0.29$ & -0.097 & $0.749 \pm 0.117$ & & & X & &\
NGC 7144 & -5 & $31.89 \pm 0.12$ & -0.074 & $0.840 \pm 0.116$ & X & & & &\
NGC 7145 & -5 & $31.79 \pm 0.21$ & -0.218 & $0.761 \pm 0.082$ & X & & X & &\
NGC 7192 & -4 & $32.83 \pm 0.32$ & -0.080 & $0.665 \pm 0.117$ & & & X & &\
IC 1459 & -5 & $32.27 \pm 0.28$ & 0.145 & $0.912 \pm 0.116$ & X & & & &\
NGC 7457 & -3 & $30.55 \pm 0.21$ & -0.444 & $0.550 \pm 0.060$ & & & & X & X\
NGC 7507 & -5 & $31.93 \pm 0.17$ & 0.042 & $0.801 \pm 0.082$ & X & & X & &\
NGC 7619 & -5 & $33.56 \pm 0.31$ & 0.175 & $1.002 \pm 0.116$ & X & & & &\
]{}

Transformations to the $B$-band {#ss:colors}
-------------------------------

For comparison to results at intermediate redshifts it is important to have access to $M/L$ values in the rest-frame $B$-band. We therefore took the published values[^3] and transformed them to $B$-band mass-to-light ratios $M/L_B$ for the distances 