Abstract
The IceCube detector took data in its 22-string configuration in 2007-2008. This data has been analyzed to search for extraterrestrial point sources of neutrinos using several methods. Two main methods are discussed and compared here: the binned and the unbinned maximum likelihood method. The best sky-averaged sensitivity (90% C.L.) is E2 Φνμ = 1.3 × 10- 11 TeVcm- 2 s- 1 to a generic E-2 flux of νμ over the energy range from 3 TeV to 3 PeV. No neutrino point sources are found from the individual directions of a pre-selected catalogue nor in a search extended to the northern sky. Limits are improved by a factor of two compared to the total statistics collected with the AMANDA-II detector and represent the best results to date.
Original language | English |
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Pages (from-to) | 267-269 |
Number of pages | 3 |
Journal | Nuclear Physics B - Proceedings Supplements |
Volume | 188 |
Issue number | C |
DOIs | |
State | Published - Mar 2009 |
Externally published | Yes |