\begin{table}%t2 \caption{\label{tab:parameters}Stellar parameters, ages, and radial velocities for the sample of microlensed dwarf stars\tablefootmark{\dagger}.} \small%\centering \par \begin{tabular}{rlllccrr} \hline\hline \noalign{\smallskip} \multicolumn{1}{c}{Object} & \multicolumn{1}{c}{$T_{\rm eff}$} & \multicolumn{1}{c}{$\log g$} & \multicolumn{1}{c}{$\xi_{\rm t}$} & \multicolumn{1}{c}{[Fe/H]} & $N_{\ion{Fe}{i}}$,~~ $N_{\ion{Fe}{ii}}$ & \multicolumn{1}{c}{Age} & \multicolumn{1}{c}{$v_{\rm r}$} \\ & \multicolumn{1}{c}{$\rm [K]$} & \multicolumn{1}{c}{$\rm [cgs]$} & \multicolumn{1}{c}{$\rm [\kms]$} & & & \multicolumn{1}{c}{[Gyr]} & \multicolumn{1}{c}{[$\kms$]} \\ %\noalign{\smallskip} \hline %\noalign{\smallskip} %\multicolumn{12}{c}{\underline{\sl Microlensed dwarf stars}} \\ %\noalign{\smallskip} OGLE-2009-BLG-076S & $5877\pm96$ & $4.30\pm0.18$ & $1.61\pm0.16$ & $-0.72\pm0.07$ & \phantom{3}66,~~~ \phantom{3}7 & $11.7 \pm 1.9$ & $+128.7$ \\ MOA-2009-BLG-493S & $5457\pm98$ & $4.50\pm0.22$ & $0.83\pm0.30$ & $-0.70\pm0.14$ & \phantom{3}80,~~~ \phantom{3}5 & $ 9.1 \pm 4.0$ & $ -14.5$ \\ MOA-2009-BLG-133S & $5597\pm92$ & $4.40\pm0.27$ & $1.15\pm0.27$ & $-0.64\pm0.17$ & \phantom{3}68,~~~ \phantom{3}7 & $ 9.4 \pm 4.0$ & $ +91.6$ \\ MOA-2009-BLG-475S & $5843\pm173$ & $4.40\pm0.30$ & $1.31\pm0.31$ & $-0.54\pm0.17$ & \phantom{3}53,~~~ \phantom{3}4 & $ 9.1 \pm 3.7$ & $+137.8$ \\ MACHO-1999-BLG-022S & $5650\pm106$ & $4.05\pm0.20$ & $0.30\pm0.45$ & $-0.49\pm0.14$ & \phantom{3}97,~~~ 10 & $11.7 \pm 2.3$ & $ +37.6$ \\ OGLE-2008-BLG-209S & $5243\pm65$ & $3.82\pm0.16$ & $1.01\pm0.11$ & $-0.30\pm0.06$ & 146,~~~ 19 & $ 9.5 \pm 3.1$ & $-173.6$ \\ MOA-2009-BLG-489S & $5634\pm89$ & $4.30\pm0.18$ & $0.68\pm0.17$ & $-0.18\pm0.11$ & 114,~~~ 15 & $11.0 \pm 2.3$ & $ +96.5$ \\ MOA-2009-BLG-456S & $5700\pm93$ & $4.24\pm0.18$ & $1.00\pm0.20$ & $+0.12\pm0.09$ & \phantom{3}91,~~~ 14 & $ 7.9 \pm 1.6$ & $-164.6$ \\ OGLE-2007-BLG-514S & $5644\pm130$ & $4.10\pm0.28$ & $1.55\pm0.29$ & $+0.27\pm0.09$ & \phantom{3}49,~~~ \phantom{3}8 & $ 6.9 \pm 1.6$ & $+158.8$ \\ MOA-2009-BLG-259S & $5000\pm400$ & $4.50\pm0.50$ & $0.50\pm0.75$ & $+0.33\pm0.40$ & \phantom{3}16,~~~ \phantom{3}3 & $ 9.4 \pm 4.0$ & $ +83.2$ \\ MOA-2008-BLG-311S & $5944\pm68$ & $4.40\pm0.13$ & $1.17\pm0.12$ & $+0.36\pm0.07$ & 118,~~~ 16 & $ 2.3 \pm 1.0$ & $ -34.1$ \\ MOA-2008-BLG-310S & $5704\pm65$ & $4.30\pm0.12$ & $1.05\pm0.11$ & $+0.42\pm0.08$ & 122,~~~ 20 & $ 4.5 \pm 1.0$ & $ +77.5$ \\ OGLE-2007-BLG-349S & $5229\pm63$ & $4.18\pm0.13$ & $0.78\pm0.13$ & $+0.42\pm0.08$ & 103,~~~ 18 & $13.6 \pm 1.0$ & $+113.0$ \\ MOA-2006-BLG-099S & $5741\pm87$ & $4.47\pm0.15$ & $0.84\pm0.14$ & $+0.44\pm0.10$ & 119,~~~ 21 & $ 2.8 \pm 1.3$ & $ +99.0$ \\ OGLE-2006-BLG-265S & $5486\pm70$ & $4.24\pm0.15$ & $1.17\pm0.12$ & $+0.47\pm0.06$ & \phantom{3}92,~~~ 14 & $ 7.9 \pm 1.3$ & $-154.0$ \\ \noalign{\smallskip} \hline \end{tabular} \tablefoot{\tablefoottext{\dagger}{For the four stars analysed in \cite{bensby2009}: OGLE-2008-BLG-209S, MOA-2006-BLG-099S, OGLE-2006-BLG-265S, and OGLE-2007-BLG-349S, we have here updated the estimations of the uncertainties using the method outlined in \cite{epstein2010}.}} \end{table}