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ANTARES search for point-sources of neutrinos using astrophysical catalogs: a likelihood stacking analysis

A search for astrophysical point-like neutrino sources using the data collected by the ANTARES detector between January 29, 2007 and December 31, 2017 is presented. A likelihood stacking method is used to assess the significance of an excess of muon neutrinos inducing track-like events in correlatio...

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Published in:arXiv.org 2020-12
Main Authors: Albert, A, Anghinolfi, M, Anton, G, Aublin, J, Baret, B, Basa, S, Belhorma, B, Biagi, S, Bissinger, M, Boumaaza, J, Bouta, M, Bouwhuis, M C, Branzas, H, Bruijn, R, Busto, J, Capone, A, Caramete, L, Carretero, V, Celli, S, Chabab, M, Chau, T N, Moursli, R, Chiarusi, T, Circella, M, Colomer-Molla, M, Coniglione, R, Coyle, P, Creusot, A, Diaz, A F, Deschamps, A, Distefano, C, I di Palma, Donzaud, C, Dornic, D, Eberl, T, Enzenhofer, A, Fermani, P, Filippini, F, Fusco, L, Gatelet, Y, Gay, P, Glotin, H, Gozzini, R, Gracia, R, Graf, K, Guidi, C, Haren, H, Heijboer, A J, Hello, Y, Hernandez-Rey, J J, Hössl, J, Huang, F, Jisse-Jung, B, Jong, P, Kadler, M, Kalekin, O, Katz, U, Kouchner, A, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Breton, R, Lefèvre, D, Levi, G, Lincetto, M, Lopez-Coto, D, Maderer, L, Manczak, J, Marcelin, M, Mazzou, S, Melis, K, Migliozzi, P, Moser, M, Moussa, A, Muller, R, Navas, S, Nezri, E, Nunez-Castineyra, A, Palavas, G E, Pellegrino, C, Perrin-Terrin, M, Piattelli, P, Popa, V, Pradier, T, Riccobene, G, Samtleben, D F, Sanchez-Losa, A, Schussler, F, Spurio, M, Stolarczyk, Th, Taiuti, M, Tayalati, Y, Thakore, T, Vallage, B, Elewyck, V, Viola, S, Wilms, J, Zornoza, J D, Zuniga, J, Buson, S
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creator Albert, A
Anghinolfi, M
Anton, G
Aublin, J
Baret, B
Basa, S
Belhorma, B
Biagi, S
Bissinger, M
Boumaaza, J
Bouta, M
Bouwhuis, M C
Branzas, H
Bruijn, R
Busto, J
Capone, A
Caramete, L
Carretero, V
Celli, S
Chabab, M
Chau, T N
Moursli, R
Chiarusi, T
Circella, M
Colomer-Molla, M
Coniglione, R
Coyle, P
Creusot, A
Diaz, A F
Deschamps, A
Distefano, C
I di Palma
Donzaud, C
Dornic, D
Eberl, T
Enzenhofer, A
Fermani, P
Filippini, F
Fusco, L
Gatelet, Y
Gay, P
Glotin, H
Gozzini, R
Gracia, R
Graf, K
Guidi, C
Haren, H
Heijboer, A J
Hello, Y
Hernandez-Rey, J J
Hössl, J
Huang, F
Jisse-Jung, B
Jong, P
Kadler, M
Kalekin, O
Katz, U
Kouchner, A
Kreykenbohm, I
Kulikovskiy, V
Lahmann, R
Breton, R
Lefèvre, D
Levi, G
Lincetto, M
Lopez-Coto, D
Maderer, L
Manczak, J
Marcelin, M
Mazzou, S
Melis, K
Migliozzi, P
Moser, M
Moussa, A
Muller, R
Navas, S
Nezri, E
Nunez-Castineyra, A
Palavas, G E
Pellegrino, C
Perrin-Terrin, M
Piattelli, P
Popa, V
Pradier, T
Riccobene, G
Samtleben, D F
Sanchez-Losa, A
Schussler, F
Spurio, M
Stolarczyk, Th
Taiuti, M
Tayalati, Y
Thakore, T
Vallage, B
Elewyck, V
Viola, S
Wilms, J
Zornoza, J D
Zuniga, J
Buson, S
