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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.accessioned2019-07-30T17:38:09Z
dc.date.available2019-07-30T17:38:09Z
dc.date.issued2010-03
dc.date.submitted2009-11
dc.identifier.issn1748-0221
dc.identifier.urihttps://hdl.handle.net/1721.1/121948
dc.description.abstractThis paper describes the calibration procedure for the drift tubes of the CMS barrel muon system and reports the main results obtained with data collected during a high statistics cosmic ray data-taking period. The main goal of the calibration is to determine, for each drift cell, the minimum time delay for signals relative to the trigger, accounting for the drift velocity within the cell. The accuracy of the calibration procedure is influenced by the random arrival time of the cosmic muons relative to the LHC clock cycle. A more refined analysis of the drift velocity was performed during the offline reconstruction phase, which takes into account this feature of cosmic ray events.en_US
dc.language.isoen
dc.relation.isversionofhttp://dx.doi.org/10.1088/1748-0221/5/03/T03016en_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.titleCalibration of the CMS drift tube chambers and measurement of the drift velocity with cosmic raysen_US
dc.typeArticleen_US
dc.identifier.citationChatrchyan, S. et al. "Calibration of the CMS drift tube chambers and measurement of the drift velocity with cosmic rays." Journal of Instrumentation 5 (March 2010): T03016 © 2010 IOP Publishing and SISSAen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Nuclear Science and Engineeringen_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.updated2019-06-19T11:46:43Z
dspace.date.submission2019-06-19T11:46:44Z
mit.journal.volume5en_US


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