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|Type:||Artigo de evento|
|Title:||Amplification Of The Signal-to-noise Ratio In Cosmic Ray Maps Using The Mexican Hatwavelet Family|
|Abstract:||In this work we analyze the effect of smoothing maps containing arrival directions of cosmic rays with a gaussian kernel and kernels of the mexican hat wavelets of orders 1, 2 and 3. The analysis is performed by calculating the amplification of the signal-to-noise ratio for several background patterns (noise) and different number of events coming from a simulated source (signal) for an ideal detector capable of observing the full sky with uniform coverage. We extend this analysis for a virtual observatory with two sites, one in the northern hemisphere, the other in the southern, considering an acceptance law.|
|Editor:||Institute of High Energy Physics|
|Appears in Collections:||Unicamp - Artigos e Outros Documentos|
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