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Table 2.

Results of the observations for the sample sources.

ID (a) [C II] freq. (b) z[C II](c) rms (d) Speak(e) FWHM Scont(f) LIR(g)
[GHz] [mJy beam−1] [mJy] [km s−1] [mJy] [1012 L⊙]
PSO J007.0273+04.9571 271.463 6.001 0.39 4.89 965 1.87 ± 0.04 2.09 ± 0.48
PSO J009.7355–10.4316 271.364 6.004 0.36 17.32 583 1.60 ± 0.04 1.78 ± 0.41
SDSS J0129–0035 280.390 5.778 0.10 10.60 384 2.65 ± 0.02 2.9 ± 0.7
VST-ATLAS J025.6821–33.4627 259.010 6.338 0.70 12.16 656 1.19 ± 0.05 1.4 ± 0.3
PSO J065.4085–26.9543 264.429 6.187 0.79 7.12 854 1.00 ± 0.05 1.2 ± 0.3
PSO J065.5041–19.4579 266.753 6.125 0.73 3.47 777 0.38 ± 0.05 0.4 ± 0.1
VDES J0454–4448 269.272 6.058 0.62 1.68 726 0.55 ± 0.04 0.6 ± 0.1
PSO J159.2257–02.5438 257.450 6.382 0.54 3.90 717 0.53 ± 0.04 0.6 ± 0.1
SDSS J1044–0125 280.106 5.786 0.24 4.16 895 3.03 ± 0.02 3.3 ± 0.8
VIK J1048–0109 247.600 6.676 0.49 7.42 707 2.50 ± 0.04 3.1 ± 0.7
PSO J167.6415–13.4960 252.932 6.514 0.21 7.97 1003 0.58 ± 0.04 0.7 ± 0.2
VIK J1152+0055 258.045 6.365 0.74 2.27 386 0.09 ± 0.03 0.1 ± 0.04
PSO J183.1124+05.0926 255.500 6.438 0.66 19.05 763 3.99 ± 0.05 5 ± 1
SDSS J1306+0356 270.181 6.034 0.76 9.46 598 0.82 ± 0.04 0.9 ± 0.2
ULAS J1319+0950 266.431 6.133 0.37 9.05 1016 4.59 ± 0.03 5 ± 1
CFQS J1509–1749 266.859 6.122 0.66 3.54 1135 1.46 ± 0.04 1.7 ± 0.4
PSO J231.6576–20.83335 250.490 6.587 0.68 8.13 922 3.34 ± 0.12 4 ± 1
PSO J308.0416–21.2339 262.616 6.237 0.56 6.20 1128 0.53 ± 0.05 6.1 ± 0.1
SDSS J2054–0005 270.007 6.039 0.33 13.81 441 2.60 ± 0.03 2.9 ± 0.7
CFQS J2100–1715 268.393 6.081 0.51 3.16 870 0.36 ± 0.05 0.4 ± 0.1
VIK J2211–3206 258.963 6.339 0.57 0.71 807 0.59 ± 0.03 0.7 ± 0.2
VIMOS2911001793 265.832 6.14 0.22 8.8 270 0.76 ± 0.03 0.86 ± 0.19
SDSS J2310+1855 271.397 6.003 0.38 19.71 788 6.97 ± 0.05 8 ± 2
VIK J2318–3113 255.329 6.443 0.84 2.96 609 0.36 ± 0.04 0.4 ± 0.1
VIK J2318–3029 265.960 6.146 0.93 7.36 582 2.33 ± 0.06 2.7 ± 0.6
PSO J359.1352–06.3831 265.007 6.172 0.84 6.53 626 0.60 ± 0.06 0.7 ± 0.2

Notes. Only sources with a [C II] detection are included here (see Table 1).

(a)

Source ID.

(b)

Observed [C II] frequency.

(c)

[C II] redshift calculated from the observed line.

(d)

The rms of the spectrum from the final imaging with beamsize of 0.8″×0.8″, and channelwidths of 30 km s−1.

(e)

The peak flux density of the [C II] line.

(f)

The band-6 continuum flux density.

(g)

The IR (8–1000 μm) luminosity calculated from the band-6 continuum. In bold we highlight the sources included in the max sub-sample.

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