\begin{table}%t5
\caption{Results for the fit of {\tt ATLAS~9} and {\tt PHOENIX}~model
atmospheres to our interferometric VLTI/VINCI and NPOI~data sets
of $\gamma$~Sagittae.}
\label{tab:results}
%\centering
\small
\begin{tabular}{lrr}
\hline\hline
Model atmosphere & NPOI (526~nm to 852~nm)& VLTI/VINCI (2190~nm)\\\hline
{\tt ATLAS~9}, plane-parallel, $T_{\rm eff}=$ 3750~K, $\log g$~= 1.0 & 
$\Theta_{\rm LD}=6.18\pm0.06$~mas & $\Theta_{\rm LD}=6.08\pm0.02$~mas\\
& $\chi^2_\nu=2.2$  & $\chi^2_\nu=0.6$  \\[4ex]
{\tt PHOENIX}, plane-parallel, $T_{\rm eff}=3750$~K, $\log g=1.0$ &
$\Theta_{\rm LD}=6.11\pm0.06$~mas & $\Theta_{\rm LD}=6.09\pm0.02$~mas\\
& $\chi^2_\nu=2.3$ & $\chi^2_\nu=0.6$ \\[4ex]
{\tt PHOENIX}, spherical, $T_{\rm eff}=3750$~K, $\log g=1.0$, $M=1.3~M_\odot$ &
$\Theta_{\rm LD}=6.30\pm0.06$~mas & $\Theta_{\rm LD}=6.34\pm0.02$~mas\\
& $\chi^2_\nu=2.4$ & $\chi^2_\nu=0.6$ \\
&$\Theta_{\rm Ross}=6.02\pm0.06$~mas& $\Theta_{\rm Ross}=6.06\pm0.02$~mas\\
& \multicolumn{2}{c}{$\overline{\Theta_{\rm Ross}}=6.06\pm0.02$~mas}\\\hline 
\end{tabular}
\end{table}