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An ALMA survey of the SCUBA 2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties

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Figure

Figure 1. A sample of the multi-wavelength coverage of the AS2UDS sample which motivates this extra-galactic field being chosen forhigh resolution ALMA follow-up
Figure 2. The distribution of the rms noise estimates from the0′′.5 uv-tapered detection maps for the different cycles used inAS2UDS
Figure 3. HST I814J125H160-band colour images (5′′.4 square) of the 47 ALMA SMGs in our sample that lie in the CANDELS region.Contours are taken from the tapered ALMA maps, and denote the 870 µm emission, and start at 3 σ and are incremented by 3 σ
Figure 4. Left:flux limit the completeness declines, reaching 50 % at 1.3 mJy for the ALMA maps that were observed twice
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