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The IceCube Realtime Alert System

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arxiv 1612.06028 v2 pith:JWCE6Z4Z submitted 2016-12-19 astro-ph.HE astro-ph.IM

IceCube Collaboration: M. G. Aartsen , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , K. Andeen
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T. Anderson I. Ansseau G. Anton M. Archinger C. Argüelles J. Auffenberg S. Axani X. Bai S. W. Barwick V. Baum R. Bay J. J. Beatty J. Becker Tjus K.-H. Becker S. BenZvi D. Berley E. Bernardini A. Bernhard D. Z. Besson G. Binder D. Bindig M. Bissok E. Blaufuss S. Blot C. Bohm M. Börner F. Bos D. Bose S. Böser O. Botner J. Braun L. Brayeur H.-P. Bretz S. Bron A. Burgman T. Carver M. Casier E. Cheung D. Chirkin A. Christov K. Clark L. Classen S. Coenders G. H. Collin J. M. Conrad D. F. Cowen R. Cross M. Day J. P. A. M. de André C. De Clercq E. del Pino Ro sendo H. Dembinski S. De Ridder P. Desiati K. D. de Vries G. de Wasseige M. de With T. DeYoung J. C. Díaz-Vélez V. di Lorenzo H. Dujmovic J. P. Dumm M. Dunkman B. Eberhardt T. Ehrhardt B. Eichmann P. Eller S. Euler P. A. Evenson S. Fahey A. R. Fazely J. Feintzeig J. Felde K. Filimonov C. Finley S. Flis C.-C. Fösig A. Francko wiak E. Friedman T. Fuchs T. K. Gaisser J. Gallagher L. Gerhardt K. Ghorbani W. Giang L. Gladstone T. Glauch T. Glüsenkamp A. Goldschmidt J. G. Gonzalez D. Grant Z . Griffith C. Haack A. Hallgren F. Halzen E. Hansen T. Hansmann K. Hanson D. Hebecker D. Heereman K. Helbing R. Hellauer S. Hickford J. Hignight G. C. Hill K. D. Hof fman R. Hoffmann K. Hoshina F. Huang M. Huber K. Hultqvist S. In A. Ishihara E. Jacobi G. S. Japaridze M. Jeong K. Jero B. J. P. Jones W. Kang A. Kappes T. Karg A. Karle U. Katz M. Kauer A. Keivani J. L. Kelley A. Kheirandish J. Kim M. Kim T. Kintscher J. Kiryluk T. Kittler S. R. Klein G. Kohnen R. Koirala H. Kolanoski R. Konietz L. Köpke C. Kopper S. Kopper D. J. Koskinen M. Kowalski K. Krings M. Kroll G. Krückl C. Krüger J. Kunnen S. Kunwar N. Kurahashi T. Kuwabara M. Labare J. L. Lanfranchi M. J. Larson F. Lauber D. Lennarz M. Lesiak-Bzdak M. Leuermann L. Lu J. Lünemann J. Madsen G. Maggi K. B. M. Mahn S. Mancina M. Mandelartz R. Maruy ama K. Mase R. Maunu F. McNally K. Meagher M. Medici M. Meier A. Meli T. Menne G. Merino T. Meures S. Miarecki T. Montaruli M. Moulai R. Nahnhauer U. Naumann G. Neer H. Niederhausen S. C. Nowicki D. R. Nygren A. Obertacke Pollmann A. Olivas A. O'Murchadha T. Palczewski H. Pandya D. V. Pankova P. Peiffer Ö. Penek J. A. Pepper C. Pérez de los Heros D. Pieloth E. Pinat P. B. Price G. T. Przybylski M. Quinnan C. Raab L. Rädel M. Rameez K. Rawlins R. Reimann B. Relethford M. Relich E. Resc oni W. Rhode M. Richman B. Riedel S. Robertson M. Rongen C. Rott T. Ruhe D. Ryckbosch D. Rysewyk L. Sabbatini S. E. Sanchez Herrera A. Sandrock J. Sandroos S. Sarkar K. Satalecka P. Schlunder T. Schmidt S. Schoenen S. Schöneberg L. Schumacher D. Seckel S. Seunarine D. Soldin M. Song G. M. Spiczak C. Spiering T. Stanev A. Stasik J. Stettner A. Steuer T. Stezelberger R. G. Stokstad A. Stö{ss}l R. Ström N. L. Strotjohann G. W. Sullivan M. Sutherland H. Taavola I. Taboada J. Tatar F. Tenholt S. Ter-Antonyan A. Terliuk G. Tešić S. Tilav P. A. Toale M. N. Tobin S. Toscano D. Tosi M. Tselengidou A. Turcati E. Unger M. Usner J. Vandenbroucke N. van Eijn dhoven S. Vanheule M. van Rossem J. van Santen M. Vehring M. Voge E. Vogel M. Vraeghe C. Walck A. Wallace M. Wallraff N. Wandkowsky Ch. Weaver M. J. Weiss C. Wendt S. Westerhoff B. J. Whelan S. Wickmann K. Wiebe C. H. Wiebusch L. Wille D. R. Williams L. Wills M. Wolf T. R. Wood E. Woolsey K. Woschnagg D. L. Xu X. W. Xu Y. Xu J. P. Yanez G. Yodh S. Yoshida M. Zoll
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keywords astrophysicalrealtimeicecubeneutrinosanalysesdetectorfollow-upframework
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Following the detection of high-energy astrophysical neutrinos 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 to 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 detector site and at IceCube facilities in the north that have enabled this fast follow-up program to be developed. 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.

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