Table 2
Far-infrared continuum fluxes measured by various satellite missions and the CBI interferometer.
| Instr | λ | K4E/ | K color | Flux | Error | Fit |
| μm | K 4P | Jy | Jy | Jy | ||
|
|
||||||
| IRAS | 60 | 1.0000 | 0.9457 | 162.3 | 52.9 | 92.6 |
| IRAS | 100 | 1.0000 | 0.9650 | 312.8 | 87.0 | 271.9 |
| PACS | 70 | 1.0000 | 0.9961 | 143.6 | 19.9 | 151.8 |
| PACS | 160 | 1.0000 | 0.9996 | 302.0 | 75.3 | 251.2 |
| SPIRE | 250 | 0.9828 | 0.9978 | 126.7 | 12.9 | 135.6 |
| SPIRE | 350 | 0.9843 | 0.9991 | 69.4 | 7.2 | 69.6 |
| SPIRE | 500 | 0.9710 | 0.9788 | 30.6 | 3.2 | 30.8 |
| Planck | 350 | 1.0000 | 1.0190 | 72.0 | 7.6 | 69.6 |
| Planck | 550 | 1.0000 | 1.0881 | 24.5 | 2.7 | 24.5 |
| Planck | 849 | 1.0000 | 1.0983 | 8.83 | 1.00 | 8.42 |
| Planck | 1382 | 1.0000 | 1.1016 | 3.27 | 0.46 | 2.81 |
| Planck | 2096 | 1.0000 | 1.0077 | 1.15 | 0.23 | 1.46 |
| Planck | 2998 | 1.0000 | 1.0695 | 0.93 | 0.17 | 1.10 |
| CBI | 9671 | 1.0000 | 1.0000 | 1.10 | 0.11 | 1.00 |
Notes. The second column gives the wavelength, the third the quoted flux, the fourth column the conversion factors from point source calibration to extended source calibration for the SPIRE data, the fifth column the color correction factor, the sixth column the actual flux with all corrections applied, the seventh column the estimated error on this flux, and the eighth column the flux value from the blackbody fit.
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