� 1 UPDATES ON NSI ANALYSIS WITH ANTARES N R K CHOWDHURY, TARAK THAKORE
� 2 ADAPTED CODE VS EVTRATE ▸ ▸ Binning scheme in E reco between (0.5, 200) GeV Binning gg in E reco 20 uniformggglogarithmic biggns between [0.5, 100] GeV 1 low energy bin with logE < 1.2. 7 energy bins between 1.2 < logE < 2. 1 bin 7 bins The implementation were different in two codes. The bin centres and bin edges were slightly different.
� 3 ADAPTED CODE VS EVTRATE ▸ Binning scheme in E reco ▸ Muon background template Thee public muon background template was different from the one used in the published paper. N 𝜈
(DIS)AGREEMENT AT THE EVENT LEVEL ▸ Link to sheets. https://docs.google.com/spreadsheets/d/1HHXzDTrHawYNKEeIBtfHiq_csU_vt35eVsuXglOwtGA/ edit?ts=5e73ef57#gid=528503813 ▸ CC-muon MC events are off my ~90 events. We were reading two different samples of MC . Δ N MC ) n e z ( s o c Random binning in panda! E reco
ADAPTED CODE VS EVTRATE ▸ Tarak’s plot. BF ϵ 𝜈𝜐 : -1.4E-3 My plot. BF ϵ 𝜈𝜐 : -1.3E-3
NEW NSI SENSITIVITY PLOT Extending the contours to four quadrants. ▸ ▸ Likelihood landscape in plane Contour plot in plane ϵ μτ − ϵ ττ ϵ μτ − ϵ ττ
NEW NSI LIMITS PLOT Extending the contours to four quadrants. ▸ Needs to extended further in y range. ▸ Likelihood landscape in plane Contour plot in plane ϵ μτ − ϵ ττ ϵ μτ − ϵ ττ
ANTARES VS ORCA ▸ Old plot New plot
SUMMARY TODO 1) Only thing left to do is to get the sensitivity bands corresponding to random MC toy event distributions.
TEXT THANKS
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