Albert A, Andre M, Anton G, Ardid M, Aubert JJ, Avgitas T, Baret B, Barrios-Marti J, Basa S, Bertin V, Biagi S, Bormuth R, Bouwhuis MC, Bruijn R, Brunner J, Busto J, Capone A, Caramete L, Carr J, Celli S, Chiarusi T, Circella M, Coleiro A, Coniglione R, Costantini H, Coyle P, Creusot A, Deschamps A, De Bonis G, Distefano C, Di Palma I, Donzaud C, Dornic D, Drouhin D, Eberl T, El Bojaddaini I, Elsasser D, Enzenhofer A, Felis I, Fusco LA, Galata S, Gay P, Geißelsöder S, Geyer K, Giordano V, Gleixner A, Glotin H, Gracia-Ruiz R, Graf K, Hallmann S, Van Haren H, Heijboer AJ, Hello Y, Hernandez-Rey JJ, Hößl J, Hofestädt J, Hugon CM, 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, Loucatos S, Marcelin M, Margiotta A, Marinelli A, Martinez-Mora JA, Mathieu A, Melis K, Michael T, Migliozzi P, Moussa A, Mueller C, Nezri E, Pavalas GE, Pellegrino C, Perrina C, Piattelli P, Popa V, Pradier T, Racca C, Riccobene GM, Roensch K, Saldana M, Samtleben DFE, Sanchez-Losa A, Sanguineti M, Sapienza P, Schnabel J, Schussler F, Seitz T, Sieger C, Spurio M, Stolarczyk T, Taiuti M, Trovato A, Tselengidou M, Turpin D, Tonnis C, Vallage B, Vallee C, Van Elewyck V, Vivolo D, Wagner S, Wilms J, Zornoza JD, Zuniga J (2017)
Publication Status: Published
Publication Type: Journal article
Publication year: 2017
Publisher: IOP PUBLISHING LTD
Article Number: ARTN 019
Journal Issue: 4
DOI: 10.1088/1475-7516/2017/04/019
ANTARES is currently the largest neutrino telescope operating in the Northern Hemisphere, aiming at the detection of high-energy neutrinos from astrophysical sources. Neutrino telescopes constantly monitor at least one complete hemisphere of the sky, and are thus well-suited to detect neutrinos produced in transient astrophysical sources. A time-dependent search has been applied to a list of 33 X-ray binaries undergoing high flaring activities in satellite data (RXTE/ASM, MAXI and Swift/BAT) and during hardness transition states in the 2008-2012 period. The background originating from interactions of charged cosmic rays in the Earth's atmosphere is drastically reduced by requiring a directional and temporal coincidence with astrophysical phenomena. The results of this search are presented together with comparisons between the neutrino flux upper limits and the neutrino flux predictions from astrophysical models. The neutrino flux upper limits resulting from this search limit the jet parameter space for some astrophysical models.
APA:
Albert, A., Andre, M., Anton, G., Ardid, M., Aubert, J.-J., Avgitas, T.,... Zuniga, J. (2017). Time-dependent search for neutrino emission from X-ray binaries with the ANTARES telescope. Journal of Cosmology and Astroparticle Physics, 4. https://doi.org/10.1088/1475-7516/2017/04/019
MLA:
Albert, A., et al. "Time-dependent search for neutrino emission from X-ray binaries with the ANTARES telescope." Journal of Cosmology and Astroparticle Physics 4 (2017).
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