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Table 1.

NOEMA observations.

Name RA, Dec z[C II] Freq. Beam RMS Sν Size
h:m:s, d:m:s (J2000.0) [GHz] [arcsec2] [μJy/beam] [μJy] [arcsec2]
J0313-1806 03:13:43.84, −18:06:36.40 7.6423 USB 92.568 13.1 × 3.7 48.5 < 100.5 (a)
LSB 78.756 16.4 × 4.3 46.3
B6 219.911 0.62 × 0.44 19 0.50 ± 0.05 0.71 × 0.55
J1243+0100 12:43:53.93, +01:00:38.50 7.0749 USB 100.310 5.8 × 2.3 16.1 119 ± 16
LSB 86.756 6.3 × 2.8 13.0 49.8 ± 12.5
B6 235.364 0.62 × 0.50 19 2.07 ± 0.09 0.78 × 0.72
J0038-1527 00:38:36.10, −15:27:23.60 7.034 USB 100.821 6.2 × 3.8 22.3 < 44.4 (a)
LSB 87.256 7.3 × 4.4 19.8
B6 236.562 0.62 × 0.55 37 1.8 ± 0.7 1.9 × 1.2
J2356+0017 23:56:46.33, +00:17:47.30 7.01 USB 101.373 4.6 × 3.5 15.8 54 ± 15
LSB 87.756 5.4 × 4.1 13.4 < 40.2
J0252-0503 02:52:16.64, −05:03:31.80 7.0006 USB 101.491 5.6 × 4.2 19.0 123.4 ± 17.8
LSB 87.756 6.6 × 4.9 15.6 76.9 ± 14.9
B6 237.852 0.56 × 0.40 35 1.04 ± 0.10 0.72 × 0.55

Notes. NOEMA fluxes are derived from a fit of the visibilities with a point source model. ALMA band 6 (B6) fluxes are the integrated emission of best-fit 2D Gaussian function model of the cleaned continuum map. Upper limits are at the 3σ significance level. RMS is estimated using a channel width of 20 MHz.

(a)

upper limits are computed for the merged USB + LSB continuum data.

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