The ARAUCARIA Project: Discovery of Cepheid Variables in NGC 300 from a Wide-Field Imaging Survey

Based on observations of NGC 300, obtained with the Wide-Field Camera at the2.2 m ESO/MPI telescope during 29 nights spread over a 5.3 month interval, 117Cepheids and 12 Cepheid candidates were found which cover the period range from115 to 5.4 days. We present a catalog which provides equatorial coordinates,period, time of maximum brightness, and intensity mean B and V magnitudes foreach variable, and we show phased B and V light curves for all the Cepheidsfound. We also present the individual B and V observations for each Cepheid inour catalog. We find very good agreement between our photometry and thatobtained by Freedman et al. from ground-based CCD data for common stars. TheCepheids delineate the spiral arms of NGC 300, and a couple of them weredetected very close to the center of the galaxy. From the color-magnitudediagram of NGC 300 constructed from our data, we expect that our Cepheiddetection is near-complete for variables with periods larger than about 10days. We present plots of the PL relations in the B and V bands obtained fromour data, which clearly demonstrate the presence of a Malmquist bias forperiods below about 10 days. A thorough discussion of the distance to NGC 300will be presented in a forthcoming paper which will include the analysis ofphotometry in longer-wavelength bands.