BL Lacertae are probable sources of the observed ultra-high energy cosmic rays
We calculate angular correlation function between ultra-high energy cosmic rays (UHECR) observed by Yakutsk and AGASA experiments, and most powerful BL Lacertae objects. We find significant correlations which correspond to the probability of statistical fluctuation less than $10^{-4}$, including pen...
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ftdatacite:10.48550/arxiv.astro-ph/0102476 2023-05-15T18:45:25+02:00 BL Lacertae are probable sources of the observed ultra-high energy cosmic rays Tinyakov, P. G. Tkachev, I. I. 2001 https://dx.doi.org/10.48550/arxiv.astro-ph/0102476 https://arxiv.org/abs/astro-ph/0102476 unknown arXiv https://dx.doi.org/10.1134/1.1434282 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2001 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0102476 https://doi.org/10.1134/1.1434282 2022-04-01T17:01:16Z We calculate angular correlation function between ultra-high energy cosmic rays (UHECR) observed by Yakutsk and AGASA experiments, and most powerful BL Lacertae objects. We find significant correlations which correspond to the probability of statistical fluctuation less than $10^{-4}$, including penatly for selecting the subset of brightest BL Lacs. We conclude that some of BL Lacs are sources of the observed UHECR and present a list of most probable candidates. : Replaced with the version accepted for publication in JETP Lett Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
language |
unknown |
topic |
Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences Tinyakov, P. G. Tkachev, I. I. BL Lacertae are probable sources of the observed ultra-high energy cosmic rays |
topic_facet |
Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
description |
We calculate angular correlation function between ultra-high energy cosmic rays (UHECR) observed by Yakutsk and AGASA experiments, and most powerful BL Lacertae objects. We find significant correlations which correspond to the probability of statistical fluctuation less than $10^{-4}$, including penatly for selecting the subset of brightest BL Lacs. We conclude that some of BL Lacs are sources of the observed UHECR and present a list of most probable candidates. : Replaced with the version accepted for publication in JETP Lett |
format |
Text |
author |
Tinyakov, P. G. Tkachev, I. I. |
author_facet |
Tinyakov, P. G. Tkachev, I. I. |
author_sort |
Tinyakov, P. G. |
title |
BL Lacertae are probable sources of the observed ultra-high energy cosmic rays |
title_short |
BL Lacertae are probable sources of the observed ultra-high energy cosmic rays |
title_full |
BL Lacertae are probable sources of the observed ultra-high energy cosmic rays |
title_fullStr |
BL Lacertae are probable sources of the observed ultra-high energy cosmic rays |
title_full_unstemmed |
BL Lacertae are probable sources of the observed ultra-high energy cosmic rays |
title_sort |
bl lacertae are probable sources of the observed ultra-high energy cosmic rays |
publisher |
arXiv |
publishDate |
2001 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0102476 https://arxiv.org/abs/astro-ph/0102476 |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
Yakutsk |
op_relation |
https://dx.doi.org/10.1134/1.1434282 |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0102476 https://doi.org/10.1134/1.1434282 |
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1766236462355841024 |