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Table 1.

Main information about the ALMA observations and source properties of the QSOs in our sample.

Source ID Beam Cont rms [CII] rms fcont Log(LFIR/L⊙) Log(LAGN/erg s−1) ( * *) Stack
[arcsec] [mJy beam−1] [mJy beam−1] [mJy beam−1] [109 L⊙] [km s−1]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
PJ007+04 6.001 0.47 × 0.69 0.05 0.58 1.87 ± 0.04 1.30 ± 0.15 365 ± 45 12.89 46.77 BF
PJ009−10 6.003 0.45 × 0.66 0.05 0.49 2.43 ± 0.12 2.28 ± 0.15 290 ± 35 12.98 46.73 AF
J0055+0146 6.005 0.60 × 0.72 0.03 0.30 0.22 ± 0.02 0.60 ± 0.07 330 ± 40 11.80 46.04 AE
J0109−3047 6.790 0.51 × 0.80 0.05 0.84 0.58 ± 0.04 1.64 ± 0.18 310 ± 40 12.30 46.37 AE
J0129−0035 5.779 0.36 × 0.45 0.02 0.24 3.04 ± 0.05 1.73 ± 0.04 200 ± 30 12.91 45.67 AF
J0142−3327 6.337 0.75 × 0.87 0.04 0.61 1.70 ± 0.06 2.94 ± 0.16 300 ± 30 12.71 47.24 BF
J0210−0456 6.433 0.61 × 0.90 0.03 0.29 0.16 ± 0.03 0.37 ± 0.04 185 ± 35 11.70 45.93 AE
J0305−3150 6.615 0.51 × 0.72 0.03 0.37 3.20 ± 0.05 2.34 ± 0.09 215 ± 30 13.02 46.59 AF
J0331−0741 4.737 0.31 × 0.40 0.05 0.45 3.75 ± 0.07 2.84 ± 0.11 475 ± 35 12.84 47.39 DF
PJ065−26 6.187 0.87 × 1.11 0.05 0.76 1.05 ± 0.07 1.94 ± 0.19 405 ± 40 12.48 47.01 DE
PJ065−19 6.125 0.75 × 1.09 0.04 1.32 0.42 ± 0.04 1.80 ± 0.40 315 ± 60 12.11 46.76 BE
J0454−4448 6.058 0.80 × 1.18 0.04 0.63 0.68 ± 0.05 0.62 ± 0.10 360 ± 70 12.30 46.68 AE
J0807+1328 4.879 0.25 × 0.40 0.03 0.67 6.64 ± 0.13 2.44 ± 0.19 435 ± 38 13.14 47.07 DF
J0842+1218 6.076 1.14 × 1.27 0.05 0.77 0.57 ± 0.04 1.62 ± 0.22 480 ± 55 12.24 46.88 DE
J0923+0247 4.655 0.29 × 0.51 0.04 0.30 2.94 ± 0.08 2.55 ± 0.09 325 ± 30 12.76 46.96 BF
J0935+0801 4.682 0.29 × 0.55 0.04 0.29 1.39 ± 0.05 0.70 ± 0.07 385 ± 40 12.48 47.25 BE
J1017+0327 4.949 0.30 × 0.38 0.03 0.32 1.23 ± 0.07 1.02 ± 0.05 270 ± 30 12.42 46.27 AE
PJ159−02 6.381 0.99 × 1.27 0.04 0.55 0.60 ± 0.05 1.24 ± 0.15 385 ± 45 12.27 46.83 BE
J1044−0125 5.785 0.66 × 0.72 0.02 0.29 3.07 ± 0.03 1.62 ± 0.08 470 ± 35 12.92 47.07 DF
J1048−0109 6.676 1.00 × 1.43 0.03 0.51 2.57 ± 0.03 2.42 ± 0.13 350 ± 35 12.94 46.51 AF
PJ167−13 6.515 0.98 × 1.27 0.04 0.51 0.69 ± 0.04 3.15 ± 0.19 480 ± 35 12.35 46.36 CE
J1120+0641 7.086 0.29 × 0.32 0.01 0.13 0.40 ± 0.02 0.69 ± 0.05 540 ± 40 12.19 46.77 DE
J1152+0055 6.365 1.02 × 1.36 0.04 0.70 0.50 ± 0.06 0.51 ± 0.10 140 ± 50 12.23 46.17 AE
J1207+0630 6.037 0.89 × 1.63 0.06 0.90 0.56 ± 0.04 1.16 ± 0.18 490 ± 95 12.20 46.77 DE
PJ183+05 6.439 1.06 × 1.24 0.04 0.59 4.62 ± 0.05 6.02 ± 0.19 370 ± 30 13.17 46.93 BF
J1306+0356 6.033 0.98 × 1.17 0.05 0.74 1.20 ± 0.05 1.87 ± 0.17 265 ± 35 12.53 46.84 BE
J1319+0950 6.132 1.10 × 1.26 0.03 0.43 5.00 ± 0.05 3.85 ± 0.18 520 ± 35 13.17 46.93 DF
