Photographic photometry of Magellanic Cloud cepheids

Bibliography: pages 167-169.Photographic (B,V) light curves of 213 LMC and 180 SMC cepheids (and W Virginis stars) have been obtained and the relevant light-curve parameters derived. Comparison of this work with stars in common with photoelectric data indicate that the and ( - ) magnitudes differ from their photoelectric counterparts by ±0ᵐ.09 and ±0ᵐ.12 respectively for the fainter cepheids (log P 0.8)