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---+!! Analyzing Monojet Dark Matter %TOC% ---++ Purpose of this page In order to have information about the steps of the analysis centralized, we could write down any significant information, making it up to dated. ---++ How to produce ntuples ---+++ How to produce distributions from LHE %RED% Will come soon. %ENDCOLOR% ---+++ How to do full simulation %RED% Will come soon. %ENDCOLOR% ---+++ Producing Ntuples from !MiniAOD These are the instruction on how to create Ntuples from !MiniAOD via !CRAB3. %TWISTY{ mode="div" showlink="Show " hidelink="Hide " class="twikiHelp" showimgright="%ICONURLPATH{toggleopen-small}%" hideimgright="%ICONURLPATH{toggleclose-small}%" }% First, setup the working area (instruction from Chang-Seong): <verbatim> cmsrel CMSSW_7_4_1 cd CMSSW_7_4_1/src cmsenv git cms-merge-topic 9003 rm -rf RecoEgamma/ElectronIdentification/data git clone https://github.com/cms-data/RecoEgamma-ElectronIdentification.git RecoEgamma/ElectronIdentification/data rm -rf RecoEgamma/PhotonIdentification/data git clone https://github.com/cms-data/RecoEgamma-PhotonIdentification.git RecoEgamma/PhotonIdentification/data </verbatim> Copy directory from Angelo's public are using scp: =assantos@access.sprace.org.br:/home/assantos/Public/DarkMatter/WorkingAread_27Jul2015/MonoXAnalysis/= If wanting to produce Ntuples in signal region (0) or control region (1), edit file =MonoXAnalysis/AnalysisStep/plugins/MonoJetTreeMaker.cc= selecting <verbatim> cleanMuonJet=0; // (1) for Muon control regtion // (0) for Muon signal regtion cleanElectronJet=0; // (1) for Electron control regtion // (0) for Electron signal regtion cleanPhotonJet=0; // (1) for Photon control regtion // (0) for Photon signal regtion </verbatim> Then compile the working area: =scramv1 b -j 10=. Then go to =MonoXAnalysis/AnalysisStep/test/= and apply the proper modifications in =tree.py= and =crabConfig.py= if running over Data or MC. Current !JSON files are: * [[https://cms-service-dqm.web.cern.ch/cms-service-dqm/CAF/certification/Collisions15/13TeV/Cert_246908-251883_13TeV_PromptReco_Collisions15_JSON.txt][Golden JSON files]] * [[https://cms-service-dqm.web.cern.ch/cms-service-dqm/CAF/certification/Collisions15/13TeV/Cert_246908-251883_13TeV_PromptReco_Collisions15_JSON_MuonPhys_v2.txt][JSON files for Muon Physics]] Setup CRAB with =source /cvmfs/cms.cern.ch/crab3/crab.sh= and submit jobs with =crab submit -c crabConfig.py=. For further details on how to work with CRAB3, see [[https://twiki.cern.ch/twiki/bin/view/CMSPublic/WorkBookCRAB3Tutorial][here]]. %ENDTWISTY% ---++ Samples for Run2 (data, background and signal) ---+++ List of samples from Data Run2 The following table contains the list of Data samples (=Run2015B-PromptReco-v1=), as well as the correspondent number of events and luminosity. | *Data Run2 (Run2015B-PromptReco-v1 from DAS)* | *Number of events (from DAS)* | *Luminosity (1/pb)* | | =/MET/Run2015B-PromptReco-v1/MINIAOD= | 299090 | 40.215 | | =/DoubleMuon/Run2015B-PromptReco-v1/MINIAOD= | 1631653 | 46.337 | | =/SingleMuon/Run2015B-PromptReco-v1/MINIAOD= | 3633477 | 46.337 | | =/DoubleEG/Run2015B-PromptReco-v1/MINIAOD= | 5018488 | 40.240 | | =/SingleElectron/Run2015B-PromptReco-v1/MINIAOD= | 2718409 | 40.240 | | =/SinglePhoton/Run2015B-PromptReco-v1/MINIAOD= | 737246 | 40.240 | These are the instructions to compute luminosity: %TWISTY{ mode="div" showlink="Show " hidelink="Hide " class="twikiHelp" showimgright="%ICONURLPATH{toggleopen-small}%" hideimgright="%ICONURLPATH{toggleclose-small}%" }% Firstly, run <verbatim> crab report -d <path_to_your_crab_directory/> </verbatim> You get a file in =lumiSummary.json= format inside =<path_to_your_crab_directory/results/>=. Then, copy file =lcr2.py= from =/afs/cern.ch/user/m/marlow/public/lcr2/= into your =lxplus= and run =python lcr2.py -i lumiSummary.json= which will show the luminosity for that dataset. For further details, see [[https://twiki.cern.ch/twiki/bin/view/CMS/lcr2][here]]. %ENDTWISTY% The following table shows the paths to the Data Ntuples in =T2_SPRACE= which includes events after the good vertex selection: * =offlineSlimmedPrimaryVertices= * =!isFake && ndof > 4 && abs(z) < 24 && position.Rho < 2= | *Path of Ntuple for Data Run2 (Run2015B-PromptReco-v1) in T2_SPRACE* | *Number of events* | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/MET_Run2015B.root= | 137584 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/DoubleMuon_Run2015B.root= | 1152197 