Table A.9.
Spectroscopic redshifts and emission line properties: HerBS sources from Neri et al. (2020).
| Source | Observed Position | zspec | Emission Lines | |||||||
|---|---|---|---|---|---|---|---|---|---|---|
| RA | Dec. | ΔV | Line | Line Flux | Line | Line Flux | Line | Line Flux | ||
| (J2000) | (km s−1) | (Jy km s−1) | (Jy km s−1) | (Jy km s−1) | ||||||
| HerBS-34 | 13:34:13.87 | 26:04:57.5 | 2.6637(2) | 330±10* | CO(3-2) | 2.8±0.4 | CO(5-4) | 8.4±0.8 | ||
| HerBS-43a | 13:24:18.79 | 32:07:54.4 | 3.2121(1) | 1070±90* | CO(4-3) | 5.5±0.8 | CO(5-4) | 6.7±0.8 | ||
| HerBS-43b | 13:24:19.24 | 32:07:49.2 | 4.0543(7) | 800±50* | CO(4-3) | 1.7±0.3 | CO(5-4) | 1.5±0.3 | CO(6-5) | 4.8±0.9 |
| HerBS-44 | 13:32:55.85 | 34:22:08.4 | 2.9268(2) | 520±50* | CO(3-2) | 4.9±0.5 | CO(5-4) | 12.5±1.2 | ||
| HerBS-54 | 13:15:40.72 | 26:23:19.6 | 2.4417(3) | 1020±190 | CO(3-2) | 4.3±0.4 | CO(4-3) | 8.5±0.8 | ||
| HerBS-58 | 13:03:33.17 | 24:46:42.3 | 2.0842(1) | 970±50* | CO(3-2) | 5.3±1.0 | CO(4-3) | 5.2±1.5 | [CI](1-0) | 4.7±0.5 |
| HerBS-70 E | 13:01:40.33 | 29:29:16.2 | 2.3077(4) | 770±50* | CO(3-2) | 1.8±0.5 | CO(4-3) | 3.4±0.3 | [CI](1-0) | 3.5±0.7 |
| HerBS-70 W | 13:01:39.31 | 29:29:25.2 | 2.3115(1) | 140±20 | CO(3-2) | 1.7±0.3 | CO(4-3) | 2.0±0.3 | ||
| HerBS-79 | 13:14:34.08 | 33:52:20.1 | 2.0782(8) | 870±70* | CO(3-2) | 4.1±0.8 | CO(4-3) | 5.5±0.5 | ||
| HerBS-89a | 13:16:11.52 | 28:12:17.7 | 2.9497(1) | 1102±83* | CO(3-2) | 4.00±0.60 | CO(5-4) | 8.40±0.80 | ||
| HerBS-95 E | 13:43:42.73 | 26:39:18.0 | 2.9718(3) | 870±50* | CO(3-2) | 1.0±0.1 | CO(5-4) | 3.6±0.3 | ||
| HerBS-95 W | 13:43:41.55 | 26:39:22.7 | 2.9729(2) | 540±30* | CO(3-2) | 2.4±0.4 | CO(5-4) | 3.5±0.3 | ||
| HerBS-113 | 13:12:11.35 | 32:38:37.8 | 2.7870(8) | 900±200* | CO(3-2) | 6.1±1.2 | CO(5-4) | 13.5±1.4 | ||
| HerBS-154 | 13:22:58.11 | 32:50:51.7 | 3.7070(5) | 310±40 | CO(6-5) | 7.6±0.7 | [CI](1-0) | 1.3±0.4 | H2O (211-202) | 1.5±0.3 |
Notes. The uncertainties in the spectroscopic redshifts, zspec, given in brackets, correspond to the errors derived from Gaussian fits to the line profiles. ΔV values are the mean linewidths (FWHM) weighted by the peak intensities of the detected CO emission lines. Emission lines fitted with double Gaussians are highlighted with an asterisk after the value of ΔV - the reader is referred to Neri et al. (2020) for further details.
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