\begin{table}%t2
\caption{Log of observations of \gem\ and \psh\  
with the Subaru.\label{t:log}} 
%\centerline
{\begin{tabular}{lllcll}
\hline\hline
   PSR       &       UT   &Exp.   &Band   &Seeing$^a$& Sec~$z$   \\
	     & 21 Jan. 2001&s     &       &arcsec&         \\
\hline
  Geminga    & 05:17:26.9 & 332.3 & $I$ & 0.66 & 1.56   \\
  Geminga    & 05:30:12.6 & 300.0 & $I$ & 0.66 & 1.47   \\
  Geminga    & 05:42:29.2 & 300.0 & $I$ & 0.70 & 1.39   \\
  Geminga    & 05:51:53.6 & 300.0 & $I$ & 0.65 & 1.35   \\
  Geminga    & 06:01:30.5 & 300.0 & $I$ & 0.68 & 1.30   \\
  Geminga    & 06:31:27.7 & 300.0 & $I$ & 0.55 & 1.19   \\
  Geminga    & 06:40:32.8 & 300.0 & $I$ & 0.55 & 1.16   \\
  Geminga    & 06:49:38.0 & 400.0 & $I$ & 0.55 & 1.13   \\
  Geminga    & 07:00:22.8 & 400.0 & $I$ & 0.60 & 1.11   \\
  Geminga    & 07:11:07.8 & 400.0 & $I$ & 0.58 & 1.09   \\
  Geminga    & 07:21:52.8 & 400.0 & $I$ & 0.60 & 1.07   \\
  Geminga    & 07:32:38.2 & 400.0 & $I$ & 0.60 & 1.05   \\
  Geminga    & 07:43:23.9 & 400.0 & $I$ & 0.60 & 1.04   \\
  Geminga    & 08:07:55.3 & 400.0 & $I$ & 0.61 & 1.01   \\
  Geminga    & 08:26:36.9 & 400.0 & $I$ & 0.62 & 1.00   \\
  B0656+14   & 08:46:10.7 & 400.0 & $I$ & 0.65 & 1.01   \\
  B0656+14   & 08:56:55.8 & 400.0 & $I$ & 0.65 & 1.01   \\
  B0656+14   & 09:07:40.9 & 400.0 & $I$ & 0.73 & 1.00   \\
  B0656+14   & 09:18:26.0 & 400.0 & $I$ & 0.67 & 1.00   \\
  B0656+14   & 09:29:10.9 & 400.0 & $I$ & 0.65 & 1.01   \\
  B0656+14   & 09:39:55.9 & 400.0 & $I$ & 0.63 & 1.01   \\
  B0656+14   & 10:22:05.8 & 510.0 & $R$ & 0.60 & 1.04   \\
  B0656+14   & 10:34:41.0 & 510.0 & $R$ & 0.60 & 1.06   \\
  Geminga    & 10:47:15.8 & 510.0 & $R$ & 0.61 & 1.13   \\
  Geminga    & 10:59:58.6 & 510.0 & $R$ & 0.68 & 1.17   \\
  Geminga    & 11:12:33.8 & 510.0 & $R$ & 0.61 & 1.21   \\
  Geminga    & 11:25:09.0 & 510.0 & $R$ & 0.60 & 1.25   \\
  B0656+14   & 11:54:36.9 & 600.0 & $B$     & 0.65 & 1.28   \\
  B0656+14   & 12:08:42.3 & 600.0 & $B$     & 0.66 & 1.35   \\
  B0656+14   & 12:22:47.8 & 600.0 & $B$     & 0.69 & 1.43   \\
\hline
\end{tabular}}
\par
\smallskip
$^a$~FWHM of the stellar profile in the individual images.    
\par
\end{table}