Photometric recovery of crowded stellar fields observed with HST/WFPC2 andthe effects of confusion noise on the extragalactic distance scale

We explore the limits of photometric reductions of crowded stellar fields o bserved with the Wide Field and Planetary Camera 2 on board the Hubble Spac e Telescope. Two photometric procedures, based on the DoPHOT and DAOPHOT/AL LFRAME programs, are tested, and the effects of crowding, complex sky backg round, and cosmic-ray contamination are discussed using an extensive set of artificial star simulations. As a specific application of the results pres ented in this paper, we assess the magnitude of photometric biases on progr ams aimed at finding Cepheids and determining distances. We find that while the photometry in individual images can be biased too bright by up to 0.2 mag in the most crowded fields due to confusion noise, the effects on dista nce measurements based on Cepheid variables are insignificant, less than 0. 02 mag (1% in distance) even in the most problematic cases. This result, wh ich is at odds with claims that have recently surfaced in the literature, i s due to the strict criteria applied in the selection of the variable stars , and the photometric cross-checks made possible by the availability of mul tiple exposures in different filters which characterize Cepheid observation s.