Construction and response of a highly granular scintillator-based electromagnetic calorimeter

dc.contributor.authorRepond, J.
dc.contributor.authorXia, L.
dc.contributor.authorEigen, G.
dc.contributor.authorPrice, T.
dc.contributor.authorWatson, N. K.
dc.contributor.authorWinter, A.
dc.contributor.authorThomson, M. A.
dc.date.accessioned2024-03-13T10:35:07Z
dc.date.available2024-03-13T10:35:07Z
dc.date.issued2018
dc.departmentİstanbul Beykent Üniversitesien_US
dc.description.abstractA highly granular electromagnetic calorimeter with scintillator strip readout is being developed for future linear collider experiments. A prototype of 21.5 X-0 depth and 180 x 180 mm(2) transverse dimensions was constructed, consisting of 2160 individually read out 10 x 45 x 3 mm(3) scintillator strips. This prototype was tested using electrons of 2-32 GeV at the Fermilab Test Beam Facility in 2009. Deviations from linear energy response were less than 1.1%, and the intrinsic energy resolution was determined to be (12.5 +/- 0.1(stat.)+/- 0.4(syst.))%/root E[GeV]circle plus (1.2 +/- 0.1(stat.)(-0.7)(+0.6)(syst.))%, where the uncertainties correspond to statistical and systematic sources, respectively. (C) 2018 Elsevier B.V. All rights reserved.en_US
dc.description.sponsorshipFWO, Belgium; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Youth and Sports of the Czech Republic; European Union's Horizon 2020 Research and Innovation programme [654168]; European Commission within Framework Programme 7 Capacities [262025]; Alexander von Humboldt Stiftung (AvH), Germany; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Deutsche Forschungsgemeinschaft (DFG), Germany; Helmholtz-Gemeinschaft (HGF), Germany; I-CORE Program of the Planning and Budgeting Committee, Israel; Nella and Leon Benoziyo Center for High Energy Physics, Israel; Israeli Science Foundation, Israel; JSPS KAKENHI, Japan [17340071, 223000002]; National Research Foundation of Korea; Korea-EU cooperation programme of National Research Foundation of Korea [2014K1A3A7A03075053]; Russian Ministry of Education and Science [3.2989.2017, 14.A12.31.0006]; Spanish Ministry of Economy and Competitiveness [FPA2014-53938-C3-R2, MDM-2015-0509]; Science and Technology Facilities Council, UK; US Department of Energy; National Science Foundation of the United States of America; Nuclear Physics, Particle Physics, Astrophysics and Cosmology Initiative, a Laboratory Directed Research, USA; Grants-in-Aid for Scientific Research [15H02083, 17340071] Funding Source: KAKEN; Direct For Mathematical & Physical Scien; Division Of Physics [1506017] Funding Source: National Science Foundation; Division Of Physics; Direct For Mathematical & Physical Scien [1607262] Funding Source: National Science Foundationen_US
dc.description.sponsorshipWe gratefully acknowledge the Fermilab managements for their support and hospitality, and their accelerator staff for the reliable and efficient beam operation. This work was supported by the FWO, Belgium; by the Natural Sciences and Engineering Research Council of Canada; by the Ministry of Education, Youth and Sports of the Czech Republic; by the European Union's Horizon 2020 Research and Innovation programme under Grant Agreement 654168; by the European Commission within Framework Programme 7 Capacities, Grant Agreement 262025; by the Alexander von Humboldt Stiftung (AvH), Germany; by the Bundesministerium fur Bildung und Forschung (BMBF), Germany; by the Deutsche Forschungsgemeinschaft (DFG), Germany; by the Helmholtz-Gemeinschaft (HGF), Germany; by the I-CORE Program of the Planning and Budgeting Committee, Israel; by the Nella and Leon Benoziyo Center for High Energy Physics, Israel; by the Israeli Science Foundation, Israel; by the JSPS KAKENHI Grant-in-Aid for Scientific Research (B) No. 17340071 and specially promoted research No. 223000002, Japan; by the National Research Foundation of Korea; by the Korea-EU cooperation programme of National Research Foundation of Korea, Grant Agreement 2014K1A3A7A03075053; by the Russian Ministry of Education and Science contracts 3.2989.2017 and 14.A12.31.0006; by the Spanish Ministry of Economy and Competitiveness FPA2014-53938-C3-R2 and Grant MDM-2015-0509; by the Science and Technology Facilities Council, UK; by the US Department of Energy; by the National Science Foundation of the United States of America, and by the Nuclear Physics, Particle Physics, Astrophysics and Cosmology Initiative, a Laboratory Directed Research, USA.en_US
dc.identifier.doi10.1016/j.nima.2018.01.016
dc.identifier.endpage168en_US
dc.identifier.issn0168-9002
dc.identifier.issn1872-9576
dc.identifier.scopus2-s2.0-85041462993en_US
dc.identifier.scopusqualityQ1en_US
dc.identifier.startpage150en_US
dc.identifier.urihttps://doi.org/10.1016/j.nima.2018.01.016
dc.identifier.urihttps://hdl.handle.net/20.500.12662/4246
dc.identifier.volume887en_US
dc.identifier.wosWOS:000427814400022en_US
dc.identifier.wosqualityQ2en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.relation.ispartofNuclear Instruments & Methods In Physics Research Section A-Accelerators Spectrometers Detectors And Associated Equipmenten_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectParticle flowen_US
dc.subjectElectromagnetic calorimeteren_US
dc.subjectScintillatoren_US
dc.subjectMPPCen_US
dc.subjectSiPMen_US
dc.subjectGranularen_US
dc.titleConstruction and response of a highly granular scintillator-based electromagnetic calorimeteren_US
dc.typeArticleen_US

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