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CMS data processing workflows during an extended cosmic ray run

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, Teng
dc.contributor.authorMiller, Mark
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, Si
dc.contributor.authorYilmaz, Yetkin
dc.contributor.authorYoon, A. S.
dc.contributor.authorCMS Collaboration
dc.contributor.authorNahn, Steven
dc.date.accessioned2019-07-03T18:51:23Z
dc.date.available2019-07-03T18:51:23Z
dc.date.issued2010-03
dc.date.submitted2009-11
dc.identifier.issn1748-0221
dc.identifier.urihttps://hdl.handle.net/1721.1/121490
dc.description.abstractThe CMS Collaboration conducted a month-long data taking exercise, the Cosmic Run At Four Tesla, during October-November 2008, with the goal of commissioning the experiment for extended operation. With all installed detector systems participating, CMS recorded 270 million cosmic ray events with the solenoid at a magnetic field strength of 3.8 T. This paper describes the data flow from the detector through the various online and offline computing systems, as well as the workflows used for recording the data, for aligning and calibrating the detector, and for analysis of the data.en_US
dc.language.isoen
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/1748-0221/5/03/T03006en_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.titleCMS data processing workflows during an extended cosmic ray runen_US
dc.typeArticleen_US
dc.identifier.citationChatrchyan et al. "CMS data processing workflows during an extended cosmic ray run." Journal of Instrumentation 5 (March 2010): T03006 © 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.updated2019-06-19T11:49:49Z
dspace.date.submission2019-06-19T11:49:50Z
mit.journal.volume5en_US


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