Table 6.
Median physical properties of the total sample of 27 OFGs.
| Derived from SED fitting with median stacked photometry ( * ) | ||
|---|---|---|
| zphot(a) | 4.5 ± 0.2 | |
| M⋆(b) | M⊙ | (2.8 ) × 1010 |
| LIR(c) | L⊙ | (1.6 ± 0.3) × 1012 |
| AV(b) | mag | 0.9 |
| Mdust(c) | M⊙ | (1.2 ± 0.2) × 108 |
| Tdust(d) | K | 45.5 |
| Median stacked photometry | ||
| H | mag | 27.4 ± 0.1 |
| [4.5] | mag | 23.92 ± 0.04 |
| S1.13 mm | μJy | 334 ± 24 |
| S3 GHz | μJy | 4.1 ± 0.7 |
| Derived quantities ( * *) | ||
| L1.4 GHz(e) | erg s−1 Hz−1 | (9.53 ± 1.53) × 1030 |
| qTIR(f) | 2.23 ± 0.03 | |
| SFRrad, med(g) | M⊙ yr−1 | 287.59 ± 53.86 |
| SFRIR, med(h) | M⊙ yr−1 | 235.33 |
| SFRUV, med(i) | M⊙ yr−1 | 0.33 ± 0.02 |
| ΔMS (j) | 1.45 |
|
| Mgas(k) | M⊙ | (2.6 ± 0.4) × 1010 |
| fgas(l) | 0.48 ± 0.05 | |
| τdep(m) | Myr | 110 |
Notes. ( * )Uncertainties are the 16–84th percentile ranges of the probability distribution function given by the SED fitting. ( * *)Uncertainties on derived quantities were calculated from the propagation of the errors in the parameter values.
Measured by MBB model fit (see Sect. 4.5).
Derived from S3 GHz assuming a radio spectral index α = −0.75 (see Eq. (10)).
Calculated from the IR-radio correlation (see Eq. (12)).
Calculated following Delhaize et al. (2017; see Eq. (9)), which was simply estimated from the radio emission without correction for AGN.
Derived following Kennicutt & Evans (2012; see Eq. 2).
Derived following Daddi et al. (2004), scaled to a Chabrier (2003) IMF (see Eq. (2)).
Distance to the SFMS: ΔMS = SFR/SFRMS, where SFRMS is the average SFR of MS galaxies at fixed stellar mass and redshift (Schreiber et al. 2015, see Fig. 9 and Sect. 5.4).
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