Estimating the angular resolution of tracks in neutrino telescopes based on a likelihood analysis

Details Estimating the angular resolution of tracks in neutrino telescopes based on a likelihood analysis Estimating the angular resolution of tracks in neutrino telescopes based on a likelihood analysis

2004-03-16

arxiv.org/abs/astro-ph/0403367v1

Astropart.Phys. 25 (2006) 220-225

Astronomy and Astrophysics

Astrophysics

11 pages, 4 figures, submitted to Astropart. Phys

Scientific paper

10.1016/j.astropartphys.2006.01.

A semianalytic method to estimate the angular resolution of tracks, that have
been reconstructed by a likelihood approach, is presented. The optimal choice
of coordinate systems and resolution parameters, as well as tests of the method
are discussed based on an application for a neutrino telescope.

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