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First Search For Point Sources Of High-Energy Cosmic Neutrinos With The Antares Neutrino Telescope

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First Search For Point Sources Of High-Energy Cosmic Neutrinos With The Antares Neutrino Telescope

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dc.contributor.author	ANTARES Collaboration
dc.contributor.author	Aguilar Sánchez, Juan Antonio
dc.contributor.author	Bigongiari, C.
dc.contributor.author	Dornic, Damien
dc.contributor.author	Emanuele, U.
dc.contributor.author	Gómez González, Juan Pablo
dc.contributor.author	Hernández Rey, Juan José
dc.contributor.author	Mangano, Salvatore
dc.contributor.author	Ruiz-Rivas Onsés, Joaquín
dc.contributor.author	Salesa Greus, Francisco
dc.contributor.author	Sánchez Losa, Agustín
dc.contributor.author	Toscano, S.
dc.contributor.author	Yepes Ramírez, Harold
dc.contributor.author	Zornoza Gómez, Juan de Dios
dc.contributor.author	Zúñiga Román, Juan
dc.date.accessioned	2016-05-20T12:18:09Z
dc.date.available	2016-05-20T12:18:09Z
dc.date.issued	2011
dc.identifier.citation	ANTARES Collaboration Aguilar Sánchez, Juan Antonio Bigongiari, C. Dornic, Damien Emanuele, U. Gómez González, Juan Pablo Hernández Rey, Juan José Mangano, Salvatore Ruiz-Rivas Onsés, Joaquín Salesa Greus, Francisco Sánchez Losa, Agustín Toscano, S. Yepes Ramírez, Harold Zornoza Gómez, Juan de Dios Zúñiga Román, Juan 2011 First Search For Point Sources Of High-Energy Cosmic Neutrinos With The Antares Neutrino Telescope Astrophysical Journal Letters 743 1 L14
dc.identifier.uri	http://hdl.handle.net/10550/53649
dc.description.abstract	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.
dc.language.iso	eng
dc.relation.ispartof	Astrophysical Journal Letters, 2011, vol. 743, num. 1, p. L14
dc.subject	Física nuclear
dc.title	First Search For Point Sources Of High-Energy Cosmic Neutrinos With The Antares Neutrino Telescope
dc.type	journal article	es_ES
dc.date.updated	2016-05-20T12:18:10Z
dc.identifier.doi	10.1088/2041-8205/743/1/L14
dc.identifier.idgrec	070477
dc.rights.accessRights	open access	es_ES