New young star candidates in Taurus-Auriga (Rebull+, 2011)

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Photometry: Infrared, Ysos, Surveys, Stars: Pre-Main Sequence, Molecular Clouds

Scientific paper

In the context of Rebull et al. (2010ApJS..186..259R), we assembled a substantial multi-wavelength database, spanning Sloan u through Spitzer/MIPS 160um (with some X-rays) for point sources throughout the Taurus region. We use that catalog as the core for our analysis here, updating it with confirmed Taurus members from, e.g., Kenyon et al. (2008hsf1.book..405K) and Luhman et al. (2010ApJS..186..111L) outside of our original Spitzer map. We have also searched SIMBAD (and literature references therein) for known galaxies and other contaminants in this vicinity. Our Taurus Spitzer Survey spanned ~44deg2 (figure 1). WISE data acquisition and reduction are discussed in Wright et al. (2010AJ....140.1868W), Jarrett et al. (2011, ApJ, submitted), and in the Explanatory Supplement to the WISE Preliminary Data Release Products. There are four WISE bands, with central wavelengths at 3.4, 4.6, 12, and 22um, and a spatial resolution of 6" (12" at 22um).
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