Table 2.
Estimated star formation rates (SFRs) of high-redshift galaxies at the main sequence (SFRMS) compared with the SFR of the nearby galaxies selected to act as AGN hosts in the mock HARMONI simulations (see Table A.1 for SFR0 values).
| Hosts | ||||
|---|---|---|---|---|
| Lenticular | Spiral | Interaction | ||
| SFRMS | 1.02 | 1.16 | 1.49 | |
| z = 0.76 | ΔSFR0 − MS | −0.61 | −1.26 | −0.09 |
| AGN host | S-F | Q | S-F | |
| SFRMS | 1.38 | 1.55 | 1.94 | |
| z = 1.50 | ΔSFR0 − MS | −0.97 | −1.65 | −0.54 |
| AGN host | S-F | Q | S-F | |
| SFRMS | 1.68 | 1.89 | 2.37 | |
| z = 2.30 | ΔSFR0 − MS | −1.27 | −1.99 | −0.97 |
| AGN host | Q | Q | S-F | |
Notes. Units of SFR and ΔSFR0 − MS are in log M⊙ yr−1 and 1 dex, respectively. S-F and Q classify the galaxy as star-forming or quenched, respectively, based on the distance to the MS criteria.
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