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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 III Jun 28-30, 2006. Jan Conrad Study.
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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 III Jun 28-30, 2006
Jan Conrad Study • Jan studied the statistical properties of the Fit (with Toby’s function) and Counting (histogram quantiles) method for the PSF error estimation. • He generated random data followinf Toby’s and Landau’s function and then applied the two methods: • Fit for Toby’s Function • Counting for Landau’s function Conclusion: The two methods give consistent results
Our Mc Data • Tagged gammas: • 4.5 M e- /angle (0, 20, 40 deg) • Beam Energy 1 GeV and 2.5 GeV • do not cover all the energy range • but we (almost) have the two ends of the energy spectrum
Tagger Resolution: Close End setup From L. Latronico, G. Spandre, A. Brez VRVS 20 Jun 2006 Align at close end (beam on Al window) The range for 2500 MeV Beam has been extrapolated
Tagger Resolution: Far End setup From L. Latronico, G. Spandre, A. Brez VRVS 20 Jun 2006 Align at far end (beam away from Al frame) The range for 2500 MeV Beam has been extrapolated
Tail Structure PSF Fit Thanks Benoit !!
PSF68 - Beam 0 Deg – Close End Front Back Number of Gammas within the Energy Acceptance Range
200k 250k PSF68 - Beam 0 Deg – Close End Front Back
PSF95 – Beam 0 Deg – Close Enad Front Back
PSF95 – Beam 0 Deg – Close End Front Back
200k 400k PSF68 - Beam 40 Deg – Close End Front Back
PSF95 - Beam 40 Deg – Close End Front Back
PSF68 - Beam 0 Deg – Far End Front Back
200k 250k PSF68 - Beam 0 Deg – Far End Front Back
250k 300k PSF68 - Beam 40 Deg – Far End Front Back
25k 30k If NumTracks>0 PSF68 - Beam 0 Deg – Close End If the Trigger could Select only events with NumTracks>0 Front Back
25k 40k If NumTracks>0 PSF68 - Beam 40 Deg – Close End Front If the Trigger could Select only events with NumTracks>0 Back
25k 30k If NumTracks>0 PSF68 - Beam 0 Deg – Far End If the Trigger could Select only events with NumTracks>0 Front Back
30k 50k If NumTracks>0 PSF68 - Beam 40 Deg – Far End If the Trigger could Select only events with NumTracks>0 Front Back
Statistics Summary Tables Ask For 250-300k per Beam Energy ? Ask For 30-40k per Beam Energy ?
Jan Conrad Study II As Jan anticipated the Fit and Counting method lead to similar errors Jan is talking about events in the histograms therefore we have to compare his results with ours for NumTracks>0 Since we divided front and back events and we are dealing with “real” Mc Data, Jan’s estimation of 10k events to reach the 1% error level is in agreement with our result (events in histogram ~30k/2 )
Beam Position Tower Border Tower Center Tower Crack
Tower Center – Tower Border PSF68 Beam 2.5 GeV – 0 deg Front Back
Tower Center – Tower Crack Front PSF68 Beam 2.5 GeV – 0 deg Back
MCS Options Comparison Front
Conclusions • Number of needed gammas: • seems to be almost independent from the Beam Energy and the Tagger setup (close end, far end) • needed gammas within energy acceptance: • 250 k • 30 k if NumTracks>0 • Beam Position: • Tower Border seems not to affect the PSF • maybe our beem was too far from the Tower edge • Tower Crack affect performances • smaller efficiency • bigger amount of dead material spoil PSF • Multiple gammas: • affect the PSF • way to select single gammas not found yet • MCS: • small difference between Native G4 and OLD32 • difference bigger than 1%
Final Remarks and Wishes • From our experience different positions (except tower cracks) should not affect significantly the PSF • Energy and angle dependency are rather smooth • Angular error tails have complex structures (see also Emanueles’ Talk) • we would prefer to have few well measured pointsin order to study the tails accurately • Minimal Configurations Proposal: • Tower Center • 0 deg , 40 deg • Number of gammas in the energy acceptance • 250k/ BeamEnergy • 30k/ BeamEnergy if NumTracks>0 • Extra useful configureations (peresonal priority order): • Higher number of gammas will allow to study the PSF tails more deeply • 60 deg Beam (enahnce thick layers conversion and PSF tails…) • Tower Crack @ 0 deg