|H-ATLAS ID||SDSS ID||Sp. type||Distance (pc)||F250 (mJy)||F350 (mJy)||F500 (mJy)||T (K)||Dust mass ( )|
Notes. Spectral types are estimated from the (g - i) colour relation of Covey et al. (2007) and distances from the photometric parallax from Davenport et al. (2006). Temperatures are estimated by a greybody fit to the 250, 350 and 500 m fluxes and the upper limits of 140 mJy at 160 m, and 105 mJy at 110 m with a fixed (Wyatt et al. 2005). Masses are calculated using the standard technique with a mass absorption coefficient cm2 g-1 at 850 m (Sheret et al. 2004).
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