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Performance of the CMS drift tube chambers with cosmic rays

dc.contributor.authorAlver, Burak Han
dc.contributor.authorBauer, Gerry P
dc.contributor.authorBendavid, Joshua L.
dc.contributor.authorBusza, Wit
dc.contributor.authorButz, Erik M.
dc.contributor.authorCali, Ivan Amos
dc.contributor.authorChan, M.
dc.contributor.authorD'Enterria, David
dc.contributor.authorEveraerts, Pieter Bruno Bart
dc.contributor.authorGomez-Ceballos, Guillelmo
dc.contributor.authorHahn, Kristian Allan
dc.contributor.authorHarris, Philip Coleman
dc.contributor.authorJaditz, Stephen Hunter
dc.contributor.authorKim, Y.
dc.contributor.authorKlute, Markus
dc.contributor.authorLee, Y.-J.
dc.contributor.authorLi, W.
dc.contributor.authorLoizides, Constantinos
dc.contributor.authorMa, T.
dc.contributor.authorMiller, M.
dc.contributor.authorPaus, Christoph M. E.
dc.contributor.authorRoland, Christof E
dc.contributor.authorRoland, Gunther M
dc.contributor.authorRudolph, Matthew Scott
dc.contributor.authorStephans, George S. F.
dc.contributor.authorSumorok, Konstanty C
dc.contributor.authorSung, K.
dc.contributor.authorVaurynovich, Siarhei S.
dc.contributor.authorWenger, Edward Allen
dc.contributor.authorWyslouch, Boleslaw
dc.contributor.authorXie, S.
dc.contributor.authorYilmaz, Yetkin
dc.contributor.authorYoon, A. S.
dc.contributor.authorCMS Collaboration
dc.contributor.authorNahn, Steven
dc.date.accessioned2019-08-01T20:05:10Z
dc.date.available2019-08-01T20:05:10Z
dc.date.issued2010-03
dc.date.submitted2009-11
dc.identifier.issn1748-0221
dc.identifier.urihttps://hdl.handle.net/1721.1/121960
dc.description.abstractStudies of the performance of the CMS drift tube barrel muon system are described, with results based on data collected during the CMS Cosmic Run at Four Tesla. For most of these data, the solenoidal magnet was operated with a central field of 3.8 T. The analysis of data from 246 out of a total of 250 chambers indicates a very good muon reconstruction capability, with a coordinate resolution for a single hit of about 260 μm, and a nearly 100% efficiency for the drift tube cells. The resolution of the track direction measured in the bending plane is about 1.8 mrad, and the efficiency to reconstruct a segment in a single chamber is higher than 99%. The CMS simulation of cosmic rays reproduces well the performance of the barrel muon detector.en_US
dc.language.isoen
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/1748-0221/5/03/T03015en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titlePerformance of the CMS drift tube chambers with cosmic raysen_US
dc.typeArticleen_US
dc.identifier.citationChatrchyan, S. et al. "Performance of the CMS drift tube chambers with cosmic rays." Journal of Instrumentation 5 (March 2010): T03015 © 2010 IOP Publishing Ltd and SISSAen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Nuclear Science and Engineeringen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.relation.journalJournal of Instrumentationen_US
dc.eprint.versionOriginal manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2019-06-19T13:45:03Z
dspace.date.submission2019-06-19T13:45:05Z
mit.journal.volume5en_US


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