{"paper":{"title":"Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Capone, A. Creusot, A. Deschamps, A. Dumas, A. Enzenhofer, A. Gleixner, A. J. Heijboer, A. Kouchner, A. Margiotta, A. Marinelli, A. Mathieu, A. Moussa, ANTARES Collaboration: S. Adrian-Mart\\'inez, A. S\\'anchez-Losa, A. Trovato, B. Baret, B. Vallage, C. Distefano, C. Donzaud, C. Hugon, C. Muller, C. Pellegrino, C. Perrina, C. Racca, C. Sieger, C. Tamburini, C. Tonnis, C. Vall\\'ee, C. W. James, D. Dornic, D. Drouhin, D. Elsasser, D. F. E. Samtleben, D. Kiessling, D. Lef\\`evre, D. Vivolo, E. Leonora, E. Nezri, E. Visser, F. Folger, F. Schussler, G. Anton, G. De Bonis, G. E. Pavalas, G. Riccobene, H. Costantini, H. van Haren, I. Dekeyser, I. Felis, I. Kreykenbohm, J. A. Mart\\'inez-Mora, J. Barrios-Marti, J. Brunner, J. Busto, J. Carr, J. D. Zornoza, J. Hoessl, J. Hofestadt, J.-J. Aubert, J. J. Hern\\`andez-Rey, J. J. M. Steijger, J. Schmid, J. Schnabel, J. Wilms, J. Z\\'u\\~niga, K. Fehn, K. Geyer, K. Graf, K. Roensch, L. A. Fusco, L. Caramete, M. Andr\\'e, M. Anghinolfi, M. Ardid, M. C. Bouwhuis, M. Circella, M. de Jong, M. Kadler, M. Kreter, M. Marcelin, M. Salda\\~na, M. Sanguineti, M. Spurio, M. Taiuti, M. Tselengidou, O. Kalekin, P. Coyle, P. Fermani, P. Gay, P. Kooijman, P. Migliozzi, P. Piattelli, P. Sapienza, R. Bormuth, R. Bruijn, R. Coniglione, R. Gracia-Ruiz, R. Lahmann, R. Richter, S. Basa, S. Biagi, S. Galat\\`a, S. Geisselsoeder, S. Hallmann, S. Loucatos, S. Wagner, T. Chiarusi, T. Eberl, Th. Stolarczyk, T. Michael, T. Pradier, T. Seitz, U. Katz, V. Bertin, V. Giordano, V. Kulikovskiy, V. Popa, V. Van Elewyck, Y. Hello","submitted_at":"2016-08-31T13:28:17Z","abstract_excerpt":"A search for high-energy neutrino emission correlated with gamma-ray bursts outside the electromagnetic prompt-emission time window is presented. Using a stacking approach of the time delays between reported gamma-ray burst alerts and spatially coincident muon-neutrino signatures, data from the Antares neutrino telescope recorded between 2007 and 2012 are analysed. One year of public data from the IceCube detector between 2008 and 2009 have been also investigated. The respective timing profiles are scanned for statistically significant accumulations within 40 days of the Gamma Ray Burst, as ex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.08840","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}