Table A.1
Photometric data of the Spitzer/MIPS 24 µm and Herschel/PACS (70 µm and 160 µm) and SPIRE (250 µm, 350 µm, and 500 µm) counterparts of the clumps in G1.75-0.08 and G11.36+0.80.
| Source | S24 [mJy] | S70 [Jy] | S160 [Jy] | S250 [Jy] | S350 [Jy] | S500 [Jy] |
|---|---|---|---|---|---|---|
| G1.75-0.08 | ||||||
| Clump A | … | … | 17.77 ± 1.09 | 80.71 ± 2.16 | 64.36 ± 2.67 | 38.96 ± 4.40 |
| Clump B | … | … | …a | 60.41 ± 1.40 | 51.52 ± 2.15 | 29.15 ± 2.11 |
| G11.36+0.80 | ||||||
| Clump A | … | 0.38 ± 0.02 | 2.15 ± 0.18 | 14.04 ± 0.43 | 16.69 ± 0.79 | 25.80 ± 1.38 |
| Clump B | … | 0.22 ± 0.03 | 1.26 ± 0.19 | 26.39 ± 2.15 | 16.01 ± 0.57 | 23.04 ± 0.79 |
| Clump C | 246.61 ± 4.64 | 6.44 ± 0.09 | 17.51 ± 0.31 | 28.29 ± 0.64 | 26.95 ± 0.71 | 28.81 ± 1.56 |
| Clump D | 78.63 ± 1.79 | 4.51 ± 0.08 | 16.43 ± 0.26 | 13.77 ± 0.39 | 17.85 ± 0.74 | 10.13 ± 1.74 |
Notes. The flux densities were taken from the MIPSGAL and Hi-GAL catalogues unless otherwise stated. (a)No counterpart was found from the Hi-GAL catalogue. If the 160 µm flux density is determined from the PACS image within an aperture that corresponds to the 3σ level of the LABOCA emission, the value is S160 = 56.1 ± 3.5 Jy.
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