\begin{table} %t3
\caption{\label{table:fluxratios} Model parameters for several possible configurations of the 85~Peg system
and flux ratios as measured through the MOST custom filter.} 
%\centerline
 {
\begin{tabular}{c c c c c c c}        
\hline\hline
Star 	&  $M$          	&  $R$        		&  $T_{\rm eff}$  	&	$\Delta T^{i}$ 		&	Flux ratio 	& $A_{{\rm obs}}^{ii}$ 		\\
       	& ($M_{\odot}$)		& ($R_{\odot}$) 		&  (K)            	&   ($\sigma$) 		& A/B 	& (mmag)						\\
\hline       
 A    	&  0.90            	&  0.92        		&   5460    		&	3				& 14.1        	& 4.5          			\\
 Ba  	&  0.55            	&  0.48        		&   4200         	&   0            	&				&						\\ 
 Bb   	& \ldots           	&  \ldots  		   	&   \ldots   	    &   \ldots     		&				&						\\
\hline
 A    	&  0.77            	&  0.74        		&   4845        	&	15				& 1.5 			& 0.48					\\   
 Ba  	&  0.72            	&  0.68        		&   4605          	&	2				&               &						\\ 
 Bb   	&  \ldots            &  \ldots        	&   \ldots        	&	\ldots			&               & 						\\
\hline
 A    	&  0.90           	&  0.92          	&   5460          	& 	3				& 15.2			& 4.9					\\
 Ba   	&  0.52          	&  0.46          	&   4160          	&   0.2				&				&			         \\
 Bb   	&  0.20          	&  0.21          	&   3650           	&   \ldots			&				&			            \\
\hline
 A    	&  0.77            	&  0.74        		&   4845          	&  	15				& 5.4 			& 1.7  		 	       \\   
 Ba  	&  0.52            	&  0.46        		&   4160           	&   0.2   			&				&						\\ 
 Bb   	& 0.20            	&  0.21        		&   3650           	&   \ldots			&				&						    \\
\hline               
\end{tabular}}
\medskip
\par
$^{i}$ The deviations in temperature to the observed value 
given in \citet{dantona} are given in terms of the standard deviation $\sigma$. \newline
$^{ii}$ $A_{{\rm obs}}$ indicates the observed amplitude scaled with the corresponding 
flux ratio. The expected amplitude due to backheating of star Bb on star Ba is about 0.1--0.2~mmag.
\end{table}