J1321+0038 4.722 0.34 × 0.39 0.02 0.19 1.49 ± 0.04 1.19 ± 0.06 560 ± 35 12.47 46.70 CE
J1328−0224 4.646 0.31 × 0.48 0.04 0.37 1.58 ± 0.04 1.56 ± 0.06 300 ± 30 12.49 47.05 BE
J1341+0141 4.700 0.30 × 0.38 0.06 0.45 17.74 ± 0.33 3.06 ± 0.15 435 ± 35 13.55 47.50 DF
J1404+0314 4.924 0.34 × 0.40 0.05 0.58 10.98 ± 0.20 3.14 ± 0.15 515 ± 35 13.37 47.02 DF
PJ217−16 6.149 0.92 × 1.19 0.05 0.71 0.40 ± 0.02 0.89 ± 0.17 510 ± 70 12.14 46.89 DE
J1433+0227 4.727 0.34 × 0.44 0.05 0.43 7.69 ± 0.13 2.52 ± 0.08 415 ± 30 13.19 47.37 DF
J1509−1749 6.122 0.92 × 1.43 0.04 0.67 1.34 ± 0.04 1.72 ± 0.20 615 ± 75 12.59 46.9 DE
J1511+0408 4.679 0.31 × 0.53 0.06 0.46 10.08 ± 0.19 2.78 ± 0.18 580 ± 45 13.30 47.25 DF
PJ231−20 6.587 0.94 × 1.29 0.04 0.66 3.80 ± 0.10 2.97 ± 0.21 410 ± 35 13.09 46.99 DF
J1554+1937 4.627 0.74 × 1.26 0.16 1.67 11.98 ± 0.42 6.86 ± 0.43 800 ± 45 13.37 47.70 DF
PJ308−21 6.234 0.68 × 0.89 0.03 0.54 1.12 ± 0.08 2.17 ± 0.18 575 ± 45 12.53 46.65 CE
J2054−0005 6.039 0.73 × 0.76 0.02 0.40 2.89 ± 0.04 2.46 ± 0.07 230 ± 30 12.92 46.60 AF
J2100−1715 6.082 0.66 × 0.78 0.05 0.60 0.46 ± 0.02 1.27 ± 0.17 390 ± 60 12.22 46.33 AE
J2229+1457 6.151 0.70 × 0.80 0.03 0.42 0.14 ± 0.02 0.34 ± 0.06 240 ± 50 11.62 46.03 AE
J2244+1346 4.661 0.33 × 0.40 0.03 0.31 3.26 ± 0.05 1.74 ± 0.04 270 ± 30 12.80 46.58 AF
W2246−0526 4.601 0.35 × 0.37 0.05 0.52 7.18 ± 0.12 6.12 ± 0.19 740 ± 35 13.14 48.12 DF
J2310+1855 6.002 0.79 × 1.18 0.04 0.41 7.62 ± 0.12 5.74 ± 0.15 405 ± 30 13.34 47.23 DF
J2318−3029 6.148 0.75 × 0.87 0.05 0.82 2.87 ± 0.05 1.73 ± 0.18 275 ± 35 12.93 46.60 AF
J2318−3113 6.444 0.79 × 0.89 0.06 0.92 0.32 ± 0.04 1.26 ± 0.20 305 ± 55 12.00 46.56 AE
J2348−3054 6.902 0.62 × 0.82 0.05 0.79 1.90 ± 0.05 1.52 ± 0.23 455 ± 65 12.82 46.43 CF
PJ359−06 6.172 0.64 × 1.14 0.07 0.77 0.76 ± 0.05 1.66 ± 0.17 305 ± 40 12.46 46.83 BE

Notes. Columns give the following information: (1) source ID, (2) [CII]-based redshift, (3) x, (4) continuum rms sensitivity, (5) representative rms of the [CII] spectral region for a channel width of 30 km s−1, (6) continuum flux, (7) [CII] luminosity, (8) FWHM of the [CII] line, (9) FIR luminosity in the range 8–1000 μm derived from the ALMA continuum flux, (10) AGN bolometric luminosity. ( * ) Given the statistical error on the centroid of the best-fit Gaussian modelling the [CII] line and the systematics associated with the 30 km s−1 channel width of our ALMA spectra, the typical error on redshift is Δz[CII] = 0.001.

( * *) We consider as error on LAGN the 0.1 dex scatter associated with the bolometric correction by Runnoe et al. (2012).

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