Chasing the Neutrino Blazar Candidates
In our study of the correlations between IceCube-detected neutrino events and γ -ray properties of blazars, we recognize the inherent challenges posed by the limited detection of neutrinos. In this paper, we explore few-shot learning to deal with the class imbalance and few-shot issues presented in...
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creator | Zhu, Jingtian Cao, Haitao Xiao, Hubing Pei, Zhiyuan Fan, JunHui Bastieri, Denis |
description | In our study of the correlations between IceCube-detected neutrino events and
γ
-ray properties of blazars, we recognize the inherent challenges posed by the limited detection of neutrinos. In this paper, we explore few-shot learning to deal with the class imbalance and few-shot issues presented in the incremental version of the 12 yr Fermi-LAT
γ
-ray source catalog (4FGL_ DR3). Specifically, we train a triplet network to transform the blazars with neutrino emission (NBs) and nonblazar samples into an embedding space where their similarities can be measured. With two-way three-shot learning, 199 out of 3708 blazars without neutrino emission (non-NBs) are considered as the potential blazars emitting neutrinos (NB candidates, or NBCs for short), with a similarity score against NBs exceeding 98%. Moreover, the Kolmogorov–Smirnov test supports our identification of NBCs. |
doi_str_mv | 10.3847/1538-4365/ad7730 |
format | Article |
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γ
-ray properties of blazars, we recognize the inherent challenges posed by the limited detection of neutrinos. In this paper, we explore few-shot learning to deal with the class imbalance and few-shot issues presented in the incremental version of the 12 yr Fermi-LAT
γ
-ray source catalog (4FGL_ DR3). Specifically, we train a triplet network to transform the blazars with neutrino emission (NBs) and nonblazar samples into an embedding space where their similarities can be measured. With two-way three-shot learning, 199 out of 3708 blazars without neutrino emission (non-NBs) are considered as the potential blazars emitting neutrinos (NB candidates, or NBCs for short), with a similarity score against NBs exceeding 98%. Moreover, the Kolmogorov–Smirnov test supports our identification of NBCs.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.3847/1538-4365/ad7730</identifier><language>eng</language><publisher>Saskatoon: The American Astronomical Society</publisher><subject>Blazars ; Emission ; Emissions ; Gamma ray sources ; Learning ; Neutrinos</subject><ispartof>The Astrophysical journal. Supplement series, 2024-11, Vol.275 (1), p.11</ispartof><rights>2024. The Author(s). Published by the American Astronomical Society.</rights><rights>2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c299t-2bcf0dfdd172aafb7ae02c6aad518371ba33ebd6dcb7b8447474e3302fa0cf063</cites><orcidid>0000-0002-8626-8686 ; 0000-0002-5929-0968 ; 0000-0001-8244-1229 ; 0000-0002-8206-5080 ; 0000-0002-4970-3108 ; 0000-0002-6954-8862</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4365/ad7730/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,777,781,861,2096,27905,27906,38871,53848</link.rule.ids></links><search><creatorcontrib>Zhu, Jingtian</creatorcontrib><creatorcontrib>Cao, Haitao</creatorcontrib><creatorcontrib>Xiao, Hubing</creatorcontrib><creatorcontrib>Pei, Zhiyuan</creatorcontrib><creatorcontrib>Fan, JunHui</creatorcontrib><creatorcontrib>Bastieri, Denis</creatorcontrib><title>Chasing the Neutrino Blazar Candidates</title><title>The Astrophysical journal. Supplement series</title><addtitle>APJS</addtitle><addtitle>Astrophys. J. Suppl</addtitle><description>In our study of the correlations between IceCube-detected neutrino events and
γ
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γ
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γ
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γ
-ray source catalog (4FGL_ DR3). Specifically, we train a triplet network to transform the blazars with neutrino emission (NBs) and nonblazar samples into an embedding space where their similarities can be measured. With two-way three-shot learning, 199 out of 3708 blazars without neutrino emission (non-NBs) are considered as the potential blazars emitting neutrinos (NB candidates, or NBCs for short), with a similarity score against NBs exceeding 98%. Moreover, the Kolmogorov–Smirnov test supports our identification of NBCs.</abstract><cop>Saskatoon</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4365/ad7730</doi><tpages>16</tpages><orcidid>https://orcid.org/0000-0002-8626-8686</orcidid><orcidid>https://orcid.org/0000-0002-5929-0968</orcidid><orcidid>https://orcid.org/0000-0001-8244-1229</orcidid><orcidid>https://orcid.org/0000-0002-8206-5080</orcidid><orcidid>https://orcid.org/0000-0002-4970-3108</orcidid><orcidid>https://orcid.org/0000-0002-6954-8862</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Blazars Emission Emissions Gamma ray sources Learning Neutrinos |
title | Chasing the Neutrino Blazar Candidates |
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