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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, K. A.
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.accessioned2019-07-10T17:32:03Z
dc.date.available2019-07-10T17:32:03Z
dc.date.issued2010-03
dc.date.submitted2009-10
dc.identifier.issn1748-0221
dc.identifier.urihttps://hdl.handle.net/1721.1/121569
dc.description.abstractThe CMS silicon tracker, consisting of 1440 silicon pixel and 15 148 silicon strip detector modules, has been aligned using more than three million cosmic ray charged particles, with additional information from optical surveys. The positions of the modules were determined with respect to cosmic ray trajectories to an average precision of 3-4 microns RMS in the barrel and 3-14 microns RMS in the endcap in the most sensitive coordinate. The results have been validated by several studies, including laser beam cross-checks, track fit self-consistency, track residuals in overlapping module regions, and track parameter resolution, and are compared with predictions obtained from simulation. Correlated systematic effects have been investigated. The track parameter resolutions obtained with this alignment are close to the design performance.en_US
dc.language.isoen
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/1748-0221/5/03/T03009en_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.titleAlignment of the CMS silicon tracker during commissioning with cosmic raysen_US
dc.typeArticleen_US
dc.identifier.citationChatrchyan, S. et al. "Alignment of the CMS silicon tracker during commissioning with cosmic rays." Journal of Instrumentation 5 (March 2010): T03009 © 2010 IOP Publishing Ltd 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.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-06-19T11:42:23Z
dspace.date.submission2019-06-19T11:42:24Z
mit.journal.volume5en_US


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