Table B.1.
SED fits with all wavelength combinations.
| Band (μm) | (160–500) | (250–500) | (250–850) | (160–850) | (160–500) | (250–500) | (250–850) | (160–850) |
|---|---|---|---|---|---|---|---|---|
| Clump | ⟨T⟩ | ⟨N(H2)⟩ | ||||||
| type | (K) | (1021cm−2) | ||||||
| All | 15.5 ± 5.3 | 16.1 ± 6.3 | 14.3 ± 6.4 | 14.9 ± 5.3 | 18.3 ± 56.8 | 15.4 ± 31.4 | 21.5 ± 30.3 | 20.5 ± 57.4 |
| PS-C | 15.9 ± 1.3 | 16.2 ± 0.3 | 12.7 ± 0.2 | 14.2 ± 0.6 | 6.3 ± 2.4 | 8.2 ± 5.4 | 19.4 ± 13.1 | 10.2 ± 5.1 |
| PS | 14.8 ± 3.6 | 17.1 ± 7.1 | 16.0 ± 7.7 | 13.8 ± 3.9 | 7.4 ± 3.0 | 6.8 ± 4.3 | 16.5 ± 24.7 | 16.2 ± 15.7 |
| PRE | 16.1 ± 5.5 | 16.5 ± 6.4 | 15.1 ± 6.7 | 15.6 ± 5.5 | 20.9 ± 66.0 | 17.0 ± 36.1 | 22.2 ± 33.7 | 20.7 ± 62.7 |
| SL | 14.0 ± 4.8 | 14.6 ± 5.7 | 11.9 ± 4.4 | 12.8 ± 4.5 | 12.6 ± 18.4 | 12.4 ± 14.4 | 20.3 ± 18.5 | 20.9 ± 42.7 |
| SL PRE | 15.6 ± 5.4 | 16.0 ± 6.3 | 14.3 ± 6.3 | 14.9 ± 5.4 | 18.7 ± 57.6 | 15.9 ± 32.2 | 21.8 ± 30.6 | 20.7 ± 58.3 |
| PS PS-C | 15.1 ± 3.2 | 17.0 ± 6.6 | 15.6 ± 7.3 | 13.9 ± 3.3 | 7.1 ± 2.9 | 7.0 ± 4.5 | 16.9 ± 23.6 | 14.5 ± 13.8 |
| Band (μm) | (160–500) | (250–500) | (250–850) | (160–850) | (160–500) | (250–500) | (250–850) | (160–850) |
| Clump | ⟨M⟩ | β | ||||||
| type | (M⊙) | |||||||
| All | 154 ± 276 | 137 ± 258 | 149 ± 262 | 139 ± 249 | 1.88 ± 0.66 | 1.86 ± 0.63 | 2.2 ± 0.66 | 2.03 ± 0.62 |
| PS-C | 10 ± 2 | 10 ± 3 | 16 ± 5 | 12 ± 3 | 1.44 ± 0.07 | 1.45 ± 0.09 | 2.03 ± 0.17 | 1.77 ± 0.03 |
| PS | 14 ± 9 | 31 ± 40 | 34 ± 38 | 45 ± 68 | 1.5 ± 0.47 | 1.74 ± 0.32 | 2.04 ± 0.85 | 1.84 ± 0.55 |
| PRE | 209 ± 309 | 175 ± 287 | 191 ± 290 | 176 ± 275 | 1.95 ± 0.68 | 1.92 ± 0.67 | 2.18 ± 0.68 | 2.03 ± 0.65 |
| SL | 18 ± 29 | 17 ± 31 | 20 ± 31 | 18 ± 30 | 1.73 ± 0.59 | 1.7 ± 0.54 | 2.29 ± 0.52 | 2.07 ± 0.54 |
| SL PRE | 159 ± 279 | 143 ± 264 | 156 ± 268 | 144 ± 254 | 1.89 ± 0.66 | 1.87 ± 0.64 | 2.21 ± 0.65 | 2.04 ± 0.62 |
| PS PS-C | 13 ± 8 | 29 ± 38 | 31 ± 36 | 41 ± 65 | 1.49 ± 0.40 | 1.7 ± 0.31 | 2.04 ± 0.79 | 1.82 ± 0.47 |
Notes. Results of the MBB fit to different wavelength ranges, with opacity spectral index as a free parameter. Temperature and column density are the average value over the clump footprint. To ensure consistency between SPIRE, PACS, and SCUBA-2 data, the background has been subtracted from all fields. The errors are the standard deviation of the distribution. This table includes only those fields for which distances (to calculate mass) are available.
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