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next milestone (post Period D) - and toward the results in Moriond recommendation #70

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YasuyukiOkumura opened this issue Oct 1, 2015 · 0 comments

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@YasuyukiOkumura
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Dear Gabriel and Brian,

I summarized information in order to restart the Z+b-jet activity
Feel free to add and modify the information, and let's have a meeting to set the strategy up
( who will do what and by when? ) when everyone has time!

Data

  • Good runs list with 336pb-1 (v65 - September 23rd)
    https://atlasdqm.web.cern.ch/atlasdqm/grlgen/All_Good/data15_13TeV.periodAllYear_HEAD_DQDefects-00-01-02_PHYS_StandardGRL_All_Good.xml
  • available data runs
    279598
    data15_13TeV:data15_13TeV.00279598.physics_Main.merge.DAOD_JETM3.f628_m1497_p2419/
    279515
    data15_13TeV:data15_13TeV.00279515.physics_Main.merge.DAOD_JETM3.f628_m1497_p2425/
    279284
    data15_13TeV:data15_13TeV.00279284.physics_Main.merge.DAOD_JETM3.f628_m1497_p2425/
    279279
    data15_13TeV:data15_13TeV.00279279.physics_Main.merge.DAOD_JETM3.f628_m1497_p2425/
    279259
    data15_13TeV:data15_13TeV.00279259.physics_Main.merge.DAOD_JETM3.f628_m1497_p2419/
    279169
    data15_13TeV:data15_13TeV.00279169.physics_Main.merge.DAOD_JETM3.f628_m1497_p2419/
    278968
    data15_13TeV:data15_13TeV.00278968.physics_Main.merge.DAOD_JETM3.f628_m1497_p2425/
    278912
    data15_13TeV:data15_13TeV.00278912.physics_Main.merge.DAOD_JETM3.f628_m1497_p2419/
    278880
    data15_13TeV:data15_13TeV.00278880.physics_Main.merge.DAOD_JETM3.f628_m1497_p2425/
    276954
    data15_13TeV:data15_13TeV.00276954.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276952
    data15_13TeV:data15_13TeV.00276952.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276790
    data15_13TeV:data15_13TeV.00276790.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276778
    data15_13TeV:data15_13TeV.00276778.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276731
    data15_13TeV:data15_13TeV.00276731.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276689
    data15_13TeV:data15_13TeV.00276689.physics_Main.merge.DAOD_JETM3.f623_m1480_p2425/
    276511
    data15_13TeV:data15_13TeV.00276511.physics_Main.merge.DAOD_JETM3.f620_m1480_p2411/
    276416
    data15_13TeV:data15_13TeV.00276416.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276336
    data15_13TeV:data15_13TeV.00276336.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/
    276329
    data15_13TeV:data15_13TeV.00276329.physics_Main.merge.DAOD_JETM3.f620_m1480_p2411/
    276262
    data15_13TeV:data15_13TeV.00276262.physics_Main.merge.DAOD_JETM3.f620_m1480_p2425/

MC

  • powheg sample
    mc15_13TeV.361106.PowhegPythia8EvtGen_AZNLOCTEQ6L1_Zee.merge.DAOD_JETM3.e3601_s2576_s2132_r6765_r6282_p2401
    mc15_13TeV.361107.PowhegPythia8EvtGen_AZNLOCTEQ6L1_Zmumu.merge.DAOD_JETM3.e3601_s2576_s2132_r6765_r6282_p2401
    mc15_13TeV.361108.PowhegPythia8EvtGen_AZNLOCTEQ6L1_Ztautau.merge.DAOD_JETM3.e3601_s2576_s2132_r6765_r6282_p2401
  • sherpa sample (up to pT_{V} 500 GeV)
    mc15_13TeV.361372.Sherpa_CT10_Zee_Pt0_70_CVetoBVeto.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361373.Sherpa_CT10_Zee_Pt0_70_CFilterBVeto.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361374.Sherpa_CT10_Zee_Pt0_70_BFilter.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361375.Sherpa_CT10_Zee_Pt70_140_CVetoBVeto.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361376.Sherpa_CT10_Zee_Pt70_140_CFilterBVeto.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361377.Sherpa_CT10_Zee_Pt70_140_BFilter.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361378.Sherpa_CT10_Zee_Pt140_280_CVetoBVeto.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361379.Sherpa_CT10_Zee_Pt140_280_CFilterBVeto.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361380.Sherpa_CT10_Zee_Pt140_280_BFilter.merge.DAOD_JETM3.e3651_s2586_s2174_r6869_r6282_p2401
    mc15_13TeV.361381.Sherpa_CT10_Zee_Pt280_500_CVetoBVeto.merge.DAOD_JETM3.e4133_s2608_s2183_r6869_r6282_p2401
    mc15_13TeV.361382.Sherpa_CT10_Zee_Pt280_500_CFilterBVeto.merge.DAOD_JETM3.e4133_s2608_s2183_r6869_r6282_p2401
    mc15_13TeV.361383.Sherpa_CT10_Zee_Pt280_500_BFilter.merge.DAOD_JETM3.e4133_s2608_s2183_r6869_r6282_p2401

Information of the samples (dumped from AMI)
https://okumura.web.cern.ch/okumura/tmp/ZjetAmiDumpInfo.v20151001.txt

selection criteria harmonization

Shall we restart with p3 criteria? https://indico.cern.ch/event/449765/contribution/4/attachments/1163086/1675523/ZJet_Zbjet_insitu_update_JetEtmiss_30thSep.pdf

I guess the current electron channel is the easiest one to apply for our case, i.e.

  • pT_{2}<min(15, 0.2*pT_{1})
  • delta phi < Pi - 0.5
  • Z mass window 15 GeV

TO DO LIST

  • implement the uncertainty
    • lepton energy scale
    • lepton energy resolution
    • b-tag SF uncertainty
    • different generators (Powheg vs Sherpa)
  • implementation of bootstrap tool
  • have preliminary "complete" results

Time scale

The primary target will be including our results in Moriond recommendation.
This will need to be ready for collaboration in Christmas time scale,
and we need to have the results by the biggining of December with full data set!

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