\begin{table}%t1
\caption{\label{catalog}HST photometry for SN2000ft and reference star clusters.}             
\small%\centerline
{ 
\begin{tabular}{c c c c c c c c}     
\hline\hline  \noalign{\smallskip}     
Region & ${\it {\it F330W}}$ & ${\it F547M}$ & ${\it {\it F606W}}$ & ${\it F814W}$ & 
\normalsize{$\frac{\it F547M}{\it {\it F606W}}$} & \normalsize{$\frac{\it F814W}{\it {\it F606W}}$} & 
\normalsize{$\frac{\it {\it F330W}}{\it {\it F606W}}$} \\
(1)$^a$ & (2)$^b$ & (3) & (4) & (5) & (6)$^c$ & (7) & (8) \\
\hline  \noalign{\smallskip}                  
C2 &   1.69~$\times$~10$^{-16}$ &  1.05~$\times$~10$^{-16}$ &  8.85~$\times$~10$^{-17}$ &  4.95~$\times$~10$^{-17}$ &      1.2 &      0.6 &      1.9 \\
C3 &   7.38~$\times$~10$^{-17}$ &  6.74~$\times$~10$^{-17}$ &  4.94~$\times$~10$^{-17}$ &  2.36~$\times$~10$^{-17}$ &      1.4 &      0.5 &      1.5 \\
C5 &   6.42~$\times$~10$^{-17}$ &  4.03~$\times$~10$^{-17}$ &  4.67~$\times$~10$^{-17}$ &  2.27~$\times$~10$^{-17}$ &      0.9 &      0.5&      1.4 \\
Mean & \dots & \dots & \dots & \dots & 1.1~$\pm$~0.2 & 0.51~$\pm$~0.04 & 1.6~$\pm$~0.2\\
\hline\noalign{\smallskip}
C24$^d$ &   3.54~$\times$~10$^{-17}$ & \dots &  1.60~$\times$~10$^{-17}$ &   \dots
&  \dots &   \dots &    2.2 \\
C24(fit)$^e$ & 2.90~$\times$~10$^{-17}$ & 1.97~$\times$~10$^{-17}$ & 1.63~$\times$~10$^{-17}$ & 1.01~$\times$~10$^{-17}$ & 1.2 & 0.6 & 1.8 \\
SN\_Region$^f$ & 1.48~$\times$~10$^{-17}$ & \dots & 1.43~$\times$~10$^{-17}$ & \dots & \dots & \dots & 1.0 \\
SN~2000ft$^g$ & \dots & 6.83~$\times$~10$^{-17}$ & \dots & 1.08~$\times$~10$^{-16}$ & 4.8 &
     7.6 & \dots \\
\hline                  
\end{tabular}}
\smallskip
$^a$ Cluster label after D\'iaz-Santos et~al. (2007).
$^b$  Measured fluxes in Cols.~(2) to (5) given 
in erg~s$^{-1}$~cm$^{-2}$~\AA$^{-1}$. $^c$  Flux ratios for the different regions
as obtained from the measured fluxes given in previous columns. $^d$  Photometry of the closest cluster (C24) identified at a distance of 0\farcs1 from SN~2000ft. No measurement is given for filters {\it F547M} and {\it F814W} due to its
close distance to SN~2000ft. $^e$  Flux values for the corresponding filters, obtained from the best-fitted spectral energy distribution to the cluster C24 photometry covering the ultraviolet to near-infrared range (\mbox{D\'iaz-Santos} et~al. 2007). $^f$  {\it F330W} and {\it F606W} values represent the fluxes measured
through an aperture of 0\farcs14 diameter centered at the position where SN~2000ft
is detected in the {\it F547M} and {\it F814W} images. $^g$  Photometry of SN~2000ft in {\it F547M} and {\it F814W} images taken in May 13, 2000.
\end{table}