\begin{table}%T4 \caption{\label{table:btf:M/L-ratios}Stellar, gas, and baryonic masses.} \small %\centerline { \begin{tabular}{lccccccc} \hline\hline\noalign{\smallskip} \multicolumn{1}{c}{ID}& $\Upsilon_*^I$ (Bell) & $\Upsilon_*^I$ (Portinari) & $\langle \Upsilon_*^I \rangle$ & $M_{\rm{gas}}$ & $M_*$ (Bell) & $M_*$ (Portinari) & $\langle M_{\rm{bar}} \rangle$ \\ \multicolumn{1}{c}{} & & & & $10^8$ \Msun & $10^8$ \Msun & $10^8$ \Msun & $10^8$ \Msun \\ \multicolumn{1}{c}{(1)} & (2) & (3) & (4) & (5) & (6) & (7) & (8) \\ \hline D500-2 & 0.35 & 0.12 & 0.24 $\pm$ 0.12 & 12.19 & 0.73 & 0.26 & 12.69\\ D500-3 & 0.26 & 0.09 & 0.18 $\pm$ 0.09 & 0.92 & 0.28 & 0.09 & 1.11\\ D512-2 & 0.90 & 0.37 & 0.64 $\pm$ 0.27 & 0.98 & 0.93 & 0.38 & 1.63\\ D564-8 & 1.24 & 0.54 & 0.89 $\pm$ 0.35 & 0.22 & 0.14 & 0.06 & 0.32\\ D572-5 & 0.44 & 0.16 & 0.30 $\pm$ 0.14 & 1.20 & 0.19 & 0.07 & 1.33\\ D575-1 & 0.70 & 0.28 & 0.49 $\pm$ 0.21 & 0.53 & 0.26 & 0.10 & 0.71\\ D575-2 & 1.07 & 0.45 & 0.76 $\pm$ 0.31 & 4.41 & 1.02 & 0.43 & 5.13\\ D575-5 & 0.36 & 0.13 & 0.25 $\pm$ 0.12 & 0.60 & 0.04 & 0.02 & 0.63\\ D631-7 & 0.48 & 0.18 & 0.33 $\pm$ 0.15 & 2.05 & 0.20 & 0.08 & 2.19\\ D640-13 & 0.48 & 0.18 & 0.33 $\pm$ 0.15 & 0.64 & 0.18 & 0.07 & 0.76\\ D646-7 & 0.99 & 0.41 & 0.70 $\pm$ 0.29 & 0.05 & 0.09 & 0.04 & 0.12\\\hline \end{tabular}} \smallskip Notes: (1)~galaxy identifier; (2)~stellar {\it I}-band mass-to-light ratio based on \cite{bell-2001}; (3)~stellar {\it I}-band mass-to-light ratio based on \cite{portinari-2004}; (4)~average of {\it I}-band $\Upsilon_{*}$ values listed in Cols.~(2) and~(3). For the uncertainty in $\Upsilon_{*}$, we assume half the difference between the mass-to-light ratios of the two population models; (5)~the gas mass in $10^8$~\Msun; (6)~the stellar mass based on $\Upsilon_{*}$ in Col.~(2) in units of $10^8$~\Msun; (7)~like (6), but based on $\Upsilon_{*}$\ in Col.~(3); (8)~the baryonic mass used in further analysis, derived from the gas mass in Col.~(5) and the average of the stellar masses in Cols.~(6) and~(7). \end{table}