description A search for astrophysical point-like neutrino sources using the data collected by the ANTARES detector between January 29, 2007 and December 31, 2017 is presented. A likelihood stacking method is used to assess the significance of an excess of muon neutrinos inducing track-like events in correlation with the location of a list of possible sources. Different sets of objects are tested in the analysis: a) a sub-sample of the \textit{Fermi} 3LAC catalog of blazars, b) a jet-obscured AGN population, c) a sample of soft gamma-ray selected radio galaxies, d) a star-forming galaxy catalog , and e) a public sample of 56 very-high-energy track events from the IceCube experiment. None of the tested sources shows a significant association with the sample of neutrinos detected by ANTARES. The smallest p-value is obtained for the radio galaxies catalog with an equal weights hypothesis, with a pre-trial p-value equivalent to a \(2.8 \, \sigma\) excess, equivalent to \(1.6 \, \sigma\) post-trial. In addition, the results of a dedicated analysis for the blazar MG3 J225517+2409 are also reported: this source is found to be the most significant within the \textit{Fermi} 3LAC sample, with 5 ANTARES events located at less than one degree from the source. This blazar showed evidence of flaring activity in \textit{Fermi} data, in space-time coincidence with a high-energy track detected by IceCube. An \emph{a posteriori} significance of \(2.0\, \sigma\) for the combination of ANTARES and IceCube data is reported.
doi_str_mv 10.48550/arxiv.2012.15082
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astrophysical catalogs: a likelihood stacking analysis</title><title>arXiv.org</title><description>A search for astrophysical point-like neutrino sources using the data collected by the ANTARES detector between January 29, 2007 and December 31, 2017 is presented. A likelihood stacking method is used to assess the significance of an excess of muon neutrinos inducing track-like events in correlation with the location of a list of possible sources. Different sets of objects are tested in the analysis: a) a sub-sample of the \textit{Fermi} 3LAC catalog of blazars, b) a jet-obscured AGN population, c) a sample of soft gamma-ray selected radio galaxies, d) a star-forming galaxy catalog , and e) a public sample of 56 very-high-energy track events from the IceCube experiment. None of the tested sources shows a significant association with the sample of neutrinos detected by ANTARES. The smallest p-value is obtained for the radio galaxies catalog with an equal weights hypothesis, with a pre-trial p-value equivalent to a \(2.8 \, \sigma\) excess, equivalent to \(1.6 \, \sigma\) post-trial. In addition, the results of a dedicated analysis for the blazar MG3 J225517+2409 are also reported: this source is found to be the most significant within the \textit{Fermi} 3LAC sample, with 5 ANTARES events located at less than one degree from the source. This blazar showed evidence of flaring activity in \textit{Fermi} data, in space-time coincidence with a high-energy track detected by IceCube. An \emph{a posteriori} significance of \(2.0\, \sigma\) for the combination of ANTARES and IceCube data is reported.