%2C+L">L. Morin</a>, <a href="/search/physics?searchtype=author&amp;query=Brianne%2C+E">E. Brianne</a>, <a href="/search/physics?searchtype=author&amp;query=Ebrahimi%2C+A">A. Ebrahimi</a>, <a href="/search/physics?searchtype=author&amp;query=Gadow%2C+K">K. Gadow</a>, <a href="/search/physics?searchtype=author&amp;query=G%C3%B6ttlicher%2C+P">P. G枚ttlicher</a>, <a href="/search/physics?searchtype=author&amp;query=G%C3%BCnter%2C+C">C. G眉nter</a>, <a href="/search/physics?searchtype=author&amp;query=Hartbrich%2C+O">O. Hartbrich</a>, <a href="/search/physics?searchtype=author&amp;query=Hermberg%2C+B">B. Hermberg</a> , et al. (135 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1602.08578v2-abstract-short" style="display: inline;"> The spatial development of hadronic showers in the CALICE scintillator-steel analogue hadron calorimeter is studied using test beam data collected at CERN and FNAL for single positive pions and protons with initial momenta in the range from 10 to 80 GeV/c. Both longitudinal and radial development of hadron showers are parametrised with two-component functions. The parametrisation is fit to test be&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1602.08578v2-abstract-full').style.display = 'inline'; document.getElementById('1602.08578v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1602.08578v2-abstract-full" style="display: none;"> The spatial development of hadronic showers in the CALICE scintillator-steel analogue hadron calorimeter is studied using test beam data collected at CERN and FNAL for single positive pions and protons with initial momenta in the range from 10 to 80 GeV/c. Both longitudinal and radial development of hadron showers are parametrised with two-component functions. The parametrisation is fit to test beam data and simulations using the QGSP_BERT and FTFP_BERT physics lists from Geant4 version 9.6. The parameters extracted from data and simulated samples are compared for the two types of hadrons. The response to pions and the ratio of the non-electromagnetic to the electromagnetic calorimeter response, h/e, are estimated using the extrapolation and decomposition of the longitudinal profiles. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1602.08578v2-abstract-full').style.display = 'none'; document.getElementById('1602.08578v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 March, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 February, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">38 pages, 19 figures, 5 tables; author list changed; submitted to JINST</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1602.02276">arXiv:1602.02276</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1602.02276">pdf</a>, <a href="https://arxiv.org/format/1602.02276">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/11/04/P04001">10.1088/1748-0221/11/04/P04001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First results of the CALICE SDHCAL technological prototype </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Buridon%2C+V">V. Buridon</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Caponetto%2C+L">L. Caponetto</a>, <a href="/search/physics?searchtype=author&amp;query=Et%C3%A9%2C+R">R. Et茅</a>, <a href="/search/physics?searchtype=author&amp;query=Garillot%2C+G">G. Garillot</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Han%2C+R">R. Han</a>, <a href="/search/physics?searchtype=author&amp;query=Ianigro%2C+J+C">J. C. Ianigro</a>, <a href="/search/physics?searchtype=author&amp;query=Kieffer%2C+R">R. Kieffer</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Lumb%2C+N">N. Lumb</a>, <a href="/search/physics?searchtype=author&amp;query=Mathez%2C+H">H. Mathez</a>, <a href="/search/physics?searchtype=author&amp;query=Mirabito%2C+L">L. Mirabito</a>, <a href="/search/physics?searchtype=author&amp;query=Petrukhin%2C+A">A. Petrukhin</a>, <a href="/search/physics?searchtype=author&amp;query=Steen%2C+A">A. Steen</a>, <a href="/search/physics?searchtype=author&amp;query=Antequera%2C+J+B">J. Berenguer Antequera</a>, <a href="/search/physics?searchtype=author&amp;query=Alamillo%2C+E+C">E. Calvo Alamillo</a>, <a href="/search/physics?searchtype=author&amp;query=Fouz%2C+M+-">M. -C. Fouz</a>, <a href="/search/physics?searchtype=author&amp;query=Marin%2C+J">J. Marin</a>, <a href="/search/physics?searchtype=author&amp;query=Puerta-Pelayo%2C+J">J. Puerta-Pelayo</a>, <a href="/search/physics?searchtype=author&amp;query=Verdugo%2C+A">A. Verdugo</a>, <a href="/search/physics?searchtype=author&amp;query=Gil%2C+E+C">E. Cortina Gil</a>, <a href="/search/physics?searchtype=author&amp;query=Mannai%2C+S">S. Mannai</a>, <a href="/search/physics?searchtype=author&amp;query=Cauwenbergh%2C+S">S. Cauwenbergh</a>, <a href="/search/physics?searchtype=author&amp;query=Tytgat%2C+M">M. Tytgat</a> , et al. (96 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1602.02276v2-abstract-short" style="display: inline;"> The CALICE Semi-Digital Hadronic Calorimeter (SDHCAL) prototype, built in 2011, was exposed to beams of hadrons, electrons and muons in two short periods in 2012 on two different beam lines of the CERN SPS. The prototype with its 48 active layers, made of Glass Resistive Plate Chambers and their embedded readout electronics, was run in triggerless and power-pulsing mode. The performance of the SDH&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1602.02276v2-abstract-full').style.display = 'inline'; document.getElementById('1602.02276v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1602.02276v2-abstract-full" style="display: none;"> The CALICE Semi-Digital Hadronic Calorimeter (SDHCAL) prototype, built in 2011, was exposed to beams of hadrons, electrons and muons in two short periods in 2012 on two different beam lines of the CERN SPS. The prototype with its 48 active layers, made of Glass Resistive Plate Chambers and their embedded readout electronics, was run in triggerless and power-pulsing mode. The performance of the SDHCAL during the test beam was found to be very satisfactory with an efficiency exceeding 90% for almost all of the 48 active layers. A linear response (within 5%) and a good energy resolution are obtained for a large range of hadronic energies (5-80GeV) by applying appropriate calibration coefficients to the collected data for both the Digital (Binary) and the Semi-Digital (Multi-threshold) modes of the SDHCAL prototype. The Semi-Digital mode shows better performance at energies exceeding 30GeV <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1602.02276v2-abstract-full').style.display = 'none'; document.getElementById('1602.02276v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 March, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 February, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1506.05316">arXiv:1506.05316</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1506.05316">pdf</a>, <a href="https://arxiv.org/format/1506.05316">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Construction and commissioning of a technological prototype of a high-granularity semi-digital hadronic calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Baulieu%2C+G">G. Baulieu</a>, <a href="/search/physics?searchtype=author&amp;query=Bedjidian%2C+M">M. Bedjidian</a>, <a href="/search/physics?searchtype=author&amp;query=Belkadhi%2C+K">K. Belkadhi</a>, <a href="/search/physics?searchtype=author&amp;query=Berenguer%2C+J">J. Berenguer</a>, <a href="/search/physics?searchtype=author&amp;query=Boudry%2C+V">V. Boudry</a>, <a href="/search/physics?searchtype=author&amp;query=Calabria%2C+P">P. Calabria</a>, <a href="/search/physics?searchtype=author&amp;query=Callier%2C+S">S. Callier</a>, <a href="/search/physics?searchtype=author&amp;query=Almillo%2C+E+C">E. Calvo Almillo</a>, <a href="/search/physics?searchtype=author&amp;query=Cap%2C+S">S. Cap</a>, <a href="/search/physics?searchtype=author&amp;query=Caponetto%2C+L">L. Caponetto</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Cornat%2C+R">R. Cornat</a>, <a