\begin{table}%t1
\caption{\label{phot}Parameters of the underlying photospheres for the model construction. From
the literature we also cite [A/H] given in brackets.}
%\begin{center}
{\begin{tabular}[htbp]{cccccc}
\hline\hline
Star & Other name & Spectrum used & $T_{{\rm eff}}$ [K] & log $g$ & Literature\\
\hline
AD Leo & GJ 388 & 2002-03-16 03:40:47 & 3200 & 4.5 & 3350, 4.5 (--0.75) $^{1}$\\
YZ CMi & GJ 285 & average & 3000 & 4.5 & 2925 $^{3}$\\
CN Leo & GJ 406 & 2002-03-14 03:24:38 & 2900 & 5.5 & 2900, 5.0 (0.0) $^{1}$\\
DX Cnc & GJ 1111 & average &2700 & 5.0 & 2850, 5.25 (+0.5) $^{1}$; 2775 $^{3}$\\
LHS 3003 & GJ 3877 & average &2500 & 4.5 & 2400--2650 $^{2}$\\
\hline 
\end{tabular}}
\parbox{13cm}{
$^{1}$ \citet{Jones},  
$^{2}$ \citet{Leggett},  
$^{3}$ \citet{Mohanty}.}
%\end{center}
\end{table}