\begin{table}%t3
%%\centering
\par
\caption{\label{tab:totlc}Light-curve data of the \object{GRB~060908} afterglow obtained by our collaboration.} 
\tiny \begin{tabular}{crrcc} 
\hline  \hline \noalign{\smallskip}
Band & $T-T_0$ & Bin half size & Magnitude & Telescope\\
 &  (s) &  (s) &  \\
\hline 
$U$ & 778 & 125 & $17.05 \pm 0.18$ & UVOT \\
$B$ & 2522 & 22.5 & $19.10 \pm 0.20$ & SMARTS \\
$V$ & 84 & 2.5 & $14.87 \pm 0.20$ & UVOT \\ 
& 202 & 25 & $\rm 16.38 \pm 0.21$ & UVOT \\ 
& 252 & 25 & $16.37 \pm 0.15$ & UVOT \\ 
& 302 & 25 & $16.52 \pm 0.17$ & UVOT \\ 
& 500 & 100 & $17.34 \pm 0.17$ & UVOT \\ 
& 633 & 10 & $16.88 \pm 0.26$ & REM \\
& 783 & 10 & $17.50 \pm 0.42$ & REM \\
& 1034 & 30 & $17.71 \pm 0.29$ & REM \\
& 1063 & 250 & $18.28 \pm 0.35$ & UVOT \\ 
& 1385 & 30 & $18.04 \pm 0.35$ & REM \\
& 2522 & 15 & $18.90 \pm 0.30$ & SMARTS \\
& 1~278~472 & 2100  & $25.04 \pm 0.10$ & NOT \\
$R$ & 61 & 5 & $14.02 \pm 0.04$ & REM \\
& 80 & 5 & $14.43 \pm 0.06$ & REM  \\
& 100 & 5 & $14.83 \pm 0.06$ & REM  \\
& 119 & 5 & $15.00 \pm 0.08$ & REM  \\
& 138 & 5 & $15.38 \pm 0.10$ & REM  \\
& 157 & 5 & $15.48 \pm 0.12$ & REM  \\
& 176 & 5 & $15.60 \pm 0.12$ & REM  \\
& 195 & 5 & $15.73 \pm 0.12$ & REM  \\
& 214 & 5 & $15.74 \pm 0.13$ & REM  \\
& 233 & 5 & $15.71 \pm 0.14$ & REM  \\
& 248 & 10 & $16.14 \pm 0.14$ & REM  \\
& 277 & 10 & $16.25 \pm 0.15$ & REM  \\
& 306 & 10 & $16.32 \pm 0.16$ & REM  \\
& 336 & 10 & $16.35 \pm 0.16$ & REM  \\
& 365 & 10 & $16.63 \pm 0.21$ & REM  \\
& 394 & 10 & $16.67 \pm 0.20$ & REM  \\
& 423 & 10 & $16.63 \pm 0.18$ & REM  \\
& 452 & 10 & $16.58 \pm 0.20$ & REM  \\
& 481 & 10 & $16.73 \pm 0.21$ & REM  \\
& 510 & 10 & $16.93 \pm 0.26$ & REM  \\
& 542 & 10 & $17.11 \pm 0.25$ & REM  \\
& 571 & 10 & $16.95 \pm 0.23$ & REM  \\
& 601 & 10 & $17.34 \pm 0.34$ & REM  \\
& 695 & 10 & $17.08 \pm 0.28$ & REM  \\
& 724 & 10 & $17.48 \pm 0.36$ & REM  \\
& 753 & 10 & $17.36 \pm 0.33$ & REM  \\
& 825 & 30 & $17.65 \pm 0.27$ & REM  \\
& 894 & 30 & $17.49 \pm 0.24$ & REM  \\
& 964 & 30 & $17.64 \pm 0.27$ & REM \\
& 1211 & 65 & $18.36 \pm 0.36$ & REM  \\
& 1420 & 136 & $18.37 \pm 0.34$ & REM  \\
& 2177 & 30 & $18.36 \pm 0.07$ & Danish \\ 
& 2461 & 30 & $18.56 \pm 0.06$ & Danish \\ 
& 2522 & 15 & $18.70 \pm 0.10$ & SMARTS \\
& 2652 & 60 & $18.72 \pm 0.06$ & Danish  \\ 
& 2864 & 25 & $18.29 \pm 0.40$ & REM  \\
& 2874 & 60 & $18.79 \pm 0.06$ & Danish \\ 
& 3100 & 201 & $18.77 \pm 0.40$ & REM  \\
& 3125 & 90 & $18.86 \pm 0.06$ & Danish \\ 
& 3402 & 90 & $19.00 \pm 0.06$ & Danish \\ 
& 3683 & 90 & $19.06 \pm 0.06$ & Danish \\ 
& 3787 & 334 & $19.03 \pm 0.43$ & REM  \\
& 4018 & 120 & $19.02 \pm 0.05$ & Danish \\ 
& 82~747 & 7317 & $22.83 \pm 0.16$ & Danish \\ 
& 1~113~287 & 2400 & $25.00 \pm 0.20$ & NOT \\
& 34~343~882 & 2865 & $25.63 \pm 0.25$ & TNG \\
$I$ & 740 & 85 & $17.17 \pm 0.37$  & REM   \\
& 1105 & 30 & $17.52 \pm 0.34$ & REM   \\
& 1456 & 30 & $17.55 \pm 0.32$ & REM   \\
& 2522 & 22.5 & $18.40 \pm 0.10$ & SMARTS \\
$J$ & 9819 & 405 & $19.22 \pm 0.06$  & UKIRT \\
$H$ & 10~039 & 405 & $18.65 \pm 0.08$ & UKIRT  \\
$K$ & 8586 & 520 & $17.80 \pm 0.03$ & UKIRT \\
White & 100 & 5 & $15.23 \pm 0.11$ & UVOT \\
& 110 & 5 & $15.44 \pm 0.10$ & UVOT \\ 
& 120 & 5 & $15.60 \pm 0.10$ & UVOT \\ 
& 130 & 5 & $15.67 \pm 0.10$ & UVOT \\
& 140 & 5 & $15.69 \pm 0.10$ & UVOT \\ 
\hline
& 150 & 5 & $15.76 \pm 0.10$ & UVOT \\ 
& 160 & 5 & $15.92 \pm 0.11$ & UVOT \\ 
& 170 & 5 & $15.94 \pm 0.10$ & UVOT \\ 
& 180 & 5 & $16.06 \pm 0.11$ & UVOT \\ 
& 190 & 5 & $16.28 \pm 0.12$ & UVOT \\ 
& 720 & 25 & $17.57 \pm 0.30$ & UVOT \\ 
& 820 & 25 & $17.58 \pm 0.33$ & UVOT \\ 
\hline
\end{tabular}
\tablefoot{The time delay from the burst was updated as $T_0 = T_{\rm BAT}-12.96$~s (see Sect.~\ref{sec:databat}). Galactic extinction has not been removed from these data.}
\end{table}