{"paper":{"title":"Optical and X-ray early follow-up of ANTARES neutrino alerts","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. Herrero, A.J. Heijboer, A. Klotz, A. Kouchner, A. Le Van Suu, A. Margiotta, A. Mathieu, A. Moussa, A. Rostovtsev, A. Sanchez-Losa, A. Trovato, B. Baret, B. Vallage, C. Akerlof, C. Bogazzi, C. Distefano, C. Donzaud, C. Hugon, C. Mueller, C. Pellegrino, C. Perrina, C. Racca, C. Sieger, C. Tamburini, C. Tonnis, C. Vallee, C.W James, D. Dornic, D. Drouhin, D. Elsasser, D. F. E. Samtleben, D. Kie{\\ss}ling, D. Lattuada, D. Lefevre, D.M. Coward, D. Turpin, D. Vivolo, E. Leonora, E. Nezri, E. Visser, F. Folger, F. Sch\\\"ussler, G. Anton, G. De Bonis, G.E. Pavalas, G. Lambard, G. Riccobene, H. Costantini, H. van Haren, I. Al Samarai, I. Dekeyser, I. Felis, I. Kreykenbohm, J.A. Martinez-Mora, J. Barrios-Marti, J. Brunner, J. Busto, J. Carr, J.D. Zornoza, J. Hofestadt, J. Ho{\\ss}l, J.-J. Aubert, J.J. Hernandez-Rey, J.J.M. Steijger, J. Kennea, J.P. Osborne, J. Schmid, J. Schnabel, J. Wilms, J. Zuniga, K. Fehn, K. Geyer, K. Graf, K. Roensch, L.A. Fusco, L. Caramete, M. Ageron, M. Andre, M. Ardid, M. Boer, M. Bou-Cabo, M.C. Bouwhuis, M. Circella, M. de Jong, M. Kadler, M. Marcelin, M. Neff, M. Saldana, M. Sanguineti, M. Spurio, M. Taiuti, M. Tselengidou, M. Vecchi, N. Gehrels, O. Kalekin, P. Coyle, P. Evans, 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. Adrian-Martinez, S. Basa, S. Biagi, S. Galata, S. Gei{\\ss}elsoder, S. Loucatos, S. Mangano, S. Martini, S. Schulte, 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, W. Zheng, Y. Hello","submitted_at":"2015-08-05T19:08:04Z","abstract_excerpt":"High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. Even with the recent detection of extraterrestrial high-energy neutrinos by the IceCube experiment, no astrophysical neutrino source has yet been discovered. Transient sources, such as gamma-ray bursts, core-collapse supernovae, or active galactic nuclei are promising candidates. Multi-messenger programs offer a unique opportunity to detect these transient sources. By combining the information provided by the ANTARES neutrino telescope with information c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.01180","kind":"arxiv","version":1},"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"}