Table 5.
Infrared luminosities, dust masses, dust temperatures, and spectral emissivity indices.
| Source | μLL(MBB) (1012 L⊙) | μLL(DL07) (1012 L⊙) | μLMdust(MBB) | Tdust(MBB) | μLMdust(DL07) | β |
|---|---|---|---|---|---|---|
| 50−1000 μm | 8−1000 μm | (1010 M⊙) | (K) | (1010 M⊙) | ||
| HerBS-34 | 24.8 ± 0.6 | 40.6 ± 2.4 | 1.00 ± 0.07 | 33.0 ± 1.2 | 1.16 ± 0.07 | 1.87 ± 0.08 |
| HerBS-43a | 19.8 ± 0.8 | 33.4 ± 4.1 | 0.53 ± 0.05 | 34.6 ± 1.7 | 0.69 ± 0.04 | 1.91 ± 0.11 |
| HerBS-43b | 10.0 ± 1.3 | 15.0 ± 2.0 | 0.58 ± 0.12 | 29.1 ± 5.1 | 0.45 ± 0.04 | 2.21 ± 0.39 |
| HerBS-44 | 33.1 ± 0.7 | 108.1 ± 7.8 | 0.49 ± 0.05 | 34.8 ± 1.4 | 0.70 ± 0.04 | 2.26 ± 0.11 |
| HerBS-54 | 14.9 ± 0.6 | 23.6 ± 1.6 | 1.33 ± 0.16 | 26.7 ± 1.6 | 1.25 ± 0.12 | 2.15 ± 0.16 |
| HerBS-58 | 10.4 ± 0.4 | 17.7 ± 1.3 | 0.98 ± 0.09 | 24.1 ± 1.3 | 0.83 ± 0.06 | 2.36 ± 0.15 |
| HerBS-70E | 12.6 ± 0.6 | 40.5 ± 5.2 | 0.42 ± 0.04 | 26.3 ± 1.5 | 0.37 ± 0.02 | 2.62 ± 0.14 |
| HerBS-70W | 3.0 ± 0.5 | 8.7 ± 4.2 | 0.10 ± 0.04 | 31.5 ± 9.9 | 0.09 ± 0.02 | 2.43 ± 0.53 |
| HerBS-79 | 10.5 ± 0.4 | 18.1 ± 1.2 | 0.81 ± 0.14 | 24.0 ± 1.5 | 0.83 ± 0.18 | 2.52 ± 0.19 |
| HerBS-89a | 19.3 ± 0.8 | 29.0 ± 1.5 | 1.40 ± 0.09 | 27.6 ± 1.4 | 1.35 ± 0.06 | 2.08 ± 0.11 |
| HerBS-95E | 7.8 ± 0.7 | 11.4 ± 1.9 | 0.53 ± 0.07 | 27.2 ± 3.6 | 0.50 ± 0.05 | 2.22 ± 0.33 |
| HerBS-95W | 10.9 ± 0.8 | 16.1 ± 1.8 | 1.00 ± 0.09 | 24.2 ± 2.1 | 0.77 ± 0.04 | 2.46 ± 0.24 |
| HerBS-113 | 18.9 ± 0.8 | 29.6 ± 2.8 | 0.57 ± 0.07 | 31.8 ± 1.9 | 0.72 ± 0.06 | 2.11 ± 0.15 |
| HerBS-154 | 25.7 ± 1.1 | 81.3 ± 7.3 | 0.38 ± 0.03 | 38.2 ± 2.3 | 0.46 ± 0.03 | 2.10 ± 0.14 |
| HerBS-173 | 10.9 ± 0.5 | 18.5 ± 1.4 | 0.62 ± 0.11 | 25.8 ± 1.5 | 0.51 ± 0.04 | 2.44 ± 0.15 |
| HerBS-204 | 9.9 ± 0.4 | 16.4 ± 1.0 | 0.85 ± 0.15 | 21.6 ± 0.9 | 0.45 ± 0.04 | 2.96 ± 0.09 |
Notes. The infrared luminosities and dust masses are not corrected for amplification (μL is the magnification factor). Regarding the sources that are double, appropriate corrections were applied to estimate the flux densities of each source at 250, 350, and 500 μm (see text for details). For the sources HerBS-204 and HerBS-173, we used the stacked continuum data (see Sect. 3.1). In the case of HerBS-204, we adopt a redshift zspec = 2.37, as the higher value (zspec = 3.49) yields a dust temperature of 40 K, which is slightly higher than the values derived for the other sources in this sample (see Sect. 3.1). The MBB luminosities, dust masses, and temperatures include the effects of the CMB (see Sect. 4.2). The quoted errors on the SED-fitting derived quantities are 1σ.
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