\begin{table}%T1
\caption{\label{tab:sample_properties}Parameters of the sample galaxies.}
%\centerline
{
\begin{tabular}{lllrrcrrrrrcc}
\hline\hline
\multicolumn{1}{c}{Object} &
\multicolumn{2}{c}{Type} &
\multicolumn{1}{c}{$B_T$} &
\multicolumn{1}{c}{PA} &
\multicolumn{1}{c}{$i$} &
\multicolumn{1}{c}{$V_{\odot}$} &
\multicolumn{1}{c}{$D$} &
\multicolumn{1}{c}{Scale} &
\multicolumn{1}{c}{$R_{25}$} &
\multicolumn{1}{c}{$M_{B_T}^0$} &
\multicolumn{2}{c}{$R_{\rm last}/R_{25}$} \\
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{[stars]} &
\multicolumn{1}{c}{[gas]} \\
\multicolumn{1}{c}{[name]} &
\multicolumn{1}{c}{[RSA]} &
\multicolumn{1}{c}{[RC3]} &
\multicolumn{1}{c}{[mag]} &
\multicolumn{1}{c}{[\degr]} &
\multicolumn{1}{c}{[\degr]} &
\multicolumn{1}{c}{[\kms]} &
\multicolumn{1}{c}{[Mpc]} &
\multicolumn{1}{c}{[pc$/''$]} &
\multicolumn{1}{c}{[$''$]} &
\multicolumn{1}{c}{[mag]} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} \\
\multicolumn{1}{c}{$^{(1)}$} &
\multicolumn{1}{c}{$^{(2)}$} &
\multicolumn{1}{c}{$^{(3)}$} &
\multicolumn{1}{c}{$^{(4)}$} &
\multicolumn{1}{c}{$^{(5)}$} &
\multicolumn{1}{c}{$^{(6)}$} &
\multicolumn{1}{c}{$^{(7)}$} &
\multicolumn{1}{c}{$^{(8)}$} &
\multicolumn{1}{c}{$^{(9)}$} &
\multicolumn{1}{c}{$^{(10)}$} &
\multicolumn{1}{c}{$^{(11)}$} &
\multicolumn{1}{c}{$^{(12)}$} &
\multicolumn{1}{c}{$^{(13)}$} \\
\hline
\object{NGC~210}  & Sb(rs)  & SABb(s)     & 11.60 & 165 & 49 & 1650 & 23.2 & 113 & 150 &~$-20.5$ & 0.3&0.8 \\
\object{NGC~615}  & Sb(r)   & SAb(rs)     & 12.47 & 155 & 67 & 1849 & 25.7 & 125 & 108 &~$-20.3$ & 0.7&0.9 \\
\object{NGC~1620} & --     & SABbc(rs)   & 13.08 &  25 & 70 & 3509 & 46.1 & 224 &  86 &~$-21.1$ & 0.7&1.2 \\
\object{NGC~2590} & --     & SAbc(s):    & 13.94 &  77 & 72 & 4960 & 63.4 & 308 &  67 &~$-21.0$ & 0.5&1.0 \\
\object{NGC~2708} & --     & SABb(s)pec? & 12.80 &  25 & 60 & 1984 & 23.5 & 114 &  78 &~$-19.4$ & 0.6&0.8 \\
\object{NGC~2815} & Sb(s)   & SBb(r):     & 12.81 &  10 & 72 & 2535 & 30.0 & 145 & 104 &~$-21.0$ & 0.4&1.0 \\
\object{NGC~3054} & SBbc(s) & SABb(r)     & 12.35 & 118 & 52 & 2430 & 28.5 & 138 & 114 &~$-20.3$ & 0.5&0.9 \\
\object{NGC~3200} & Sb(r)   & SABc(rs):   & 12.83 & 169 & 73 & 3526 & 43.4 & 211 & 125 &~$-21.5$ & 0.5&0.9 \\
\object{NGC~3717} & Sb(s)   & SAb:sp      & 12.24 &  33 & 81 & 1748 & 19.6 &  95 & 180 &~$-20.5$ & 0.4&0.5 \\
\object{NGC~4682} & Sc(s)   & SABcd(s)    & 13.14 &  83 & 61 & 2344 & 28.8 & 140 &  77 &~$-20.0$ & 0.3&0.8 \\
\object{NGC~5530} & Sc(s)   & SAbc(rs)    & 11.79 & 127 & 62 & 1092 & 11.7 &  57 & 125 &~$-19.4$ & 0.6&0.9 \\
\object{NGC~6118} & Sc(s)   & SAcd(s)     & 12.42 &  58 & 65 & 1580 & 21.4 & 104 & 140 &~$-20.4$ & 0.6&0.8 \\
\object{NGC~6878} & Sc(r)   & SAb(s)      & 13.45 & 125 & 40 & 5821 & 77.3 & 375 &  48 &~$-21.3$ & 0.6&1.0 \\
\object{NGC~6925} & Sbc(r)  & SAbc(s)     & 12.07 &   5 & 75 & 2783 & 37.7 & 183 & 134 &~$-21.9$ & 0.6&0.9 \\
\object{NGC~7083} & Sb(s)   & SAbc(s)     & 11.87 &   5 & 53 & 3093 & 39.7 & 192 & 116 &~$-21.5$ & 0.5&1.0 \\
\object{NGC~7412} & Sc(rs)  & SBc(s)      & 11.88 &  65 & 42 & 1712 & 22.7 & 110 & 116 &~$-20.1$ & 0.4&0.8 \\
\object{NGC~7531} & Sbc(r)  & SABbc(r)    & 12.04 &  15 & 67 & 1591 & 20.9 & 102 & 134 &~$-20.2$ & 0.4&0.6 \\
\hline
\end{tabular}}
\smallskip
NOTES --~$^{(2)}$ Morphological classification from Sandage \& Tammann
         (1981, RSA hereafter).
$^{(3)}$ Morphological classification from~RC3.
$^{(4)}$~Total observed blue magnitude from~RC3 except for
         NGC~3954, NGC~4682 and NGC~5530 (LEDA).
$^{(5)}$ Major-axis position angle from~RC3.
$^{(6)}$~Inclination, derived as~$\cos^{2}{i}~=~(q^2-q_0^2)/(1-q_0^2)$. The observed axial ratio~$q$
         is taken from~RC3 and the intrinsic flattening~$q_0=0.11$ has been
         assumed following Guthrie (\cite{Guthrie1992}).
$^{(7)}$ Heliocentric velocity of the galaxy derived at the centre of
         symmetry of the rotation curve of the gas.~$\Delta V_\odot = 10$~{\kms}.
$^{(8)}$ Distance obtained as~$V_0/H_0$ with~$H_0=75$~\kms~Mpc$^{-1}$ and~$V_0$, the systemic velocity derived from~$V_\odot$
         corrected for the motion of the Sun with respect to the Local Group,
         as in~RSA.
$^{(10)}$ Radius of the 25~$B$~mag~arcsec$^{-2}$ isophote derived as~$R_{25} = D_{25}/2$ with~$D_{25}$ from~RC3.
$^{(11)}$ Absolute total blue magnitude corrected for
          inclination and extinction from~RC3.
$^{(12)}$ Radial extension of the stellar rotation curve
          in units of~$R_{25}$ from this paper.
$^{(13)}$ Radial extension of the ionized gas rotation curve
          in units of~$R_{25}$ from this paper.
\end{table}