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.
x . | a . | b . | R2 . | Spearman r . | p . |
---|---|---|---|---|---|
LoM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.12 ± 0.00 | −0.69 ± 0.02 | 0.96 | 0.99 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.22 ± 0.05 | −0.52 ± 0.11 | 0.22 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.32 ± 0.05 | 0.32 | 0.61 | <0.01 |
log10Z/Z⊙ | −0.18 ± 0.08 | 0.01 ± 0.02 | 0.08 | −0.22 | 0.07 |
[Mg/Fe] | 0.16 ± 0.10 | −0.02 ± 0.01 | 0.04 | 0.21 | 0.09 |
log10re/kpc | −0.04 ± 0.04 | −0.01 ± 0.02 | 0.02 | −0.06 | 0.65 |
log10M⋆,Chab | 0.08 ± 0.03 | −0.92 ± 0.29 | 0.12 | 0.38 | <0.01 |
MK − 5log10h | −0.02 ± 0.01 | −0.53 ± 0.25 | 0.06 | −0.26 | 0.03 |
log10MBH/M⋆ | 0.11 ± 0.02 | 0.31 ± 0.06 | 0.34 | 0.46 | <0.01 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.15 ± 0.02 | −0.59 ± 0.09 | 0.37 | 0.56 | <0.01 |
HiM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.07 ± 0.01 | −0.51 ± 0.03 | 0.87 | 0.91 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.19 ± 0.08 | −0.52 ± 0.15 | 0.18 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.38 ± 0.04 | 0.53 | 0.68 | <0.01 |
log10Z/Z⊙ | 0.13 ± 0.06 | −0.22 ± 0.04 | 0.15 | 0.39 | 0.04 |
[Mg/Fe] | 0.39 ± 0.05 | −0.19 ± 0.01 | 0.72 | 0.81 | <0.01 |
log10re/kpc | 0.12 ± 0.08 | −0.24 ± 0.06 | 0.09 | 0.24 | 0.21 |
log10M⋆,Chab | 0.09 ± 0.04 | −1.10 ± 0.40 | 0.17 | 0.36 | 0.06 |
MK − 5log10h | −0.02 ± 0.02 | −0.66 ± 0.34 | 0.08 | −0.21 | 0.26 |
log10MBH/M⋆ | −0.01 ± 0.02 | −0.16 ± 0.06 | <0.01 | 0.24 | 0.21 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.08 ± 0.05 | −0.40 ± 0.15 | 0.10 | 0.36 | 0.06 |
x . | a . | b . | R2 . | Spearman r . | p . |
---|---|---|---|---|---|
LoM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.12 ± 0.00 | −0.69 ± 0.02 | 0.96 | 0.99 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.22 ± 0.05 | −0.52 ± 0.11 | 0.22 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.32 ± 0.05 | 0.32 | 0.61 | <0.01 |
log10Z/Z⊙ | −0.18 ± 0.08 | 0.01 ± 0.02 | 0.08 | −0.22 | 0.07 |
[Mg/Fe] | 0.16 ± 0.10 | −0.02 ± 0.01 | 0.04 | 0.21 | 0.09 |
log10re/kpc | −0.04 ± 0.04 | −0.01 ± 0.02 | 0.02 | −0.06 | 0.65 |
log10M⋆,Chab | 0.08 ± 0.03 | −0.92 ± 0.29 | 0.12 | 0.38 | <0.01 |
MK − 5log10h | −0.02 ± 0.01 | −0.53 ± 0.25 | 0.06 | −0.26 | 0.03 |
log10MBH/M⋆ | 0.11 ± 0.02 | 0.31 ± 0.06 | 0.34 | 0.46 | <0.01 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.15 ± 0.02 | −0.59 ± 0.09 | 0.37 | 0.56 | <0.01 |
HiM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.07 ± 0.01 | −0.51 ± 0.03 | 0.87 | 0.91 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.19 ± 0.08 | −0.52 ± 0.15 | 0.18 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.38 ± 0.04 | 0.53 | 0.68 | <0.01 |
log10Z/Z⊙ | 0.13 ± 0.06 | −0.22 ± 0.04 | 0.15 | 0.39 | 0.04 |
[Mg/Fe] | 0.39 ± 0.05 | −0.19 ± 0.01 | 0.72 | 0.81 | <0.01 |
log10re/kpc | 0.12 ± 0.08 | −0.24 ± 0.06 | 0.09 | 0.24 | 0.21 |
log10M⋆,Chab | 0.09 ± 0.04 | −1.10 ± 0.40 | 0.17 | 0.36 | 0.06 |
MK − 5log10h | −0.02 ± 0.02 | −0.66 ± 0.34 | 0.08 | −0.21 | 0.26 |
log10MBH/M⋆ | −0.01 ± 0.02 | −0.16 ± 0.06 | <0.01 | 0.24 | 0.21 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.08 ± 0.05 | −0.40 ± 0.15 | 0.10 | 0.36 | 0.06 |
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.
