  We present results of the long term monitoring of the gravitationally lensed
quasar HE1104-1805. The photometric data were collected between August 1997 and
January 2002 as a subproject of the OGLE survey.
  We determine the time delay in the light curves of images A and B of
HE1104-1805 to be equal to 157+/-21 days with the variability in the image B
light curve leading variability of the image A. The result is in excellent
agreement with the earlier determination by Ofek and Maoz.
  OGLE photometry of HE1104-1805 is available to the astronomical community
from the OGLE Internet archive.
