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Table 3
Observed flux densities and their corresponding errors.
| Survey | λ | F ν |
| (μm) | (mJy) | |
|
|
||
| GALEX | 0.153 | 1.02 ± 0.48 |
| GALEX | 0.226 | 1.90 ± 0.35 |
| FTS | 0.45 | 40.27 ± 4.3 |
| FTS | 0.55 | 70.22 ± 6.6 |
| FTS | 0.66 | 97.6 ± 8.8 |
| 2MASS | 1.25 | 250.0 ± 16.4 |
| 2MASS | 1.64 | 346.8 ± 19.5 |
| 2MASS | 2.17 | 290.9 ± 14.5 |
| WISE | 3.4 | 127.3 ± 5.4 |
| Spitzer | 3.6 | 156.3 ± 7.6 |
| WISE | 4.6 | 88.2 ± 3.7 |
| WISE | 12 | 218.2 ± 6.8 |
| WISE | 22 | 187.9 ± 7.7 |
| PACS | 100 | 5824 ± 508 |
| PACS | 160 | 9937 ± 654 |
| SPIRE | 250 | 6720 ± 477 |
| SPIRE | 350 | 3511 ± 256 |
| Planck | 350 | 3499 ± 552 |
| SPIRE | 500 | 1419 ± 115 |
| Planck | 550 | 1180 ± 290 |
| Planck | 850 | 313 ± 174 |
Notes. Correction for Galactic extinction (where applicable) has been applied according to Schlafly & Finkbeiner (2011). The masked objects were replaced by the interpolated values using a Gaussian weights kernel.
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