Notice

This is not the latest version of this item. The latest version can be found at:https://dspace.mit.edu/handle/1721.1/133915.2

Show simple item record

dc.date.accessioned2021-10-27T19:57:12Z
dc.date.available2021-10-27T19:57:12Z
dc.date.issued2017
dc.identifier.urihttps://hdl.handle.net/1721.1/133915
dc.description.abstract© 2017 Elsevier B.V. Although high-energy astrophysical neutrinos were discovered in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory. Several analyses selecting neutrinos of astrophysical origin are now operating in realtime at the detector site in Antarctica and are producing alerts for the community to enable rapid follow-up observations. The goal of these observations is to locate the astrophysical objects responsible for these neutrino signals. This paper highlights the infrastructure in place both at the South Pole site and at IceCube facilities in the north that have enabled this fast follow-up program to be implemented. Additionally, this paper presents the first realtime analyses to be activated within this framework, highlights their sensitivities to astrophysical neutrinos and background event rates, and presents an outlook for future discoveries.
dc.language.isoen
dc.publisherElsevier BV
dc.relation.isversionof10.1016/J.ASTROPARTPHYS.2017.05.002
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs License
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.sourcearXiv
dc.titleThe IceCube realtime alert system
dc.typeArticle
dc.relation.journalAstroparticle Physics
dc.eprint.versionAuthor's final manuscript
dc.type.urihttp://purl.org/eprint/type/JournalArticle
eprint.statushttp://purl.org/eprint/status/PeerReviewed
dc.date.updated2019-09-18T12:40:47Z
dspace.orderedauthorsAartsen, MG; Ackermann, M; Adams, J; Aguilar, JA; Ahlers, M; Ahrens, M; Altmann, D; Andeen, K; Anderson, T; Ansseau, I; Anton, G; Archinger, M; Argüelles, C; Auffenberg, J; Axani, S; Bai, X; Barwick, SW; Baum, V; Bay, R; Beatty, JJ; Becker Tjus, J; Becker, K-H; BenZvi, S; Berley, D; Bernardini, E; Bernhard, A; Besson, DZ; Binder, G; Bindig, D; Bissok, M; Blaufuss, E; Blot, S; Bohm, C; Börner, M; Bos, F; Bose, D; Böser, S; Botner, O; Braun, J; Brayeur, L; Bretz, H-P; Bron, S; Burgman, A; Carver, T; Casier, M; Cheung, E; Chirkin, D; Christov, A; Clark, K; Classen, L; Coenders, S; Collin, GH; Conrad, JM; Cowen, DF; Cross, R; Day, M; de André, JPAM; De Clercq, C; del Pino Rosendo, E; Dembinski, H; De Ridder, S; Desiati, P; de Vries, KD; de Wasseige, G; de With, M; DeYoung, T; Díaz-Vélez, JC; di Lorenzo, V; Dujmovic, H; Dumm, JP; Dunkman, M; Eberhardt, B; Ehrhardt, T; Eichmann, B; Eller, P; Euler, S; Evenson, PA; Fahey, S; Fazely, AR; Feintzeig, J; Felde, J; Filimonov, K; Finley, C; Flis, S; Fösig, C-C; Franckowiak, A; Friedman, E; Fuchs, T; Gaisser, TK; Gallagher, J; Gerhardt, L; Ghorbani, K; Giang, W; Gladstone, L; Glauch, T; Glüsenkamp, T; Goldschmidt, A; Gonzalez, JG; Grant, D; Griffith, Z; Haack, C; Hallgren, A; Halzen, F; Hansen, E; Hansmann, T; Hanson, K; Hebecker, D; Heereman, D; Helbing, K; Hellauer, R; Hickford, S; Hignight, J; Hill, GC; Hoffman, KD; Hoffmann, R; Hoshina, K; Huang, F; Huber, M; Hultqvist, K; In, S; Ishihara, A; Jacobi, E; Japaridze, GS; Jeong, M; Jero, K; Jones, BJP; Kang, W; Kappes, A; Karg, T; Karle, A; Katz, U; Kauer, M; Keivani, A; Kelley, JL; Kheirandish, A; Kim, J; Kim, M; Kintscher, T; Kiryluk, J; Kittler, T; Klein, SR; Kohnen, G; Koirala, R; Kolanoski, H; Konietz, R; Köpke, L; Kopper, C; Kopper, S; Koskinen, DJ; Kowalski, M; Krings, K; Kroll, M; Krückl, G; Krüger, C; Kunnen, J; Kunwar, S; Kurahashi, N; Kuwabara, T; Labare, M; Lanfranchi, JL; Larson, MJ; Lauber, F; Lennarz, D; Lesiak-Bzdak, M; Leuermann, M; Lu, L; Lünemann, J; Madsen, J; Maggi, G; Mahn, KBM; Mancina, S; Mandelartz, M; Maruyama, R; Mase, K; Maunu, R; McNally, F; Meagher, K; Medici, M; Meier, M; Meli, A; Menne, T; Merino, G; Meures, T; Miarecki, S; Montaruli, T; Moulai, M; Nahnhauer, R; Naumann, U; Neer, G; Niederhausen, H; Nowicki, SC; Nygren, DR; Obertacke Pollmann, A; Olivas, A; O’Murchadha, A; Palczewski, T; Pandya, H; Pankova, DV; Peiffer, P; Penek, Ö; Pepper, JA; Pérez de los Heros, C; Pieloth, D; Pinat, E; Price, PB; Przybylski, GT; Quinnan, M; Raab, C; Rädel, L; Rameez, M; Rawlins, K; Reimann, R; Relethford, B; Relich, M; Resconi, E; Rhode, W; Richman, M; Riedel, B; Robertson, S; Rongen, M; Rott, C; Ruhe, T; Ryckbosch, D; Rysewyk, D; Sabbatini, L; Sanchez Herrera, SE; Sandrock, A; Sandroos, J; Sarkar, S; Satalecka, K; Schlunder, P; Schmidt, T; Schoenen, S; Schöneberg, S; Schumacher, L; Seckel, D; Seunarine, S; Soldin, D; Song, M; Spiczak, GM; Spiering, C; Stanev, T; Stasik, A; Stettner, J; Steuer, A; Stezelberger, T; Stokstad, RG; Stößl, A; Ström, R; Strotjohann, NL; Sullivan, GW; Sutherland, M; Taavola, H; Taboada, I; Tatar, J; Tenholt, F; Ter-Antonyan, S; Terliuk, A; Tešić, G; Tilav, S; Toale, PA; Tobin, MN; Toscano, S; Tosi, D; Tselengidou, M; Turcati, A; Unger, E; Usner, M; Vandenbroucke, J; van Eijndhoven, N; Vanheule, S; van Rossem, M; van Santen, J; Vehring, M; Voge, M; Vogel, E; Vraeghe, M; Walck, C; Wallace, A; Wallraff, M; Wandkowsky, N; Weaver, C; Weiss, MJ; Wendt, C; Westerhoff, S; Whelan, BJ; Wickmann, S; Wiebe, K; Wiebusch, CH; Wille, L; Williams, DR; Wills, L; Wolf, M; Wood, TR; Woolsey, E; Woschnagg, K; Xu, DL; Xu, XW; Xu, Y; Yanez, JP; Yodh, G; Yoshida, S; Zoll, M
dspace.date.submission2019-09-18T12:40:48Z
mit.journal.volume92
mit.metadata.statusAuthority Work and Publication Information Needed


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

VersionItemDateSummary

*Selected version