Panels A and B: distance from the ALMA sources in the 100% pure main catalog to the closest IRAC counterpart in Ashby et al. (2015) (panel A) and VLA counterpart at 3 GHz (Rujopakarn et al., in prep.) (panel B). Panel A: sources whose coordinates were corrected accounting for blending in IRAC are highlighted in green (see main text). Panels C, D, E, and F: number of positive (yellow histogram) and negative (black histogram) detections in the σ_p = 3.0 blind detection in the combined dataset map with an IRAC counterpart at (panel C) and (panel E) or with a VLA counterpart at (panel D) and (panel F) as a function of stellar mass.