\begin{table}%t2   
\caption{Spot configuration for VY~Ari.  The stellar parameters used in the solution are:
unspotted effective temperature, $T_{\rm max}$~= 4916~K; limb-darkening coefficients at~$V$ and
at~6200~\AA, $\mu_{\rm V}$~= 0.77, $\mu_{6200}$~= 0.63; inclination, $i$~= 65$^{\circ}$.}
\label{tab:parameters_vy}
%\centerline
{
\begin{tabular}{lcrccc}
\hline
\hline
 \noalign{\smallskip}
 Model  &    Radius  &  Lon.$^{a}$  &   Lat.  &  $\frac{T_{\rm sp}}{T_{\rm ph}}$ &
  $A_{\rm rel}$$^{b}$ \\
    \noalign{\smallskip}
\hline
 Planck   & 28$\fdg$0	&  355$\degr$  &  35$\degr$  & 0.786 $\pm$ 0.016 & 0.135 $\pm$ 0.012 \\
  "  "    & 31$\fdg$8	&   90$\degr$  &  35$\degr$  & 0.786 $\pm$ 0.016 &	             \\
 Kurucz   & 29$\fdg$5	&  355$\degr$  &  35$\degr$  & 0.830 $\pm$ 0.024 & 0.144 $\pm$ 0.013  \\
  "  "    & 32$\fdg$5	&   90$\degr$  &  35$\degr$  & 0.830 $\pm$ 0.024 &	             \\
 NextG    & 28$\fdg$7	&  355$\degr$  &  35$\degr$  & 0.840 $\pm$ 0.018 &  0.147 $\pm$ 0.015  \\
  "  "    & 34$\fdg$1	&   90$\degr$  &  35$\degr$  & 0.840 $\pm$ 0.018 &	             \\
\hline
\end{tabular}}
\medskip
$^{a}$ Longitude increases with phase, and 0$\degr$ longitude
corresponds to phase~0$\fp$0. \\
$^{b}$ Total fractional area of the two spots in units of the star surface. 
\end{table}