LAr Response to pions: Data vs MC (work in progress) S.Paganis (Wisconsin) withIsabelle,Martin LAr+Tile H8 pion CTB Meeting, CERN, 19-April-2005.

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LAr Response to pions: Data vs MC (work in progress) S.Paganis (Wisconsin) withIsabelle,Martin LAr+Tile H8 pion CTB Meeting, CERN, 19-April-2005

19-Apr-2005LAr response to pions2 Analysis ( data+MC)  Run: GeV pions Fully combined, have shown previously problems in LAr rec. energy  Parabola Energy reconstruction 50MeV “cubicADCcut” in LArRawChannelSimpleBuilder.cxx  A2MEV numbers from EMTB  EMTB 3x3 clustering  No cluster corrections, No Long. weigths  No shower cuts yet.  MC New “pythonized” version (powerful) Charge collection corrections Tried to get “correct” beam profile … ADC2MEV in Digitization step (parabola is the default)

19-Apr-2005LAr response to pions3 Program Flow ( release ): Analysis C++ Package MC: ADC2MEV happens here Thanks to: Manuel Galas Final Physics Plots jobOptions.G4Ctb_Dig.py Reconstruction ESD and CBNT Data: ADC2MEV here CTB04 Data jobOptions.G4Ctb_Sim.py TBAnalysis on ESD miniCBNT +G4Apps

19-Apr-2005LAr response to pions4 ADC -> MeV for MC and Data (10.0.2) Monte Carlo Data Differences at present : 1.Difference in the Sampling Fractions 2.Different noise normalization due to ADC2MeV (small)

19-Apr-2005LAr response to pions5 ADC2MEV (Data vs MC) ADC2DACDAC2Volt Volts2  A  A2MeV How:Ramps uA/Volt Injection Resistor (t drift *W)/e  1/SF PS (EMB1) /R=0.114 nA 1250 S1 (EMB1) nA S2 (EMB1) nA S3 (EMB1) nA MC ADC2MEV(PS) = 7.0 MC ADC2MEV(S1) = 2.5 MC ADC2MEV(S2) = 12.0 Data ADC2MEV(PS) ~ 7.2 Data ADC2MEV(S1) ~ 2.4 Data ADC2MEV(S2) ~ vary 10.0,12.0,16.0

19-Apr-2005LAr response to pions6 How to get the SF for Data (an example) SF(Presampler <0.8)=t*W/e/1250 = SF(Accordion <0.8)=t*W/e/ =

19-Apr-2005LAr response to pions7 How to get the SF for MC  Since the Sampling Fractions are the same as for ATLAS Example, for Accordion eta<0.8, SF=  They are calculated (Geant4) assuming no upstream material and compensating for charge collection effects (ON by default) Eventually we must port them to the data stream, as part of the ADC2MEV factor

19-Apr-2005LAr response to pions8 Data: 3x3 LAr vs Total tile Energy Electrons

19-Apr-2005LAr response to pions9 Beam Profiles Can do better Data MC

19-Apr-2005LAr response to pions10 Cleaning cuts: any biases?  For reconstructed energy comparisons: E(MC) = Erec * SFmc/SFdata  For visible energy comparisons: E(MC) = Erec * SFmc E(data) = Erec * SFdata  muTag to remove muons  Etile+ELAr MIP cuts to remove muons  Etile>2GeV, to remove electrons (crude) Don’t want to use shower shape cuts yet (under study) Possible Long electron tail I studied the region Etile<2GeV and ELar<14GeV and I see small discrepancies (checking also with electrons)

19-Apr-2005LAr response to pions11 Known biases:  Tile MC has no noise.  For data a LAr drift time assumption is made to get the SF  LAr MC has noise but I haven’t checked how representative is of the data  Cuts on LAr energy cause a bias when scale and shape are different  Parabolic fit at low energies? ...

19-Apr-2005LAr response to pions12 MuTag: removes a portion of muons

19-Apr-2005LAr response to pions13 LAr Energy after simple cuts Data MC

19-Apr-2005LAr response to pions14 Zoom in the MIP region (before cuts) Uncorrected MC Corrected MC for Sampling Fraction (Rear situation that data looks better than MC!)

19-Apr-2005LAr response to pions15 Zoom in the “MIP” region (after cuts) MC is broader, slow rising: due to more noise or the parabola or …?

19-Apr-2005LAr response to pions16 Visible Energy per LAr Sampling Good Agreement All Samplings have problems in the noise region; but agreement is good away from it. Normalization away from the noise region

19-Apr-2005LAr response to pions17 Total visible Energy (LAr) Normalization away from the noise region

19-Apr-2005LAr response to pions18Summary  Reasonable agreement between Data and MC: Away from the noise/MIP region After properly correcting MC for Sampling Fraction difference (however it is data SF that needs to changed in ATHENA !)  Discrepancy between DATA and MC for very small depositions. Distributions around 0 Energy look different. It is possible that MC noise is larger (at least for the middle).  Fully contained pions are being checked together with electrons I am seeing a discrepancy in this run but I’m still checking