Wavelets applied to the detection of point sources of UHECRs
ResumoIn 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 wavelet family of order 1, 2 and 3. The analysis is performed by calculating the ampliﬁcation of the signal-to-noise ratio for several anisotropy patterns (noise) and different number of events coming from a simulated source (signal) for an ideal detector capable of observing the full sky with equal probability. We extend this analysis for a virtual detector located within the array of detectors of the Pierre Auger Observatory, considering an acceptance law.
BATISTA, R.A. et al. Wavelets applied to the detection of point sources of UHECRs. Physicæ Proceedings, [S.l.], p. 1, may 2011. ISSN 2236-7535. Disponível em: <http://physicae.ifi.unicamp.br/index.php/phyproceedings/article/view/physicae.proceedings.XEJP.1>. Acesso em: 21 aug. 2017. doi: https://doi.org/10.5196/physicae.proceedings.XEJP.1.
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