Magellanic Clouds Photometric Survey Home Page

Home	The Magellanic Cloud Photometric Survey is producing a UBVI catalog of stars in the central 8 by 8 degrees of the LMC and 4 by 4 degrees of the SMC. The limiting magnitude (set primarily by crowding) is V = 21.

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P.I. Dennis Zaritsky (Univ. of Arizona)

This program is 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 institutions.