Table A.2
Photometric measurements of AS 205.
| AS 205 N | AS 205 S | ||
| Wavelength | Flux | Flux | Refs. |
| (μm) | (Jy) | (Jy) | |
|
|
|||
| 0.36 | 0.0060 ± 0.0033 | 1 | |
| 0.44 | 0.014 ± 0.001 | 1 | |
| 0.55 | 0.029 ± 0.001 | 1 | |
| 0.55 | 0.044/0.0069 | 2 | |
| 0.64 | 0.12 ± 0.01 | 1 | |
| 0.79 | 0.19 ± 0.01 | 1 | |
| 1.25 | 0.55 ± 0.07 | – | 1 |
| 1.65 | 1.1 ± 0.07 | – | 1 |
| 2.2 | 1.80 ± 0.14 | – | 1 |
| 1.25 | 0.86 ± 0.05 | 0.32 ± 0.05 | 3 |
| 1.65 | 1.40 ± 0.08 | 0.66 ± 0.08 | 3 |
| 2.2 | 2.80 ± 0.08 | 1.11 ± 0.15 | 3 |
| 3.5 | 3.10 ± 0.30 | 1.34 ± 0.13 | 3 |
| 25 | 14 ± 2 | 4 | |
| 60 | 19 ± 2 | 4 | |
| 60 | 20 ± 1 | 5 | |
| 90 | 13 ± 1 | 5 | |
| 100 | 16 ± 3.2 | 4 | |
| 170 | 9.1 ± 1.6 | 5 | |
| 350 | 3.5 ± 0.5 | 6 | |
| 450 | 2.5 ± 0.2 | 6 | |
| 800 | 1.00 ± 0.04 | 6 | |
| 859 | ~0.9 ± 0.006 | ~0.060 ± 0.001 | 7 |
| 1100 | 0.50 ± 0.02 | 6 | |
Notes.The two components could only be spatially resolved in the NIR and MIR range. Cohen & Kuhi (1979) were able to spatially resolve both components, but they missed declaring which flux belongs to which component. The southern system is a binary system, as well.
Reference. Eisner et al. (2005); 2) Cohen & Kuhi (1979); 3) Prato et al. (2003); 4) IRAS catalogue (1985); 5) ISO data archive; 6) Jensen et al. (1996); 7) Andrews et al. (2011).
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