Wavelets applied to the detection of point sources of UHECRs

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 wavelet family of order 1, 2 and 3. The analysis is performed by calculating the ampli?cation of the signal-to-noise ratio for several anisotropy pa...

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Main Authors: Batista, R. A., Kemp, E., Almeida, R. M. de, Daniel, B.
Format: Online
Language:Portuguese
Published: Universidade Estadual de Campinas 2011
Subjects:
Online Access:https://econtents.sbu.unicamp.br/eventos/index.php/phyproceedings/article/view/physicae.proceedings.XEJP.1
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author Batista, R. A.
Kemp, E.
Almeida, R. M. de
Daniel, B.
author_facet Batista, R. A.
Kemp, E.
Almeida, R. M. de
Daniel, B.
author_sort Batista, R. A.
collection Portal de Eventos Científicos da UNICAMP
container_reference Physicae Proceedings; Vol. 1 No. 1 (2010): Proceedings X EJP ; 1-6
description 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 wavelet family of order 1, 2 and 3. The analysis is performed by calculating the ampli?cation 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.
first_indexed 2025-10-08T13:49:11Z
format Online
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institution Universidade Estadual de Campinas
issn 2236-7535
language por
last_indexed 2025-10-08T13:49:11Z
publishDate 2011
publisher Universidade Estadual de Campinas
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spelling ojs-article-32072020-05-15T15:13:20Z Wavelets applied to the detection of point sources of UHECRs Batista, R. A. Kemp, E. Almeida, R. M. de Daniel, B. Cosmic rays Ultra-high energy cosmic rays 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 wavelet family of order 1, 2 and 3. The analysis is performed by calculating the ampli?cation 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. Universidade Estadual de Campinas 2011-05-01 info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion application/pdf https://econtents.sbu.unicamp.br/eventos/index.php/phyproceedings/article/view/physicae.proceedings.XEJP.1 Physicae Proceedings; Vol. 1 No. 1 (2010): Proceedings X EJP ; 1-6 Physicae Proceedings; v. 1 n. 1 (2010): Proceedings X EJP ; 1-6 2236-7535 por https://econtents.sbu.unicamp.br/eventos/index.php/phyproceedings/article/view/physicae.proceedings.XEJP.1/3150 Copyright (c) 2010 Physicae Proceedings
spellingShingle Batista, R. A.
Kemp, E.
Almeida, R. M. de
Daniel, B.
Cosmic rays
Ultra-high energy cosmic rays
Wavelets applied to the detection of point sources of UHECRs
title Wavelets applied to the detection of point sources of UHECRs
title_full Wavelets applied to the detection of point sources of UHECRs
title_fullStr Wavelets applied to the detection of point sources of UHECRs
title_full_unstemmed Wavelets applied to the detection of point sources of UHECRs
title_short Wavelets applied to the detection of point sources of UHECRs
title_sort wavelets applied to the detection of point sources of uhecrs
topic Cosmic rays
Ultra-high energy cosmic rays
url https://econtents.sbu.unicamp.br/eventos/index.php/phyproceedings/article/view/physicae.proceedings.XEJP.1
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AT almeidarmde waveletsappliedtothedetectionofpointsourcesofuhecrs
AT danielb waveletsappliedtothedetectionofpointsourcesofuhecrs