\begin{table}%t4
\caption{Derived quantities from the harmonic decomposition.}
\label{tabharm}
%\centerline
{
\begin{tabular}{lccccccccc}
\hline
  \hline
\noalign{\smallskip}
Galaxy & $\langle A_{\rm r}\rangle$ & $\langle A_{\rm r,1~kpc}\rangle$ & $\langle A_{\rm r}\rangle$/$v_{\rm rot}$ & $\langle M_{\rm res}\rangle$ & $\langle A_{\rm r,c}\rangle$ & $\langle A_{\rm r,c,1~kpc}\rangle$ & $\langle A_{\rm r,c}\rangle$/$v_{\rm rot}$ & $\langle M_{\rm res,c}\rangle$ & $r_{\rm max}$\\
& [\kms] & [\kms] & [\%] & [\kms] & [\kms] & [\%] & [\kms] & [kpc]\\
(1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) & (10)\\
\hline
\noalign{\smallskip}
NGC~2366 & $2.91^{\rm +4.09}_{-1.06}$ & $1.50^{\rm +0.42}_{-0.87}$ & 5.8 & 2.15 &
$4.81^{\rm +2.32}_{-1.83}$ & $2.08^{\rm +0.66}_{-0.67}$ & 9.6 & 1.89 & 4.1\\
\noalign{\smallskip} ESO~059-G001 & $0.77^{\rm +0.51}_{-0.09}$ &
$0.77^{\ldots}_{\ldots}$ & 1.1 & 0.43 &
$1.45^{\rm +0.62}_{-0.61}$ & $1.17^{\ldots}_{\ldots}$ & 2.1 & 0.37 & 3.2\\
\noalign{\smallskip}
ESO~215-G?009 & \ldots & \ldots & \ldots & \ldots & $6.57^{\rm +1.64}_{-1.38}$ & $5.42^{\rm +2.79}_{-3.03}$ & 8.5 & 1.99 & 7.3\\
\noalign{\smallskip} NGC~4861 & $1.54^{\rm +0.94}_{-0.46}$ &
$0.78^{\ldots}_{\ldots}$ & 3.3 & 1.04 &
$2.60^{\rm +0.78}_{-0.28}$ & $1.02^{\ldots}_{\ldots}$ & 5.7 & 1.07 & 7.1\\
\noalign{\smallskip} \noalign{\smallskip} NGC~5408 &
$2.15^{\rm +2.62}_{-0.88}$ & $2.50^{\ldots}_{\ldots}$ & 4.1 & 1.92 &
$4.08^{\rm +2.63}_{-1.79}$ & $2.54^{\ldots}_{\ldots}$ & 7.7 & 1.30 & 6.9\\
\noalign{\smallskip}
IC~5152 & $2.35^{\rm +2.27}_{-1.24}$ & $1.63^{\rm +0.99}_{-1.24}$ & 5.3 & 1.17 &
$5.38^{\rm +0.10}_{-0.64}$ & $5.38^{\rm +0.10}_{-0.64}$ & 12.2 & 1.07 & 3.9\\
\hline 
\end{tabular}}
Notes: (1) The name of the galaxy; (2) the median of the
  quadratically-added amplitude of the non-circular motions (unconstrained
  case), averaged over the entire radial range, the errors indicate the lower
  and upper quartile; (3) same as (2), but averaged over the inner 1~kpc
  only; (4) the percentage the non-circular motions contribute to the maximum
  rotation velocity; (5) the median of the \emph{reswri} absolute residual
  velocity field after the harmonic decomposition; (6), (7), (8), (9) the same
  as (2), (3), (4), (5), but for the constrained case; (10) maximum radius for
  the averaging of the quadratically-added amplitudes.
\end{table}