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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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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 |
format | article |
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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><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2012.15082</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Active galactic nuclei ; Astronomical catalogs ; Blazars ; Equivalence ; Gamma rays ; Neutrinos ; Radio galaxies ; Stacking ; Star formation</subject><ispartof>arXiv.org, 2020-12</ispartof><rights>2020. 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J</creatorcontrib><creatorcontrib>Bouta, M</creatorcontrib><creatorcontrib>Bouwhuis, M C</creatorcontrib><creatorcontrib>Branzas, H</creatorcontrib><creatorcontrib>Bruijn, R</creatorcontrib><creatorcontrib>Busto, J</creatorcontrib><creatorcontrib>Capone, A</creatorcontrib><creatorcontrib>Caramete, L</creatorcontrib><creatorcontrib>Carretero, V</creatorcontrib><creatorcontrib>Celli, S</creatorcontrib><creatorcontrib>Chabab, M</creatorcontrib><creatorcontrib>Chau, T N</creatorcontrib><creatorcontrib>Moursli, R</creatorcontrib><creatorcontrib>Chiarusi, T</creatorcontrib><creatorcontrib>Circella, M</creatorcontrib><creatorcontrib>Colomer-Molla, M</creatorcontrib><creatorcontrib>Coniglione, R</creatorcontrib><creatorcontrib>Coyle, P</creatorcontrib><creatorcontrib>Creusot, A</creatorcontrib><creatorcontrib>Diaz, A F</creatorcontrib><creatorcontrib>Deschamps, A</creatorcontrib><creatorcontrib>Distefano, C</creatorcontrib><creatorcontrib>I di Palma</creatorcontrib><creatorcontrib>Donzaud, C</creatorcontrib><creatorcontrib>Dornic, D</creatorcontrib><creatorcontrib>Eberl, T</creatorcontrib><creatorcontrib>Enzenhofer, A</creatorcontrib><creatorcontrib>Fermani, P</creatorcontrib><creatorcontrib>Filippini, F</creatorcontrib><creatorcontrib>Fusco, L</creatorcontrib><creatorcontrib>Gatelet, Y</creatorcontrib><creatorcontrib>Gay, P</creatorcontrib><creatorcontrib>Glotin, H</creatorcontrib><creatorcontrib>Gozzini, R</creatorcontrib><creatorcontrib>Gracia, R</creatorcontrib><creatorcontrib>Graf, K</creatorcontrib><creatorcontrib>Guidi, C</creatorcontrib><creatorcontrib>Haren, H</creatorcontrib><creatorcontrib>Heijboer, A J</creatorcontrib><creatorcontrib>Hello, Y</creatorcontrib><creatorcontrib>Hernandez-Rey, J J</creatorcontrib><creatorcontrib>Hössl, J</creatorcontrib><creatorcontrib>Huang, F</creatorcontrib><creatorcontrib>Jisse-Jung, B</creatorcontrib><creatorcontrib>Jong, P</creatorcontrib><creatorcontrib>Kadler, M</creatorcontrib><creatorcontrib>Kalekin, O</creatorcontrib><creatorcontrib>Katz, U</creatorcontrib><creatorcontrib>Kouchner, A</creatorcontrib><creatorcontrib>Kreykenbohm, I</creatorcontrib><creatorcontrib>Kulikovskiy, V</creatorcontrib><creatorcontrib>Lahmann, R</creatorcontrib><creatorcontrib>Breton, R</creatorcontrib><creatorcontrib>Lefèvre, D</creatorcontrib><creatorcontrib>Levi, G</creatorcontrib><creatorcontrib>Lincetto, M</creatorcontrib><creatorcontrib>Lopez-Coto, D</creatorcontrib><creatorcontrib>Maderer, L</creatorcontrib><creatorcontrib>Manczak, J</creatorcontrib><creatorcontrib>Marcelin, M</creatorcontrib><creatorcontrib>Mazzou, S</creatorcontrib><creatorcontrib>Melis, K</creatorcontrib><creatorcontrib>Migliozzi, P</creatorcontrib><creatorcontrib>Moser, M</creatorcontrib><creatorcontrib>Moussa, A</creatorcontrib><creatorcontrib>Muller, R</creatorcontrib><creatorcontrib>Navas, S</creatorcontrib><creatorcontrib>Nezri, E</creatorcontrib><creatorcontrib>Nunez-Castineyra, A</creatorcontrib><creatorcontrib>Palavas, G E</creatorcontrib><creatorcontrib>Pellegrino, C</creatorcontrib><creatorcontrib>Perrin-Terrin, M</creatorcontrib><creatorcontrib>Piattelli, P</creatorcontrib><creatorcontrib>Popa, V</creatorcontrib><creatorcontrib>Pradier, T</creatorcontrib><creatorcontrib>Riccobene, G</creatorcontrib><creatorcontrib>Samtleben, D F</creatorcontrib><creatorcontrib>Sanchez-Losa, A</creatorcontrib><creatorcontrib>Schussler, F</creatorcontrib><creatorcontrib>Spurio, M</creatorcontrib><creatorcontrib>Stolarczyk, Th</creatorcontrib><creatorcontrib>Taiuti, M</creatorcontrib><creatorcontrib>Tayalati, Y</creatorcontrib><creatorcontrib>Thakore, T</creatorcontrib><creatorcontrib>Vallage, B</creatorcontrib><creatorcontrib>Elewyck, V</creatorcontrib><creatorcontrib>Viola, S</creatorcontrib><creatorcontrib>Wilms, J</creatorcontrib><creatorcontrib>Zornoza, J D</creatorcontrib><creatorcontrib>Zuniga, J</creatorcontrib><creatorcontrib>Buson, S</creatorcontrib><title>ANTARES search for point-sources of neutrinos using 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 formation</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotkEtLw0AUhQdBsNT-AHcDrlNn7jySuiulPqAoaPflNrlppg2ZOjcR_fcGdXU2H4fvHCFutJrbwjl1h-krfM5BaZhrpwq4EBMwRmeFBbgSM-ajUgp8Ds6ZiTguX7bLt_W7ZMJUNrKOSZ5j6PqM45BKYhlr2dHQp9BFlgOH7iCR-xTPzTeHEltZYo9tPPC9RNmGE7WhibGS3GN5-qU7bEeUr8VljS3T7D-nYvuw3q6ess3r4_NqucnQAWReW8xrNH5v0frCWauAFh4tFnYBlTbkCDTsc8qdN9qVpJ2hva_I1VRrY6bi9q_2nOLHQNzvjuOS0YF3YHM7XuIdmB8NSloo</recordid><startdate>20201230</startdate><enddate>20201230</enddate><creator>Albert, A</creator><creator>Anghinolfi, M</creator><creator>Anton, G</creator><creator>Aublin, J</creator><creator>Baret, B</creator><creator>Basa, S</creator><creator>Belhorma, B</creator><creator>Biagi, S</creator><creator>Bissinger, M</creator><creator>Boumaaza, J</creator><creator>Bouta, M</creator><creator>Bouwhuis, M C</creator><creator>Branzas, H</creator><creator>Bruijn, 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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><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Database (Proquest)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Databases</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering 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> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
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issn | 2331-8422 |
language | eng |
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source | Publicly Available Content Database |
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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