\begin{table}%t3 %\centering \par %\renewcommand{\arraystretch}{1.1} \caption{Summary of optical and ultraviolet observations. All data but the point in the $R$ band were measured by \Swift-UVOT. The {$R$-band} observations is by \citet{Tristram05}. All measurements were corrected for the Galactic extinction \citep[$A_{\rm V} = 0.123$~mag;][]{Schlegel98}, assuming the Milky Way extinction curve by \citet{Pei92}. The optical-to-X-ray spectral index is $\beta_{\rm OX} = \log(F_\nu^{\rm opt}/F_\nu^{\rm X}) / \log(\nu_{\rm X}/\nu_{\rm opt})$. The X-ray frequency was set to $\nu_{\rm X} = 1.5$~keV, the logarithmic mean of the XRT observing range. The X-ray flux was computed by interpolating the XRT light curve { to} the time of the optical limit. The last column reports the ratio of the extrapolated X-ray flux to the optical one (assuming no spectral breaks between the two bands; see Fig.~\ref{fg:SED}).\label{tab:optical}} \small %\centering \begin{tabular}{lllllllll} \hline\hline \noalign{\smallskip} Time since burst &Filter & Wavelength & Exposure time & Extinction & Magnitude & Flux density &$\beta_\mathbf{OX}$ & X-ray/optical ratio\\ (s) & &(\AA) &(s) & (mag) & &($\mu$Jy) & & \\ \hline \noalign{\smallskip} 3300 &{\it UVW2} &1930 &10 &0.29 &${>} 17.41$ &${<} 99.11$ &${<} 0.52$ &$\rm {>} 23^{+8.9}_{-6.4}$\\[2mm] 3306 &$V$ &5460 &100 &0.12 &${>} 18.66$ &${<} 107.5$ &${<} 0.45$ &$\rm {>} 65 ^{+31}_{-21}$ \\[1mm] 3350 &{\it UVM2} &2220 &100 &0.36 &${>} 18.54$ &${<} 34.17$ &${<} 0.32$ &$\rm {>} 75 ^{+30}_{-21}$ \\[1mm] 3470 &{\it UVW1} &2600 &100 &0.27 &${>} 18.75$ &${<} 27.80$ &${<} 0.29$ &$\rm {>} 103^{+43}_{-30}$ \\[1mm] 5219 &$U$ &3450 &750 &0.20 &${>} 19.65$ &${<} 11.00$ &${<} 0.24$ &$\rm {>} 176^{+77}_{-54}$ \\[1mm] 9390 &$B$ &4350 &714 &0.16 &${>} 20.87$ &${<} 17.47$ &${<} 0.46$ &$\rm {>} 52 ^{+24}_{-16}$ \\ \hline \noalign{\smallskip} 24~840 &$R_{\rm MOA}$ &6399 &600 &0.10 &${>} 20.20$ &${<} 25.70$ &${<} 0.74$ &$\rm {>} 10^{+5.0}_{-3.4}$\\ \hline \end{tabular} \end{table}