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dc.contributor.authorDemir, Durmuş Ali
dc.contributor.authorCMS Collaboration
dc.date.accessioned2016-12-05T13:57:38Z
dc.date.available2016-12-05T13:57:38Z
dc.date.issued2010
dc.identifier.citationChatrchyan, S., Khachatryan, V., Sirunyan, A. M., Adam. W., Arnold, B., ...CMS Collaboration (2010). Alignment of the CMS muon system with cosmic-ray and beam-halo muons. Journal of Instrumentation, 5(3). doi:10.1088/1748-0221/5/03/T03020en_US
dc.identifier.issn1748-0221
dc.identifier.urihttp://doi.org/10.1088/1748-0221/5/03/T03020
dc.identifier.urihttp://hdl.handle.net/11147/2574
dc.description.abstractThe CMS muon system has been aligned using cosmic-ray muons collected in 2008 and beam-halo muons from the 2008 LHC circulating beam tests. After alignment, the resolution of the most sensitive coordinate is 80 microns for the relative positions of superlayers in the same barrel chamber and 270 microns for the relative positions of endcap chambers in the same ring structure. The resolution on the position of the central barrel chambers relative to the tracker is comprised between two extreme estimates, 200 and 700 microns, provided by two complementary studies. With minor modifications, the alignment procedures can be applied using muons from LHC collisions, leading to additional significant improvements.en_US
dc.description.sponsorshipCERN and other CMS Institutes; TÜBİTAK and TAEKen_US
dc.language.isoengen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionof10.1088/1748-0221/5/03/T03020en_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectMuon spectrometersen_US
dc.subjectLarge Hadron Collider (LHC)en_US
dc.subjectCompact Muon Solenoiden_US
dc.subjectMonte Carlo methoden_US
dc.titleAlignment of the CMS muon system with cosmic-ray and beam-halo muonsen_US
dc.typearticleen_US
dc.contributor.authorIDTR1918en_US
dc.contributor.iztechauthorDemir, Durmuş Ali
dc.relation.journalJournal of Instrumentationen_US
dc.contributor.departmentİYTE, Fen Fakültesi, Fizik Bölümüen_US
dc.identifier.volume5en_US
dc.identifier.issue3en_US


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