First Search for Point Sources of High Energy Cosmic Neutrinos with the   ANTARES Neutrino Telescope
  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 degrees. The neutrino flux sensitivity is 7.5 x 10-8 ~ (E/GeV)^-2 GeV^-1 s^-1 cm^-2 for the part of the sky that is always visible (declination < -48 degrees), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed. 
Antares Collaboration: S. Adri\'an-Mart\'inez, J.A. Aguilar, I. Al   Samarai, A. Albert, M. Andr\'e, M. Anghinolfi, G. Anton...
astro-ph.HE