001434719 001__ 1434719
001434719 003__ SzGeCERN
001434719 005__ 20220810225057.0
001434719 0247_ $$2DOI$$a10.1088/1748-0221/7/01/T01003
001434719 0248_ $$aoai:cds.cern.ch:1434719$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
001434719 035__ $$9Inspire$$a1091609
001434719 041__ $$aeng
001434719 100__ $$aTaki, K$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 245__ $$aLuminosity determination in $\sqrt{s}$ = 7 TeV proton collisions using the LHCf Front Counter at LHC
001434719 260__ $$c2012
001434719 520__ $$aIn the Large Hadron Collider forward (LHCf) experiment, the luminosity is determined with the counting rates of detectors called Front Counter. During the LHCf physics operation at √s = 7 TeV in 2010, two series of calibration run in the conversion factors from the counting rate to the luminosity were carried out on 26th of April and 9th of May. Using the luminosities determined in the April and May scans with 5 % and 4 % accuracy, the conversion factors were determined with 5.0 % accuracy, providing the luminosity determination at the LHCf experiment with this accuracy.
001434719 540__ $$3publication$$aOpen Access$$aCC-BY-NC-SA-3.0$$uhttp://creativecommons.org/licenses/by-nc-sa/3.0/
001434719 542__ $$3publication$$dIOP$$g2012
001434719 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
001434719 693__ $$aCERN LHC$$eLHCf
001434719 690C_ $$aARTICLE
001434719 690C_ $$aCERN
001434719 690C_ $$aLHCf_Papers
001434719 700__ $$aAdriani, O$$uINFN, Florence$$uFlorence U.
001434719 700__ $$aBonechi, L$$uINFN, Florence
001434719 700__ $$aBongi, M$$uINFN, Florence
001434719 700__ $$aCastellini, G$$uINFN, Florence$$uFlorence U.
001434719 700__ $$0AUTHOR|(CDS)2072270$$9#BEARD#$$aD'Alessandro, R$$uINFN, Florence$$uFlorence U.
001434719 700__ $$aFukatsu, K$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aHaguenauer, M$$uEcole Polytechnique
001434719 700__ $$aItow, Y$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aKasahara, K$$uWaseda U., RISE
001434719 700__ $$aMase, T$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aKawade, K$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aRicciarini, S$$uINFN, Florence
001434719 700__ $$aMacina, D$$uCERN
001434719 700__ $$aMasuda, K$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aMenjo, H$$uKMI, Nagoya
001434719 700__ $$aMitsuka, G$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aMuraki, Y$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aNoda, K$$uINFN, Catania
001434719 700__ $$aPapini, P$$uINFN, Florence
001434719 700__ $$aPerrot, A L$$uCERN
001434719 700__ $$aSako, T$$uNagoya U., Solar-Terrestrial Environ. Lab.$$uKMI, Nagoya
001434719 700__ $$aShimizu, Y$$uWaseda U., RISE
001434719 700__ $$aSuzuki, K$$uNagoya U., Solar-Terrestrial Environ. Lab.
001434719 700__ $$aSuzuki, T$$uWaseda U., RISE
001434719 700__ $$aTamura, T$$uKanagawa U.
001434719 700__ $$aTorii, S$$uKanagawa U.
001434719 700__ $$aTricomi, A$$uINFN, Catania$$uCatania U.
001434719 700__ $$aTurner, W C$$uLBL, Berkeley
001434719 773__ $$cT01003$$pJINST$$v7$$y2012
001434719 8564_ $$uhttps://cds.cern.ch/record/1434719/files/1748-0221_7_01_T01003.pdf$$yIOP Open Access article
001434719 916__ $$sh$$w201213$$ya2012
001434719 960__ $$a13
001434719 980__ $$aARTICLE
001434719 980__ $$aLHCf_Papers