Update on Data vs MC comparison
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Transcript of Update on Data vs MC comparison
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Update on Data vs MC Update on Data vs MC comparisoncomparison
- 5 energies: 20, 50, 100, 180, - 5 energies: 20, 50, 100, 180, 250GeV250GeV
- Description of cuts and MC - Description of cuts and MC scalesscales
- Comparison: Data vs MC- Comparison: Data vs MC
- Appendix: detailed plots (not - Appendix: detailed plots (not presented)presented)
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Cuts applied Cuts applied Release 10.5.0, OFC-9, latest tags from Marco et Release 10.5.0, OFC-9, latest tags from Marco et
al.al. 3x3 EMTB cluster with ncells>663x3 EMTB cluster with ncells>66 Clock>2ns (except for 100GeV, 3-16ns)Clock>2ns (except for 100GeV, 3-16ns) MC scale factors:MC scale factors:
Eps_scaled = 0.8*11/13*Eps Etot_scaled = 0.98*Etotal
Data scale factors: Data scale factors: Estips_corrected = 0.92*Estrips
Ecell_tile < 1.5GeVEcell_tile < 1.5GeV MuTag < 500 countsMuTag < 500 counts MuHalo < 700 counts (for 180GeV, 250GeV runs MuHalo < 700 counts (for 180GeV, 250GeV runs
no effect)no effect) eta/phi cuts (next page)eta/phi cuts (next page)
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eta/phi cuts (see appendix)eta/phi cuts (see appendix)
20GeV:20GeV: 0.360<eta<0.375 && 0.005<phi<0.025
50GeV50GeV 0.362<eta<0.373 && 0.004<phi<0.020
100GeV100GeV 0.362<eta<0.373 && 0.004<phi<0.017
180GeV180GeV 0.378<eta<0.383 && 0.002<phi<0.008
250GeV250GeV 0.375<eta<0.381 && 0.002<phi<0.012
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Sampling Layer <Erec> vs Beam Sampling Layer <Erec> vs Beam EnergyEnergy
DataMC
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Period 5: 20, 50, 100, 180GeVPeriod 5: 20, 50, 100, 180GeV
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250 GeV from period 6250 GeV from period 6
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Resolution stochastic termResolution stochastic term
• Const = 0.5% (assumed)• Noise = 145MeV (low gain)• E vs Clock effect was not
included!
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<Erec> vs Beam energy<Erec> vs Beam energy
DataMC
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Data vs MC difference of mean Data vs MC difference of mean EnergyEnergy
Beam profiles notwell matched
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SummarySummary Data vs MC description in agreement to better Data vs MC description in agreement to better
than 0.5% for 20-250GeV electron energy rangethan 0.5% for 20-250GeV electron energy range Caution1: CTB has tails produced ustream our area which
make comparisons challenging Caution2: When raw energies are compared the beam profiles
in data vs MC must match because we have out-of-cluster losses that are different (in %) for strips,middle and PS.
Caution3: Our MC upstream material X0 assumption may be too high by 0.02X0 or so (fine tuning).
We have different material configurations so we We have different material configurations so we can put the Data vs MC comparison to the test can put the Data vs MC comparison to the test (see Walter’s talk)(see Walter’s talk)
Why we do this? We want to calibrate the MC Why we do this? We want to calibrate the MC first and apply the constants to the data. This first and apply the constants to the data. This should work if Data vs MC comparison is good.should work if Data vs MC comparison is good.
Cell to cell (region to region) final calibration must still be done in-situ with data (Z->ee, MIPs, etc) but this is just an overall scale factor.
All we need in 2007 is a good MC description of the ATLAS material (for example ID services, SCT LMTs, ...)
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AppendixAppendix
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Sampling Layers: 20GeVSampling Layers: 20GeV
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Sampling Layers: 50GeVSampling Layers: 50GeV
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Sampling Layers: 100GeVSampling Layers: 100GeV
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Sampling Layers: 180GeVSampling Layers: 180GeV
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Sampling Layers: 250GeVSampling Layers: 250GeV
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Estrips/Emiddle all energies Estrips/Emiddle all energies (period 5)(period 5)
20GeV 50GeV
100GeV 180GeV
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Estrips/Emiddle (250GeV period Estrips/Emiddle (250GeV period 6)6)
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Eta/phi comparison (20GeV)Eta/phi comparison (20GeV)
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Eta/phi comparison (50GeV)Eta/phi comparison (50GeV)
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Eta/phi comparison (100GeV)Eta/phi comparison (100GeV)
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Eta/phi comparison (180GeV)Eta/phi comparison (180GeV)
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Eta/phi comparison (250GeV)Eta/phi comparison (250GeV)
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Energy vs ClockEnergy vs Clock
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Erec vs Clock: 250 GeVErec vs Clock: 250 GeV
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Remove MuHalo cut for 100GeVRemove MuHalo cut for 100GeV
Tails in Erec increase and we loose in resolution