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IFIC analysis (5L PS with Bbfit ) Phone call AWG. 04 June 2010. Juan Pablo Gómez, Paco Salesa, Salvatore Mangano. OUTLINE. OUTSTANDING QUESTIONS. The factor 2 in Aeff with all relevant plots updated Discrepancy in discovery potential needs to be understood
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IFIC analysis (5L PS with Bbfit)Phone callAWG 04 June 2010 Juan Pablo Gómez, Paco Salesa, Salvatore Mangano
OUTLINE OUTSTANDING QUESTIONS • The factor 2 in Aeff with all relevant plots updated • Discrepancy in discovery potential needs to be understood • Event by event comparison of relevant quantities • Check that the proper run-start is used for the event time computation • Provide tables of "the relevant data (effective area, atm neutrino flux, and signal flux)“ • Check that you always use the visibility for the 90 deg. cut in the acceptance computation, even when cutting at 80 degrees in the analysis • Include in the documentation which systematics will be applied. Including the one for the angular resolution • Include a description of the final treatment of the 10pe period and whether any overall scaling is applied to Aeff • Include in the documentation a description of which p-values will be computed and how 5Lines Analysis Juan Pablo Gómez-González
EFFECTIVE AREA Effective Area factor 2 included Effective area as a function of the neutrino energy Optimized cuts plot Factor 2 change on the Sensitivity 5Lines Analysis Juan Pablo Gómez-González
DISCOVERY POTENTIAL Discrepancy in discovery potential Checked that the different results doesn’t come from difference ways to compute the discovery power. We find compatible results with those that Garo have shown. 3.3 SIGNAL EVENTS ARE REQUIRED TO HAVE A 50% PROBABILITY OF A 3SIGMA DISCOVEY Better sg from bg discrimination 5Lines Analysis Juan Pablo Gómez-González
CALIBRATION TABLES • Event by event comparison of relevant quantities • We have found some differences between the calibration values used Production ran by Jürgen (2007-2008 Analysis with Bbfit) TVCIFIC --> 5062269 (L5) & 10756385 (L10)CPPM --> 16684668 (both for L5 y L10) 1pe One different set is used Alignment IFIC --> 5330911 CPPM --> 33512503 Updating the analysis using more recent calibration tables 5Lines Analysis Juan Pablo Gómez-González
EVENTS COMPARISONS TVC TO 1PE 0PE 233 common events same run and frame index For those events difference in relevant variables are small Not common events are closer to the chi2 cut border 5Lines Analysis Juan Pablo Gómez-González
RUN INFO AND RELEVANT DATA • Check that the proper run-start is used for the event time computation IFIC and CPPM find same time for the start time of each run A link to the table containing all the information will be available on the analysis webpage • Provide tables of the relevant data (effective area, atm neutrino flux, and signal flux) • All values will be included on the documentation 5Lines Analysis Juan Pablo Gómez-González
VISIBILITY ON EFFECTIVE AREA COMPUTATION • Check that you always use the visibility for the 90 deg. cut in the acceptance computation, even when cutting at 80 degrees in the analysis • Fraction of events generated as upgoing • (zenith > PI / 2) 5Lines Analysis Juan Pablo Gómez-González
ANGULAR RESOLUTION SYSTEMATIC • Include in the documentation which systematic will be applied. • Angular resolution Time residuals Data and atm.Neutrino mc (3 pe) (chi2<1.8 & bchi2 > 1.8 & nhit > 5 & elevation < -10) Gives confidence on the expected angular resolution 5Lines Analysis Juan Pablo Gómez-González
ACCEPTANCE SYSTEMATIC • Include in the documentation which systematic will be applied. • Acceptance systematic 5-lines muon paper systematic studies 1) Absorption length: 10% uncertainty 20% variation on the number of reconstructed tracks 2) PMT quantum & collection efficiency: 10% 30% 3) OM angular acceptance: 15% - 50% 35% / -30% 4) Timming: contribution negligible + Theoretical model 30% 5Lines Analysis Juan Pablo Gómez-González
OUTSTANDING QUESTIONS • Include in the documentation which systematic will be applied. • Acceptance systematic 30 % symmetric band to represent the systematic uncertainty How does sensitivity changes if we consider a 30% systematic on the detection efficiency use gaussian convolution 5Lines Analysis Juan Pablo Gómez-González
OUTSTANDING QUESTIONS Include a description of the final treatment of the 10pe period and whether any overall scaling is applied to Aeff Mixed noise files mc number of events ratio (before / now) neutrinos 3pe: 0.94 (6% less) neutrinos 10pe: 0.82 (28% less) muons 3pe: 0.98 (2% less) muons10pe: 0.85 (15% less) No scaling facto to be applied ~30 % of events are coming from this period (40% of live time) 5Lines Analysis Juan Pablo Gómez-González
OUTSTANDING QUESTIONS • Include in the documentation a description of which p-values will be computed and how Candidate list BIC distribution of only background BICobs 5Lines Analysis Juan Pablo Gómez-González