Albert A, Andre M, Anghinolfi M, Anton G, Ardid M, Aubert JJ, Avgitas T, Baret B, Barrios-Marti J, Basa S, Belhorma B, Bertin V, Biagi S, Bormuth R, Bourret S, Bouwhuis MC, Branza H, Bruijn R, Brunner J, Busto J, Capone A, Caramete L, Carr J, Celli S, El Moursli RC, Chiarusi T, Circella M, Coelho JAB, Coleiro A, Coniglione R, Costantini H, Coyle P, Creusot A, Diaz AF, Deschamps A, De Bonis G, Distefano C, Di Palma I, Domi A, Donzaud C, Dornic D, Drouhin D, Eberl T, El Bojaddaini I, El Khayati N, Elsasser D, Enzenhofer A, Ettahiri A, Fassi F, Felis I, Fusco LA, Gay P, Giordano V, Glotin H, Gregoire T, Ruiz RG, Graf K, Hallmann S, Van Haren H, Heijboer AJ, Hello Y, Hernandez-Rey JJ, Hößl J, Hofestädt J, Hugon C, Illuminati G, James C, De Jong M, Jongen M, Kadler M, Kalekin O, Katz U, Kießling D, Kouchner A, Kreter M, Kreykenbohm I, Kulikovskiy V, Lachaud C, Lahmann R, Lefevre D, Leonora E, Lotze M, Loucatos S, Marcelin M, Margiotta A, Marinelli A, Martinez-Mora JA, Mele R, Melis K, Michael T, Migliozzi P, Moussa A, Navas S, Nezri E, Organokov M, Pavalas GE, Pellegrino C, Perrina C, Piattelli P, Popa V, Pradier T, Quinn L, Racca C, Riccobene G, Sanchez-Losa A, Saldana M, Salvadori I, Samtleben DFE, Sanguineti M, Sapienza P, Schussler F, Sieger C, Spurio M, Stolarczyk T, Taiuti M, Tayalati Y, Trovato A, Turpin D, Tonnis C, Vallage B, Van Elewyck V, Versari F, Vivolo D, Vizzoca A, Wilms J, Zornoza JD, Zuniga J (2017)
Publication Status: Published
Publication Type: Journal article, Original article
Publication year: 2017
Publisher: SPRINGER
Book Volume: 77
Article Number: 911
Journal Issue: 12
DOI: 10.1140/epjc/s10052-017-5451-z
Advanced LIGO detected a significant gravitational wave signal (GW170104) originating from the coalescence of two black holes during the second observation run on January 4th, 2017. Anall-sky high-energy neutrino follow-up search has been made using data from the Antares neutrino telescope, including both upgoing and downgoing events in two separate analyses. No neutrino candidates were found within +/- 500 s around the GW event time nor any time clustering of events over an extended time window of +/- 3 months. The non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from GW170104 to less than similar to 1.2 x 10(55) erg for a E-2 spectrum. This constraint is valid in the energy range corresponding to the 5-95% quantiles of the neutrino flux [3.2 TeV; 3.6 PeV], if the GW emitter was below the Antares horizon at the alert time.
APA:
Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J.-J.,... Zuniga, J. (2017). All-sky search for high-energy neutrinos from gravitational wave event GW170104 with the Antares neutrino telescope: The ANTARES Collaboration. European Physical Journal C, 77(12). https://doi.org/10.1140/epjc/s10052-017-5451-z
MLA:
Albert, A., et al. "All-sky search for high-energy neutrinos from gravitational wave event GW170104 with the Antares neutrino telescope: The ANTARES Collaboration." European Physical Journal C 77.12 (2017).
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