</description><subject>Active galactic nuclei</subject><subject>Astronomical catalogs</subject><subject>Blazars</subject><subject>Equivalence</subject><subject>Gamma rays</subject><subject>Neutrinos</subject><subject>Radio galaxies</subject><subject>Stacking</subject><subject>Star 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20201230</creationdate><title>ANTARES search for point-sources of neutrinos using astrophysical catalogs: a likelihood stacking analysis</title><author>Albert, A ; Anghinolfi, M ; Anton, G ; Aublin, J ; Baret, B ; Basa, S ; Belhorma, B ; Biagi, S ; Bissinger, M ; Boumaaza, J ; Bouta, M ; Bouwhuis, M C ; Branzas, H ; Bruijn, R ; Busto, J ; Capone, A ; Caramete, L ; Carretero, V ; Celli, S ; Chabab, M ; Chau, T N ; Moursli, R ; Chiarusi, T ; Circella, M ; Colomer-Molla, M ; Coniglione, R ; Coyle, P ; Creusot, A ; Diaz, A F ; Deschamps, A ; Distefano, C ; I di Palma ; Donzaud, C ; Dornic, D ; Eberl, T ; Enzenhofer, A ; Fermani, P ; Filippini, F ; Fusco, L ; Gatelet, Y ; Gay, P ; Glotin, H ; Gozzini, R ; Gracia, R ; Graf, K ; Guidi, C ; Haren, H ; Heijboer, A J ; Hello, Y ; Hernandez-Rey, J J ; Hössl, J ; Huang, F ; Jisse-Jung, B ; Jong, P ; Kadler, M ; Kalekin, O ; Katz, U ; Kouchner, A ; Kreykenbohm, I ; Kulikovskiy, V ; Lahmann, R ; Breton, R ; Lefèvre, D ; Levi, G ; Lincetto, M ; Lopez-Coto, D ; Maderer, L ; Manczak, J ; Marcelin, M ; Mazzou, S ; Melis, K ; Migliozzi, P ; Moser, M ; Moussa, A ; Muller, R ; Navas, S ; Nezri, E ; Nunez-Castineyra, A ; Palavas, G E ; Pellegrino, C ; Perrin-Terrin, M ; Piattelli, P ; Popa, V ; Pradier, T ; Riccobene, G ; Samtleben, D F ; Sanchez-Losa, A ; Schussler, F ; Spurio, M ; Stolarczyk, Th ; Taiuti, M ; Tayalati, Y ; Thakore, T ; Vallage, B ; Elewyck, V ; Viola, S ; Wilms, J ; Zornoza, J D ; Zuniga, J ; Buson, S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a522-614a7fa36b4a46854402e96a4a8492d13e5e212b7e756315ce153eb6de5fef133</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Active galactic nuclei</topic><topic>Astronomical catalogs</topic><topic>Blazars</topic><topic>Equivalence</topic><topic>Gamma rays</topic><topic>Neutrinos</topic><topic>Radio galaxies</topic><topic>Stacking</topic><topic>Star formation</topic><toplevel>online_resources</toplevel><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>Anghinolfi, M</creatorcontrib><creatorcontrib>Anton, G</creatorcontrib><creatorcontrib>Aublin, J</creatorcontrib><creatorcontrib>Baret, B</creatorcontrib><creatorcontrib>Basa, S</creatorcontrib><creatorcontrib>Belhorma, B</creatorcontrib><creatorcontrib>Biagi, S</creatorcontrib><creatorcontrib>Bissinger, M</creatorcontrib><creatorcontrib>Boumaaza, 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collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Albert, A</au><au>Anghinolfi, M</au><au>Anton, G</au><au>Aublin, J</au><au>Baret, B</au><au>Basa, S</au><au>Belhorma, B</au><au>Biagi, S</au><au>Bissinger, M</au><au>Boumaaza, J</au><au>Bouta, M</au><au>Bouwhuis, M C</au><au>Branzas, H</au><au>Bruijn, R</au><au>Busto, J</au><au>Capone, A</au><au>Caramete, L</au><au>Carretero, V</au><au>Celli, S</au><au>Chabab, M</au><au>Chau, T N</au><au>Moursli, R</au><au>Chiarusi, T</au><au>Circella, M</au><au>Colomer-Molla, M</au><au>Coniglione, R</au><au>Coyle, P</au><au>Creusot, A</au><au>Diaz, A F</au><au>Deschamps, A</au><au>Distefano, C</au><au>I di Palma</au><au>Donzaud, C</au><au>Dornic, D</au><au>Eberl, T</au><au>Enzenhofer, A</au><au>Fermani, P</au><au>Filippini, F</au><au>Fusco, L</au><au>Gatelet, Y</au><au>Gay, P</au><au>Glotin, H</au><au>Gozzini, R</au><au>Gracia, R</au><au>Graf, K</au><au>Guidi, C</au><au>Haren, H</au><au>Heijboer, A