Table 1.
Properties for our sample of z ∼ 6 quasars available in the ALMA archive by January 2018.
| ID (a) | RA (b) | Dec (c) | z(d) | log Lbol(e) | Project (f) | [C II] (g) | Original (h) |
|---|---|---|---|---|---|---|---|
| hh:mm:ss | dd:mm:ss | detected | beamsize | ||||
| PSO J007.0273+04.9571(1, 2, 6) | 00:28:06.56 | +04:57:25.7 | 6.00 | 46.59 | C | Y | 0.65″ × 0.47″ |
| PSO J009.7355−10.4316(2, 6) | 00:38:56.52 | −10:25:53.9 | 5.95 | 46.55 | C | Y | 0.63″ × 0.44″ |
| SDSS J0129−0035(3, 16) | 01:29:58.51 | −00:35:39.7 | 5.779 | 45.59 | B | Y | 0.45″ × 0.38″ |
| VST-ATLAS J025.6821–33.4627 | 01:42:43.73 | −33:27:45.5 | 6.31 | 47.02 | C | Y | 0.87″ × 0.75″ |
| (J0142−3327)(2, 4, 6) | |||||||
| PSO J065.4085−26.9543(2, 6) | 04:21:38.05 | −26:57:15.6 | 6.14 | 46.82 | C | Y | 1.11″ × 0.83″ |
| PSO J065.5041−19.4579(2, 6) | 04:22:00.99 | −19:27:28.7 | 6.12 | 46.59 | C | Y | 1.09″ × 0.75″ |
| VDESJ0454−4448(2, 6, 13) | 04:54:01.79 | −44:48:31.1 | 6.09 | 46.53 | C | Y | 1.12″ × 0.79″ |
| SDSS J0842+1218(2, 5, 6, 8) | 08:42:29.23 | +12:18:48.2 | 6.069 | 46.69 | C | N ( * ) | 1.26″ × 1.12″ |
| PSO J159.2257−02.5438(2, 6) | 10:36:54.19 | −02:32:37.9 | 6.38 | 46.65 | C | Y | 1.28″ × 0.98″ |
| SDSS J1030+0524(2, 6) | 10:30:27.10 | +05:24:55.0 | 6.308 | 46.72 | C | N | 1.21″ × 0.98″ |
| SDSS J1044−0125(2, 3) | 10:44:33.04 | −01:25:02.2 | 5.7847 | 46.86 | B | Y | 0.74″ × 0.70″ |
| VIK J1048−0109(6, 15) | 10:48:19.09 | −01:09:40.3 | 6.661 | 46.36 | C | Y | 1.46″ × 1.00″ |
| PSO J167.6415−13.4960(2, 6, 14, 19) | 11:10:33.98 | −13:29:45.6 | 6.508 | 46.22 | A,C | Y | 0.77″ × 0.63″ |
| ULAS J1148+0702(2, 6) | 11:48:03.29 | +07:02:08.3 | 6.32 | 46.54 | C | N | 1.32″ × 1.08″ |
| VIK J1152+0055(2, 6, 10) | 11:52:21.27 | +00:55:36.7 | 6.37 | 46.04 | C | Y | 1.26″ × 1.02″ |
| ULAS J1207+0630(2, 6) | 12:07:37.44 | +06:30:10.4 | 6.04 | 46.59 | C | N ( * ) | 1.73″ × 0.89″ |
| PSO J183.1124+05.0926(2, 6) | 12:12:26.98 | +05:05:33.5 | 6.4039 | 46.73 | C | Y | 1.25″ × 1.05″ |
| SDSS J1306+0356(2, 6, 7) | 13:06:08.26 | +03:56:26.3 | 6.016 | 46.66 | C | Y | 1.11″ × 0.90″ |
| ULAS J1319+0950(2, 6, 12) | 13:19:11.29 | +09:50:51.4 | 6.133 | 46.74 | B | Y | 1.20″ × 1.04″ |
| PSO J217.0891−16.0453(2, 6) | 14:28:21.39 | −16:02:43.3 | 6.11 | 46.70 | C | N ( * ) | 1.17″ × 0.86″ |
| CFHQS J1509−1749(2, 6, 17) | 15:09:41.78 | −17:49:26.8 | 6.121 | 46.78 | C | Y | 1.36″ × 0.87″ |
| PSO J231.6576−20.83335(5, 6, 11) | 15:26:37.84 | −20:50:00.7 | 6.586 | 46.80 | C | Y | 1.21″ × 0.88″ |
| PSO J308.0416−21.2339(2, 5, 6) | 20:32:09.99 | −21:14:02.3 | 6.23 | 46.49 | C | Y | 0.85″ × 0.65″ |
| SDSS J2054−0005(2, 3) | 20:54:06.49 | −00:05:06.49 | 6.0391 | 46.44 | B | Y | 0.69″ × 0.67″ |
| CFHQS J2100−1715(2, 5, 6, 18) | 21:00:54.62 | −17:15:22.5 | 6.087 | 46.20 | C | Y | 0.73″ × 0.63″ |
| VIK J2211−3206(6, 15) | 22:11:12.39 | −32:06:12.9 | 6.336 | 46.62 | C | Y | 0.84″ × 0.67″ |
| VIMOS2911001793(6, 19) | 22:19:17.22 | +01:02:48.90 | 6.16 | 45.12 | A | Y | 0.77″ × 0.68″ |
| PSO J340.2041−18.6621(2, 6) | 22:40:49.00 | −18:39:43.8 | 6.01 | 46.51 | C | N | 0.78″ × 0.68″ |
| SDSS J2310+1855(2, 3, 9) | 23:10:38.88 | +18:55:19.7 | 6.0031 | 47.02 | B | Y | 1.10″ × 0.73″ |
| VIK J2318−3113(15) | 23:18:18.35 | −31:13:46.4 | 6.444 | 46.40 | C | Y | 0.82″ × 0.78″ |
| VIK J2318−3029(15) | 23:18:33.10 | −30:29:33.4 | 6.12 | 46.44 | C | Y | 0.91″ × 0.74″ |
| PSO J359.1352−063831(2, 6) | 23:56:32.00 | −06:22:59.0 | 6.15 | 46.65 | C | Y | 1.06″ × 0.62″ |
Notes.
The identification (ID) of the source, with the associated numbers corresponding to the references of the source (including Bischetti et al. 2019; Decarli et al. 2018; Willott et al. 2017, in which the ALMA data have been published).
The bolometric AGN luminosity estimated from the 1450 Å absolute magnitudes found in the literature.
The ProjectID of the ALMA project the source was observed in, where A = 2015.1.00606.S, B = 2015.1.00997.S, C = 2015.1.01115.S.
The original beamsize of the natural weighted images, before re-imaging to a 0.8″ × 0.8″ beamsize.
( * )These sources are not detected in our analysis; however if only the central pixel of the source is taken the [C II] line is detected in agreement with Decarli et al. (2018).
References.(1) Bañados et al. (2014); (2) Bañados et al. (2016); (3) Bischetti et al. (2019); (4) Carnall et al. (2015); (5) Decarli et al. (2017); (6) Decarli et al. (2018); (7) Fan et al. (2001); (8) Jiang et al. (2015); (9) Jiang et al. (2016); (10) Matsuoka et al. (2016); (11) Mazzucchelli et al. (2017); (12) Mortlock et al. (2009); (13) Reed et al. (2015); (14) Venemans et al. (2015); (15) Venemans et al. (in prep.); (16) Wang et al. (2013); (17) Willott et al. (2007); (18) Willott et al. (2010); (19) Willott et al. (2017).
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