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Table 1.

32 QSOs revealed with emission line detection significant at ≳3σ and related information about the ALMA observing project.

No. Object ID RA (J2000) Dec (J2000) zcat(a) Observed line Flags [rot, β, MBH] (b)
1 CXOCDFS J0332−2746 2.2234 CO(4–3) r, u, –
2 VHS J2101−5943 −59°43′45″ 2.313 CO(3–2) r, b, a
3 ULAS J1234+0907 2.503 CO(3–2) u, –, –
4 ULAS J2315+0143 2.560 CO(3–2) r, u, –
5 ULAS J0123+1525 2.629 CO(3–2) u, –, –
6 SDSS J1328−0224 4.62271 [CII] r, c, e
7 SDSS J0923+0247 4.66307 [CII] r, c, e
8 SDSS J0331−0741 4.72426 [CII] r, u, –
9 SDSS J0129−0035 −00°35′39″ 5.780 [CII] r, l, a
10 SDSS J1044−0125 5.800 [CII] r, c, a
11 SDSS J1306+0356 6.016 [CII] r, c, e
12 SDSS J2310+1855 6.040 [CII] r, c, e
13 SDSS J0842+1218 6.055 [CII] u, –, –
14 SDSS J2054−0005 6.062 [CII] r, c, a
15 [WMH2013] 05 6.068 [CII] u, –, –
16 CFHQS J2100−1715 6.09 [CII] u, –, –
17 DES J0454−4448 6.100 [CII] u, –, –
18 CFHQS J1509−1749 −17°49′27″ 6.120 [CII] u, –, –
19 ULAS J1319+0950 6.130 [CII] r, l, e
20 PSO J065−26 6.14 [CII] u, –, –
21 [CLM2003] J0228−04161 6.17 [CII] u, –, –
22 PSO J308−21 6.2342 [CII] r, b, u
23 VIKING J1152+0055 6.37 [CII] u, –, –
24 PSO J159−02 6.38 [CII] u, –, –
25 PSO J183+05 6.4386 [CII] r, l, u
26 PSO J167−13 6.508 [CII] r, c, e
27 PSO J231−20 6.58651 [CII] r, u, –
28 VIKING J0305−3150 6.605 [CII] r, c, e
29 VIKING J1048−0109 6.661 [CII] u, –, –
30 VIKING J0109−3047 6.750 [CII] r, u, –
31 VIKING J2348−3054 6.890 [CII] u, –, –
32 ULAS J1120+0641 7.080 [CII] u, –, –
No. (c) ALMA ID P.I. (d) σline(e) θbeam(f) Ref. No. (c) ALMA ID P.I. (d) σline(e) θbeam(f) Ref.
(mJy beam−1) (″) (mJy beam−1) (″)
1 2015.1.00228.S GP 0.60 1.66 P17 17 2015.1.01115.S FW 1.25 1.24 V18
2 2015.1.01247.S MB 0.68 5.39 B17 18 2015.1.01115.S FW 1.10 1.04 D18
3 2015.1.01247.S MB 1.20 2.65 B17 19 2012.1.00240.S RW 0.62 0.22 J17
4 2015.1.01247.S MB 0.73 2.22 B17 20 2015.1.01115.S FW 1.28 0.82 D18
5 2015.1.01247.S MB 0.74 2.58 B17 21 2013.1.00815.S CW 0.60 0.39 W15
6 2013.1.01153.S PL 0.71 0.44 T17 22 2016.A.00018.S RD 0.54 0.27 D17
7 2013.1.01153.S PL 0.69 0.45 T17 23 2015.1.01115.S FW 1.21 0.92 D18
8 2013.1.01153.S PL 1.60 0.34 T17 24 2015.1.01115.S FW 1.20 0.89 D18
9 2012.1.00240.S RW 0.66 0.17 – 25 2016.1.00544.S EB 0.64 0.25 –
10 2011.0.00206.S RW 1.84 0.48 W13 26 2015.1.00606.S CW 0.58 0.63 W17
11 2015.1.01115.S FW 1.35 0.83 D18 27 2015.1.01115.S FW 1.37 0.97 D17
12 2011.0.00206.S RW 1.39 0.57 W13 28 2015.1.00399.S BV 0.51 0.19 –
13 2015.1.01115.S FW 1.35 0.93 D17 29 2015.1.01115.S FW 1.01 0.98 D18
14 2011.0.00206.S RW 1.81 0.45 W13 30 2012.1.00882.S BV 1.45 0.36 V16
15 2013.1.00815.S CW 0.58 0.37 W15 31 2012.1.00882.S BV 1.88 0.42 V16
16 2015.1.01115.S FW 1.30 0.62 D17 32 2012.1.00882.S BV 0.67 0.20 V17

Notes.

(a)

Top part: redshift values retrieved from SIMBAD Astronomical Database (http://simbad.u-strasbg.fr/simbad/).

(b)

The flags provide information on kinematics (rot), disc inclination angle (β) as resulting from our kinematical modelling, and black hole mass (MBH) as follows: [rot]: unresolved (u) or resolved (r) kinematics. [β]: unconstrained (u) or constrained (c) disc inclination angle, lower limit (l), bimodal distribution (b). [MBH]: unavailable in the literature (u), single-epoch virial mass estimated in this work (e) or value retrieved the literature (a).

(c)

Bottom part: identification numbers (No.) refer to those of the top table.

(d)

Principal investigator of the project: BV (Venemans, B.), CW (Willott, C.), EB (Bañados, E.), FW (Walter, F.), GP (Popping, G.), MB (Banerji, M.), PL (Lira, P.), RD (Decarli, R.), RW (Wang, R.).

(e)

Line sensitivity over 10 km s−1.

(f)

Angular resolution.

References. B17: Banerji et al. (2017), D17, D18: Decarli et al. (2017, 2018), J17: Jones et al. (2017) P17: Popping et al. (2017), T17: Trakhtenbrot et al. (2017), V16, V17, V18: Venemans et al. (2016, 2017a; 2018), W13: Wang et al. (2013), W15, W17: Willott et al. (2015b, 2017).

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