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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Veröffentlicht in:arXiv.org 2013-12
Hauptverfasser: 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
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container_title arXiv.org
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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
format Article
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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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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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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>
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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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