\begin{table}%T3
\par
  \caption{\label{table:btf:rotcur-params}Derived    parameters for the rotation curve sub-sample.}
\small
%\centerline
{
 \begin{tabular}{lccrrccrrrrrlrcc}
\hline\hline
\multicolumn{1}{c}{ID}& $\alpha_{2000}$ & $\delta_{2000}$ & \multicolumn{1}{c}{${V_{\rm sys}}$} & \multicolumn{1}{c}{D} & $M_V$ & $(V-I)$ & \multicolumn{1}{c}{$M_{\rm HI}$} & \multicolumn{1}{c}{$W_{20}$} & \multicolumn{1}{c}{$W_{50}$} &\multicolumn{1}{c}{ $W_{20}$$_{\rm{,~turb}}$} & \multicolumn{1}{c}{$W_{50}$$_{\rm{,~turb}}$} & \multicolumn{1}{c}{$i$} & \multicolumn{1}{c}{$\langle {\rm PA} \rangle$} & $V_{vf}$ & $V_{pv}$\\
~ & (h m s) & ($\circ~~~ \arcmin~~~ \arcsec$) & \multicolumn{1}{c}{~{km}~{s}$^{-1}$} & \multicolumn{1}{c}{Mpc} & mag  & & \multicolumn{1}{c}{$10^7$~\Msun} & \multicolumn{1}{c}{~{km}~{s}$^{-1}$} & \multicolumn{1}{c}{~{km}~{s}$^{-1}$} & \multicolumn{1}{c}{~{km}~{s}$^{-1}$} & \multicolumn{1}{c}{~{km}~{s}$^{-1}$} &\multicolumn{1}{c}{\degr} &\multicolumn{1}{c}{\degr} &~{km}~{s}$^{-1}$ &~{km}~{s}$^{-1}$\\
\multicolumn{1}{c}{(1)} & (2) & (3) & \multicolumn{1}{c}{(4)} & \multicolumn{1}{c}{(5)} & (6) & (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)} & \multicolumn{1}{c}{(14)} & (15) & (16)\\
\hline
D500-2$^*$ & 10 31 43.0 & +25 18 33 & 1259 & 17.9~ & $-$16.38 & 0.42 & 87.08 & 135 & 120 & 119 & 105 & 57 $\pm$ 6 & 345 & 68 & 68\\ 
D500-3  & 10 05 59.5 & +23 52 04 & 1327 & 18.5~ & $-$15.74 & 0.31 & 6.58 & 96 & 83 & 84 & 72 & 55$^a$ $\pm$ 6 & \nodata & \nodata & 45\\ 
D512-2 & 14 33 20.2 & +26 59 54 & 840  & 14.1~ & $-$15.22 & 0.80 & 6.96 & 88 & 74 & 78 & 65 & 56 $\pm$ 10 & 40 & 35 & 37\\ 
D564-8$^*$ & 09 02 54.0 & +20 04 28 & 478  & 6.5~ & $-$12.64 & 0.93 & 1.58 & 62 & 48 & 54 & 42 & 63 $\pm$ 7 & 13 & 25 & 29\\ 
D575-2$^*$ & 12 52 21.9 & +21 37 46 & 774  & 12.2~ & $-$15.15 & 0.78 & 31.51 & 146 & 119 & 129 & 104 & 57 $\pm$ 5 & 220 & 74 & \nodata\\ 
D631-7$^*$ & 07 57 01.8 & +14 23 27 & 311  & 5.5$^b$ & $-$14.50 & 0.55 & 14.68 & 113 & 89 & 100 & 78 & 59 $\pm$ 3 & 324 & 58 & 53\\ 
\hline
\end{tabular}}
\smallskip
$^a$ {Optical \emph{I}-band inclination from \cite{pildis-1997}.}\\
$^b$ {Distance as given in \cite{karachentsev-2003}.}\\
 {Notes:} Cols.~(1) to~(12) as in
Table~\ref{table:btf:derived-params}, except that for
the starred galaxies, the center position and $V_{{\rm sys}}$ were
derived kinematically; (13)~inclination angle (optical inclination for
D500-3, kinematic inclination otherwise). The uncertainties given for
the kinematic inclination angles represent the scatter of the values
of the individual tilted-rings. For D500-3, 
the average uncertainty of the kinematic inclination estimates is given; (14)~average position angle of the rotation curve analysis, measured
counter-clockwise from north to the receding side of the galaxy; (15)~maximum rotation velocity from the tilted-ring analysis of the
velocity field, corrected for inclination; (16)~maximum
rotation velocity from the position-velocity diagram, corrected for
inclination.
\end{table}