href="/search/physics?searchtype=author&amp;query=Gil%2C+E+C">E. Cortina Gil</a>, <a href="/search/physics?searchtype=author&amp;query=de+Callatay%2C+B">B. de Callatay</a>, <a href="/search/physics?searchtype=author&amp;query=Davin%2C+F">F. Davin</a>, <a href="/search/physics?searchtype=author&amp;query=de+la+Taille%2C+C">C. de la Taille</a>, <a href="/search/physics?searchtype=author&amp;query=Dellanegra%2C+R">R. Dellanegra</a>, <a href="/search/physics?searchtype=author&amp;query=Delaunay%2C+D">D. Delaunay</a>, <a href="/search/physics?searchtype=author&amp;query=Doizon%2C+F">F. Doizon</a>, <a href="/search/physics?searchtype=author&amp;query=Dulucq%2C+F">F. Dulucq</a>, <a href="/search/physics?searchtype=author&amp;query=Eynard%2C+A">A. Eynard</a>, <a href="/search/physics?searchtype=author&amp;query=Fouz%2C+M">M-C. Fouz</a>, <a href="/search/physics?searchtype=author&amp;query=Gastaldi%2C+F">F. Gastaldi</a>, <a href="/search/physics?searchtype=author&amp;query=Germani%2C+L">L. Germani</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a> , et al. (21 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1506.05316v2-abstract-short" style="display: inline;"> A large prototype of 1.3m3 was designed and built as a demonstrator of the semi-digital hadronic calorimeter (SDHCAL) concept proposed for the future ILC experiments. The prototype is a sampling hadronic calorimeter of 48 units. Each unit is built of an active layer made of 1m2 Glass Resistive Plate Chamber(GRPC) detector placed inside a cassette whose walls are made of stainless steel. The casset&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1506.05316v2-abstract-full').style.display = 'inline'; document.getElementById('1506.05316v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1506.05316v2-abstract-full" style="display: none;"> A large prototype of 1.3m3 was designed and built as a demonstrator of the semi-digital hadronic calorimeter (SDHCAL) concept proposed for the future ILC experiments. The prototype is a sampling hadronic calorimeter of 48 units. Each unit is built of an active layer made of 1m2 Glass Resistive Plate Chamber(GRPC) detector placed inside a cassette whose walls are made of stainless steel. The cassette contains also the electronics used to read out the GRPC detector. The lateral granularity of the active layer is provided by the electronics pick-up pads of 1cm2 each. The cassettes are inserted into a self-supporting mechanical structure built also of stainless steel plates which, with the cassettes walls, play the role of the absorber. The prototype was designed to be very compact and important efforts were made to minimize the number of services cables to optimize the efficiency of the Particle Flow Algorithm techniques to be used in the future ILC experiments. The different components of the SDHCAL prototype were studied individually and strict criteria were applied for the final selection of these components. Basic calibration procedures were performed after the prototype assembling. The prototype is the first of a series of new-generation detectors equipped with a power-pulsing mode intended to reduce the power consumption of this highly granular detector. A dedicated acquisition system was developed to deal with the output of more than 440000 electronics channels in both trigger and triggerless modes. After its completion in 2011, the prototype was commissioned using cosmic rays and particles beams at CERN. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1506.05316v2-abstract-full').style.display = 'none'; document.getElementById('1506.05316v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 24 October, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 June, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">49 pages, 41 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1412.2653">arXiv:1412.2653</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1412.2653">pdf</a>, <a href="https://arxiv.org/format/1412.2653">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/10/04/P04014">10.1088/1748-0221/10/04/P04014 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Pion and proton showers in the CALICE scintillator-steel analogue hadron calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=The+CALICE+Collaboration"> The CALICE Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Bilki%2C+B">B. Bilki</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Xia%2C+L">L. Xia</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a>, <a href="/search/physics?searchtype=author&amp;query=Khoulaki%2C+Y">Y. Khoulaki</a>, <a href="/search/physics?searchtype=author&amp;query=Chang%2C+S">S. Chang</a>, <a href="/search/physics?searchtype=author&amp;query=Khan%2C+A">A. Khan</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+D+H">D. H. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kong%2C+D+J">D. J. Kong</a>, <a href="/search/physics?searchtype=author&amp;query=Oh%2C+Y+D">Y. D. Oh</a>, <a href="/search/physics?searchtype=author&amp;query=Blazey%2C+G+C">G. C. Blazey</a>, <a href="/search/physics?searchtype=author&amp;query=Dyshkant%2C+A">A. Dyshkant</a>, <a href="/search/physics?searchtype=author&amp;query=Francis%2C+K">K. Francis</a>, <a href="/search/physics?searchtype=author&amp;query=Lima%2C+J+G+R">J. G. R. Lima</a>, <a href="/search/physics?searchtype=author&amp;query=Salcido%2C+R">R. Salcido</a>, <a href="/search/physics?searchtype=author&amp;query=Zutshi%2C+V">V. Zutshi</a>, <a href="/search/physics?searchtype=author&amp;query=Salvatore%2C+F">F. Salvatore</a>, <a href="/search/physics?searchtype=author&amp;query=Kawagoe%2C+K">K. Kawagoe</a>, <a href="/search/physics?searchtype=author&amp;query=Miyazaki%2C+Y">Y. Miyazaki</a>, <a href="/search/physics?searchtype=author&amp;query=Sudo%2C+Y">Y. Sudo</a> , et al. (147 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1412.2653v3-abstract-short" style="display: inline;"> Showers produced by positive hadrons in the highly granular CALICE scintillator-steel analogue hadron calorimeter were studied. The experimental data were collected at CERN and FNAL for single particles with initial momenta from 10 to 80 GeV/c. The calorimeter response and resolution and spatial characteristics of shower development for proton- and pion-induced showers for test beam data and simul&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1412.2653v3-abstract-full').style.display = 'inline'; document.getElementById('1412.2653v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1412.2653v3-abstract-full" style="display: none;"> Showers produced by positive hadrons in the highly granular CALICE scintillator-steel analogue hadron calorimeter were studied. The experimental data were collected at CERN and FNAL for single particles with initial momenta from 10 to 80 GeV/c. The calorimeter response and resolution and spatial characteristics of shower development for proton- and pion-induced showers for test beam data and simulations using Geant4 version 9.6 are compared. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1412.2653v3-abstract-full').style.display = 'none'; document.getElementById('1412.2653v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 March, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 December, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2014. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">26 pages, 16 figures, JINST style, changes in the author list, typos corrected, new section added, figures regrouped. Accepted for publication in JINST</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1404.6454">arXiv:1404.6454</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1404.6454">pdf</a>, <a href="https://arxiv.org/format/1404.6454">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/9/07/P07022">10.1088/1748-0221/9/07/P07022 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Time Structure of Hadronic Showers in highly granular Calorimeters with Tungsten and Steel Absorbers </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adloff%2C+C">C. Adloff</a>, <a href="/search/physics?searchtype=author&amp;query=Blaising%2C+J+-">J. -J. Blaising</a>, <a href="/search/physics?searchtype=author&amp;query=Chefdeville%2C+M">M. Chefdeville</a>, <a href="/search/physics?searchtype=author&amp;query=Drancourt%2C+C">C. Drancourt</a>, <a href="/search/physics?searchtype=author&amp;query=Gaglione%2C+R">R. Gaglione</a>, <a href="/search/physics?searchtype=author&amp;query=Geffroy%2C+N">N. Geffroy</a>, <a href="/search/physics?searchtype=author&amp;query=Karyotakis%2C+Y">Y. Karyotakis</a>, <a href="/search/physics?searchtype=author&amp;query=Koletsou%2C+I">I. Koletsou</a>, <a href="/search/physics?searchtype=author&amp;query=Prast%2C+J">J. Prast</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+G+V+J">G. Vouters J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Schlereth%2C+J">J. Schlereth</a>, <a href="/search/physics?searchtype=author&amp;query=Baldolemar%2C+L+X+E">L. Xia E. Baldolemar</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+J">J. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+S+T">S. T. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Sosebee%2C+M">M. Sosebee</a>, <a href="/search/physics?searchtype=author&amp;query=White%2C+A+P">A. P. White</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a>, <a href="/search/physics?searchtype=author&amp;query=Apostolakis%2C+Y+K+J">Y. Khoulaki J. Apostolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Arfaoui%2C+S">S. Arfaoui</a>, <a href="/search/physics?searchtype=author&amp;query=Benoit%2C+M">M. Benoit</a> , et al. (188 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1404.6454v2-abstract-short" style="display: inline;"> The intrinsic time structure of hadronic showers influences the timing capability and the required integration time of hadronic calorimeters in particle physics experiments, and depends on the active medium and on the absorber of the calorimeter. With the CALICE T3B experiment, a setup of 15 small plastic scintillator tiles read out with Silicon Photomultipliers, the time structure of showers is m&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1404.6454v2-abstract-full').style.display = 'inline'; document.getElementById('1404.6454v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1404.6454v2-abstract-full" style="display: none;"> The intrinsic time structure of hadronic showers influences the timing capability and the required integration time of hadronic calorimeters in particle physics experiments, and depends on the active medium and on the absorber of the calorimeter. With the CALICE T3B experiment, a setup of 15 small plastic scintillator tiles read out with Silicon Photomultipliers, the time structure of showers is measured on a statistical basis with high spatial and temporal resolution in sampling calorimeters with tungsten and steel absorbers. The results are compared to GEANT4 (version 9.4 patch 03) simulations with different hadronic physics models. These comparisons demonstrate the importance of using high precision treatment of low-energy neutrons for tungsten absorbers, while an overall good agreement between data and simulations for all considered models is observed for steel. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1404.6454v2-abstract-full').style.display = 'none'; document.getElementById('1404.6454v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 July, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 25 April, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2014. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">24 pages including author list, 9 figures, published in JINST</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> MPP-2014-147 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 9 (2014) P07022 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1311.3761">arXiv:1311.3761</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1311.3761">pdf</a>, <a href="https://arxiv.org/ps/1311.3761">ps</a>, <a href="https://arxiv.org/format/1311.3761">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2014.06.039">10.1016/j.nima.2014.06.039 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Performance of the first prototype of the CALICE scintillator strip electromagnetic calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=CALICE+Collaboration"> CALICE Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Francis%2C+K">K. Francis</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Schlereth%2C+J">J. Schlereth</a>, <a href="/search/physics?searchtype=author&amp;query=Smith%2C+J">J. Smith</a>, <a href="/search/physics?searchtype=author&amp;query=Xia%2C+L">L. Xia</a>, <a href="/search/physics?searchtype=author&amp;query=Baldolemar%2C+E">E. Baldolemar</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+J">J. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+S+T">S. T. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Sosebee%2C+M">M. Sosebee</a>, <a href="/search/physics?searchtype=author&amp;query=White%2C+A+P">A. P. White</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Mikami%2C+Y">Y. Mikami</a>, <a href="/search/physics?searchtype=author&amp;query=Watson%2C+N+K">N. K. Watson</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a>, <a href="/search/physics?searchtype=author&amp;query=Khoulaki%2C+Y">Y. Khoulaki</a>, <a href="/search/physics?searchtype=author&amp;query=Apostolakis%2C+J">J. Apostolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Dotti%2C+A">A. Dotti</a>, <a href="/search/physics?searchtype=author&amp;query=Folger%2C+G">G. Folger</a>, <a href="/search/physics?searchtype=author&amp;query=Ivantchenko%2C+V">V. Ivantchenko</a>, <a href="/search/physics?searchtype=author&amp;query=Ribon%2C+A">A. Ribon</a> , et al. (169 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1311.3761v2-abstract-short" style="display: inline;"> A first prototype of a scintillator strip-based electromagnetic calorimeter was built, consisting of 26 layers of tungsten absorber plates interleaved with planes of 45x10x3 mm3 plastic scintillator strips. Data were collected using a positron test beam at DESY with momenta between 1 and 6 GeV/c. The prototype&#39;s performance is presented in terms of the linearity and resolution of the energy measur&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1311.3761v2-abstract-full').style.display = 'inline'; document.getElementById('1311.3761v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1311.3761v2-abstract-full" style="display: none;"> A first prototype of a scintillator strip-based electromagnetic calorimeter was built, consisting of 26 layers of tungsten absorber plates interleaved with planes of 45x10x3 mm3 plastic scintillator strips. Data were collected using a positron test beam at DESY with momenta between 1 and 6 GeV/c. The prototype&#39;s performance is presented in terms of the linearity and resolution of the energy measurement. These results represent an important milestone in the development of highly granular calorimeters using scintillator strip technology. This technology is being developed for a future linear collider experiment, aiming at the precise measurement of jet energies using particle flow techniques. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1311.3761v2-abstract-full').style.display = 'none'; document.getElementById('1311.3761v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 June, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 November, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Inst. and Methods in Physics Research, A (2014), pp. 278-289 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1311.3505">arXiv:1311.3505</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1311.3505">pdf</a>, <a href="https://arxiv.org/format/1311.3505">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/9/01/P01004">10.1088/1748-0221/9/01/P01004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Shower development of particles with momenta from 1 to 10 GeV in the CALICE Scintillator-Tungsten HCAL </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adloff%2C+C">C. Adloff</a>, <a href="/search/physics?searchtype=author&amp;query=Blaising%2C+J+-">J. -J. Blaising</a>, <a href="/search/physics?searchtype=author&amp;query=Chefdeville%2C+M">M. Chefdeville</a>, <a href="/search/physics?searchtype=author&amp;query=Drancourt%2C+C">C. Drancourt</a>, <a href="/search/physics?searchtype=author&amp;query=Gaglione%2C+R">R. Gaglione</a>, <a href="/search/physics?searchtype=author&amp;query=Geffroy%2C+N">N. Geffroy</a>, <a href="/search/physics?searchtype=author&amp;query=Karyotakis%2C+Y">Y. Karyotakis</a>, <a href="/search/physics?searchtype=author&amp;query=Koletsou%2C+I">I. Koletsou</a>, <a href="/search/physics?searchtype=author&amp;query=Prast%2C+J">J. Prast</a>, <a href="/search/physics?searchtype=author&amp;query=Vouters%2C+G">G. Vouters</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Schlereth%2C+J">J. Schlereth</a>, <a href="/search/physics?searchtype=author&amp;query=Smith%2C+J">J. Smith</a>, <a href="/search/physics?searchtype=author&amp;query=Xia%2C+L">L. Xia</a>, <a href="/search/physics?searchtype=author&amp;query=Baldolemar%2C+E">E. Baldolemar</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+J">J. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+S+T">S. T. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Sosebee%2C+M">M. Sosebee</a>, <a href="/search/physics?searchtype=author&amp;query=White%2C+A+P">A. P. White</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a> , et al. (194 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1311.3505v2-abstract-short" style="display: inline;"> Lepton colliders are considered as options to complement and to extend the physics programme at the Large Hadron Collider. The Compact Linear Collider (CLIC) is an $e^+e^-$ collider under development aiming at centre-of-mass energies of up to 3 TeV. For experiments at CLIC, a hadron sampling calorimeter with tungsten absorber is proposed. Such a calorimeter provides sufficient depth to contain hig&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1311.3505v2-abstract-full').style.display = 'inline'; document.getElementById('1311.3505v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1311.3505v2-abstract-full" style="display: none;"> Lepton colliders are considered as options to complement and to extend the physics programme at the Large Hadron Collider. The Compact Linear Collider (CLIC) is an $e^+e^-$ collider under development aiming at centre-of-mass energies of up to 3 TeV. For experiments at CLIC, a hadron sampling calorimeter with tungsten absorber is proposed. Such a calorimeter provides sufficient depth to contain high-energy showers, while allowing a compact size for the surrounding solenoid. A fine-grained calorimeter prototype with tungsten absorber plates and scintillator tiles read out by silicon photomultipliers was built and exposed to particle beams at CERN. Results obtained with electrons, pions and protons of momenta up to 10 GeV are presented in terms of energy resolution and shower shape studies. The results are compared with several GEANT4 simulation models in order to assess the reliability of the Monte Carlo predictions relevant for a future experiment at CLIC. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1311.3505v2-abstract-full').style.display = 'none'; document.getElementById('1311.3505v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 January, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 14 November, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">28 pages, 23 figures, 3 tables</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 9 P01004 January 2014 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1305.7027">arXiv:1305.7027</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1305.7027">pdf</a>, <a href="https://arxiv.org/format/1305.7027">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Track segments in hadronic showers in a highly granular scintillator-steel hadron calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=CALICE+Collaboration"> CALICE Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Adloff%2C+C">C. Adloff</a>, <a href="/search/physics?searchtype=author&amp;query=Blaising%2C+J+-">J. -J. Blaising</a>, <a href="/search/physics?searchtype=author&amp;query=Chefdeville%2C+M">M. Chefdeville</a>, <a href="/search/physics?searchtype=author&amp;query=Drancourt%2C+C">C. Drancourt</a>, <a href="/search/physics?searchtype=author&amp;query=Gaglione%2C+R">R. Gaglione</a>, <a href="/search/physics?searchtype=author&amp;query=Geffroy%2C+N">N. Geffroy</a>, <a href="/search/physics?searchtype=author&amp;query=Karyotakis%2C+Y">Y. Karyotakis</a>, <a href="/search/physics?searchtype=author&amp;query=Koletsou%2C+I">I. Koletsou</a>, <a href="/search/physics?searchtype=author&amp;query=Prast%2C+J">J. Prast</a>, <a href="/search/physics?searchtype=author&amp;query=Vouters%2C+G">G. Vouters</a>, <a href="/search/physics?searchtype=author&amp;query=Francis%2C+K">K. Francis</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Schlereth%2C+J">J. Schlereth</a>, <a href="/search/physics?searchtype=author&amp;query=Smith%2C+J">J. Smith</a>, <a href="/search/physics?searchtype=author&amp;query=Xia%2C+L">L. Xia</a>, <a href="/search/physics?searchtype=author&amp;query=Baldolemar%2C+E">E. Baldolemar</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+J">J. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+S+T">S. T. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Sosebee%2C+M">M. Sosebee</a>, <a href="/search/physics?searchtype=author&amp;query=White%2C+A+P">A. P. White</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Mikami%2C+Y">Y. Mikami</a>, <a href="/search/physics?searchtype=author&amp;query=Watson%2C+N+K">N. K. Watson</a> , et al. (184 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1305.7027v3-abstract-short" style="display: inline;"> We investigate the three dimensional substructure of hadronic showers in the CALICE scintillator-steel hadronic calorimeter. The high granularity of the detector is used to find track segments of minimum ionising particles within hadronic showers, providing sensitivity to the spatial structure and the details of secondary particle production in hadronic cascades. The multiplicity, length and angul&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.7027v3-abstract-full').style.display = 'inline'; document.getElementById('1305.7027v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1305.7027v3-abstract-full" style="display: none;"> We investigate the three dimensional substructure of hadronic showers in the CALICE scintillator-steel hadronic calorimeter. The high granularity of the detector is used to find track segments of minimum ionising particles within hadronic showers, providing sensitivity to the spatial structure and the details of secondary particle production in hadronic cascades. The multiplicity, length and angular distribution of identified track segments are compared to GEANT4 simulations with several different shower models. Track segments also provide the possibility for in-situ calibration of highly granular calorimeters. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.7027v3-abstract-full').style.display = 'none'; document.getElementById('1305.7027v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 July, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 30 May, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">27 pages, 17 figures, accepted for publication in JINST</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> MPP-2013-143 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1211.5698">arXiv:1211.5698</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1211.5698">pdf</a>, <a href="https://arxiv.org/format/1211.5698">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2012.11.029">10.1016/j.nima.2012.11.029 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> High Rate Resistive Plate Chamber for LHC detector upgrades </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Haddad%2C+Y">Y. Haddad</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Lumb%2C+N">N. Lumb</a>, <a href="/search/physics?searchtype=author&amp;query=Cauwenbergh%2C+S">S. Cauwenbergh</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1211.5698v1-abstract-short" style="display: inline;"> The limitation of the detection rate of standard bakelite resistive plate chambers (RPC) used as muon detectors in the LHC experiments has prevented the use of such detectors in the high rate regions in both CMS and ATLAS detectors. One alternative to these detectors are RPCs made with low resistivity glass plates ($10^{10} {\rm 惟.cm}$), a beam test at DESY has shown that such detectors can operat&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1211.5698v1-abstract-full').style.display = 'inline'; document.getElementById('1211.5698v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1211.5698v1-abstract-full" style="display: none;"> The limitation of the detection rate of standard bakelite resistive plate chambers (RPC) used as muon detectors in the LHC experiments has prevented the use of such detectors in the high rate regions in both CMS and ATLAS detectors. One alternative to these detectors are RPCs made with low resistivity glass plates ($10^{10} {\rm 惟.cm}$), a beam test at DESY has shown that such detectors can operate at few thousand Hz/cm$^2$ with high efficiency(&gt; 90%) <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1211.5698v1-abstract-full').style.display = 'none'; document.getElementById('1211.5698v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 24 November, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2012. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1111.5630">arXiv:1111.5630</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1111.5630">pdf</a>, <a href="https://arxiv.org/format/1111.5630">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/7/04/P04009">10.1088/1748-0221/7/04/P04009 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First test of a power-pulsed electronics system on a GRPC detector in a 3-Tesla magnetic field </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Caponetto%2C+L">L. Caponetto</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=de+la+Taille%2C+C">C. de la Taille</a>, <a href="/search/physics?searchtype=author&amp;query=Dulucq%2C+F">F. Dulucq</a>, <a href="/search/physics?searchtype=author&amp;query=Kieffer%2C+R">R. Kieffer</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Lumb%2C+N">N. Lumb</a>, <a href="/search/physics?searchtype=author&amp;query=Mirabito%2C+L">L. Mirabito</a>, <a href="/search/physics?searchtype=author&amp;query=Seguin-Moreau%2C+N">N. Seguin-Moreau</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1111.5630v1-abstract-short" style="display: inline;"> An important technological step towards the realization of an ultra-granular hadronic calorimeter to be used in the future International Linear Collider (ILC) experiments has been made. A 33X50 cm2 GRPC detector equipped with a power-pulsed electronics board offering a 1cm2 lateral segmentation was successfully tested in a 3-Tesla magnet operating at the H2 beam line of the CERN SPS. An important&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.5630v1-abstract-full').style.display = 'inline'; document.getElementById('1111.5630v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1111.5630v1-abstract-full" style="display: none;"> An important technological step towards the realization of an ultra-granular hadronic calorimeter to be used in the future International Linear Collider (ILC) experiments has been made. A 33X50 cm2 GRPC detector equipped with a power-pulsed electronics board offering a 1cm2 lateral segmentation was successfully tested in a 3-Tesla magnet operating at the H2 beam line of the CERN SPS. An important reduction of power consumption with no deterioration of the detector performance is obtained when the power-pulsing mode is applied. This important result shows that ultra-granular calorimeters for ILC experiments are not only an attractive but also a realistic option. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.5630v1-abstract-full').style.display = 'none'; document.getElementById('1111.5630v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 November, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">10 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1011.5969">arXiv:1011.5969</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1011.5969">pdf</a>, <a href="https://arxiv.org/format/1011.5969">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/6/02/P02001">10.1088/1748-0221/6/02/P02001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Performance of Glass Resistive Plate Chambers for a high granularity semi-digital calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Bedjidian%2C+M">M. Bedjidian</a>, <a href="/search/physics?searchtype=author&amp;query=Belkadhi%2C+K">K. Belkadhi</a>, <a href="/search/physics?searchtype=author&amp;query=Boudry%2C+V">V. Boudry</a>, <a href="/search/physics?searchtype=author&amp;query=Combaret%2C+C">C. Combaret</a>, <a href="/search/physics?searchtype=author&amp;query=Decotigny%2C+D">D. Decotigny</a>, <a href="/search/physics?searchtype=author&amp;query=Gil%2C+E+C">E. Cortina Gil</a>, <a href="/search/physics?searchtype=author&amp;query=de+la+Taille%2C+C">C. de la Taille</a>, <a href="/search/physics?searchtype=author&amp;query=Dellanegra%2C+R">R. Dellanegra</a>, <a href="/search/physics?searchtype=author&amp;query=Gapienko%2C+V+A">V. A. Gapienko</a>, <a href="/search/physics?searchtype=author&amp;query=Grenier%2C+G">G. Grenier</a>, <a href="/search/physics?searchtype=author&amp;query=Jauffret%2C+C">C. Jauffret</a>, <a href="/search/physics?searchtype=author&amp;query=Kieffer%2C+R">R. Kieffer</a>, <a href="/search/physics?searchtype=author&amp;query=Fouz%2C+M+-">M. -C. Fouz</a>, <a href="/search/physics?searchtype=author&amp;query=Han%2C+R">R. Han</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Lumb%2C+N">N. Lumb</a>, <a href="/search/physics?searchtype=author&amp;query=Manai%2C+K">K. Manai</a>, <a href="/search/physics?searchtype=author&amp;query=Mannai%2C+S">S. Mannai</a>, <a href="/search/physics?searchtype=author&amp;query=Mathez%2C+H">H. Mathez</a>, <a href="/search/physics?searchtype=author&amp;query=Mirabito%2C+L">L. Mirabito</a>, <a href="/search/physics?searchtype=author&amp;query=Pelayo%2C+J+P">J. Puerta Pelayo</a>, <a href="/search/physics?searchtype=author&amp;query=Ruan%2C+M">M. Ruan</a>, <a href="/search/physics?searchtype=author&amp;query=Schirra%2C+F">F. Schirra</a>, <a href="/search/physics?searchtype=author&amp;query=Seguin-Moreau%2C+N">N. Seguin-Moreau</a>, <a href="/search/physics?searchtype=author&amp;query=Tromeur%2C+W">W. Tromeur</a> , et al. (3 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1011.5969v2-abstract-short" style="display: inline;"> A new design of highly granular hadronic calorimeter using Glass Resistive Plate Chambers (GRPCs) with embedded electronics has been proposed for the future International Linear Collider (ILC) experiments. It features a 2-bit threshold semi-digital read-out. Several GRPC prototypes with their electronics have been successfully built and tested in pion beams. The design of these detectors is presen&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1011.5969v2-abstract-full').style.display = 'inline'; document.getElementById('1011.5969v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1011.5969v2-abstract-full" style="display: none;"> A new design of highly granular hadronic calorimeter using Glass Resistive Plate Chambers (GRPCs) with embedded electronics has been proposed for the future International Linear Collider (ILC) experiments. It features a 2-bit threshold semi-digital read-out. Several GRPC prototypes with their electronics have been successfully built and tested in pion beams. The design of these detectors is presented along with the test results on efficiency, pad multiplicity, stability and reproducibility. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1011.5969v2-abstract-full').style.display = 'none'; document.getElementById('1011.5969v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 December, 2010; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 November, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">16 pages, 15 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 6:P02001,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1004.4996">arXiv:1004.4996</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1004.4996">pdf</a>, <a href="https://arxiv.org/ps/1004.4996">ps</a>, <a href="https://arxiv.org/format/1004.4996">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/5/05/P05007">10.1088/1748-0221/5/05/P05007 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Study of the interactions of pions in the CALICE silicon-tungsten calorimeter prototype </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adloff%2C+C">C. Adloff</a>, <a href="/search/physics?searchtype=author&amp;query=Karyotakis%2C+Y">Y. Karyotakis</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Mikami%2C+Y">Y. Mikami</a>, <a href="/search/physics?searchtype=author&amp;query=Watson%2C+N+K">N. K. Watson</a>, <a href="/search/physics?searchtype=author&amp;query=Wilson%2C+J+A">J. A. Wilson</a>, <a href="/search/physics?searchtype=author&amp;query=Goto%2C+T">T. Goto</a>, <a href="/search/physics?searchtype=author&amp;query=Mavromanolakis%2C+G">G. Mavromanolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Yan%2C+W">W. Yan</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a>, <a href="/search/physics?searchtype=author&amp;query=Khoulaki%2C+Y">Y. Khoulaki</a>, <a href="/search/physics?searchtype=author&amp;query=Apostolakis%2C+J">J. Apostolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Ribon%2C+A">A. Ribon</a>, <a href="/search/physics?searchtype=author&amp;query=Uzhinskiy%2C+V">V. Uzhinskiy</a>, <a href="/search/physics?searchtype=author&amp;query=Benyamna%2C+M">M. Benyamna</a>, <a href="/search/physics?searchtype=author&amp;query=C%C3%A2rloganu%2C+C">C. C芒rloganu</a>, <a href="/search/physics?searchtype=author&amp;query=Fehr%2C+F">F. Fehr</a>, <a href="/search/physics?searchtype=author&amp;query=Gay%2C+P">P. Gay</a>, <a href="/search/physics?searchtype=author&amp;query=Blazey%2C+G+C">G. C. Blazey</a>, <a href="/search/physics?searchtype=author&amp;query=Chakraborty%2C+D">D. Chakraborty</a> , et al. (133 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1004.4996v1-abstract-short" style="display: inline;"> A prototype silicon-tungsten electromagnetic calorimeter for an ILC detector was tested in 2007 at the CERN SPS test beam. Data were collected with electron and hadron beams in the energy range 8 to 80 GeV. The analysis described here focuses on the interactions of pions in the calorimeter. One of the main objectives of the CALICE program is to validate the Monte Carlo tools available for the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.4996v1-abstract-full').style.display = 'inline'; document.getElementById('1004.4996v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1004.4996v1-abstract-full" style="display: none;"> A prototype silicon-tungsten electromagnetic calorimeter for an ILC detector was tested in 2007 at the CERN SPS test beam. Data were collected with electron and hadron beams in the energy range 8 to 80 GeV. The analysis described here focuses on the interactions of pions in the calorimeter. One of the main objectives of the CALICE program is to validate the Monte Carlo tools available for the design of a full-sized detector. The interactions of pions in the Si-W calorimeter are therefore confronted with the predictions of various physical models implemented in the GEANT4 simulation framework. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.4996v1-abstract-full').style.display = 'none'; document.getElementById('1004.4996v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 April, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 5:P05007,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1003.2662">arXiv:1003.2662</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1003.2662">pdf</a>, <a href="https://arxiv.org/format/1003.2662">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/5/05/P05004">10.1088/1748-0221/5/05/P05004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Construction and Commissioning of the CALICE Analog Hadron Calorimeter Prototype </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adloff%2C+C">C. Adloff</a>, <a href="/search/physics?searchtype=author&amp;query=Karyotakis%2C+Y">Y. Karyotakis</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Brandt%2C+A">A. Brandt</a>, <a href="/search/physics?searchtype=author&amp;query=Brown%2C+H">H. Brown</a>, <a href="/search/physics?searchtype=author&amp;query=De%2C+K">K. De</a>, <a href="/search/physics?searchtype=author&amp;query=Medina%2C+C">C. Medina</a>, <a href="/search/physics?searchtype=author&amp;query=Smith%2C+J">J. Smith</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+J">J. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Sosebee%2C+M">M. Sosebee</a>, <a href="/search/physics?searchtype=author&amp;query=White%2C+A">A. White</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a>, <a href="/search/physics?searchtype=author&amp;query=Buanes%2C+T">T. Buanes</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">G. Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Mikami%2C+Y">Y. Mikami</a>, <a href="/search/physics?searchtype=author&amp;query=Miller%2C+O">O. Miller</a>, <a href="/search/physics?searchtype=author&amp;query=Watson%2C+N+K">N. K. Watson</a>, <a href="/search/physics?searchtype=author&amp;query=Wilson%2C+J+A">J. A. Wilson</a>, <a href="/search/physics?searchtype=author&amp;query=Goto%2C+T">T. Goto</a>, <a href="/search/physics?searchtype=author&amp;query=Mavromanolakis%2C+G">G. Mavromanolakis</a>, <a href="/search/physics?searchtype=author&amp;query=Thomson%2C+M+A">M. A. Thomson</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D+R">D. R. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Yan%2C+W">W. Yan</a>, <a href="/search/physics?searchtype=author&amp;query=Benchekroun%2C+D">D. Benchekroun</a>, <a href="/search/physics?searchtype=author&amp;query=Hoummada%2C+A">A. Hoummada</a> , et al. (205 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1003.2662v1-abstract-short" style="display: inline;"> An analog hadron calorimeter (AHCAL) prototype of 5.3 nuclear interaction lengths thickness has been constructed by members of the CALICE Collaboration. The AHCAL prototype consists of a 38-layer sandwich structure of steel plates and highly-segmented scintillator tiles that are read out by wavelength-shifting fibers coupled to SiPMs. The signal is amplified and shaped with a custom-designed ASIC.&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1003.2662v1-abstract-full').style.display = 'inline'; document.getElementById('1003.2662v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1003.2662v1-abstract-full" style="display: none;"> An analog hadron calorimeter (AHCAL) prototype of 5.3 nuclear interaction lengths thickness has been constructed by members of the CALICE Collaboration. The AHCAL prototype consists of a 38-layer sandwich structure of steel plates and highly-segmented scintillator tiles that are read out by wavelength-shifting fibers coupled to SiPMs. The signal is amplified and shaped with a custom-designed ASIC. A calibration/monitoring system based on LED light was developed to monitor the SiPM gain and to measure the full SiPM response curve in order to correct for non-linearity. Ultimately, the physics goals are the study of hadron shower shapes and testing the concept of particle flow. The technical goal consists of measuring the performance and reliability of 7608 SiPMs. The AHCAL was commissioned in test beams at DESY and CERN. The entire prototype was completed in 2007 and recorded hadron showers, electron showers and muons at different energies and incident angles in test beams at CERN and Fermilab. