Table 4.
CMB impact on observables.
| ID | LIR |
 |
 |
 |
 |
 |
 |
 |
 |
 |
λeff |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [1012 L⊙] | [K] | [K] | [K] | [108 M⊙] | [108 M⊙] | [108 M⊙] | [μm] | ||||
| (Cold) | |||||||||||
| 3117 | 6.24 ± 2.62 | 2.5 ± 0.2 | 2.3 ± 0.2 | 2.2 ± 0.2 | 25 ± 4 | 26 ± 4 | 30 ± 9 | 20.0 ± 4.0 | 26.5 ± 7.8 | 21.2 ± 9.1 | 100 ± 23 |
| 5340 | 5.85 ± 0.81 | 2.7 ± 0.2 | 2.4 ± 0.1 | 2.2 ± 0.2 | 25 ± 1 | 26 ± 1 | 41 ± 10 | 12.2 ± 1.1 | 17.9 ± 2.3 | 8.0 ± 3.7 | 150 ± 30 |
| 6309 | 4.82 ± 0.84 | 2.6 ± 0.2 | 2.3 ± 0.2 | 2.3 ± 0.3 | 24 ± 2 | 25 ± 2 | 42 ± 6 | 16.3 ± 1.6 | 23.5 ± 3.5 | 8.7 ± 2.9 | 200 ± 19 |
| 7549 | 4.90 ± 0.87 | 2.6 ± 0.2 | 2.1 ± 0.2 | 2.1 ± 0.2 | 22 ± 2 | 24 ± 3 | 36 ± 7 | 38.2 ± 4.3 | 61.6 ± 1.6 | 25.7 ± 5.8 | 200 ± 23 |
| 12646 | 3.50 ± 0.61 | 2.5 ± 0.2 | 2.2 ± 0.2 | 2.2 ± 0.2 | 26 ± 2 | 27 ± 2 | 43 ± 9 | 8.8 ± 0.9 | 12.9 ± 1.8 | 6.1 ± 2.5 | 175 ± 24 |
| (Warm) | |||||||||||
| 9316 | 10.01 ± 2.48 | 1.8 ± 0.1 | 1.6 ± 0.1 | 1.6 ± 0.2 | 36 ± 3 | 37 ± 3 | 46 ± 8 | 19.0 ± 2.2 | 23.1 ± 3.4 | 16.5 ± 4.4 | 100 ± 28 |
Notes. LIR: IR luminosity at 8–1000 μm rest-frame corrected for CMB effect; 
, 
and 
: Rayleigh-Jeans slope, dust temperature, and dust mass from optically thin MBB fits without accounting for CMB; 
, 
, and 
: Rayleigh-Jeans slope, dust temperature, and dust mass from optically thin MBB fits accounting for CMB effect; 
, 
, and 
: Rayleigh-Jeans slope, dust temperature, and dust mass from optically thick MBB fits accounting for CMB effect; λeff: effective wavelength of optical depth τ = 1.
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