High-energy gamma-ray astronomy is now a well-established field, and severa
l sources have been discovered in the region from a few giga-electron volts
up to several tera-electron volts. If sources involving hadronic processes
exist, the production of photons would be accompanied by neutrinos too. Ot
her possible neutrino sources could be related to the annihilation of weakl
y interacting, massive particles (WIMPs) at the center of galaxies with bla
ck holes. We present the results of a search for pointlike sources using 11
00 upward-going muons produced by neutrino interactions in the rock below a
nd inside the Monopole Astrophysics and Cosmic Ray Observatory (MACRO) dete
ctor in the underground Gran Sasso Laboratory. These data show no evidence
of a possible neutrino pointlike source or of possible correlations between
gamma-ray bursts and neutrinos. They have been used to set flux upper limi
ts for candidate pointlike sources which are in the range 10(-14)-10(-15) c
m(-2) s(-1).