Optical and Infrared Properties of Sources Observed by the Two Micron All Sky Survey and the Sloan Digital Sky Survey

Mathematics – Logic

Scientific paper

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Scientific paper

We positionally match sources observed by the Sloan Digital Sky Survey (SDSS) to sources observed by the Two Micron All Sky Survey (2MASS) in ~200 deg2 of high-latitude sky along the Celestial Equator. There are ~3*E6 SDSS sources and ~2*E5 2MASS sources in this region. Practically all ( ~99%) 2MASS sources are matched to an SDSS source within 1 arcsec, and ~12% of them are galaxies resolved in SDSS imaging data. Only ~25% of the optically resolved galaxies are also resolved in 2MASS data. We discuss the optical and infrared color-color and color-magnitude diagrams for the matched sources and show that stars, galaxies and quasars can be cleanly separated even without morphological information using only the optical-infrared colors. We calculate the K-band luminosity function for galaxies and find it consistent with previous work but with five times smaller error bars.

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