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Table 3

Scaling relation parameters across quenching stages.

log(SFR) = q + m log(M*)
Group m q ⟨x⟩ ⟨y⟩ Scatter rP rS
SF 0.76−0.02+0.02$\[0.76_{-0.02}^{+0.02}\]$ −7.54−0.21+0.22$\[-7.54_{-0.21}^{+0.22}\]$ 10.21 0.23 0.06 0.77 0.76
QnR 0.38−0.28+0.28$\[0.38_{-0.28}^{+0.28}\]$ −3.92−3.01+3.04$\[-3.92_{-3.01}^{+3.04}\]$ 10.76 0.21 0.20 0.23 0.38
cQ 0.72−0.10+0.10$\[0.72_{-0.10}^{+0.10}\]$ −7.71−1.07+1.06$\[-7.71_{-1.07}^{+1.06}\]$ 10.77 0.02 0.26 0.61 0.62
MX 0.98−0.09+0.09$\[0.98_{-0.09}^{+0.09}\]$ −10.95−0.97+0.99$\[-10.95_{-0.97}^{+0.99}\]$ 10.75 −0.45 0.68 0.64 0.40
nR 0.54−0.11+0.11$\[0.54_{-0.11}^{+0.11}\]$ −7.57−1.15+1.16$\[-7.57_{-1.15}^{+1.16}\]$ 11.05 −1.82 0.77 0.39 0.17
fR 0.77−0.10+0.09$\[0.77_{-0.10}^{+0.09}\]$ −10.94−1.01+1.01$\[-10.94_{-1.01}^{+1.01}\]$ 10.9 −2.63 0.32 0.58 0.46
log(SFR) = q + m log(Mmol)
Group m q ⟨x⟩ ⟨y⟩ Scatter rP rS
SF 0.79−0.02+0.02$\[0.79_{-0.02}^{+0.02}\]$ −7.06−0.20+0.19$\[-7.06_{-0.20}^{+0.19}\]$ 0.23 9.25 0.13 0.82 (0.85) 0.86 (0.85)
QnR 0.78−0.09+0.12$\[0.78_{-0.09}^{+0.12}\]$ −7.03−1.13+0.83$\[-7.03_{-1.13}^{+0.83}\]$ 0.21 9.46 0.10 0.64 (0.52) 0.65 (0.69)
cQ 1.32−0.13+0.16$\[1.32_{-0.13}^{+0.16}\]$ −11.95−1.46+1.17$\[-11.95_{-1.46}^{+1.17}\]$ 0.03 9.07 0.26 0.66 (0.83) 0.75 (0.84)
MX 1.54−0.08+0.09$\[1.54_{-0.08}^{+0.09}\]$ −14.32−0.81+0.71$\[-14.32_{-0.81}^{+0.71}\]$ −0.46 9.01 0.24 0.80 (0.65) 0.72 (0.66)
nR 2.11−0.17+0.21$\[2.11_{-0.17}^{+0.21}\]$ −19.84−1.84+1.49$\[-19.84_{-1.84}^{+1.49}\]$ −1.83 8.6 0.21 0.66 (0.53) 0.62 (0.49)
fR 1.58−0.11+0.13$\[1.58_{-0.11}^{+0.13}\]$ −15.40−1.08+0.91$\[-15.40_{-1.08}^{+0.91}\]$ −2.6 8.06 0.15 0.69 (0.58) 0.71 (0.43)
log(Mmol) = q + m log(M*)
Group m q ⟨x⟩ ⟨y⟩ Scatter rP rS
SF 1.08−0.03+0.03$\[1.08_{-0.03}^{+0.03}\]$ −1.88−0.29+0.29$\[-1.88_{-0.29}^{+0.29}\]$ 10.21 9.25 0.15 0.84 (0.86) 0.81 (0.85)
QnR 1.09−0.31+0.32$\[1.09_{-0.31}^{+0.32}\]$ −2.43−3.39+3.34$\[-2.43_{-3.39}^{+3.34}\]$ 10.76 9.46 0.27 0.52 (0.80) 0.57 (0.72)
cQ 0.92−0.09+0.09$\[0.92_{-0.09}^{+0.09}\]$ −0.73−0.91+0.95$\[-0.73_{-0.91}^{+0.95}\]$ 10.77 9.05 0.24 0.70 (0.78) 0.62 (0.69)
MX 0.75−0.07+0.07$\[0.75_{-0.07}^{+0.07}\]$ 0.89−0.73+0.71$\[0.89_{-0.73}^{+0.71}\]$ 10.75 9.01 0.44 0.63 (0.44) 0.36 (0.34)
nR 0.59−0.06+0.06$\[0.59_{-0.06}^{+0.06}\]$ 2.09−0.63+0.62$\[2.09_{-0.63}^{+0.62}\]$ 11.08 8.6 0.23 0.64 (0.51) 0.44 (0.30)
fR 0.57−0.07+0.07$\[0.57_{-0.07}^{+0.07}\]$ 1.85−0.79+0.78$\[1.85_{-0.79}^{+0.78}\]$ 10.89 8.05 0.23 0.55 (0.40) 0.49 (0.63)

Notes. Slope (m), intercept (q), median x–quantity, median y–quantity, intrinsic scatter, and correlation coefficient for the SFR-M*, Mmol − M*, and SFR-Mmol relations for galaxies at a given quenching stage (as indicated in the first column). Quantities (expect rP and rS) are obtained via the linmix algorithm. Slope and intercept are provided as median with the uncertainties giving the interval between the median and the 25th percentile (–) or between the 75th percentile and the median (+). The intrinsic scatters are provided as medians of the relative posterior distributions. The Pearson (rP) and Spearman (rS) correlation coefficients for the full sample and for the sample of only CO-detected galaxies (within brackets) are indicated.

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