Magellanic Clouds Photometric Survey

The Magellanic Clouds Photometric Survey is a 4-band (UBVI) survey of the Large and Small Magellanic Clouds. We provide a catalog of stars in the central 8x8 degrees of the LMC and 4x4 degrees of the SMC, to a typical limiting magnitude of V = 21 (set primarily by crowding)

Welcome to the MCPS site

P.I. Dennis Zaritsky

This program was supported by the National Science Foundation through grant AST-9619576, a NASA LTSA award, two Hubble Fellowships from STScI, a fellowship from the David and Lucile Packard Foundation, a fellowship from the Sloan Foundation, a Fullam grant from the Dudley Observatory, and the Carnegie Institution of Washington. Any opinions, findings, and conclusions expressed in this material are those of the authors and do not necessarily reflect the views of any of the supporting agencies or institutions.