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1003.2662v1-abstract-full').style.display = 'none'; document.getElementById('1003.2662v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 March, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">36 pages, 32 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> DESY 10-032 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 5 (2010) P05004 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0707.1245">arXiv:0707.1245</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0707.1245">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> CALICE Report to the Calorimeter R&amp;D Review Panel </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Brient%2C+J">J-C Brient</a>, <a href="/search/physics?searchtype=author&amp;query=Dauncey%2C+P">P Dauncey</a>, <a href="/search/physics?searchtype=author&amp;query=Garutti%2C+E">E. Garutti</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Poeschl%2C+R">R. Poeschl</a>, <a href="/search/physics?searchtype=author&amp;query=Repond%2C+J">J. Repond</a>, <a href="/search/physics?searchtype=author&amp;query=Sefkow%2C+F">F. Sefkow</a>, <a href="/search/physics?searchtype=author&amp;query=Takeshita%2C+T">T. Takeshita</a>, <a href="/search/physics?searchtype=author&amp;query=Ward%2C+D">D. Ward</a>, <a href="/search/physics?searchtype=author&amp;query=Yu%2C+J">J. Yu</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0707.1245v1-abstract-short" style="display: inline;"> The report describes the status of the calorimeter R&amp;D for ILC detector performed in the CALICE collaboration. This status has been presented to the review panel at the LCWS07 workshop at DESY in June 2007. </span> <span class="abstract-full has-text-grey-dark mathjax" id="0707.1245v1-abstract-full" style="display: none;"> The report describes the status of the calorimeter R&amp;D for ILC detector performed in the CALICE collaboration. This status has been presented to the review panel at the LCWS07 workshop at DESY in June 2007. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0707.1245v1-abstract-full').style.display = 'none'; document.getElementById('0707.1245v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 9 July, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">77 pages</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> ILC-DET-2007-024 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0705.3102">arXiv:0705.3102</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0705.3102">pdf</a>, <a href="https://arxiv.org/ps/0705.3102">ps</a>, <a href="https://arxiv.org/format/0705.3102">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/2/05/P05004">10.1088/1748-0221/2/05/P05004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Track reconstruction in the emulsion-lead target of the OPERA experiment using the ESS microscope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Arrabito%2C+L">L. Arrabito</a>, <a href="/search/physics?searchtype=author&amp;query=Bozza%2C+C">C. Bozza</a>, <a href="/search/physics?searchtype=author&amp;query=Buontempo%2C+S">S. Buontempo</a>, <a href="/search/physics?searchtype=author&amp;query=Consiglio%2C+L">L. Consiglio</a>, <a href="/search/physics?searchtype=author&amp;query=Cozzi%2C+M">M. Cozzi</a>, <a href="/search/physics?searchtype=author&amp;query=D%27Ambrosio%2C+N">N. D&#39;Ambrosio</a>, <a href="/search/physics?searchtype=author&amp;query=De+Lellis%2C+G">G. De Lellis</a>, <a href="/search/physics?searchtype=author&amp;query=De+Serio%2C+M">M. De Serio</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Capua%2C+F">F. Di Capua</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Ferdinando%2C+D">D. Di Ferdinando</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Marco%2C+N">N. Di Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Ereditato%2C+A">A. Ereditato</a>, <a href="/search/physics?searchtype=author&amp;query=Esposito%2C+L+S">L. S. Esposito</a>, <a href="/search/physics?searchtype=author&amp;query=Fini%2C+R+A">R. A. Fini</a>, <a href="/search/physics?searchtype=author&amp;query=Giacomelli%2C+G">G. Giacomelli</a>, <a href="/search/physics?searchtype=author&amp;query=Giorgini%2C+M">M. Giorgini</a>, <a href="/search/physics?searchtype=author&amp;query=Grella%2C+G">G. Grella</a>, <a href="/search/physics?searchtype=author&amp;query=Ieva%2C+M">M. Ieva</a>, <a href="/search/physics?searchtype=author&amp;query=Csathy%2C+J+J">J. Janicsko Csathy</a>, <a href="/search/physics?searchtype=author&amp;query=Juget%2C+F">F. Juget</a>, <a href="/search/physics?searchtype=author&amp;query=Kreslo%2C+I">I. Kreslo</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Manai%2C+K">K. Manai</a>, <a href="/search/physics?searchtype=author&amp;query=Mandrioli%2C+G">G. Mandrioli</a>, <a href="/search/physics?searchtype=author&amp;query=Marotta%2C+A">A. Marotta</a> , et al. (22 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0705.3102v1-abstract-short" style="display: inline;"> The OPERA experiment, designed to conclusively prove the existence of $\rm 谓_渭\to 谓_蟿$ oscillations in the atmospheric sector, makes use of a massive lead-nuclear emulsion target to observe the appearance of $\rm 谓_蟿$&#39;s in the CNGS $\rm 谓_渭$ beam. The location and analysis of the neutrino interactions in quasi real-time required the development of fast computer-controlled microscopes able to rec&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0705.3102v1-abstract-full').style.display = 'inline'; document.getElementById('0705.3102v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0705.3102v1-abstract-full" style="display: none;"> The OPERA experiment, designed to conclusively prove the existence of $\rm 谓_渭\to 谓_蟿$ oscillations in the atmospheric sector, makes use of a massive lead-nuclear emulsion target to observe the appearance of $\rm 谓_蟿$&#39;s in the CNGS $\rm 谓_渭$ beam. The location and analysis of the neutrino interactions in quasi real-time required the development of fast computer-controlled microscopes able to reconstruct particle tracks with sub-micron precision and high efficiency at a speed of 20 cm^2 / h. This paper describes the performance in particle track reconstruction of the European Scanning System, a novel automatic microscope for the measurement of emulsion films developed for OPERA. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0705.3102v1-abstract-full').style.display = 'none'; document.getElementById('0705.3102v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 May, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">13 pages, 10 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 2:P05004,2007 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0701192">arXiv:physics/0701192</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0701192">pdf</a>, <a href="https://arxiv.org/ps/physics/0701192">ps</a>, <a href="https://arxiv.org/format/physics/0701192">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/2/02/P02001">10.1088/1748-0221/2/02/P02001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Electron/pion separation with an Emulsion Cloud Chamber by using a Neural Network </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Arrabito%2C+L">L. Arrabito</a>, <a href="/search/physics?searchtype=author&amp;query=Autiero%2C+D">D. Autiero</a>, <a href="/search/physics?searchtype=author&amp;query=Bozza%2C+C">C. Bozza</a>, <a href="/search/physics?searchtype=author&amp;query=Buontempo%2C+S">S. Buontempo</a>, <a