Fig. B.3
All point sources detected by ALMA (this study), but missing Spitzer counterparts (Megeath et al. 2012), ordered by millimeter flux. Solid contours show the 3, 6, 12, and 24σ noise levels of the ALMA observations; dashed contours show the 1σ flux. The background is the VISTA Ks image from Meingast et al. (2016). Small labels indicate the types of nearby objects in this survey.
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