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/SingleMuon_Run2015B.root= | 2010988 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/DoubleEG_Run2015B.root= | 4773783 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/SingleElectron_Run2015B.root= | 2217177 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/SinglePhoton_Run2015B.root= | 561242 | %RED% The following table contains the list of Data samples (=Run2015B-17Jul2015-v1=) *INTENDED* to be produced in Ntuple format, as well as the correspondent number of events and luminosity. According to [[https://twiki.cern.ch/twiki/bin/view/CMSPublic/WorkBookMiniAOD2015#ETmiss_filters][MiniAOD Analysis Documentation]], this datasets correctly include E<sub>T</sub><sup>missing</sup> filters. It is important to use the recommendations provided by MET group concerning Spring15 MC and 50 ns about: %ENDCOLOR% * [[https://twiki.cern.ch/twiki/bin/viewauth/CMS/MissingETRun2Corrections][Met corrections for Run-II]]; and * [[https://twiki.cern.ch/twiki/bin/viewauth/CMS/MissingETOptionalFiltersRun2][MET Filters for Run II]]. | *Data Run2 (Run2015B-17Jul2015-v1 from DAS)* | *Number of events (from DAS)* | *Luminosity (1/pb)* | | =/MET/Run2015B-17Jul2015-v1/MINIAOD= | 75938 | | | =/DoubleMuon/Run2015B-17Jul2015-v1/MINIAOD= | 497402 | | | =/SingleMuon/Run2015B-17Jul2015-v1/MINIAOD= | 1039658 | | | =/DoubleEG/Run2015B-17Jul2015-v1/MINIAOD= | 4567275 | | | =/SingleElectron/Run2015B-17Jul2015-v1/MINIAOD= | 1027225 | | | =/SinglePhoton/Run2015B-17Jul2015-v1/MINIAOD= | 323203 | | ---+++ List of MC samples for background (Run2 Spring15) The following table contains the list of MC background samples (Run2 Spring15) with correspondent number of events and cross sections (from different sources). As mentioned in the [[https://twiki.cern.ch/twiki/bin/view/CMS/ExoDiBosonResonancesRun2#Backgrounds][Exo Diboson twiki page]], _"If only the lepton decay of the W is included in the sample, the cross section is multiplied by BR(W->lv) = 0.322 with l = e, mu, tau"_, and the references for cross sections come from: * [1] https://twiki.cern.ch/twiki/bin/viewauth/CMS/StandardModelCrossSectionsat13TeVInclusive * [2] https://twiki.cern.ch/twiki/bin/view/LHCPhysics/TtbarNNLO * [3] https://twiki.cern.ch/twiki/bin/viewauth/CMS/SingleTopSigma * [4] [[https://cmsweb.cern.ch/das/][DAS]] | *MC Background Spring15 (from DAS)* | *Number of events (from !DAS)* | *Cross Section (pb) from DAS* | *Cross Section (pb) from other reference* | | =/WJetsToLNu_TuneCUETP8M1_13TeV-amcatnloFXFX-pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 24089991 | 60290 | 61526.7 (NNLO) [1] | | =/TTJets_TuneCUETP8M1_13TeV-madgraphMLM-pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 4992231 | 502.2 | 502.2 (NNLO) [2] | | =/ST_t-channel_top_4f_leptonDecays_13TeV-powheg-pythia8_TuneCUETP8M1/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 1273800 | 103.02 | 136.02*0.322 (NLO) [3] | | =/ST_t-channel_antitop_4f_leptonDecays_13TeV-powheg-pythia8_TuneCUETP8M1/RunIISpring15DR74-Asympt25ns_MCRUN2_74_V9-v1/MINIAODSIM= | 1695400 | 80.95 | 80.95*0.322 (NLO) [3] | | =/ST_tW_top_5f_inclusiveDecays_13TeV-powheg-pythia8_TuneCUETP8M1/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 998400 | 38.09 | 35.6 (NNLO) [3] | | =/ST_tW_antitop_5f_inclusiveDecays_13TeV-powheg-pythia8_TuneCUETP8M1/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= | 1000000 | 38.09 | 35.6 (NNLO) [3] | | =/WW_TuneCUETP8M1_13TeV-pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 989608 | 63.21 | 118.7 (NNLO) [1] | | =/WZ_TuneCUETP8M1_13TeV-pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= | 996920 | 22.82 | 66.1 (NLO) [1] | | =/ZZ_TuneCUETP8M1_13TeV-pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= | 998848 | 10.32 | 15.4 (NLO) [1] | | =/QCD_Pt_120to170_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 3446207 | 471100 | --- | | =/QCD_Pt_170to300_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= %RED% (Being produced)%ENDCOLOR% | 3438066 | 117276 | --- | | =/QCD_Pt_300to470_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 2930578 | 7823 | --- | | =/QCD_Pt_470to600_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= %RED%(Being produced)%ENDCOLOR% | 1939229 | 648.2 | --- | | =/QCD_Pt_600to800_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= %RED%(Being produced)%ENDCOLOR% | 1890256 | 186.9 | --- | | =/QCD_Pt_800to1000_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= %RED%(Being produced)%ENDCOLOR% | 1911296 | 32.293 | --- | | =/QCD_Pt_1000to1400_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= %RED%(Being