x . | a . | b . | R2 . | Spearman r . | p . |
---|---|---|---|---|---|
LoM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.12 ± 0.00 | −0.69 ± 0.02 | 0.96 | 0.99 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.22 ± 0.05 | −0.52 ± 0.11 | 0.22 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.32 ± 0.05 | 0.32 | 0.61 | <0.01 |
log10Z/Z⊙ | −0.18 ± 0.08 | 0.01 ± 0.02 | 0.08 | −0.22 | 0.07 |
[Mg/Fe] | 0.16 ± 0.10 | −0.02 ± 0.01 | 0.04 | 0.21 | 0.09 |
log10re/kpc | −0.04 ± 0.04 | −0.01 ± 0.02 | 0.02 | −0.06 | 0.65 |
log10M⋆,Chab | 0.08 ± 0.03 | −0.92 ± 0.29 | 0.12 | 0.38 | <0.01 |
MK − 5log10h | −0.02 ± 0.01 | −0.53 ± 0.25 | 0.06 | −0.26 | 0.03 |
log10MBH/M⋆ | 0.11 ± 0.02 | 0.31 ± 0.06 | 0.34 | 0.46 | <0.01 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.15 ± 0.02 | −0.59 ± 0.09 | 0.37 | 0.56 | <0.01 |
HiM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.07 ± 0.01 | −0.51 ± 0.03 | 0.87 | 0.91 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.19 ± 0.08 | −0.52 ± 0.15 | 0.18 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.38 ± 0.04 | 0.53 | 0.68 | <0.01 |
log10Z/Z⊙ | 0.13 ± 0.06 | −0.22 ± 0.04 | 0.15 | 0.39 | 0.04 |
[Mg/Fe] | 0.39 ± 0.05 | −0.19 ± 0.01 | 0.72 | 0.81 | <0.01 |
log10re/kpc | 0.12 ± 0.08 | −0.24 ± 0.06 | 0.09 | 0.24 | 0.21 |
log10M⋆,Chab | 0.09 ± 0.04 | −1.10 ± 0.40 | 0.17 | 0.36 | 0.06 |
MK − 5log10h | −0.02 ± 0.02 | −0.66 ± 0.34 | 0.08 | −0.21 | 0.26 |
log10MBH/M⋆ | −0.01 ± 0.02 | −0.16 ± 0.06 | <0.01 | 0.24 | 0.21 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.08 ± 0.05 | −0.40 ± 0.15 | 0.10 | 0.36 | 0.06 |
x . | a . | b . | R2 . | Spearman r . | p . |
---|---|---|---|---|---|
LoM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.12 ± 0.00 | −0.69 ± 0.02 | 0.96 | 0.99 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.22 ± 0.05 | −0.52 ± 0.11 | 0.22 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.32 ± 0.05 | 0.32 | 0.61 | <0.01 |
log10Z/Z⊙ | −0.18 ± 0.08 | 0.01 ± 0.02 | 0.08 | −0.22 | 0.07 |
[Mg/Fe] | 0.16 ± 0.10 | −0.02 ± 0.01 | 0.04 | 0.21 | 0.09 |
log10re/kpc | −0.04 ± 0.04 | −0.01 ± 0.02 | 0.02 | −0.06 | 0.65 |
log10M⋆,Chab | 0.08 ± 0.03 | −0.92 ± 0.29 | 0.12 | 0.38 | <0.01 |
MK − 5log10h | −0.02 ± 0.01 | −0.53 ± 0.25 | 0.06 | −0.26 | 0.03 |
log10MBH/M⋆ | 0.11 ± 0.02 | 0.31 ± 0.06 | 0.34 | 0.46 | <0.01 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.15 ± 0.02 | −0.59 ± 0.09 | 0.37 | 0.56 | <0.01 |
HiM-50 | |||||
|$\log _{10} P_{\rm birth}/(\, {\rm K}\, {\rm cm}^{-3})$| | 0.07 ± 0.01 | −0.51 ± 0.03 | 0.87 | 0.91 | <0.01 |
|$\log _{10}\sigma _e/(\, {\rm km}\, {\rm s}^{-1})$| | 0.19 ± 0.08 | −0.52 ± 0.15 | 0.18 | 0.48 | <0.01 |
log10Age/Gyr | 0.34 ± 0.06 | −0.38 ± 0.04 | 0.53 | 0.68 | <0.01 |
log10Z/Z⊙ | 0.13 ± 0.06 | −0.22 ± 0.04 | 0.15 | 0.39 | 0.04 |
[Mg/Fe] | 0.39 ± 0.05 | −0.19 ± 0.01 | 0.72 | 0.81 | <0.01 |
log10re/kpc | 0.12 ± 0.08 | −0.24 ± 0.06 | 0.09 | 0.24 | 0.21 |
log10M⋆,Chab | 0.09 ± 0.04 | −1.10 ± 0.40 | 0.17 | 0.36 | 0.06 |
MK − 5log10h | −0.02 ± 0.02 | −0.66 ± 0.34 | 0.08 | −0.21 | 0.26 |
log10MBH/M⋆ | −0.01 ± 0.02 | −0.16 ± 0.06 | <0.01 | 0.24 | 0.21 |
|$\log _{10} \sigma _e^2/r_e\ [{\rm km^2\, s^{-2}\, kpc^{-1}}]$| | 0.08 ± 0.05 | −0.40 ± 0.15 | 0.10 | 0.36 | 0.06 |
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