The luminosity function of the globular cluster Palomar 1 is determined tog
ether with its confidence interval by applying an adaptive kernel estimator
to data from the Isaac Newton Telescope. The luminosity function of Paloma
r 1 has two minima in the V band and one in the I band. The cluster con con
tains a relatively high fraction of bright stars, indicative of mass segreg
ation. (C) 2000 MAIK "Nauka/lnterperionica".