\begin{table}%t5
\caption{Geminga  in the NIR-optical-NUV-FUV range. \label{t:633_fl}}
%\centerline
{\begin{tabular}{lccc}
\hline\hline
Filter/  & Log ${\nu}$        & $F_{\nu}$   & $F_{\nu}$   \\
 Telescope                         &              &
 observed         &dereddened$^a$   \\
                   &  Hz            & $\mu$Jy          &$\mu$Jy    \\
\hline
\multicolumn{4}{c}{NIR} \\
${\it F160W}$/HST          & 14.273($^{\rm +58}_{-51}$)          &
0.230(25)$^{b,c}$      &0.233(25)   \\
${\it F110W}$/HST          & 14.436($^{\rm +138}_{-105}$)           &
0.166(21)$^{b,c}$      &0.170(21)   \\
\hline
\multicolumn{4}{c}{Optical} \\
$I$/Subaru           & 14.571($^{\rm +44}_{-40}$)    &
0.193$^{+19}_{-21}$$^c$&0.201$^{\rm +20}_{-22}$   \\
$R$/Subaru           & 14.658($^{\rm +55}_{-49}$)    &
0.172$^{+17}_{-18}$$^c$&$\rm 0.181^{+18}_{-19}$   \\
${\it F555W}$/HST          & 14.734($^{\rm +62}_{-54}$)           &
0.170(20)$^d$            &0.182(21)   \\
${\it F555W}$/HST          & 14.734($^{\rm +62}_{-54}$)           &
0.146(13)$^c$          &0.156(14)   \\
${\it F430W}$/HST          &14.882($^{\rm +49}_{-44}$)            &
0.146(11)$^c$          &0.160(12)   \\
\hline
\multicolumn{4}{c}{NUV} \\
${\it F342W}$/HST          & 14.944($^{\rm +47}_{-43}$)           &
0.201(10)$^c$          &0.224(11)   \\
${\it F25SRF}$/HST       & 15.116($^{\rm +122}_{-95}$)         
&0.261(26)$^d$     &  0.315(31) \\
{\it F195W}/HST          & 15.104($^{\rm +159}_{-39}$)           &
0.288(30)$^c$          &0.344(36)  \\
\hline
\multicolumn{4}{c}{FUV} \\
$G140L$/HST         & 15.322(84)            &0.455(29)$^d$  
     & 0.546(35) \\      
\hline
\end{tabular}}
\par
\smallskip
$^a$~$E(B-V)=0.023$;   $^b$~Harlow \etal~(\cite{Harlow});  
$^c$~this work; $^d$~Kargaltsev \etal~(\cite{Karg05}) using ACS    and STIS/MAMA NUV and FUV. 
\end{table}