\begin{table}%t4
\caption{\label{Tab4}Gas kinematic results.}
%\centerline
 {\small \begin{tabular}{lccc}
\hline\hline
Galaxy  & $cz_{{\rm nuc, H}\alpha}$ & $\Delta v_{{\rm H}\alpha}$       & 
$\sigma_{{\rm nuc, H}\alpha}$\\ 
(1) & (2) & (3) & (4) \\
\hline
%\hline
NGC~23	       & $4495\pm 9$ & $-215$, $+236$ & $139\pm 17$ \\
MCG~+12-02-001 & $4732\pm 8$ & $-110$, $+156$ & $105\pm 14$\\
UGC~1845       & $4796\pm 9$ & $-237$, $+181$ & $142\pm 17$\\
NGC~2388       & $4093\pm 9$ & $-157$, $+163$ & $115\pm 15$\\
MCG~+02-20-003 & $4950\pm 9$ & $-141$, $+110$ & $96\pm 13$\\
IC~860$^*$     & $4146\pm 13$ & $\cdots$      & $\cdots$  \\
NGC~5936       & $3984\pm 13$ & $-66$, $+179$ & $66\pm 15$\\
NGC~6701       & $3946\pm 13$ & $-41$, $+102$ & $92\pm 16$\\  
NGC~7469       & $4946\pm 9^{**}$  & $-110$,$+207$$^{**}$ & $125\pm 16^{**}$ \\
NGC~7591       & $4869\pm 9$ & $-179$, $+345$  & $144 \pm 17$\\     
NGC~7771       & $4334\pm 9$ & $-181$, $+199$ & $106\pm 14$\\
\hline
\end{tabular} }
\medskip
Notes. --  Column~(2): $cz_{{\rm nuc, H}\alpha}$ is the H$\alpha$ velocity of the  nucleus, defined as the peak of the 6200~\AA \ continuum, except
  for NGC~7771 where it is refered to the position that makes the
  velocity field gradient symmetric (see text and Fig.~\ref{Fig3}c). 
Column~(3): $\Delta v_{{\rm H}\alpha}$ is the H$\alpha$
peak-to-peak velocity range over the PMAS FoV. Column~(4): 
$\sigma_{{\rm nuc, H}\alpha}$ is the nuclear H$\alpha$ velocity dispersion
(corrected for instrumental effects). All measurements are  in km~s$^{-1}$, and are not corrected for inclination and/or angular resolution effects; $^*$~for IC~860 $cz_{\rm nuc}$ is from  [N~{\sc ii}]$\lambda$6584 and 
[S~{\sc ii}]$\lambda\lambda$6717,6731. We note that NED quotes a value of $3347~{\rm km~s}^{-1}$ from 21~cm H~{\sc i} measurements, whereas our value of the velocity is confirmed by measurements of the mid-infrared emission lines with {\it Spitzer}/IRS (Pereira-Santaella et~al. \cite{perezgonzalez2005}, in preparation); $^{**}$~for NGC~7469 the measurements are from [N~{\sc ii}]$\lambda$6584.
\end{table}