Adrian-Martinez S, Aguilar JA, Al Samarai I, Albert A, Andre M, Anghinolfi M, Anton G, Anvar S, Ardid M, Jesus ACA, Astraatmadja T, Aubert JJ, Baret B, Basa S, Bertin V, Biagi S, Bigi A, Bigongiari C, Bogazzi C, Bou-Cabo M, Bouhou B, Bouwhuis MC, Brunner J, Busto J, Camarena F, Capone A, Carloganu C, Carminati G, Carr J, Cecchini S, Charif Z, Charvis P, Chiarusi T, Circella M, Coniglione R, Costantini H, Coyle P, Curtil C, Decowski MP, Dekeyser I, Deschamps A, Distefano C, Donzaud C, Dornic D, Dorosti Q, Drouhin D, Eberl T, Emanuele U, Enzenhöfer A, Ernenwein JP, Escoffier S, Fermani P, Ferri M, Flaminio V, Folger F, Fritsch U, Fuda JL, Galata S, Gay P, Giacomelli G, Giordano V, Gomez-Gonzalez JP, Graf K, Guillard G, Halladjian G, Hallewell G, Van Haren H, Hartman J, Heijboer AJ, Hello Y, Hernandez-Rey JJ, Herold B, Hößl J, Hsu CC, De Jong M, Kadler M, Kalekin O, Kappes A, Katz U, Kavatsyuk O, Kooijman P, Kopper C, Kouchner A, Kreykenbohm I, Kulikovskiy V, Lahmann R, Lamare P, Larosa G, Lattuada D, Lefevre D, Lim G, Lo Presti D, Loehner H, Loucatos S, Mangano S, Marcelin M, Margiotta A, Martinez-Mora JA, Meli A, Montaruli T, Moscoso L, Motz H, Neff M, Nezri E, Palioselitis D, Pavalas GE, Payet K, Payre P, Petrovic J, Piattelli P, Picot-Clemente N, Popa V, Pradier T, Presani E, Racca C, Reed C, Richardt C, Richter R, Riviere C, Robert A, Roensch K, Rostovtsev A, Ruiz-Rivas J, Rujoiu M, Russo GV, Salesa F, Samtleben DFE, Sapienza P, Schoeck F, Schuller JP, Schuessler F, Seitz T, Shanidze R, Simeone F, Spies A, Spurio M, Steijger JJM, Stolarczyk T, Sanchez-Losa A, Taiuti M, Tamburini C, Toscano S, Vallage B, Van Elewyck V, Vannoni G, Vecchi M, Vernin P, Wagner S, Wijnker G, Wilms J, De Wolf E, Yepes H, Zaborov D, Zornoza JD, Zuniga J (2011)
Publication Status: Published
Publication Type: Journal article
Publication year: 2011
Publisher: IOP PUBLISHING LTD
Book Volume: 743
Article Number: ARTN L14
Journal Issue: 1
DOI: 10.1088/2041-8205/743/1/L14
Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 +/- 0.1 deg. The neutrino flux sensitivity is 7.5 x 10(-8)(E(v)/GeV)(-2) GeV(-1) s(-1) cm(-2) for the part of the sky that is always visible (delta < -48 deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.
APA:
Adrian-Martinez, S., Aguilar, J.A., Al Samarai, I., Albert, A., Andre, M., Anghinolfi, M.,... Zuniga, J. (2011). FIRST SEARCH FOR POINT SOURCES OF HIGH-ENERGY COSMIC NEUTRINOS WITH THE ANTARES NEUTRINO TELESCOPE. Astrophysical Journal Letters, 743(1). https://doi.org/10.1088/2041-8205/743/1/L14
MLA:
Adrian-Martinez, S., et al. "FIRST SEARCH FOR POINT SOURCES OF HIGH-ENERGY COSMIC NEUTRINOS WITH THE ANTARES NEUTRINO TELESCOPE." Astrophysical Journal Letters 743.1 (2011).
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