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Table 1
Characteristics of the FIR/submm data used in this study.
| Data | λref | νref | θ | σII | σabs |
| [μm] | [GHz] | [arcmin] | [MJysr-1] | [%] | |
|
|
|||||
| IRAS | 100 | 2997.92 | 4.30 | 0.06 | 13.6 †‡ |
| HFI | 349.82 | 857 | 3.67 | 0.12♭ | 7% |
| HFI | 550.08 | 545 | 3.80 | 0.12♭ | 7% |
| HFI | 849.27 | 353 | 4.43 | 0.08♭ | ≲2% |
| HFI | 1381.5 | 217 | 4.68 | 0.08♭ | ≲2% |
| HFI | 2096.4 | 143 | 7.04 | 0.08♭ | ≲2% |
| HFI | 2997.9 | 100 | 9.37 | 0.07♭ | ≲2% |
| LFI | 4285.7 | 70.3 | 13.01 | – | 5.0 |
| LFI | 6818.2 | 44.1 | 27.92 | – | 5.0 |
| LFI | 10000 | 28.5 | 32.65 | – | 5.0 |
| WMAP | 3200 | 93.69 | 13.2 | 1.76♯ | 1.0 |
| WMAP | 4900 | 61.18 | 21.0 | 0.36♯ | 1.0 |
| WMAP | 7300 | 41.07 | 30.6 | 0.11♯ | 1.0 |
| WMAP | 9100 | 32.94 | 39.6 | 0.05♯ | 1.0 |
| WMAP | 13000 | 23.06 | 52.8 | 0.02♯ | 1.0 |
Notes.
(†)
Assumed to be for the average IRAS coverage. σII computed by rescaling this value to actual coverage.
(♭)
1σ average value in one beam scaled from Planck HFI Core Team (2011b). We actually use the internal variance maps for σII.
(♯)
From Bennett et al. (2003).
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