Transcript ppt
Gamma-ray Large Area Space Telescope Study of the ToT on the full LAT data sample: corrections & updates F. Loparco INFN Bari 1 What was wrong? • IA Workshop 6: • discrepancies between results in full LAT configuration and previous results • We did not take the ACD into account! (thanks Anders!) • Analysis cut correction: • muons are tagged by GemConditionWord=3 instead of GemConditionWord=2 2 List of the runs analyzed A data samples of 20 runs has been analyzed: 135005345, 135005347, 135005349, 135005351, 135005355, 135005357, 135005359, 135005363, 135005365, 135005367, 135005371, 135005373, 135005375, 135005377, 135005379, 135005381, 135005383, 135005385, 135005387, 135005389 These runs have been performed on Jan 14-15, 2006 in the B2 configuration 3 Event selection & definitions Event Selection: Trigger from 3 consecutive layers: GemConditionWord=2 = 3!!!! Single tower events: GemTkrVector[tower] ≠ 0 for only one tower Single muon tracks in the TKR: TkrNumTracks=1 Triggering Layers = Layers in both views from GltLayer (First Triggering Layer) to GltLayer+2 (Last Triggering Layer) Track Layers = Layers in both views from Tkr1FirstLayer (First layer in the track) to Tkr1LastLayer (Last layer in the track) 0 left ToT ToT right ToT left and right ToTs if both left and right ToT 0 or NA if right ToT 0 or NA if left ToT 0 or NA if both left and right ToTs 0 4 cosθ distributions In central bays tracks with large zenith angles are ruled out 5 Azimuth angle φ distributions Symmetries reflect the TKR geometry! 6 ToT distributions for triggering layers 7 Evaluation of the hit capture efficiency 1 - ε f(ToT 0) With the exception of bay 0, for all towers 1-ε < 0.1% 8 ToT vs track parameters Z Track length l 1/cos X Projected track length Y l cos 2 sin 2 cos 2 , for X layers l' 2 2 2 l cos sin sin , for Y layers 9 ToT vs zenith angle 10 ToT vs zenith angle: linear fit results The previous histograms have been fitted with a linear function: ToT a b/cos • Fit results slightly changed with respect to the ones shown at the IA workshop 6 • As expected, the fit results are similar for all integrated towers 11 ToT vs l/l’ 12 ToT vs l/l’: linear fit results The previous histograms have been fitted with a linear function: ToT a b(l/l ) • Fit results changed with respect to IA workshop 6 • a small; b 40 ToT is almost proportional to the ratio l/l’ 13 Are results compatible with previous ones? Yes, now they are! 14 Conclusions • The ToT dependence on the track parameters has been investigated • The analysis cuts have been corrected • Symmetries in the angular distributions of muon tracks can be explained taking the geometry into account • Results in the full LAT configuration are compatible with previous analysis 15