Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/108172
Type: Artigo de evento
Title: Amplification Of The Signal-to-noise Ratio In Cosmic Ray Maps Using The Mexican Hatwavelet Family
Author: Batista R.A.
Kemp E.
Daniel B.
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
Rights: fechado
Identifier DOI: 10.7529/ICRC2011/V02/1327
Address: http://www.scopus.com/inward/record.url?eid=2-s2.0-84899530354&partnerID=40&md5=039c0a82dee74c0798e0445d967fa5db
Date Issue: 2011
Appears in Collections:Unicamp - Artigos e Outros Documentos

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