one publication added to basket [284447] | Stacked search for time shifted high energy neutrinos from gamma ray bursts with the Antares neutrino telescope
Adrián-Martínez, S.; Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.-J.; Baret, B.; Barrios-Marti, J.; Basa, S.; Bertin, V.; Biagi, S.; Bormuth, R.; Bouwhuis, M.C.; Bruijn, R.; Brunner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Chiarusi, T.; Circella, M.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; Dekeyser, I.; Deschamps, A.; De Bonis, G.; Distefano, C.; Donzaud, C.; Dornic, D.; Drouhin, D.; Dumas, A.; Eberl, T.; Elsässer, D.; Enzenhöfer, A.; Fehn, K.; Felis, I.; Fermani, P.; Folger, F.; Fusco, L.A.; Galatà, S.; Gay, P.; Geißelsöder, S.; Geyer, K.; Giordano, V.; Gleixner, A.; Gracia-Ruiz, R.; Graf, K.; Hallmann, S.; van Haren, H.; Heijboer, A.J.; Hello, Y.; Hernández-Rey, J.J.; Hößl, J.; Hofestädt, J.; Hugon, C.; James, C.W.; de Jong, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kooijman, P.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lahmann, R.; Lefèvre, D.; Leonora, E.; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez-Mora, J.A.; Mathieu, A.; Michael, T.; Migliozzi, P.; Moussa, A.; Müller, C.; Nezri, E.; Pavalas, G.E.; Pellegrino, C.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Racca, C.; Riccobene, G.; Richter, R.; Roensch, K.; Saldaña, M.; Samtleben, D.F.E.; Sánchez-Losa, A.; Sanguineti, M.; Sapienza, P.; Schmid, J.; Schnabel, J.; Schüssler, F.; Seitz, T.; Sieger, C.; Spurio, M.; Steijger, J.J.M.; Stolarczyk, T.; Taiuti, M.; Tamburini, C.; Trovato, A.; Tselengidou, M.; Tönnis, C.; Vallage, B.; Vallée, C.; Van Elewyck, V.; Visser, E.; Vivolo, D.; Wagner, S.; Wilms, J.; Zornoza, J.D.; Zúñiga, J. (2017). Stacked search for time shifted high energy neutrinos from gamma ray bursts with the Antares neutrino telescope. Eur. Phys. J. C 77(1): 20. https://dx.doi.org/10.1140/epjc/s10052-016-4496-8
In: The European Physical Journal C. Springer: Berlin. ISSN 1434-6044; e-ISSN 1434-6052, meer
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Auteurs | | Top |
- Adrián-Martínez, S.
- Albert, A.
- André, M.
- Anghinolfi, M.
- Anton, G.
- Ardid, M.
- Aubert, J.-J.
- Baret, B.
- Barrios-Marti, J.
- Basa, S.
- Bertin, V.
- Biagi, S.
- Bormuth, R.
- Bouwhuis, M.C.
- Bruijn, R.
- Brunner, J.
- Busto, J.
- Capone, A.
- Caramete, L.
- Carr, J.
- Chiarusi, T.
- Circella, M.
- Coniglione, R.
- Costantini, H.
- Coyle, P.
- Creusot, A.
- Dekeyser, I.
- Deschamps, A.
- De Bonis, G.
- Distefano, C.
- Donzaud, C.
- Dornic, D.
- Drouhin, D.
- Dumas, A.
- Eberl, T.
- Elsässer, D.
- Enzenhöfer, A.
- Fehn, K.
- Felis, I.
- Fermani, P.
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- Folger, F.
- Fusco, L.A.
- Galatà, S.
- Gay, P.
- Geißelsöder, S.
- Geyer, K.
- Giordano, V.
- Gleixner, A.
- Gracia-Ruiz, R.
- Graf, K.
- Hallmann, S.
- van Haren, H.
- Heijboer, A.J.
- Hello, Y.
- Hernández-Rey, J.J.
- Hößl, J.
- Hofestädt, J.
- Hugon, C.
- James, C.W.
- de Jong, M.
- Kadler, M.
- Kalekin, O.
- Katz, U.
- Kießling, D.
- Kooijman, P.
- Kouchner, A.
- Kreter, M.
- Kreykenbohm, I.
- Kulikovskiy, V.
- Lahmann, R.
- Lefèvre, D.
- Leonora, E.
- Loucatos, S.
- Marcelin, M.
- Margiotta, A.
- Marinelli, A.
- Martínez-Mora, J.A.
- Mathieu, A.
- Michael, T.
- Migliozzi, P.
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- Moussa, A.
- Müller, C.
- Nezri, E.
- Pavalas, G.E.
- Pellegrino, C.
- Perrina, C.
- Piattelli, P.
- Popa, V.
- Pradier, T.
- Racca, C.
- Riccobene, G.
- Richter, R.
- Roensch, K.
- Saldaña, M.
- Samtleben, D.F.E.
- Sánchez-Losa, A.
- Sanguineti, M.
- Sapienza, P.
- Schmid, J.
- Schnabel, J.
- Schüssler, F.
- Seitz, T.
- Sieger, C.
- Spurio, M.
- Steijger, J.J.M.
- Stolarczyk, T.
- Taiuti, M.
- Tamburini, C.
- Trovato, A.
- Tselengidou, M.
- Tönnis, C.
- Vallage, B.
- Vallée, C.
- Van Elewyck, V.
- Visser, E.
- Vivolo, D.
- Wagner, S.
- Wilms, J.
- Zornoza, J.D.
- Zúñiga, J.
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Abstract |
A search for high-energy neutrino emission correlatedwith gamma-ray bursts outside the electromagneticprompt-emission time window is presented. Using a stackingapproach of the time delays between reported gammarayburst alerts and spatially coincident muon-neutrino signatures,data from the Antares neutrino telescope recordedbetween 2007 and 2012 are analysed. One year of public datafrom the IceCube detector between 2008 and 2009 have beenalso investigated. The respective timing profiles are scannedfor statistically significant accumulations within 40 days ofthe Gamma Ray Burst, as expected from Lorentz InvarianceViolation effects and some astrophysical models. No significantexcess over the expected accidental coincidence ratecould be found in either of the two data sets. The averagestrength of the neutrino signal is found to be fainter than onedetectable neutrino signal per hundred gamma-ray bursts inthe Antares data at 90% confidence level. |
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