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Experimental setup (SPICE)

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Presentation on theme: "Experimental setup (SPICE)"— Presentation transcript:

1 Experimental setup (SPICE)

2 Dust logger/EDML log matching
prediction for precision of extrapolation outside IceCube is based on the correlation with SPICE model: 14% Correlation with SPICE ice model Merging Dust Logger and EDML logs

3 fit region (inside detector)
black line: 7-string fit to flasher data gray band: scaled merged dust log (m-1) (m) extrapolation region fit region (inside detector) (outside detector)

4 fit region (inside detector)
black line: 7-string fit to flasher data gray band: scaled merged dust log (m-1) (m) extrapolation region fit region (inside detector) (outside detector)

5 fit region (inside detector)
black line: 7-string fit to flasher data gray band: scaled merged dust log (m) extrapolation region fit region (inside detector) (outside detector)

6 fit region (inside detector)
black line: 7-string fit to flasher data gray band: scaled merged dust log (m) extrapolation region fit region (inside detector) (outside detector)

7 Model error of SPICE: ~10%
> 0, 1, 10, 100, 400 p.e./event 19, 24, 57, 62, 80, 81+63 with LED pattern unfolding + with DOM efficiencies

8 Timeline AMANDA ice models:
bulk, f125, mam, mamint, stdkurt, sudkurt, kgm, … millennium (published 2006)  AHA (2007) % IceCube ice models: cont.  WHAM (2011) % SPICE 1 (2009) % SPICE 2, 2+, 2x, 2y (2010) added ice layer tilt SPICE Mie (2010) fit to scattering function 29% SPICE Lea (2012) fit to scattering anisotropy 20% SPICE Next (2013) 7-string, LED unfolding 17% SPICE Next New (2014) llh fixes, DOM sensitivity fits 12%


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