  We analysed the arrival directions of single muons detected by the first LVD
tower from November, 1994 till January, 1998. The moon shadowing effect has
been observed. To search for point sources of high energy photons we have
analysed muons crossing the rock thickness greater than 3, 5 and 7 km w.e.,
which corresponds to the mean muon energies 1.6, 3.9 and 8.4 TeV at the
surface, respectively. Upper limits on steady muon fluxes for selected
astrophysical sources for different muon energies are presented.