produced)%ENDCOLOR% | 1461216 | 9.4183 | --- | | =/QCD_Pt_1400to1800_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 197959 | 0.84265 | --- | | =/QCD_Pt_1800to2400_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 194924 | 0.114943 | --- | | =/QCD_Pt_2400to3200_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 198383 | 0.00682981 | --- | | =/QCD_Pt_3200toInf_TuneCUETP8M1_13TeV_pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v1/MINIAODSIM= | 188696 | 0.000165445 | --- | | =/DYJetsToLL_M-50_TuneCUETP8M1_13TeV-amcatnloFXFX-pythia8/RunIISpring15DR74-Asympt50ns_MCRUN2_74_V9A-v2/MINIAODSIM= | 19925500 | 6104 | 6025.2 (NNLO) [1] | The following table shows the paths to the MC background Ntuples in =T2_SPRACE= site which includes events after the good vertex selection: * =offlineSlimmedPrimaryVertices= * =!isFake && ndof > 4 && abs(z) < 24 && position.Rho < 2= | *Path of Ntuple for MC Spring15 in T2_SPRACE* | *Number of events* | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/WJetsToLNu.root= | 24089978 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/TTJets.root= | 4992231 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/ST_t-channel_top_4f_leptonDecays.root= | 1273800 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/ST_t-channel_antitop_4f_leptonDecays.root= | 1695400 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/ST_tW_top_5f_inclusiveDecays.root= | 998400 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/ST_tW_antitop_5f_inclusiveDecays.root= | 1000000 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/WW.root= | 989608 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/WZ.root= | 996920 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/ZZ.root= | 998847 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/QCD_Pt_120to170.root= | 3446207 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/QCD_Pt_300to470.root= | 2930577 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/QCD_Pt_1400to1800.root= | 197959 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/QCD_Pt_1800to2400.root= | 194924 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/QCD_Pt_2400to3200.root= | 198383 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/QCD_Pt_3200toInf.root= | 188696 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/RunIISamples_25Jul2015/Ntuples_DataMC_27Jul2015/DYJetsToLL_M-50.root= | 19925488 | ---+++ List of MC samples for background (Phys14) The following table contains the list of MC background samples (Phys14) with correspondent number of events and cross sections. | *MC Background Phy14 (from DAS)* | *Number of events (from !DAS)* | *Cross Section (pb) from DAS* | | =/ZJetsToNuNu_HT-100to200_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4986424 | 372.6 | | =/ZJetsToNuNu_HT-200to400_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4546470 | 100.8 | | =/ZJetsToNuNu_HT-400to600_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v2/MINIAODSIM= | 4433784 | 11.99 | | =/ZJetsToNuNu_HT-600toInf_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4463806 | 4.113 | | =/WJetsToLNu_HT-100to200_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 5262265 | 1817.0 | | =/WJetsToLNu_HT-200to400_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4936077 | 471.6 | | =/WJetsToLNu_HT-400to600_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4640594 | 55.61 | | =/WJetsToLNu_HT-600toInf_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4581841 | 18.81 | | =/TTJets_MSDecaysCKM_central_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 25446993 | 831.76 | | =/TToLeptons_s-channel-CSA14_Tune4C_13TeV-aMCatNLO-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 500000 | 2.3328 | | =/TToLeptons_t-channel-CSA14_Tune4C_13TeV-aMCatNLO-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 3991000 | 136.02 | | =/T_tW-channel-DR_Tune4C_13TeV-CSA14-powheg-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 986100 | 35.6 | | =/TBarToLeptons_s-channel-CSA14_Tune4C_13TeV-aMCatNLO-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 250000 | 1.34784 | | =/TBarToLeptons_t-channel_Tune4C_CSA14_13TeV-aMCatNLO-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 1999800 | 26.2278 | | =/Tbar_tW-channel-DR_Tune4C_13TeV-CSA14-powheg-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 971800 | 35.6 | | =/QCD_HT-100To250_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4123612 | 28730000 | | =/QCD_HT_250To500_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 971800 | 670500 | | =/QCD_HT-500To1000_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 849033 | 26740.0 | | =/QCD_HT_1000ToInf_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 333733 | 769.7 | | =/QCD_HT_250To500_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1_ext1-v2/MINIAODSIM= | 2004219 | 670500 | | =/QCD_HT-500To1000_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1_ext1-v1/MINIAODSIM= | 3214312 | 26740.0 | | =/QCD_HT_1000ToInf_13TeV-madgraph/Phys14DR-PU20bx25_PHYS14_25_V1_ext1-v1/MINIAODSIM= | 1130720 | 769.7 | | =/DYJetsToLL_M-50_HT-100to200_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4054159 | 194.3 | | =/DYJetsToLL_M-50_HT-200to400_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4666496 | 52.24 | | =/DYJetsToLL_M-50_HT-400to600_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4931372 | 6.546 | | =/DYJetsToLL_M-50_HT-600toInf_Tune4C_13TeV-madgraph-tauola/Phys14DR-PU20bx25_PHYS14_25_V1-v1/MINIAODSIM= | 4493574 | 2.179 | The following table shows the paths to the MC background Ntuples in =T2_SPRACE= site which includes events after the good vertex selection. | *Path of Ntuple for MC Phys14 in T2_SPRACE* | *Number of events* | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/ZJetsToNuNu_HT-100to200_PHYS14.root= | 4986410 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/ZJetsToNuNu_HT-200to400_PHYS14.root= | 4546455 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/ZJetsToNuNu_HT-400to600_PHYS14.root= | 4433769 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/ZJetsToNuNu_HT-600toInf_PHYS14.root= | 4463773 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/WJetsToLNu_HT-100to200_PHYS14.root= | 5262249 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/WJetsToLNu_HT-200to400_PHYS14.root= | 4936055 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/WJetsToLNu_HT-400to600_PHYS14.root= | 4640575 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/WJetsToLNu_HT-600toInf_PHYS14.root= | 4581825 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/TTJets_MSDecaysCKM_centra.root= | 25446877 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/TToLeptons_s-channel_PHYS14.root= | 499999 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/TToLeptons_t-channel_PHYS14.root= | 3990985 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/T_tW-channel-DR_PHYS14.root= | 986096 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/TBarToLeptons_s-channel_PHYS14.root= | 250000 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/TBarToLeptons_t-channel_PHYS14.root= | 1999793 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/Tbar_tW-channel-DR_PHYS14.root= | 971797 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT-100To250_PHYS14.root= | 4123591 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT_250to500_PHYS14.root= | 663953 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT_500to1000_PHYS14.root= | 849028 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT_1000toInf_PHYS14.root= | 333732 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT_250to500_ext1_PHYS14.root= | 2004211 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT_500to1000_ext1_PHYS14.root= | 3214303 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/QCD_HT_1000toInf_ext1_PHYS14.root= | 1130715 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/DYJetsToLL_HT-100to200_PHYS14.root= | 4054144 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/DYJetsToLL_HT-200to400_PHYS14.root= | 4666479 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/DYJetsToLL_HT-400to600_PHYS14.root= | 4931352 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/Backgrounds_18Jun2015/DYJetsToLL_HT-600toInf_PHYS14.root= | 4493550 | ---+++ List of MC samples for signal (i2HDM) The following table shows the path of MC samples for i2HDM signal in T2_SPRACE, as well as the number of generated events, the number events after the good primary vertex selection, and the cross section. There are samples considering cases of *%BLUE%h1h1%ENDCOLOR%* and *%BLUE%h1h2%ENDCOLOR%* DM production. | *Path of Ntuple for i2HDM signal in T2_SPRACE* | *Number of generated events (from LHE)* | *Number of events in level of Ntuple* | *Cross Section (pb)* | | *h1h1 DM production* |||| | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM1_h1h1j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.17 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM2_h1h1j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.77 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM3_h1h1j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.000043 