A Search for Neutrino Emission from the Fermi Bubbles with the ANTARES Telescope
Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma...
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creator | ANTARES Collaboration Adrián-Martínez, S Albert, A I Al Samarai André, M Anton, G Anvar, S Astraatmadja, T J-J Aubert Baret, B Basa, S Biagi, S Bigongiari, C Bogazzi, C Bouhou, B Brunner, J Capone, A Cârloganu, C Carr, J Charif, Z Charvis, Ph Chiarusi, T Circella, M Core, L Costantini, H Creusot, A Curtil, C Dekeyser, I Donzaud, C Dornic, D Dumas, A Eberl, T Escoffier, S Fermani, P Flaminio, V Folger, F Fritsch, U Fusco, L A Galatà, S Gay, P Geißelsöder, S Geyer, K Gleixner, A Gómez-González, J P Graf, K Guillard, G H van Haren Hello, Y Hernández-Rey, J J Hößl, J Hugon, C de Jong, M Kadler, M Kalekin, O Kappes, A Kooijman, P Kouchner, A Lahmann, R Lambard, E Larosa, G Lefèvre, D Leonora, E D Lo Presti Loehner, H Marcelin, M Margiotta, A Martínez-Mora, J A Martini, S Michael, T Müller, C Neff, M Nezri, E Palioselitis, D Păvălaş, G E Popa, V Pradier, T Racca, C Richter, R Roensch, K Rostovtsev, A Samtleben, D F E Schmid, J Schüssler, F Seitz, T Shanidze, R Simeone, F Spies, A Spurio, M Stolarczyk, Th Sánchez-Losa, A Tamburini, C Tayalati, Y Trovato, A Vallage, B Vallée, C Vecchi, M Vernin, P de Wolf, E Yatkin, K Zornoza, J D |
description | Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source. |
doi_str_mv | 10.48550/arxiv.1308.5260 |
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Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1308.5260</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Bubbles ; Emission analysis ; Fluxes ; Gamma rays ; Neutrinos ; Physics - High Energy Astrophysical Phenomena ; Visibility</subject><ispartof>arXiv.org, 2013-12</ispartof><rights>2013. 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P</creatorcontrib><creatorcontrib>de Wolf, E</creatorcontrib><creatorcontrib>Yatkin, K</creatorcontrib><creatorcontrib>Zornoza, J D</creatorcontrib><title>A Search for Neutrino Emission from the Fermi Bubbles with the ANTARES Telescope</title><title>arXiv.org</title><description>Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source.</description><subject>Bubbles</subject><subject>Emission analysis</subject><subject>Fluxes</subject><subject>Gamma rays</subject><subject>Neutrinos</subject><subject>Physics - High Energy Astrophysical 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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><scope>GOX</scope></search><sort><creationdate>20131203</creationdate><title>A Search for Neutrino Emission from the Fermi Bubbles with the ANTARES Telescope</title><author>ANTARES Collaboration ; Adrián-Martínez, S ; Albert, A ; I Al Samarai ; André, M ; Anton, G ; Anvar, S ; Astraatmadja, T ; J-J Aubert ; Baret, B ; Basa, S ; Biagi, S ; Bigongiari, C ; Bogazzi, C ; Bouhou, B ; Brunner, J ; Capone, A ; Cârloganu, C ; Carr, J ; Charif, Z ; Charvis, Ph ; Chiarusi, T ; Circella, M ; Core, L ; Costantini, H ; Creusot, A ; Curtil, C ; Dekeyser, I ; Donzaud, C ; Dornic, D ; Dumas, A ; Eberl, T ; Escoffier, S ; Fermani, P ; Flaminio, V ; Folger, F ; Fritsch, U ; Fusco, L A ; Galatà, S ; Gay, P ; Geißelsöder, S ; Geyer, K ; Gleixner, A ; Gómez-González, J P ; Graf, K ; Guillard, G ; H van Haren ; Hello, Y ; Hernández-Rey, J J ; Hößl, J ; Hugon, C ; de Jong, M ; Kadler, M ; Kalekin, O ; Kappes, A ; Kooijman, P ; Kouchner, A ; Lahmann, R ; Lambard, E ; Larosa, G ; Lefèvre, D ; Leonora, E ; D Lo Presti ; Loehner, H ; Marcelin, M ; Margiotta, A ; Martínez-Mora, J