  The results of a search for point sources of high energy neutrinos in the
northern hemisphere using data collected by AMANDA-II in the years 2000, 2001
and 2002 are presented. In particular, a comparison with the single-year result
previously published shows that the sensitivity was improved by a factor of
2.2. The muon neutrino flux upper limits on selected candidate sources,
corresponding to an E^{-2} neutrino energy spectrum, are included. Sky grids
were used to search for possible excesses above the background of cosmic ray
induced atmospheric neutrinos. This search reveals no statistically significant
excess for the three years considered.
