\begin{table}%t1
\caption{\label{Table:datamrk1418}Basic data for Mrk~1418.}
\small%\centerline
 {
\begin{tabular}{ll}     
\hline
\hline
Parameter      &  Value  \\
\hline
RA (2000)				       &  \phantom{+}09:40:27  	     \\
Dec (2000)			               &  +48:20:16		     \\
$v_{\rm helio}$ (km~s$^{-1}$)	       &  $773\pm11$		     \\
$D$ (Mpc)				       &  $14.6\pm1.0$ 		     \\
$A_{B}$ (mag)$^{a}$		       &  0.098		             \\
$m_{B}$ (mag)$^{b}$		       &  $13.86\pm0.03$	     \\
$m_{R}$ (mag)$^{b}$		       &  $12.61\pm0.19$	     \\
$M_{B}$ (mag)$^{c}$		       &  $-16.96$		     \\
$F(\Ha)$ (erg s$^{-1}$ cm $^{-2})^{b}$ &  $95\pm16 \times 10^{-14}$  \\       
$m_{J}$ (mag)$^{d}$		       &  $12.08\pm0.03$	     \\
$m_{H}$ (mag)$^{d}$		       &  $11.46\pm0.04$	     \\
$m_{K_{\rm s}}$ (mag)$^{d}$  	       &  $11.41\pm0.05$	     \\
$M_{\rm HI}\;(M_{\odot})^{e}$         &  $2.30\times10^{8}$         \\
\hline
\end{tabular}}
\medskip
Notes: RA, Dec, heliocentric velocity, $v_{\rm helio}$, and distance, $D$~(Mpc), all taken from NED (\url{http://nedwww.ipac.caltech.edu/}). Distance calculated using a Hubble constant of 73~km~s$^{-1}$~Mpc$^{-1}$, and taking  the influence of the Virgo Cluster, the Great 
Attractor, and the Shapley supercluster into account. \\
$^{{a}}$ Absorption coefficient in the $B$~band, from \cite{Schlegel1998}. \\
$^{{b}}$ $B$- and $R$-band integrated magnitudes, their $1\sigma$~uncertainty and integrated \Ha~flux, corrected for Galactic extinction \citep{GildePaz2003}. \\
$^{{c}}$ Absolute magnitude in the $B$ band, computed from the above tabulated $B$ integrated magnitude and distance. \\
$^{{d}}$ Total magnitudes from 2MASS.  \\
$^{{e}}$ Neutral hydrogen mass $M_{\rm HI}$ from \cite{VanZee2001}, who adopted a distance of 10.8~Mpc.
\end{table}