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Measurement of the Jet Energy Scale in the CMS experiment ... - IIHE

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CHAPTER 5: Estimat<strong>in</strong>g <strong>of</strong> <strong>the</strong> <strong>Jet</strong> <strong>Energy</strong> <strong>Scale</strong> Calibration Factor 1090.28%, for light quark and b quark jets respectively. These numbers are corrected for<strong>the</strong> non-unity width <strong>of</strong> <strong>the</strong> pull distributions, too. Therefore, <strong>the</strong> results <strong>of</strong> bias onboth <strong>the</strong> light and <strong>the</strong> b jet energy corrections, which were quoted <strong>in</strong> Table 5.6, arere-estimated us<strong>in</strong>g <strong>the</strong> corrected statistical errors and summarized <strong>in</strong> Table 5.13.∆ε expl(%) ∆ε estl(%) ∆ε estl− ∆ε expl(%)-8.67±0.23(stat.)±1.2(sys.) -10.12±0.18(stat.) -1.45±0.29(stat.)±1.2(sys.)∆ε expb(%) ∆ε estb(%)∆ε estb− ∆ε expb(%)-2.08±0.36(stat.)±2.5(sys.) -1.31±0.28(stat.) 0.77±0.46(stat.)±2.5(sys.)Table 5.13: The f<strong>in</strong>al estimated residual jet energy corrections obta<strong>in</strong>ed for 100pb −1 .The correspond<strong>in</strong>g expected residual corrections and <strong>the</strong> possible bias are also shown.The quoted estimated results are corrected for <strong>the</strong> non-unity width <strong>of</strong> <strong>the</strong> pull distributions.The systematical uncerta<strong>in</strong>ties on <strong>the</strong> expected results are mentioned s<strong>in</strong>ceone cannot fit <strong>the</strong> distributions <strong>of</strong> ∆ε expl,bbetter than <strong>the</strong> quoted values which shouldbe taken <strong>in</strong>to account when estimat<strong>in</strong>g <strong>the</strong> bias.Also <strong>in</strong> Table 5.13, <strong>the</strong> systematical uncerta<strong>in</strong>ty on <strong>the</strong> expected residual jet energycorrections are mentioned. S<strong>in</strong>ce one cannot fit <strong>the</strong> distributions <strong>of</strong> ∆ε expl,bbetter than<strong>the</strong> quoted uncerta<strong>in</strong>ties which have to be considered <strong>in</strong> <strong>the</strong> f<strong>in</strong>al estimation <strong>of</strong> <strong>the</strong> bias.5.6 A First Application on <strong>the</strong> 2010 Collision DataSo far, <strong>the</strong> method to estimate <strong>the</strong> residual jet energy scale calibration factors has been<strong>in</strong>troduced and <strong>the</strong> performance <strong>of</strong> <strong>the</strong> method on simulated data has been described.In this section, <strong>the</strong> method is applied for <strong>the</strong> first time on <strong>the</strong> collision data whichis accumulated <strong>in</strong> 2010 and correspond<strong>in</strong>g to 36pb −1 <strong>of</strong> proton-proton collisions at acenter <strong>of</strong> mass energy <strong>of</strong> 7 TeV. The event selection cuts are slightly different comparedto those <strong>in</strong>troduced <strong>in</strong> Section 4.4, and are listed <strong>in</strong> <strong>the</strong> next section. Also <strong>in</strong> order toillustrate how well <strong>the</strong> simulated data predict <strong>the</strong> collision data, some control plots areshown <strong>in</strong> Section 5.6.2 to compare <strong>the</strong> simulated versus collision data. The simulatedsamples which are compared to <strong>the</strong> collision data, are different from what have beenused <strong>in</strong> previous sections because <strong>the</strong>y need to match with <strong>the</strong> collision and detectorparameters <strong>in</strong> <strong>the</strong> low data tak<strong>in</strong>g period. They are listed <strong>in</strong> Table 5.14. Also <strong>the</strong>names <strong>of</strong> 2010 collision data sets are given <strong>in</strong> <strong>the</strong> same table.The method to estimate <strong>the</strong> residual jet energy correction factors has been alreadyapplied on <strong>the</strong> simulated data and <strong>the</strong> results are obta<strong>in</strong>ed for 100pb −1 <strong>of</strong> <strong>in</strong>tegratedlum<strong>in</strong>osity. Although <strong>the</strong> performance <strong>of</strong> <strong>the</strong> method was checked us<strong>in</strong>g a huge amount<strong>of</strong> statistics compared to <strong>the</strong> accumulated collision data, it is still <strong>in</strong>terest<strong>in</strong>g to <strong>in</strong>ves-

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