Table 1.

Fit parameters to the r-band mass-to-light ratio excess, MLEr, for mock C13 galaxies in our variable IMF simulations. Columns 2 and 3 show the result of a linear least-squares fit of the relation between each parameter (indicated in Column 1) individually and MLEr, of the form MLEr = ax + b. Column 4 shows the coefficient of determination, while columns 5 and 6 show the Spearman-r value and the corresponding p-value.

xabR2Spearman rp
LoM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.12 ± 0.00−0.69 ± 0.020.960.99<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.22 ± 0.05−0.52 ± 0.110.220.48<0.01
log10Age/Gyr0.34 ± 0.06−0.32 ± 0.050.320.61<0.01
log10Z/Z−0.18 ± 0.080.01 ± 0.020.08−0.220.07
[Mg/Fe]0.16 ± 0.10−0.02 ± 0.010.040.210.09
log10re/kpc−0.04 ± 0.04−0.01 ± 0.020.02−0.060.65
log10M⋆,Chab0.08 ± 0.03−0.92 ± 0.290.120.38<0.01
MK − 5log10h−0.02 ± 0.01−0.53 ± 0.250.06−0.260.03
log10MBH/M0.11 ± 0.020.31 ± 0.060.340.46<0.01
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.15 ± 0.02−0.59 ± 0.090.370.56<0.01
HiM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.07 ± 0.01−0.51 ± 0.030.870.91<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.19 ± 0.08−0.52 ± 0.150.180.48<0.01
log10Age/Gyr0.34 ± 0.06−0.38 ± 0.040.530.68<0.01
log10Z/Z0.13 ± 0.06−0.22 ± 0.040.150.390.04
[Mg/Fe]0.39 ± 0.05−0.19 ± 0.010.720.81<0.01
log10re/kpc0.12 ± 0.08−0.24 ± 0.060.090.240.21
log10M⋆,Chab0.09 ± 0.04−1.10 ± 0.400.170.360.06
MK − 5log10h−0.02 ± 0.02−0.66 ± 0.340.08−0.210.26
log10MBH/M−0.01 ± 0.02−0.16 ± 0.06<0.010.240.21
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.08 ± 0.05−0.40 ± 0.150.100.360.06
xabR2Spearman rp
LoM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.12 ± 0.00−0.69 ± 0.020.960.99<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.22 ± 0.05−0.52 ± 0.110.220.48<0.01
log10Age/Gyr0.34 ± 0.06−0.32 ± 0.050.320.61<0.01
log10Z/Z−0.18 ± 0.080.01 ± 0.020.08−0.220.07
[Mg/Fe]0.16 ± 0.10−0.02 ± 0.010.040.210.09
log10re/kpc−0.04 ± 0.04−0.01 ± 0.020.02−0.060.65
log10M⋆,Chab0.08 ± 0.03−0.92 ± 0.290.120.38<0.01
MK − 5log10h−0.02 ± 0.01−0.53 ± 0.250.06−0.260.03
log10MBH/M0.11 ± 0.020.31 ± 0.060.340.46<0.01
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.15 ± 0.02−0.59 ± 0.090.370.56<0.01
HiM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.07 ± 0.01−0.51 ± 0.030.870.91<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.19 ± 0.08−0.52 ± 0.150.180.48<0.01
log10Age/Gyr0.34 ± 0.06−0.38 ± 0.040.530.68<0.01
log10Z/Z0.13 ± 0.06−0.22 ± 0.040.150.390.04
[Mg/Fe]0.39 ± 0.05−0.19 ± 0.010.720.81<0.01
log10re/kpc0.12 ± 0.08−0.24 ± 0.060.090.240.21
log10M⋆,Chab0.09 ± 0.04−1.10 ± 0.400.170.360.06
MK − 5log10h−0.02 ± 0.02−0.66 ± 0.340.08−0.210.26
log10MBH/M−0.01 ± 0.02−0.16 ± 0.06<0.010.240.21
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.08 ± 0.05−0.40 ± 0.150.100.360.06
Table 1.