A ; Martini, S ; Michael, T ; Müller, C ; Neff, M ; Nezri, E ; Palioselitis, D ; Păvălaş, G E ; Popa, V ; Pradier, T ; Racca, C ; Richter, R ; Roensch, K ; Rostovtsev, A ; Samtleben, D F E ; Schmid, J ; Schüssler, F ; Seitz, T ; Shanidze, R ; Simeone, F ; Spies, A ; Spurio, M ; Stolarczyk, Th ; Sánchez-Losa, A ; Tamburini, C ; Tayalati, Y ; Trovato, A ; Vallage, B ; Vallée, C ; Vecchi, M ; Vernin, P ; de Wolf, E ; Yatkin, K ; Zornoza, J D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a512-91cb68f365d323497fb060fe692d8f31f2b43f6b45964338fa45aed4abfa3f6b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Bubbles</topic><topic>Emission analysis</topic><topic>Fluxes</topic><topic>Gamma rays</topic><topic>Neutrinos</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Visibility</topic><toplevel>online_resources</toplevel><creatorcontrib>ANTARES Collaboration</creatorcontrib><creatorcontrib>Adrián-Martínez, S</creatorcontrib><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>I Al Samarai</creatorcontrib><creatorcontrib>André, M</creatorcontrib><creatorcontrib>Anton, G</creatorcontrib><creatorcontrib>Anvar, S</creatorcontrib><creatorcontrib>Astraatmadja, T</creatorcontrib><creatorcontrib>J-J Aubert</creatorcontrib><creatorcontrib>Baret, B</creatorcontrib><creatorcontrib>Basa, 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P</creatorcontrib><creatorcontrib>Flaminio, V</creatorcontrib><creatorcontrib>Folger, F</creatorcontrib><creatorcontrib>Fritsch, U</creatorcontrib><creatorcontrib>Fusco, L A</creatorcontrib><creatorcontrib>Galatà, S</creatorcontrib><creatorcontrib>Gay, P</creatorcontrib><creatorcontrib>Geißelsöder, S</creatorcontrib><creatorcontrib>Geyer, K</creatorcontrib><creatorcontrib>Gleixner, A</creatorcontrib><creatorcontrib>Gómez-González, J P</creatorcontrib><creatorcontrib>Graf, K</creatorcontrib><creatorcontrib>Guillard, G</creatorcontrib><creatorcontrib>H van Haren</creatorcontrib><creatorcontrib>Hello, Y</creatorcontrib><creatorcontrib>Hernández-Rey, J J</creatorcontrib><creatorcontrib>Hößl, J</creatorcontrib><creatorcontrib>Hugon, C</creatorcontrib><creatorcontrib>de Jong, M</creatorcontrib><creatorcontrib>Kadler, M</creatorcontrib><creatorcontrib>Kalekin, O</creatorcontrib><creatorcontrib>Kappes, A</creatorcontrib><creatorcontrib>Kooijman, P</creatorcontrib><creatorcontrib>Kouchner, A</creatorcontrib><creatorcontrib>Lahmann, R</creatorcontrib><creatorcontrib>Lambard, E</creatorcontrib><creatorcontrib>Larosa, G</creatorcontrib><creatorcontrib>Lefèvre, D</creatorcontrib><creatorcontrib>Leonora, E</creatorcontrib><creatorcontrib>D Lo Presti</creatorcontrib><creatorcontrib>Loehner, H</creatorcontrib><creatorcontrib>Marcelin, M</creatorcontrib><creatorcontrib>Margiotta, A</creatorcontrib><creatorcontrib>Martínez-Mora, J A</creatorcontrib><creatorcontrib>Martini, S</creatorcontrib><creatorcontrib>Michael, T</creatorcontrib><creatorcontrib>Müller, C</creatorcontrib><creatorcontrib>Neff, M</creatorcontrib><creatorcontrib>Nezri, E</creatorcontrib><creatorcontrib>Palioselitis, D</creatorcontrib><creatorcontrib>Păvălaş, G E</creatorcontrib><creatorcontrib>Popa, V</creatorcontrib><creatorcontrib>Pradier, T</creatorcontrib><creatorcontrib>Racca, C</creatorcontrib><creatorcontrib>Richter, R</creatorcontrib><creatorcontrib>Roensch, K</creatorcontrib><creatorcontrib>Rostovtsev, A</creatorcontrib><creatorcontrib>Samtleben, D F