2005 AMANDA Point Source Analysis | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Data Sample Simulation Event Selection Methodology Sensitivity, Discovery Potential, & Systematics Unblinding Proposal Results Questions and Answers |
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Unblinding ResultsFull Sky Search6001 events are shown (887 events >100o zenith) from the 2005 dataset.![]() The likelihood ratio is evaluated on a 0.25ox0.25o grid ranging from -5o<δ<82.5o. At each point the significance is calculated, resulting in the following map of log10(p-value) ![]() The maximum significance obtained is 3.58σ near 2.75h, +48o. Out of 100 sets of randomized data, 69 have a maximum significance equal to or greater than 3.58σ. The quantity γbest from the likelihood maximization is plotted for the skymap: ![]() The fitted spectral index at the 3.58σ fluctuation near 2.75h, +48o is slightly greater than 3. Locations in white have a negative fluctuation in number of signal events, so spectral index information is meaningless. Search Based on a List of Candidate SourcesThe method is applied to the locations of sources in the IC-9 point source catalog and the limits (E2Φ < μ90*10-11 TeV cm-2s-1) and p-values (probability the result is due to background alone) are summarized in the table below. No excess near the Crab is observed in 2005
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