href="/search/physics?searchtype=author&amp;query=Caffari%2C+Y">Y. Caffari</a>, <a href="/search/physics?searchtype=author&amp;query=Consiglio%2C+L">L. Consiglio</a>, <a href="/search/physics?searchtype=author&amp;query=Cozzi%2C+M">M. Cozzi</a>, <a href="/search/physics?searchtype=author&amp;query=D%27Ambrosio%2C+N">N. D&#39;Ambrosio</a>, <a href="/search/physics?searchtype=author&amp;query=De+Lellis%2C+G">G. De Lellis</a>, <a href="/search/physics?searchtype=author&amp;query=De+Serio%2C+M">M. De Serio</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Capua%2C+F">F. Di Capua</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Ferdinando%2C+D">D. Di Ferdinando</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Marco%2C+N">N. Di Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Ereditato%2C+A">A. Ereditato</a>, <a href="/search/physics?searchtype=author&amp;query=Esposito%2C+L+S">L. S. Esposito</a>, <a href="/search/physics?searchtype=author&amp;query=Gagnebin%2C+S">S. Gagnebin</a>, <a href="/search/physics?searchtype=author&amp;query=Giacomelli%2C+G">G. Giacomelli</a>, <a href="/search/physics?searchtype=author&amp;query=Giorgini%2C+M">M. Giorgini</a>, <a href="/search/physics?searchtype=author&amp;query=Grella%2C+G">G. Grella</a>, <a href="/search/physics?searchtype=author&amp;query=Hauger%2C+M">M. Hauger</a>, <a href="/search/physics?searchtype=author&amp;query=Ieva%2C+M">M. Ieva</a>, <a href="/search/physics?searchtype=author&amp;query=Csathy%2C+J+J">J. Janicsko Csathy</a>, <a href="/search/physics?searchtype=author&amp;query=Juget%2C+F">F. Juget</a>, <a href="/search/physics?searchtype=author&amp;query=Kreslo%2C+I">I. Kreslo</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a> , et al. (24 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="physics/0701192v1-abstract-short" style="display: inline;"> We have studied the performance of a new algorithm for electron/pion separation in an Emulsion Cloud Chamber (ECC) made of lead and nuclear emulsion films. The software for separation consists of two parts: a shower reconstruction algorithm and a Neural Network that assigns to each reconstructed shower the probability to be an electron or a pion. The performance has been studied for the ECC of t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0701192v1-abstract-full').style.display = 'inline'; document.getElementById('physics/0701192v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0701192v1-abstract-full" style="display: none;"> We have studied the performance of a new algorithm for electron/pion separation in an Emulsion Cloud Chamber (ECC) made of lead and nuclear emulsion films. The software for separation consists of two parts: a shower reconstruction algorithm and a Neural Network that assigns to each reconstructed shower the probability to be an electron or a pion. The performance has been studied for the ECC of the OPERA experiment [1]. The $e/蟺$ separation algorithm has been optimized by using a detailed Monte Carlo simulation of the ECC and tested on real data taken at CERN (pion beams) and at DESY (electron beams). The algorithm allows to achieve a 90% electron identification efficiency with a pion misidentification smaller than 1% for energies higher than 2 GeV. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0701192v1-abstract-full').style.display = 'none'; document.getElementById('physics/0701192v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 January, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 2:P02001,2007 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0604043">arXiv:physics/0604043</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0604043">pdf</a>, <a href="https://arxiv.org/ps/physics/0604043">ps</a>, <a href="https://arxiv.org/format/physics/0604043">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2006.06.072">10.1016/j.nima.2006.06.072 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Hardware performance of a scanning system for high speed analysis of nuclear emulsions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Arrabito%2C+L">L. Arrabito</a>, <a href="/search/physics?searchtype=author&amp;query=Barbuto%2C+E">E. Barbuto</a>, <a href="/search/physics?searchtype=author&amp;query=Bozza%2C+C">C. Bozza</a>, <a href="/search/physics?searchtype=author&amp;query=Buontempo%2C+S">S. Buontempo</a>, <a href="/search/physics?searchtype=author&amp;query=Consiglio%2C+L">L. Consiglio</a>, <a href="/search/physics?searchtype=author&amp;query=Coppola%2C+D">D. Coppola</a>, <a href="/search/physics?searchtype=author&amp;query=Cozzi%2C+M">M. Cozzi</a>, <a href="/search/physics?searchtype=author&amp;query=Damet%2C+J">J. Damet</a>, <a href="/search/physics?searchtype=author&amp;query=D%27Ambrosio%2C+N">N. D&#39;Ambrosio</a>, <a href="/search/physics?searchtype=author&amp;query=De+Lellis%2C+G">G. De Lellis</a>, <a href="/search/physics?searchtype=author&amp;query=De+Serio%2C+M">M. De Serio</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Capua%2C+F">F. Di Capua</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Ferdinando%2C+D">D. Di Ferdinando</a>, <a href="/search/physics?searchtype=author&amp;query=Di+Marco%2C+N">N. Di Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Esposito%2C+L+S">L. S. Esposito</a>, <a href="/search/physics?searchtype=author&amp;query=Giacomelli%2C+G">G. Giacomelli</a>, <a href="/search/physics?searchtype=author&amp;query=Grella%2C+G">G. Grella</a>, <a href="/search/physics?searchtype=author&amp;query=Hauger%2C+M">M. Hauger</a>, <a href="/search/physics?searchtype=author&amp;query=Juget%2C+F">F. Juget</a>, <a href="/search/physics?searchtype=author&amp;query=Kreslo%2C+I">I. Kreslo</a>, <a href="/search/physics?searchtype=author&amp;query=Giorgini%2C+M">M. Giorgini</a>, <a href="/search/physics?searchtype=author&amp;query=Ieva%2C+M">M. Ieva</a>, <a href="/search/physics?searchtype=author&amp;query=Laktineh%2C+I">I. Laktineh</a>, <a href="/search/physics?searchtype=author&amp;query=Manai%2C+K">K. Manai</a>, <a href="/search/physics?searchtype=author&amp;query=Mandrioli%2C+G">G. Mandrioli</a> , et al. (23 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="physics/0604043v2-abstract-short" style="display: inline;"> The use of nuclear emulsions in very large physics experiments is now possible thanks to the recent improvements in the industrial production of emulsions and to the development of fast automated microscopes. In this paper the hardware performances of the European Scanning System (ESS) are described. The ESS is a very fast automatic system developed for the mass scanning of the emulsions of the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0604043v2-abstract-full').style.display = 'inline'; document.getElementById('physics/0604043v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0604043v2-abstract-full" style="display: none;"> The use of nuclear emulsions in very large physics experiments is now possible thanks to the recent improvements in the industrial production of emulsions and to the development of fast automated microscopes. In this paper the hardware performances of the European Scanning System (ESS) are described. The ESS is a very fast automatic system developed for the mass scanning of the emulsions of the OPERA experiment, which requires microscopes with scanning speeds of about 20 cm^2/h in an emulsion volume of 44 micron thickness. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0604043v2-abstract-full').style.display = 'none'; document.getElementById('physics/0604043v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 July, 2006; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 April, 2006; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2006. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">16 pages, 12 figures, Accepted by Nucl. Instrum. Meth. A</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl.Instrum.Meth.A568:578-587,2006 </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 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