2005 AMANDA Point Source Analysis
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Data Sample
Simulation
Event Selection
Methodology
Sensitivity, Discovery Potential, & Systematics
Unblinding Proposal
Results
Questions and Answers
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 | | NASA/ESA Hubble |
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Simulation
Signal MC is generated using Simuperl with the following configuration
| Generator | NUSIM |
| Energy Range | 10^1 - 10^8 GeV |
| Zenith Range | 80 < Zenith < 180 |
| Events/File | 10000 |
| Photon Simulation | PTD |
| Ice Model | MAM |
| AMASIM | Aluminum-opt5 |
| OM Sensitivity | Standard |
Background MC
- ~5.6 days dcorsika (Photonics + Aluminum-fix)
- 16k events coincident-muon (Photonics + Aluminum-fix)
Files
| Diffuse neutrino | 300+300 files | /net/user/jbraun/analysis/point_source/amanda/2005/sim/nusim_ptd_new/ |
| Declination bands spaced by 5 degrees | 5+5 files per band | /data/sim/AMANDA/2005/point_source |
| dCORSIKA | ~5.6 days LT | /data/sim/AMANDA/2005/dcorsika |
| Coincident-muon | 16k events | /data/sim/AMANDA/2005/coinc_mu |
Processing
AMASIM output is filtered identically to the filtered data, except for the obvious removal of the SPASE stream and associated processing.
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