\begin{table}%t3
  \caption{\label{tab:LDevents}Photometric temperatures and $I$-band limb-darkening coefficients of
  K Bulge giants for OGLE~2008--BLG--290 and other published
  microlensing events with source stars of similar spectral type.}
  \small
  %\centering
\par
    \begin{tabular}{lccccccc}
      \hline\hline \noalign{\smallskip}
      \multicolumn{1}{c}{Event} & \multicolumn{4}{c}{Source characteristics} &
 Measured LLDC & ATLAS LLDC \\ %\cline{2-5}
      & Type  & ${T_{\rm eff}}$ & $\logg$ & [\element{Fe}/\element{H}] & $u_I$ & $u_I$ \\
      \hline 
      EROS~2000--BLG--5   & K3~III & 4200~K & $2.3$ & $0.3$ & $0.54$\tablefootmark{a} & $0.62$ \\
      OGLE~2003--BLG--238 & K2~III & 4400~K & $2.0$ & $0.0$ & $0.58 \pm 0.06$ & $0.59$ \\
      OGLE~2004--BLG--254 & K3~III & 4500~K & $2.0$ & $0.3$ & $0.62 \pm 0.07$ & $0.59$ \\
      OGLE~2008--BLG--290 & K3~III & 4200~K & $2.5$ & $0.2$ & $0.539 \pm 0.033$ & $0.61$ \\
      \hline
    \end{tabular}
\tablefoot{\tablefoottext{a}{One-parameter fit cannot properly describe the LD profile:
see \Sec{sec:LDmeasure} for details.}} 
\end{table}