H->bb Weekly Meeting Ricardo Gonçalo (RHUL) HSG5 H->bb weekly meeting, 16 August 2011.

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Presentation transcript:

H->bb Weekly Meeting Ricardo Gonçalo (RHUL) HSG5 H->bb weekly meeting, 16 August 2011

News! News! News! Peak stable lumi 2.2x10 33 cm -2 s -1 LHC delivered about 0.5fb -1 in one week! 2.3fb -1 with stable beams collected so far Peak pileup around 12 – bunches in the machine – maximum for 50ns Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20112

News! News! News! Our H->bb poster for LP2011 got cancelled for lack of presenter…  It turned out that Dilip could not present 2 posters (he was already presenting one for HSG3) Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20113

News! News! News! Top group tools Some uniformization of non-Athena code is being tried by the top group: – Using RootCore package to provide a common way to build Root-based code for top analyses. – See: Benefits: – Most of the Makefile is written in one place – Dependencies are resolved and the packages are built automatically in order – Given one package the others are checked out as needed – All package dependencies can be built in one go Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20114

News! News! News! Fast simulation workshop – Fast simulation will be more and more needed with increased statistics – Already successfully used for SUSY results for EPS – Workshop dedicated to fast simulations and the new integrated simulation framework on 7 th September 2011: Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20115

News! News! News! Trigger problems in run Prescale information on run is wrong in AODs, ESDs and D3PDs filled using TrigDecisionTool Trigger decision information is correct Luminosity information for this run should only be obtained from LumiCalc: This problem will be corrected in rel.17 reprocessing Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20116

Trigger! Be worried! Be very worried! Higher-threshold triggers in use since period K – 3x10 33 prescale set used since 4 th August, run – Several combined MET chains and and L1_MU10 unprescaled in last part of each fill Single-electron triggers will use isolation – Problem for fake electron background estimation – Nice page from Will Bell (top group) with list of planned studies: Triggers Triggers A new sample T was just produced for trigger studies – Using AtlasTrigMC cache; AMI tag: r2597 – Sample names start with "valid”: valid1.*.recon.AOD.e598_s933_s946_r2597_tid… – Useful for looking at recent changes for the 3e33 menu (e.g. e22_medium, e22_medium1, etc) – Similar sample may be produced with 17.0.X.Y if there’s enough popular demand – See: Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20117 Disabled or prescaled from run : 2b10_medium_4L1J10 2b10_medium_L1_2J10J50 2b10_medium_3L1J20 2e12_medium 2mu4_DiMu 3b15_loose_4L1J15 3j75_a4tc_EFFS L1FJ75_NoAlg e15_medium_e12_medium e20_loose e20_loose1 e20_looseTrk e20_medium e20_medium1 e20_medium2 e20_medium_SiTrk e20_medium_TRT e7_tight_e14_etcut_Jpsi g40_loose_EFxe40_noMu ht350_a4tc_EFFS_L2je255 j100_a4tc_EFFS_ht350 j75_2j30_a4tc_EFSF_ht350 j75_j30_a4tc_EFFS_anymct150 j75_j30_a4tc_EFFS_anymct175 mu15i_medium tau100_medium tau125_medium tau16_loose tau16_loose_e15_medium tau16_loose_mu15 tau16_medium_mu10 tau29_loose

Data skims for H->bb We need to have data skims to avoid pain of running over too much data – both for inclusive and boosted analyses (ZH inclusive already using HSG2 skims) Plan to join the DPD train: – The code to produce DAODs or D3PDs should be in AtlasPhysics cache and fully tested – The production needs to be done with a single Reco_trf.py instruction (fully tested standalone) – Write the data to Higgs group space – DPD production done in Tier1 from AODs – Skims should be small enough for this to make sense Once code is running, need to get the ok from the Higgs conveners and production manager Should test asap on rel.16 AODs to be ready for production after reprocessing Any news on the skimming code? Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20118

Releases, data and Monte Carlo All 2011 data will be reprocessed with rel.17 – We should move to rel.17 and MC11 asap – Rel.17 MC11A validation samples available: tag r2585, MC samples: – Missing a few inclusive signal (WH/ZH) samples 135GeV for WH and ZH (since we have 130 and 140) Extend up to 150GeV? (σ×BR ≈0.05 – 10× smaller than at 115GeV) Re-do WH samples at 110 and 140 since the current ones were done with a lepton filter by mistake – MC samples for boosted channels Wbb background with Sherpa to compare to Alpgen – How much do we need? Who will prepare job options? Boosted VH signal – Only have WH (Herwig, m H =120GeV, p T H >150GeV) at the moment – What’s the status of this? ttH? VBF? Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/20119

Backup Slides Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/201110

Post-mortem of WH/ZH results M bb resolution is extremely poor – Should try to get a peak, but this needs work on jet (and b-jet) energy scale – Try to think about this together with jet/E T miss people – Could we improve other things in jet reco to improve m bb ? – In ZH->llbb could try to use ll vs bb p T balance to do in-situ calibration? B-tagging systematic uncertainty dominates by far – 16% vs 7-9% for JES and ≈1-2% others – Should be possible to improve this, since the error is dominated by the statistics used in b-tagging studies – Would improve limits by up to 25-30% – Think about this with b-tagging people Limits: must get help from roostats experts to understand the difference between expected and observed WH cuts on exactly 2 jets – A lot of signal is lost there – can it be improved? WH backgrounds: – Top and W+jets background estimate using simultaneous template fit to m bb sidebands (<80GeV and GeV) – Probably should try to also constrain jet energy scale from this fit – JES changes m bb distribution and could affect normalization of backgrounds – In light of H->WW results, should move upper sideband to e.g GeV – at m H =150GeV, σ*BR already 1/10 of value at 115GeV, but H->WW and H->bb resolution is very broad – Can top background be reduced further? ZH background from Z+bb seems irreducible – can it be improved? Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/201111

WH/ZH analysis plans We can still try to improve cut based analysis: – Get a m bb peak, improve b-tagging systematics, constrain JES in WH, etc… – Reduce top background in WH: Try using looser leptons or extending lepton id to forward region to veto tt->lvlvbb Loosen jet η cut (at |η| lvjjbb/jjjjjbb – But… must keep pileup and JVF in mind Reduce Z+bb background in ZH? Would probably need a clever new variable like cos * θ Then clearly we should include multivariate methods – Used intensively by Tevatron – e.g. use NN to target top background – may allow to relax 2-jet cut in WH – NN may also help in rejecting Z+bb background in ZH? – See if MV method can improve existing b-tagging Add more channels! – Can something be done with ZH->ννbb? Very good channel in Tevatron, but complex and mature analysis Academia Sinica group plans to work on this But trigger is the crucial part – Boosted VH is clearly the next thing to push! WH->lνbb and ZH->llbb, but also ZH->ννbb UCL and Edinburgh working on this – should be enough manpower now, but need to get results soon – ttH has been slowly building up in Glasgow – will push for this to happen together with Chris Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/201112

Boosted VH Data Format Had a phone meeting two weeks ago to discuss a common D3PD format for boosted VH analyses Will use “official” Jet/ETmiss D3PD maker code by Bertrand Capleau to produce SM W/Z D3PDs including jet substructure variables – – Filtered Cambridge-Aachen jets and their constituent jets etc – Need to run b-tagging on sub-jets – Edinburgh (Robert H.) working on this with help from UCL Then the idea is to make data skims to ease running on new data Ricardo GonçaloHSG5 H->bb Weekly Meeting - 16/8/201113