Table 2
Photometric data of the analysed sources.
| Source | S22 | S25 | S60 | S70 | S100 | S160 | S350 | S870 |
|---|---|---|---|---|---|---|---|---|
| [Jy] | [Jy] | [Jy] | [Jy] | [Jy] | [Jy] | [Jy] | [Jy] | |
| SMM 1a | … | … | … | … | 2.59 ± 0.11 | 8.04 ± 0.87 | 4.04 ± 1.24 | 0.75 ± 0.09 |
| SMM 1b |  |
… | … | 0.95 ± 0.05 | 1.60 ± 0.15 | … | 4.15 ± 1.28 | 0.78 ± 0.09 |
| SMM 2 | 0.35 ± 0.01 | … | … | 1.10 ± 0.05 | 1.65 ± 0.06 | 3.73 ± 0.87 | 2.18 ± 0.69 | 0.63 ± 0.06 |
| SMM 3 |  |
… | … | … | 4.62 ± 0.39 | 10.72 ± 2.38 | 3.58 ± 1.11 | 0.82 ± 0.11 |
| SMM 4a | 0.03 ± 0.01 | … | … | … | 3.32 ± 1.28 | … | 4.98 ± 1.53 | 0.75 ± 0.09 |
| IRAS 13037 | 3.27 ± 0.05 | 5.23 ± 0.42 | 47.69 ± 7.63 | 24.08 ± 1.02 | 33.51 ± 3.45 | 56.34 ± 8.01 | 3.74 ± 1.15 | 0.77 ± 0.09 |
| –6112a | <144.25 | |||||||
| IRAS 13037 |  |
2.18 ± 0.17 | 17.27 ± 2.76 | 8.72 ± 1.17 | 12.14 ± 1.83 | … | 2.27 ± 0.72 | 0.47 ± 0.05 |
| –6112b | <52.25 | |||||||
| SMM 6a | 0.28 ± 0.01 | … | … | 7.33 ± 0.52 | … | … | 4.97 ± 0.70 | 0.34 ± 0.05 |
| SMM 7 |  |
… | … | 1.19 ± 0.17 | 2.40 ± 0.46 | … | 2.12 ± 0.68 | 0.52 ± 0.07 |
| IRAS 13039 | 3.33 ± 0.05 | 7.43 ± 0.59 | 105.6 ± 14.8 | … | … | … | 5.88 ± 1.80 | 1.17 ± 0.13 |
| –6108a | 196.5 ± 35.4 | |||||||
| SMM 9 | … | … | … | 3.52 ± 0.07 | 7.84 ± 0.19 | 13.10 ± 1.29 | 3.61 ± 1.12 | 0.83 ± 0.10 |
| IRAS 13042 | 0.46 ± 0.01 | 0.67 ± 0.08 | <4.97 | 2.73 ± 0.03 | 4.77 ± 0.13 | 6.58 ± 0.84 | 1.27 ± 0.44 | 0.23 ± 0.05 |
| –6105 | <196.5 |
Notes. The WISE flux densities listed in the second column were computed from the AllWISE catalogue’s Vega magnitudes by applying the colour corrections under the assumption of a Sν ∝ ν−2 power-law spectrum. Moreover, an additional W4 correction was applied to calculate the final 22 μm flux density (see Cutri et al. 2012). For the IRAS sources, the 100 μm flux density could be obtained from both Herschel/PACS and IRAS (given below the PACS value). However, IRAS 13039-6108a could not be found from the PACS Point Source Catalogue, and hence only the IRAS 100 μm flux density is given in the table.
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