Table A.1.
Colour corrections 𝒞 (Eq. (A.2)) for dusty star-forming galaxies are given for two different CIB spectral energy distributions (“model” refers to the model of Béthermin et al. (2012a), while “measure” refers to the Gispert et al. (2000) fit of FIRAS measurements).
| Experiment | Frequency | 𝒞model | 𝒞measure |
|---|---|---|---|
| [GHz] | |||
| 100 | 1.0759 | 1.0824 | |
| 143 | 1.0171 | 1.0124 | |
| Planck/HFI | 217 | 1.1190 | 1.1076 |
| 353 | 1.0973 | 1.0941 | |
| 545 | 1.0677 | 1.0675 | |
| 857 | 0.9948 | 0.9939 | |
| IRAS | 3000 | 0.9605 | 0.9446 |
| 148 | 1.0720 | 1.0719 | |
| ACT | 218 | 1.0422 | 1.0384 |
| 277 | 1.0227 | 1.0217 | |
| 150 | 1.1411 | 1.1350 | |
| SPT | 220 | 1.0059 | 1.0046 |
| 95 | 1.1386 | 1.1525 | |
| 1200 | 0.9880 | 0.9808 | |
| Herschel/SPIRE | 857 | 0.9887 | 0.9875 |
| (extended RSRF) | 600 | 0.9739 | 0.9763 |
| 1200 | 1.0053 | 0.9945 | |
| Herschel/SPIRE | 857 | 1.0193 | 1.0187 |
| (point-source RSRF) | 600 | 1.0469 | 1.0503 |
Notes. For SPIRE, we give the colour corrections for the two spectral responses (extended or point-source RSRF).
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