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM4_h1h1j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.00012 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM5_h1h1j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.000023 | | *h1h2 DM production* |||| | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM1_h1h2j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.17 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM2_h1h2j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.77 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM3_h1h2j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.000043 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM4_h1h2j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.00012 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/I2HDM_13TeV/i2HDM_Ntuples_30Jul2015/i2hdm_BM5_h1h2j_13tev-single_Ntuple.root= | 50000 | 50000 | 0.000023 | ---+++ List of MC samples for signal (EFT) The following table shows the path of MC samples for EFT signal in T2_SPRACE, as well as the number of generated events, the number events after the good primary vertex selection, and the cross section (from [[https://twiki.cern.ch/twiki/bin/viewauth/CMS/Monojet][Monojet twiki page]]). These are samples with *%BLUE%Axial-Vector%ENDCOLOR%* and *%BLUE%Vector%ENDCOLOR%* cases. | *Path of Ntuple for EFT signal in T2_SPRACE* | *Events in MiniAOD (from DAS)* | *Number of events in level of Ntuple* | *Cross Section (pb)* | | *Axial-Vector* |||| | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet1_M-1_AV_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 194600 | 194598 | 9.5695x10-7 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet2_M-10_AV_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 190400 | 190399 | 9.5381x10-7 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet3_M-100_AV_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 190000 | 190000 | 8.0087x10-7 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet7_M-1000_V_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 194800 | 194798 | 4.6629x10-8 | | *Vector* |||| | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet5_M-10_V_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 191800 | 191799 | 9.5463x10-7 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet6_M-100_V_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 189400 | 189399 | 9.0451x10-7 | | =/pnfs/sprace.org.br/data/cms/store/user/adesouza/DarkMatter/EFT_Samples_30Jul2015/Monojet7_M-1000_V_Tune4C_13TeV_PU20bx25_tsg_PHYS14_25_V1.root= | 197200 | 197198 | 1.2438x10-7 | ---++ Kinematic selections This is the list of the [[https://twiki.cern.ch/twiki/bin/viewauth/CMS/Monojet][standard Monojet selection]] applied in the signal region: * 1 or 2 jets in the event * p<sub>T</sub>(Jet1) > 110 !GeV * !CH fraction > 0.2 * !NH fraction < 0.7 * !EM fraction < 0.7 * !CEM fraction < 0.99 * p<sub>T</sub>(Jet2) > 30 !GeV * !NH fraction < 0.7 * !EM fraction < 0.9 * ΔΦ(Jet1, Jet2) < 2.5 * lepton veto * photon veto * !MET > 200 !GeV (!PF !MET with Type-1 corrections) ---++ Kinematic distributions Here we create distributions from Ntuples ---+++ Results from Physics14 samples These figures were made with Physics14 samples for background while Spring15 samples are not ready. It does not have any selection other than good primary vertex. %TWISTY{ mode="div" showlink="Show " hidelink="Hide " class="twikiHelp" showimgright="%ICONURLPATH{toggleopen-small}%" hideimgright="%ICONURLPATH{toggleclose-small}%" }% <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_njets.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_t1pfmet.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljetpt.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_secondjetpt.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljeteta.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_secondjeteta.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_jetjetdphi.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_nvtx.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljetmetdphi.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_secondjetmetdphi.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljetCHfrac.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljetNHfrac.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljetEMfrac.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_signaljetCEMfrac.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_secondjetNHfrac.