Fit parameters to the r-band mass-to-light ratio excess, MLEr, for mock C13 galaxies in our variable IMF simulations. Columns 2 and 3 show the result of a linear least-squares fit of the relation between each parameter (indicated in Column 1) individually and MLEr, of the form MLEr = ax + b. Column 4 shows the coefficient of determination, while columns 5 and 6 show the Spearman-r value and the corresponding p-value.

xabR2Spearman rp
LoM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.12 ± 0.00−0.69 ± 0.020.960.99<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.22 ± 0.05−0.52 ± 0.110.220.48<0.01
log10Age/Gyr0.34 ± 0.06−0.32 ± 0.050.320.61<0.01
log10Z/Z−0.18 ± 0.080.01 ± 0.020.08−0.220.07
[Mg/Fe]0.16 ± 0.10−0.02 ± 0.010.040.210.09
log10re/kpc−0.04 ± 0.04−0.01 ± 0.020.02−0.060.65
log10M⋆,Chab0.08 ± 0.03−0.92 ± 0.290.120.38<0.01
MK − 5log10h−0.02 ± 0.01−0.53 ± 0.250.06−0.260.03
log10MBH/M0.11 ± 0.020.31 ± 0.060.340.46<0.01
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.15 ± 0.02−0.59 ± 0.090.370.56<0.01
HiM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.07 ± 0.01−0.51 ± 0.030.870.91<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.19 ± 0.08−0.52 ± 0.150.180.48<0.01
log10Age/Gyr0.34 ± 0.06−0.38 ± 0.040.530.68<0.01
log10Z/Z0.13 ± 0.06−0.22 ± 0.040.150.390.04
[Mg/Fe]0.39 ± 0.05−0.19 ± 0.010.720.81<0.01
log10re/kpc0.12 ± 0.08−0.24 ± 0.060.090.240.21
log10M⋆,Chab0.09 ± 0.04−1.10 ± 0.400.170.360.06
MK − 5log10h−0.02 ± 0.02−0.66 ± 0.340.08−0.210.26
log10MBH/M−0.01 ± 0.02−0.16 ± 0.06<0.010.240.21
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.08 ± 0.05−0.40 ± 0.150.100.360.06
xabR2Spearman rp
LoM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.12 ± 0.00−0.69 ± 0.020.960.99<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.22 ± 0.05−0.52 ± 0.110.220.48<0.01
log10Age/Gyr0.34 ± 0.06−0.32 ± 0.050.320.61<0.01
log10Z/Z−0.18 ± 0.080.01 ± 0.020.08−0.220.07
[Mg/Fe]0.16 ± 0.10−0.02 ± 0.010.040.210.09
log10re/kpc−0.04 ± 0.04−0.01 ± 0.020.02−0.060.65
log10M⋆,Chab0.08 ± 0.03−0.92 ± 0.290.120.38<0.01
MK − 5log10h−0.02 ± 0.01−0.53 ± 0.250.06−0.260.03
log10MBH/M0.11 ± 0.020.31 ± 0.060.340.46<0.01
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.15 ± 0.02−0.59 ± 0.090.370.56<0.01
HiM-50
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$|0.07 ± 0.01−0.51 ± 0.030.870.91<0.01
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$|0.19 ± 0.08−0.52 ± 0.150.180.48<0.01
log10Age/Gyr0.34 ± 0.06−0.38 ± 0.040.530.68<0.01
log10Z/Z0.13 ± 0.06−0.22 ± 0.040.150.390.04
[Mg/Fe]0.39 ± 0.05−0.19 ± 0.010.720.81<0.01
log10re/kpc0.12 ± 0.08−0.24 ± 0.060.090.240.21
log10M⋆,Chab0.09 ± 0.04−1.10 ± 0.400.170.360.06
MK − 5log10h−0.02 ± 0.02−0.66 ± 0.340.08−0.210.26
log10MBH/M−0.01 ± 0.02−0.16 ± 0.06<0.010.240.21
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$|0.08 ± 0.05−0.40 ± 0.150.100.360.06
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