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Table 1

ALMA survey fields used in this paper, sorted by sensitivity.

Project ν obs σ λ Area Field
code [GHz] [μJy beam-1] [mm] [10-4 deg2]
(1) (2) (3) (4)

2012.A.00040.S 230 7.8 1.28 1.17 a
2012.1.00374.S 225 14.5 1.31 1.17 b
2012.1.00719.S 230 17.7 1.30 1.17 c
2011.1.00115.S 260 18.6 1.16 0.87 d
2012.1.00719.S 244 19.5 1.23 1.06 e
2011.1.00243.S 250 20.9 1.2 0.97 f
2011.0.00767.S 230 20.9 1.30 1.17 g
2012.1.00142.S 230 26.3 1.28 1.07 h
2011.1.00243.S 249 28.9 1.2 0.97 i
2012.1.00523.S 286 29.9 1.05 0.72 j
2012.1.00523.S 295 30.0 1.02 0.71 k
2012.1.00523.S 286 30.3 1.05 0.72 l
2012.1.00523.S 289 33.1 1.05 0.72 m
2012.1.00523.S 290 36.3 1.03 0.71 n
2012.1.00523.S 289 38.1 1.05 0.72 o
2012.1.00523.S 289 41.8 1.05 0.72 p
2012.1.00523.S 292 49.1 1.02 0.71 q
2012.1.00523.S 292 52.1 1.02 0.71 r

Notes. (1) Frequency in the observed frame corresponding to the mean frequency of the four ALMA spectral window. (2) rms measured in each continuum map before primary beam correction. (3) Central wavelength in the observed frame. (4) Area in two primary beams. The size of the primary beam scales linearly with wavelength.

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