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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Main Authors: Tinyakov, P. G., Tkachev, I. I.
Format: Text
Language:unknown
Published: arXiv 2001
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0102476
https://arxiv.org/abs/astro-ph/0102476
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spelling 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
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id 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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