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

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62 CHAPTER 4: Reconstruct<strong>in</strong>g and Select<strong>in</strong>g Physics Event#Events410310tt+jets semi-ele (1022.1 entries)tt+jets o<strong>the</strong>r (310.1 entries)t+jets, (all channels) (149.1 entries)Z+jets (1045.4 entries)W+jets (5314.5 entries)Multi-jets (12144.0 entries)210101-110-0.5 0 0.5 1 1.5 2 2.5 3 3.5 4 4.5Nr. <strong>of</strong> Loose MuonsFigure 4.13: Muon multiplicity per event which passed <strong>the</strong> Second Electron Veto cut.At Least Four <strong>Jet</strong>sAt <strong>the</strong> pre-selection step, all events are required to have at least four reconstructed jets<strong>in</strong> <strong>the</strong>ir f<strong>in</strong>al states. By tighten<strong>in</strong>g <strong>the</strong> thresholds on <strong>the</strong> jet k<strong>in</strong>ematics and also by apply<strong>in</strong>gsome identification criteria, <strong>the</strong> probability <strong>of</strong> select<strong>in</strong>g <strong>the</strong> four jets orig<strong>in</strong>at<strong>in</strong>gfrom <strong>the</strong> quarks com<strong>in</strong>g out <strong>of</strong> <strong>the</strong> hard scatter<strong>in</strong>g process becomes higher. The eventis required to have at least four selected jets with p T greater than 30GeV. Also jets,<strong>in</strong> order to be labeled as selected, are asked to pass identification cuts that are brieflydescribed below.• f EM which is called <strong>the</strong> electromagnetic energy fraction and is def<strong>in</strong>ed as <strong>the</strong>fraction <strong>of</strong> <strong>the</strong> jet energy measured <strong>in</strong> <strong>the</strong> ECAL. This parameter is useful <strong>in</strong>differentiat<strong>in</strong>g between electrons and jets s<strong>in</strong>ce jets with a high value <strong>of</strong> f EMprobably are electrons with energy deposits also used <strong>in</strong> <strong>the</strong> jet reconstructionalgorithm. The upper limit <strong>of</strong> this variable is set to be 0.9. Also <strong>in</strong> order tosuppress those jets which are actually pure electronic noise, a lower limit equalto 0.05 is put on this parameter.• n90Hits is def<strong>in</strong>ed as <strong>the</strong> m<strong>in</strong>imal number <strong>of</strong> reconstructed hits conta<strong>in</strong><strong>in</strong>g 90%<strong>of</strong> <strong>the</strong> jet energy and is ano<strong>the</strong>r observable that is used for <strong>the</strong> jet identification.The selected jets are required to have a n90Hits variable exceed<strong>in</strong>g 4.• f HPD is def<strong>in</strong>ed as <strong>the</strong> fraction <strong>of</strong> energy <strong>in</strong> <strong>the</strong> hottest HPD readout. The selectedjets are asked to fulfill f HPD < 0.98.The distributions <strong>of</strong> <strong>the</strong> various identification variables <strong>of</strong> all reconstructed jets forthose events that already passed <strong>the</strong> Muon Veto cut, are shown <strong>in</strong> Figure 4.14.Look<strong>in</strong>g at <strong>the</strong> distribution <strong>of</strong> <strong>the</strong> electromagnetic energy fraction, <strong>the</strong>re is a clearpeak at ∼1 represent<strong>in</strong>g <strong>the</strong> electrons which are re-reconstructed as jets. Ano<strong>the</strong>r plotthat shows <strong>the</strong> jet collection <strong>in</strong>cludes electrons and <strong>the</strong>refore needs to be cleaned, is<strong>the</strong> distance between <strong>the</strong> selected electron and <strong>the</strong> closest jet among all reconstructed

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