Table 1.
Sample of quasars studied in this work.
| Full name | Target | RA | Dec | z | Fcont (1 mm) | LIR | L[CII] | Ref |
|---|---|---|---|---|---|---|---|---|
| (J2000.0) | (J2000.0) | [mJy] | [1012 L⊙] | [109 L⊙] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| PSO J036.5078+03.0498 | PJ036+03 | 02:26:01.876 | +03:02:59.39 | 6.5412 | 2.5 ± 0.5 | 6.5 |
 |
3 |
| SDSS J0338+0021 | J0338+0021 | 03:38:29.310 | +00:21:56.30 | 5.0267 | 2.98 ± 0.05 | 12.0 ( † ) |
 |
2 |
| PSO J159.2257–02.5438 | PJ159–02 | 10:36:54.191 | –02:32:37.94 | 6.3809 | 0.65 ± 0.03 | 1.6 |
 |
6 |
| VIK J1048–0109 | J1048–0109 | 10:48:19.086 | –01:09:40.29 | 6.6759 | 2.84 ± 0.03 | 7.7 |
 |
6 |
| DELS J1104+2134 | J1104+2134 | 11:04:21.580 | +21:34:28.85 | 6.7662 | 1.8 ± 0.05 | 5.0 |
 |
7 |
| ULAS J1319+0950 | J1319+0950 | 13:19:11.302 | +09:50:51.49 | 6.1331 | 5.23 ± 0.10 | 10.7 ( † ) |
 |
1,2 |
| SDSS J2054–0005 | J2054–0005 | 20:54:06.481 | –00:05:14.80 | 6.0391 | 2.98 ± 0.05 | 8.0 ( † ) |
 |
1,2 |
| VIMOS2911001793 | J2219+0102 | 22:19:17.217 | +01:02:48.90 | 6.1492 | 0.766 ± 0.047 | 1.8 |
 |
5 |
| PSO J338.2298+29.5089 | PJ338+29 | 22:32:55.150 | +29:30:32.23 | 6.6660 | 0.972 ± 0.215 | 2.6 |
 |
4 |
| PSO J359.1352–06.3831 | PJ359–06 | 23:56:32.455 | –06:22:59.26 | 6.1722 | 0.87 ± 0.08 | 2.1 |
 |
6 |
Notes. (1) Full quasar name. (2) Abbreviated target name. (3–4) Target coordinates. (5) Redshift. (6) Continuum flux density at the observed frequency of the [C II] line. (7) Total infrared luminosity, LIR, integrated between 8–1000 μm (rest frame), computed as described in Sect. 3.1. (8) [C II] luminosities. (9) References for [C II] and IR measurements. ( † )IR luminosity based on SED fits from the literature.
References. 1: Wang et al. (2013), 2: Leipski et al. (2014), 3: Bañados et al. (2015), 4: Mazzucchelli et al. (2017), 5: Willott et al. (2017), 6: Decarli et al. (2018), 7: Wang et al. (in prep).
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