Table 5
DGL and optical-IR-submm sky-subtracted intensities for B207.
| Wavelength | Core | Rim | DGL | fDGL |
| λ (μm) | MJy/sr | MJy/sr | MJy/sr | MJy/sr |
|
|
||||
| 0.43 | -5.43E-5 | 4.02E-3 | 9.14E-3 | 3.44E-3 |
| 0.54 | 2.44E-3 | 1.55E-2 | 1.47E-2 | 4.17E-3 |
| 0.63 | 7.89E-3 | 3.05E-2 | 1.90E-2 | 4.11E-3 |
| 0.81 | 2.74E-2 | 6.82E-2 | 1.97E-2 | 2.00E-3 |
| 1.25 | 9.06E-2 | 1.14E-1 | 1.27E-2 | 9.76E-4 |
| 1.65 | 9.90E-2 | 1.62E-1 | 7.22E-3 | 3.38E-4 |
| 2.17 | 6.66E-2 | 1.10E-1 | 3.71E-3 | 1.37E-4 |
| 3.36 | 6.64E-2 | 2.61E-2 | 7.89E-4 | 1.79E-5 |
| 4.62 | 1.02E-1 | 2.24E-2 | 1.77E-4 | 3.16E-6 |
| 100 | 9.02E+0 | 9.53E+0 | – | – |
| 160 | 6.94E+1 | 3.75E+1 | – | – |
| 250 | 1.55E+2 | 5.80E+1 | – | – |
| 350 | 1.45E+2 | 4.14E+1 | – | – |
| 500 | 8.20E+1 | 1.99E+1 | – | – |
Notes. (1) The uncertainties in the observed intensities and the DGL are about 10% and 25%, respectively. However, for H (1.65 μm) and Ks (2.17 μm) bands the uncertainties are higher than the observed sky subtracted intensities. (2) The centre of the core region is RA = 4h4m47.539s, Dec = + 26°18′51.66″. (3) The centre of the rim region is RA = 4h5m00.00s, Dec = + 26°19′00.00″. (4) The intensities are measured using the optical, NIR, MIR, and FIR wavelengths from DCT, 2MASS, WISE, and Herschel PACS and SPIRE images.
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