Table 3.
Median and fitted values for ΔsSFR–M*/SFH diagrams.
| N | ⟨ΔsSFR⟩ | ⟨M*⟩ | Linear regression | N | ⟨ΔsSFR⟩ | ⟨tlast burst⟩ | |
|---|---|---|---|---|---|---|---|
| (intercept, slope) | |||||||
| FRII | 52 | −0.57 (0.475) | 11.20 (0.532) | 51 | −0.57 (0.438) | 9.25 (0.411) | |
| FRI/FRII | 24 | −0.60 (0.564) | 11.09 (0.261) | 22 | −0.54 (0.500) | 9.15 (0.413) | |
| FRI | 29 | −0.58 (0.542) | 11.17 (0.360) | 27 | −0.58 (0.358) | 9.45 (0.377) | |
| FR | 105 | −0.58 (0.516) | 11.17 (0.440) | 1.46, −0.18 | 100 | −0.57 (0.437) | 9.25 (0.410) |
| COM AGN | 1800 | −0.60 (0.488) | 10.90 (0.558) | 0.27, −0.07 | 1738 | −0.61 (0.481) | 9.24 (0.420) |
Notes. Median values derived for the FRs and COM AGN from Fig. 11. Values in parenthesis are standard deviations. SFR, M*, and tlast burst are estimated from the fit to the IR+UV SED (Delvecchio et al. 2017). We also give values for the individual FR populations, for comparison. Note: We do not provide the results of the linear regression between ΔsSFR and tlast burst as the observed anti-correlation is artificially induced by the co-dependence between these quantities in the SED-fitting code.
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