» Introduction
» Monte Carlo sample
» Processing times
» Trigger level
» effective
area
» angular resol. vs energy
» efficiency
» energy spectra
» angular
resol. vs
declination
» events vs azimuth
» fakes
» summay table
» comparison 9,
21, 80 lines
» check retriggering
» Cut set 1
» effective area
» angular resol. vs energy
» efficiency
» energy spectra
» angular resol.
vs declination
» events vs azimuth
» fakes
» summay table
» comparison
9, 21, 80 lines
» check
retriggering
» Cut set 2
» effective area
» angular resol. vs energy
» efficiency
» energy spectra
» angular resol.
vs declination
» events vs azimuth
» fakes
» summay table
» comparison
9, 21, 80 lines
» check
retriggering
» Cut set 3
» effective area
» angular resol. vs energy
» efficiency
» energy spectra
» angular resol.
vs declination
» events vs azimuth
» fakes
» summay table
» comparison
9, 21, 80 lines
» check
retriggering
» Event
rates vs zenith cut
» corsika events
» cosmic signal
» atmospheric neutrinos
» Preliminary conclusions
Comments to:
zornoza@icecube.wisc.edu
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Cut Set 1
This cut is defined as:
- |Sdir|<0.6
- Ndir>=8
- Ldir>150 m
Effective areas
9 lines
Effective area for first guesses
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Effective area for log-likelihoods
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Effective area for different angular ranges |
21 lines
Effective area for first guesses
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Effective area for log-likelihoods
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Effective area for different angular ranges
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80 lines
Effective area for first guesses
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Effective area for log-likelihoods
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Effective area for different angular ranges
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Angular
resolution vs energy
9 lines
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21 lines
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80 lines
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Efficiency
first guesses
9 lines
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21 lines
|
80 lines
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log-likelihoods
9 lines
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21 lines
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80 lines
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Energy spectra
9 lines
corsika events
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atmospheric neutrinos
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cosmic neutrinos
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21 lines
corsika events
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atmospheric neutrinos
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cosmic neutrinos
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80 lines
corsika events
|
atmospheric neutrinos
|
cosmic neutrinos
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Angular
resolution vs declination
9 lines
corsika events
|
atmospheric neutrinos
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cosmic neutrinos
|
21 lines
corsika events
|
atmospheric neutrinos
|
cosmic neutrinos
|
80 lines
corsika events
|
atmospheric neutrinos
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cosmic neutrinos
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Events vs. azimuth
9 lines
|
21 lines
|
80 lines
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Cumulative
distributions
9 lines
corsika events
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atmospheric neutrinos
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cosmic neutrinos
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corsika events
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atmospheric neutrinos
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cosmic neutrinos
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21 lines
corsika events
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atmospheric neutrinos
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cosmic neutrinos
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corsika events
|
atmospheric neutrinos
|
cosmic neutrinos
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80 lines
corsika events
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atmospheric neutrinos
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cosmic neutrinos
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corsika events
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atmospheric neutrinos
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cosmic neutrinos
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Fake rates
9 lines - Corsika
9 lines - Atmospheric neutrinos
9 lines - Cosmic neutrinos
21 lines - Corsika
21 lines - Atmospheric neutrinos
21 lines - Cosmic neutrinos
80 lines - Corsika
80 lines - Atmospheric neutrinos
80 lines - Cosmic neutrinos
The tables below correspond to the following strucuture:
9
lines, corsika
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9
lines, atmospheric neutrinos
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9
lines, cosmic neutrinos
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| 21
lines, corsika |
21
lines, atmospheric neutrinos |
21
lines, cosmic neutrinos |
| 80
lines, corsika |
80
lines, atmospheric neutrinos |
80
lines, cosmic neutrinos
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Comparison
9, 21 and 80 lines
Checks on retriggering
We are using the module DAQRetriggeringModule created by Phil Roth to
retrigger files generated with 80 with only 21 lines. In order to check
that everything goes as expected, we also reconstructed some files
generated with 80 lines and retriggering them with 9 lines.
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