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dc.contributor.authorALICE Collaboration
dc.date.accessioned2018-01-22T10:44:38Z
dc.date.available2018-01-22T10:44:38Z
dc.date.issued2018
dc.identifier.citationALICE Collaboration. (2018). The ALICE Transition Radiation Detector: Construction, operation, and performance. <i>Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment</i>, <i>881</i>, 88-127. <a href="https://doi.org/10.1016/j.nima.2017.09.028" target="_blank">https://doi.org/10.1016/j.nima.2017.09.028</a>
dc.identifier.otherCONVID_27850031
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/56845
dc.description.abstractThe Transition Radiation Detector (TRD) was designed and built to enhance the capabilities of the ALICE detector at the Large Hadron Collider (LHC). While aimed at providing electron identification and triggering, the TRD also contributes significantly to the track reconstruction and calibration in the central barrel of ALICE. In this paper the design, construction, operation, and performance of this detector are discussed. A pion rejection factor of up to 410 is achieved at a momentum of 1 GeV/c in p–Pb collisions and the resolution at high transverse momentum improves by about 40% when including the TRD information in track reconstruction. The triggering capability is demonstrated both for jet, light nuclei, and electron selection.
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofseriesNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
dc.subject.othertransition radiation detector
dc.subject.othermulti-wire proportional drift chamber
dc.subject.otherfibre/foam sandwich radiator
dc.subject.otherXenon-based gas mixture
dc.subject.otherionisation energy loss
dc.subject.otherdE/dx
dc.subject.otherTR
dc.subject.otherelectron-pion identification
dc.subject.otherneural network
dc.subject.othertrigger
dc.titleThe ALICE Transition Radiation Detector: Construction, operation, and performance
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201801161218
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-01-16T13:15:26Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange88-127
dc.relation.issn0168-9002
dc.relation.numberinseries0
dc.relation.volume881
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 CERN for the benefit of the Authors. Published by Elsevier B.V. This is an open access article distributed under the terms of the Creative Commons License.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysoseuranta
jyx.subject.urihttp://www.yso.fi/onto/yso/p17497
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.nima.2017.09.028
dc.type.okmA1


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© 2017 CERN for the benefit of the Authors. Published by Elsevier B.V. This is an open access article distributed under the terms of the Creative Commons License.
Except where otherwise noted, this item's license is described as © 2017 CERN for the benefit of the Authors. Published by Elsevier B.V. This is an open access article distributed under the terms of the Creative Commons License.