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CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$

The calibration of the luminosity measurement by the CMS experiment in the 2018 proton-proton data taking at $\sqrt{s} = 13~\mathrm{TeV}$ is described. The principal calibration is derived from the analysis of the van der Meer scan program in CMS taken during LHC fill 6868. In addition, the performa...

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Autor principal: CMS Collaboration
Publicado: 2019
Materias:
Acceso en línea:http://cds.cern.ch/record/2676164
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author CMS Collaboration
author_facet CMS Collaboration
author_sort CMS Collaboration
collection CERN
description The calibration of the luminosity measurement by the CMS experiment in the 2018 proton-proton data taking at $\sqrt{s} = 13~\mathrm{TeV}$ is described. The principal calibration is derived from the analysis of the van der Meer scan program in CMS taken during LHC fill 6868. In addition, the performance and stability of the CMS luminometers are also evaluated using emittance scans taken throughout the course of the year. The systematic uncertainty in the absolute calibration from the van der Meer scan is derived with a precision of $2.1\%$, with the dominant contribution to the uncertainty arising from the $x$-$y$ nonfactorization of the beam shape. The total systematic uncertainty, including terms from stability and linearity effects, is $2.5\%$.
id cern-2676164
institution Organización Europea para la Investigación Nuclear
publishDate 2019
record_format invenio
spelling cern-26761642019-09-30T06:29:59Zhttp://cds.cern.ch/record/2676164CMS CollaborationCMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$Detectors and Experimental TechniquesThe calibration of the luminosity measurement by the CMS experiment in the 2018 proton-proton data taking at $\sqrt{s} = 13~\mathrm{TeV}$ is described. The principal calibration is derived from the analysis of the van der Meer scan program in CMS taken during LHC fill 6868. In addition, the performance and stability of the CMS luminometers are also evaluated using emittance scans taken throughout the course of the year. The systematic uncertainty in the absolute calibration from the van der Meer scan is derived with a precision of $2.1\%$, with the dominant contribution to the uncertainty arising from the $x$-$y$ nonfactorization of the beam shape. The total systematic uncertainty, including terms from stability and linearity effects, is $2.5\%$.CMS-PAS-LUM-18-002oai:cds.cern.ch:26761642019
spellingShingle Detectors and Experimental Techniques
CMS Collaboration
CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$
title CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$
title_full CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$
title_fullStr CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$
title_full_unstemmed CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$
title_short CMS luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{TeV}$
title_sort cms luminosity measurement for the 2018 data-taking period at $\sqrt{s} = 13~\mathrm{tev}$
topic Detectors and Experimental Techniques
url http://cds.cern.ch/record/2676164
work_keys_str_mv AT cmscollaboration cmsluminositymeasurementforthe2018datatakingperiodatsqrts13mathrmtev