J</au><au>Hello, Y</au><au>Hernandez-Rey, J J</au><au>Hössl, J</au><au>Huang, F</au><au>Jisse-Jung, B</au><au>Jong, P</au><au>Kadler, M</au><au>Kalekin, O</au><au>Katz, U</au><au>Kouchner, A</au><au>Kreykenbohm, I</au><au>Kulikovskiy, V</au><au>Lahmann, R</au><au>Breton, R</au><au>Lefèvre, D</au><au>Levi, G</au><au>Lincetto, M</au><au>Lopez-Coto, D</au><au>Maderer, L</au><au>Manczak, J</au><au>Marcelin, M</au><au>Mazzou, S</au><au>Melis, K</au><au>Migliozzi, P</au><au>Moser, M</au><au>Moussa, A</au><au>Muller, R</au><au>Navas, S</au><au>Nezri, E</au><au>Nunez-Castineyra, A</au><au>Palavas, G E</au><au>Pellegrino, C</au><au>Perrin-Terrin, M</au><au>Piattelli, P</au><au>Popa, V</au><au>Pradier, T</au><au>Riccobene, G</au><au>Samtleben, D F</au><au>Sanchez-Losa, A</au><au>Schussler, F</au><au>Spurio, M</au><au>Stolarczyk, Th</au><au>Taiuti, M</au><au>Tayalati, Y</au><au>Thakore, T</au><au>Vallage, B</au><au>Elewyck, V</au><au>Viola, S</au><au>Wilms, J</au><au>Zornoza, J D</au><au>Zuniga, J</au><au>Buson, S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>ANTARES search for point-sources of neutrinos using astrophysical catalogs: a likelihood stacking analysis</atitle><jtitle>arXiv.org</jtitle><date>2020-12-30</date><risdate>2020</risdate><eissn>2331-8422</eissn><abstract>A search for astrophysical point-like neutrino sources using the data collected by the ANTARES detector between January 29, 2007 and December 31, 2017 is presented. A likelihood stacking method is used to assess the significance of an excess of muon neutrinos inducing track-like events in correlation with the location of a list of possible sources. Different sets of objects are tested in the analysis: a) a sub-sample of the \textit{Fermi} 3LAC catalog of blazars, b) a jet-obscured AGN population, c) a sample of soft gamma-ray selected radio galaxies, d) a star-forming galaxy catalog , and e) a public sample of 56 very-high-energy track events from the IceCube experiment. None of the tested sources shows a significant association with the sample of neutrinos detected by ANTARES. The smallest p-value is obtained for the radio galaxies catalog with an equal weights hypothesis, with a pre-trial p-value equivalent to a \(2.8 \, \sigma\) excess, equivalent to \(1.6 \, \sigma\) post-trial. In addition, the results of a dedicated analysis for the blazar MG3 J225517+2409 are also reported: this source is found to be the most significant within the \textit{Fermi} 3LAC sample, with 5 ANTARES events located at less than one degree from the source. This blazar showed evidence of flaring activity in \textit{Fermi} data, in space-time coincidence with a high-energy track detected by IceCube. An \emph{a posteriori} significance of \(2.0\, \sigma\) for the combination of ANTARES and IceCube data is reported.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2012.15082</doi><oa>free_for_read</oa></addata></record>
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subjects Active galactic nuclei
Astronomical catalogs
Blazars
Equivalence
Gamma rays
Neutrinos
Radio galaxies
Stacking
Star formation
title ANTARES search for point-sources of neutrinos using astrophysical catalogs: a likelihood stacking analysis
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