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WATER PROPERTIES ON RECONSTRUCTION : STATUS HAROLD YEPES-RAMIREZ IFIC, March 25 th 2011. DOWN-GOING MUONS PRODUCTION FOR DIFFERENT WATER MODELS: 10 different water models processed with mupage. - PowerPoint PPT Presentation
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WATER PROPERTIES ON RECONSTRUCTION : STATUS
HAROLD YEPES-RAMIREZ
IFIC, March 25th 2011
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DOWN-GOING MUONS PRODUCTION FOR DIFFERENT WATER MODELS:
• 10 different water models processed with mupage.
• One of the models (abs63 sca53 eta0.17) matches with the new official mupage production done by Juan Pablo and presented in the last collaboration meeting @ CERN (https://sbgelog.in2p3.fr/ANALYSIS/516 ). Cross-checks at TriggerEfficiency level:
• Production is done, but i`m not exactly sure how to weight and scale such distributions for data comparison Ongoing.
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NEUTRINOS (METHODOLOGY):
Run selection:
12 lines detector simulation (r12_c00_s01.det):
Data subsample from Aafit v0r6 production (5 line data + 9,10,12 line data).
• Cut for 12 lines period.• MC Cut: 30508 < runnumber < 38216.
Data Cut (JP): 30880 < runnumber < 38052. (1752 runs)
Lifetime:
For MC:
• 365 days for each production (10 productions = 10 different water models)
For data:
• Juan Pablo Tool (Wikipage):Qbasic>=1&&Scan!=1
For 30880 < runnumber < 38052:
1903 runs in total! ≠ 1752 runs chosen.(lifetime_tool=174.709) – lifetime_set =X•runs=1903-1752=151 runs• 303 runs ≈ 16 days of lifetime•runs ≈ 8 days of lifetime.• 1752 runs -> lifetime_tool – 8 = 166.709 days
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TOTAL AMPLITUDE AND NUMBER OF HITS OF SELECTED HITS IN THE FIT
tcosth < 0.9998 && nhit > 5.0 && nline > 1 tcosth < 0.9998 && nhit > 5 && nline > 1 && run > 30880 && run < 38052
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TOTAL AMPLITUDE AND NUMBER OF HITS OF SELECTED HITS IN THE FIT
tcosth < 0.9998 && nhit > 5.0 && nline > 1 tcosth < 0.9998 && nhit > 5 && nline > 1 && run > 30880 && run < 38052
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NUMBER OF OF LINES USED IN THE FIT
lambda > -5.4 && tcosth > 0 && beta < 1 lambda > -5.4 && tcosth > 0 && beta < 1 && run > 30880 && run < 38052
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NUMBER OF OF LINES USED IN THE FIT
lambda > -5.4 && tcosth > 0 && beta < 1 lambda > -5.4 && tcosth > 0 && beta < 1 && run > 30880 && run < 38052
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RECONSTRUCTION QUALITY PARAMETER
w3*(tcosth > 0 && beta < 1)*(1.0/N*1e10) MC tcosth > 0 && beta < 1 && run > 30880 && run < 38052 DATA
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RECONSTRUCTION QUALITY PARAMETER
w3*(tcosth > 0 && beta < 1)*(1.0/N*1e10) MC tcosth > 0 && beta < 1 && run > 30880 && run < 38052 DATA
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ANGULAR ERROR
lambda > -5.4 && tcosth > 0 lambda > -5.4 && tcosth > 0 && run > 30880 && run < 38052
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ANGULAR ERROR
lambda > -5.4 && tcosth > 0 lambda > -5.4 && tcosth > 0 && run > 30880 && run < 38052
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ZENITH
lambda > -5.4 && beta < 1 lambda > -5.4 && beta < 1 && run > 30880 && run < 38052
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ZENITH
lambda > -5.4 && beta < 1 lambda > -5.4 && beta < 1 && run > 30880 && run < 38052
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AZIMUTH
lambda > -5.4 && tcosth > 0 && beta < 1 lambda > -5.4 && tcosth > 0 && beta < 1&& run > 30880 && run < 38052
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AZIMUTH
lambda > -5.4 && tcosth > 0 && beta < 1 lambda > -5.4 && tcosth > 0 && beta < 1&& run > 30880 && run < 38052
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COMMENTS:
Is it correct the run selection?It is being well weighted the MC neutrino production?