@Article{ANTARESCollaborationAdrian-Martinez_etal2011,
author="ANTARES Collaboration (Adrian-Martinez, S. et al
and Aguilar, J. A.
and Bigongiari, C.
and Dornic, D.
and Emanuele, U.
and Gomez-Gonzalez, J. P.
and Hernandez-Rey, J. J.
and Mangano, S.
and Ruiz-Rivas, J.
and Salesa, F.
and Sanchez-Losa, A.
and Toscano, S.
and Yepes, H.
and Zornoza, J. D.
and Zu{\~{n}}iga, J.",
title="First Search For Point Sources Of High-Energy Cosmic Neutrinos With The Antares Neutrino Telescope",
journal="Astrophysical Journal Letters",
year="2011",
publisher="Iop Publishing Ltd",
volume="743",
number="1",
pages="L14 - 6pp",
optkeywords="astroparticle physics; cosmic rays; neutrinos",
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.",
optnote="WOS:000297372600014",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=826), last updated on Thu, 09 Jul 2020 11:08:32 +0000",
issn="2041-8205",
doi="10.1088/2041-8205/743/1/L14",
opturl="http://arxiv.org/abs/1108.0292",
opturl="https://doi.org/10.1088/2041-8205/743/1/L14",
archivePrefix="arXiv",
eprint="1108.0292",
language="English"
}