E</creatorcontrib><creatorcontrib>Schmid, J</creatorcontrib><creatorcontrib>Schüssler, F</creatorcontrib><creatorcontrib>Seitz, T</creatorcontrib><creatorcontrib>Shanidze, R</creatorcontrib><creatorcontrib>Simeone, F</creatorcontrib><creatorcontrib>Spies, A</creatorcontrib><creatorcontrib>Spurio, M</creatorcontrib><creatorcontrib>Stolarczyk, Th</creatorcontrib><creatorcontrib>Sánchez-Losa, A</creatorcontrib><creatorcontrib>Tamburini, C</creatorcontrib><creatorcontrib>Tayalati, Y</creatorcontrib><creatorcontrib>Trovato, A</creatorcontrib><creatorcontrib>Vallage, B</creatorcontrib><creatorcontrib>Vallée, C</creatorcontrib><creatorcontrib>Vecchi, M</creatorcontrib><creatorcontrib>Vernin, P</creatorcontrib><creatorcontrib>de Wolf, E</creatorcontrib><creatorcontrib>Yatkin, K</creatorcontrib><creatorcontrib>Zornoza, J D</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</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>Access via ProQuest (Open Access)</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><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ANTARES Collaboration</au><au>Adrián-Martínez, S</au><au>Albert, A</au><au>I Al Samarai</au><au>André, M</au><au>Anton, G</au><au>Anvar, S</au><au>Astraatmadja, T</au><au>J-J Aubert</au><au>Baret, B</au><au>Basa, S</au><au>Biagi, S</au><au>Bigongiari, C</au><au>Bogazzi, C</au><au>Bouhou, B</au><au>Brunner, J</au><au>Capone, A</au><au>Cârloganu, C</au><au>Carr, J</au><au>Charif, Z</au><au>Charvis, Ph</au><au>Chiarusi, T</au><au>Circella, M</au><au>Core, L</au><au>Costantini, H</au><au>Creusot, A</au><au>Curtil, C</au><au>Dekeyser, I</au><au>Donzaud, C</au><au>Dornic, D</au><au>Dumas, A</au><au>Eberl, T</au><au>Escoffier, S</au><au>Fermani, P</au><au>Flaminio, V</au><au>Folger, F</au><au>Fritsch, U</au><au>Fusco, L A</au><au>Galatà, S</au><au>Gay, P</au><au>Geißelsöder, S</au><au>Geyer, K</au><au>Gleixner, A</au><au>Gómez-González, J P</au><au>Graf, K</au><au>Guillard, G</au><au>H van Haren</au><au>Hello, Y</au><au>Hernández-Rey, J J</au><au>Hößl, J</au><au>Hugon, C</au><au>de Jong, M</au><au>Kadler, M</au><au>Kalekin, O</au><au>Kappes, A</au><au>Kooijman, P</au><au>Kouchner, A</au><au>Lahmann, R</au><au>Lambard, E</au><au>Larosa, G</au><au>Lefèvre, D</au><au>Leonora, E</au><au>D Lo Presti</au><au>Loehner, H</au><au>Marcelin, M</au><au>Margiotta, A</au><au>Martínez-Mora, J A</au><au>Martini, S</au><au>Michael, T</au><au>Müller, C</au><au>Neff, M</au><au>Nezri, E</au><au>Palioselitis, D</au><au>Păvălaş, G E</au><au>Popa, V</au><au>Pradier, T</au><au>Racca, C</au><au>Richter, R</au><au>Roensch, K</au><au>Rostovtsev, A</au><au>Samtleben, D F E</au><au>Schmid, J</au><au>Schüssler, F</au><au>Seitz, T</au><au>Shanidze, R</au><au>Simeone, F</au><au>Spies, A</au><au>Spurio, M</au><au>Stolarczyk, Th</au><au>Sánchez-Losa, A</au><au>Tamburini, C</au><au>Tayalati, Y</au><au>Trovato, A</au><au>Vallage, B</au><au>Vallée, C</au><au>Vecchi, M</au><au>Vernin, P</au><au>de Wolf, E</au><au>Yatkin, K</au><au>Zornoza, J D</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Search for Neutrino Emission from the Fermi Bubbles with the ANTARES Telescope</atitle><jtitle>arXiv.org</jtitle><date>2013-12-03</date><risdate>2013</risdate><eissn>2331-8422</eissn><abstract>Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1308.5260</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2013-12 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_1308_5260 |
source | Freely Accessible Journals; arXiv.org |
subjects | Bubbles Emission analysis Fluxes Gamma rays Neutrinos Physics - High Energy Astrophysical Phenomena Visibility |
title | A Search for Neutrino Emission from the Fermi Bubbles with the ANTARES Telescope |
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