Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN...

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Update on Update on Beamtest 06 Beamtest 06 CU PSF study CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Gamma-ray Large Area Space Area Space Telescope Telescope Beam Test Worksop II May 15-17, 2006

Transcript of Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN...

Page 1: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

Update onUpdate on Beamtest 06 Beamtest 06 CU PSF studyCU PSF study

C. CecchiS. Germani

M. Pepe

Università di Perugia and INFN

Gamma-ray Large Area Gamma-ray Large Area Space TelescopeSpace Telescope

Beam Test Worksop II May 15-17, 2006

Page 2: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

Beam Test Worksop 2

Pisa, May 16th, 2006

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Simulated DataSimulated Data

BeamtestRelease v1r0801p0– PS simulation from beamtest06 v4r0 (updated)– 4.5M e- generated with E=2.5 GeV /angle(0°, 20°,

40°)– 4.5M e- generated with E= 1 GeV /angle– 800k e- from SLAC pipeline /angle(0°, 40°)

20°

40°

• Analyzed using Gleam v6r12 hit the towers at 3 different Beam Angles (0° and 40° are the same as Mass Production (SLAC))

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Basic Event SelectionBasic Event Selection

We used the Merit ntuple after adding PS variables

- goodCal = EvtEnergyCorr>20 && EvtEnergyCorr<BeamEnergy-goodNumTracks = TkrNumTracks > 0-goodTag = e_silicon[i] > 0 i=0, 3

e_silicon[0]e_silicon[1]

e_silicon[3]e_silicon[2]

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Vertex and TrackVertex and Track

• Good Vertex Merit Variable VtxStatus = 34 : 2 tracks vertex + two tracks share first

hit 162 : 34 + DOCA location lies inside track hits else use only BestTrack

After cuts we have roughly the same number of events in each of the two categories

Page 5: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Energy and DirectionEnergy and Direction

• Reconstructed Energy compare EvtEnergyCorr

TagEnergy (BeamEnergy – E_rec)

• Photon Direction derived using first two tag detectors (Ptag)

• PSF defined from angular error:

– good Vertex acos(Ptag·PVtx)

– best Track acos(Ptag·PTkr1)

Page 6: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Tagger Silicon DetectorTagger Silicon Detector

Page 7: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Angle Error (Vtx Scaled)Angle Error (Vtx Scaled)2 GeV (SLAC)

2.5 GeV

1 GeV

Page 8: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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McEnergy (e- 2.5 GeV)McEnergy (e- 2.5 GeV)

0 deg 40 deg

McEnergy =ΣMcEγ MultiGamma Any M_gamOne Gamma M_gam==1

The MultiGamma effect is small we can neglect to distinguish between 1 and multigamma events

Page 9: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Energy Rec. Comparison 1 Energy Rec. Comparison 1 GammaGamma

0 deg 40 deg

e- 2.5 GeVe- 2.5 GeV

Resolution of the tagger worse at low energies wrt EvtEnergy visible in the scaled PSF

Page 10: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Tagger EnergyTagger Energy

40 deg

Tagger Energy = BeamEnergy–E_rec

0 deg

e- 2.5 GeVe- 2.5 GeV

Page 11: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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EvtEnergyCorrEvtEnergyCorr

0 deg

40 deg

20 dege- 2.5 GeVe- 2.5 GeV

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McDirErr – Measured McDirErr – Measured DirErrDirErr

e- 2.5 GeVe- 2.5 GeVVtx EventsVtx Events

Page 13: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Tagger Selection (4Si vs Tagger Selection (4Si vs 2Si)2Si)

0 deg

Requiring e_silicon>0 (signal) only from the first two Tagger Planes does not affect the PSF !

e- 2.5 GeVe- 2.5 GeV

Page 14: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Electron Beam 2.5 GeV Electron Beam 2.5 GeV

Vtx Events

Tkr Events

Page 15: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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SLAC Mass Production vs 2.5 SLAC Mass Production vs 2.5 GeV GeV

Page 16: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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e- 2.5GeV – 2GeV – 1 GeVe- 2.5GeV – 2GeV – 1 GeV

Page 17: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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Evaluating PSF Evaluating PSF ErrorError

• The number of events within 68% is N68

• The error on N68 is ΔN68=sqrt(NTOT×0.68×(1-0.68)) [Binomial]

• ΔPSF68 is obtained computing the quantiles corresponding to a number of events equal to N68 ±ΔN68

68%

PSF68

Page 18: Update on Beamtest 06 CU PSF study C. Cecchi S. Germani M. Pepe Università di Perugia and INFN Gamma-ray Large Area Space Telescope Beam Test Worksop II.

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PSF Error one beam energy vs PSF Error one beam energy vs allall

Vtx 0 deg

Goal Error Level

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ConclusionConclusionss

• 1 and 2.5 GeV e- simulated on PG-farm 27M analysed • 2 GeV SLAC production 1.6M (e-) analysed

• No difference selecting 1 or M• Tag energy difference only on scaled PSF at low energies• Simulated and reconstructed energies gives same results on

PSF• Selection with only the first two silicon higher photon

energy

• Is 800K e-/angle/energy enough to reach 1% error on PSF?No at low energies...... At higher energies may depend on true rejection

• Cross check results using only not scaled PSF