\begin{table}%t3
\caption{Comparison of stellar parameters of $\eta$~Leo and $\beta$~Ori from the literature.}
\label{etaleoparams}
%\centering
$$
\begin{tabular}{lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lll}
\hline\hline
Source & \multicolumn{2}{c}{$T_{\rm eff}$~(K)} & \multicolumn{2}{c}{$\log g$~(cgs)} & \multicolumn{2}{c}{$\xi$~(km~s$^{-1}$)} & Method & Notes\\
\hline
\\[-3mm]
\multicolumn{9}{c}{      {\it HD~87737}    }\\[1mm]
This work & 9600 & 150 & 2.00 & 0.15 & 4 & 1 & NLTE \ion{H}{i}, \ion{N}{i/ii}, \ion{Mg}{i/ii}, (\ion{C}{i/ii}), & {\ldots}\\
& \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & spectrophotometry & \\
Venn~(\cite{Venn95a}) & 9700 & 200 & 2.0 & 0.2 & 4 & 1 & H$\gamma$, NLTE \ion{Mg}{i/ii} & Kurucz~(\cite{Kurucz93}) atmospheres\\ 
Lobel et~al. (\cite{Lobeletal92}) & 10~200 & 370 & 1.9 & 0.4 & 5.4 & 0.7 & LTE \ion{Fe}{i/ii} & Kurucz~(\cite{Kurucz79}) atmospheres,\\
& \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & & equivalent widths from Wolf~(\cite{Wolf71})\\
Lambert et~al. (\cite{Lambertetal88}) & \multicolumn{2}{c}{10~500} & \multicolumn{2}{c}{2.2} & \multicolumn{2}{c}{{\ldots}} & Str\"omgren photometry $+$ H$\beta$ & Kurucz~(\cite{Kurucz79}) atmospheres\\
Wolf~(\cite{Wolf71}) & 10~400 & 300 & 2.05 & 0.20 & \multicolumn{2}{c}{2{\ldots}10} & Balmer lines, Balmer jump, & early LTE atmospheres, no line-\\
& \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & LTE \ion{Mg}{i/ii}, \ion{Fe}{i/ii} & blanketing, photographic spectra\\[4mm]
\multicolumn{9}{c}{{ {\it  HD~34085     }}}\\[1mm]
This work & 12~000 & 200 & 1.75 & 0.10 & 7 & 1 & NLTE \ion{H}{i}, \ion{N}{i/ii}, \ion{O}{i/ii}, \ion{S}{ii/iii}, & {\ldots}\\
& \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & spectrophotometry & \\
McErlean et~al. (\cite{McErleanetal99}) & 13~000 & 1~000 & 1.75 & 0.2 & \multicolumn{2}{c}{10} & NLTE H$\gamma$, H$\delta$, \ion{Si}{ii/iii} & Hubeny~(\cite{Hubeny88}) H$+$He NLTE models,\\
& \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & & no line-blanketing\\
Israelian et~al. (\cite{Israelianetal97}) & 13~000 & 500 & 1.6 & 0.1 &
\multicolumn{2}{c}{7} & NLTE H$\gamma$, H$\delta$, Si & Hubeny~(\cite{Hubeny88}) H$+$He NLTE models,\\
& \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{} & & no line-blanketing\\
Takeda~(\cite{Takeda94}) & 13~000 & 500 & 2.0 & 0.3 & \multicolumn{2}{c}{7} & LTE H$\gamma$, H$\delta$, spectrophotometry & Kurucz~(\cite{Kurucz79}) atmospheres\\
Stalio et~al. (\cite{Stalioetal77}) & 12~070 & 160 & \multicolumn{2}{c}{{\ldots}} &
\multicolumn{2}{c}{{\ldots}} & angular diameter, total flux & early
line-blanketed LTE atmospheres\\
\hline
\end{tabular}
$$
\end{table}