Table 1.
Physical properties of the stacked quiescent samples.
| Redshift | N | log(M*) | SFR(UV) ( † ) | log(LIR) | Td | ⟨U⟩ | log(Mdust) |
 |
 |
|---|---|---|---|---|---|---|---|---|---|
| [M⊙] | [M⊙ yr−1] | [L⊙] | [K] | [M⊙] | [M⊙] | [%] | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| 0.30 < z < 0.65 | 563 | 11.17 ± 0.15 |
 |
9.40 ± 0.05 | 20.0 ± 4.0 | 0.6 ± 0.3 |
 |
 |
2.0 ± 1.0 |
| 0.65 < z < 1.00 | 1536 | 11.20 ± 0.17 |
 |
9.89 ± 0.05 | 19.0 ± 4.0 | 0.6 ± 0.3 |
 |
 |
5.9 ± 3.0 |
| 1.00 < z < 1.40 | 1394 | 11.16 ± 0.15 |
 |
10.20 ± 0.05 | 22.0 ± 3.0 | 1.1 ± 0.4 |
 |
 |
7.3 ± 3.0 |
| 1.50 < z < 2.20 ( ‡ ) | 997 | 11.04 ± 0.15 |
 |
10.35 ± 0.13 | 23.5 ± 2.0 | 1.8 ± 1.2 |
 |
 |
8.4 ± 3.0 |
Notes. Column 1: Redshift bin. Column 2: Number of objects in the redshift bin. Column 3: mean stellar mass. Column 4: mean SFR(UV). Column 5: total infrared luminosity from the SED fitting with Draine & Li (2007) models integrated over 8 − 1000 μm. Column 6: ‘luminosity-weighted’ Td from the SED modelling with a single-temperature modified black body. Column 7: mean intensity of the radiation field from Draine & Li (2007) models. Column 8: dust mass. Column 9: molecular gas fraction assuming a solar gas-to-dust conversion factor of GDR = 92. All quantities are computed using a Salpeter (1955) IMF. ( † )Mean and interquartile range. ( ‡ )Stacked photometry from Gobat et al. (2018) that for consistency was re-fitted here with the same method and setup as for the rest of the redshift bins.
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