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_secondjetEMfrac.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_nmuons.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_nelectrons.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_ntaus.png" height="320" /> <img width="500" alt="" src="%ATTACHURL%/Results_NoSelection_nphotons.png" height="320" /> %ENDTWISTY% ---+++ Results from Run2 Spring15 samples See [[https://indico.cern.ch/event/438011/contribution/2/attachments/1138200/1630787/15.08.10_Monojet_DM_Chang-Seong_Moon_v3.pdf][Chang-Seong's presentation in the Monojet meeting on 10/Aug/2015]]. ---++ Computing limits As preliminary results, only statistical uncertainties are taken into acccount. ---+++ Results from Run2 Spring15 samples From preliminary results, the following figures show the expected limits using Spring15 MC samples for background. To compute these limits, we use the expected number of events got from [[https://indico.cern.ch/event/438011/contribution/2/attachments/1138200/1630787/15.08.10_Monojet_DM_Chang-Seong_Moon_v3.pdf][page 19 of Chang-Seong's presentation in the Monojet meeting on 10/Aug/2015]]. ---++++ Limits considering EFT Dark Matter model * Figure on the letf (right) shows theoretical cross-sections for Axial Vector (Vector) Dark Matter. It is considered *%BLUE%Lumi = 40.03 pb<sup>-1</sup>%ENDCOLOR%*. It takes into account the *%BLUE%standard Monojet selection%ENDCOLOR%* above, which leads to EFT signal samples with efficiencies from 11 to 14%. EFT signals present very low cross sections, as is showed in the table above. <img width="400" alt="" src="%ATTACHURL%/limit_EFT_AV_CS_Spring15_40invpb_11Aug2015.png" height="400" /> <img width="400" alt="" src="%ATTACHURL%/limit_EFT_V_CS_Spring15_40invpb_11Aug2015.png" height="400" /> * Now we show the same plots, but including observed limits. Since the signal is not optimized because we are using the *%BLUE%standard monojet selections%ENDCOLOR%*, the number of observed events (940) is higher than the total number of expected events (871), leading to observed limits (30 - 40 pb) higher than the expected median limits (20 - 28 pb). <img width="400" alt="" src="%ATTACHURL%/limit_EFT_AV_CS_Data_Spring15_40invpb_13Aug2015.png" height="400" /> <img width="400" alt="" src="%ATTACHURL%/limit_EFT_V_CS_Data_Spring15_40invpb_13Aug2015.png" height="400" /> * Figure on the letf (right) shows theoretical cross-sections for Axial Vector (Vector) Dark Matter. It is considered *%BLUE%Lumi = 5 fb<sup>-1</sup>%ENDCOLOR%*. It takes into account the *%BLUE%standard Monojet selection%ENDCOLOR%* above. EFT signal samples have from 11 to 14% of efficiency. As expected, the increasing in luminosity did not bring any significant improvement. <img width="400" alt="" src="%ATTACHURL%/limit_EFT_AV_CS_Spring15_5invfb_11Aug2015.png" height="400" /> <img width="400" alt="" src="%ATTACHURL%/limit_EFT_V_CS_Spring15_5invfb_11Aug2015.png" height="400" /> * Figure on the letf (right) shows theoretical cross-sections for Axial Vector (Vector) Dark Matter. It is considered *%BLUE%Lumi = 5 fb<sup>-1</sup>%ENDCOLOR%*. It takes into account the *%BLUE%standard Monojet selection above + E<sub>T</sub><sup>missing</sup> > 500 !GeV%ENDCOLOR%*. EFT signal samples have from 1.5 to 3% of efficiency. The high E<sub>T</sub><sup>missing</sup> cut improves the expected limits by 1 order of magnitude. The limits are between 0.3 and 0.6 pb, being compatible with the 0.4 pb found in the [[http://cms.cern.ch/iCMS/user/noteinfo?cmsnoteid=CMS%20AN-2015/072][Search for New Physics in Monojet Final State (AN-15-072)]]. <img width="400" alt="" src="%ATTACHURL%/limit_EFT_AV_CS_Spring15_5invfb_MET500_12Aug2015.png" height="400" /> <img width="400" alt="" src="%ATTACHURL%/limit_EFT_V_CS_Spring15_5invfb_MET500_12Aug2015.png" height="400" /> ---++++ Limits considering i2HDM model * This figure shows limits considering the i2HDM model (with different λ<sub>345</sub> for each mass point). It is considered *%BLUE%Lumi = 40.03 pb<sup>-1</sup>%ENDCOLOR%*. It takes into account the *%BLUE%standard Monojet selection%ENDCOLOR%* above, which leads to i2HDM signal samples with efficiencies from 17 to 21%. Expected limits are around 15 pb. <img width="400" alt="" src="%ATTACHURL%/limiti2HDM_CS_Spring15_40invpb_13Aug2015.png" height="400" /> -- %USERSIG{assantos - 2015-07-24}% ---++ Comments %COMMENT%
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Macro to create Ntuples from
MiniAOD
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