\begin{table}%t6
\par
\caption{\label{tab:memK_spec}Li absorption and H$\alpha$ infilling.}
%\centerline
 {\tiny
\begin{tabular}{lcccccccccc}
\hline\hline\\[-2.8mm]
Object&$T_{\rm eff}$&$W^{\rm int}_{\rm Li}$&$W^{\rm fit}_{\rm Li}$&$W^{\rm KS05}_{\rm Li}$&$\log N^{\rm cog}_{\rm LTE}({\rm Li})$&$\log N^{\rm cog}_{\rm NLTE}({\rm Li})$&$\log N^{\rm fit}_{\rm LTE}({\rm Li})$&$\log N^{\rm KS05}_{\rm LTE}({\rm Li})$&\multicolumn{1}{c}{H$\alpha$ core}&\multicolumn{1}{c}{$F_{\rm H\alpha}$ [$10^5$~erg~cm$^{-2}$~s$^{-1}$]}\\[0.5mm]
&[K]&[m{\AA}]&[m{\AA}]&[m{\AA}]&&&&&\multicolumn{1}{c}{[\%]}&\\
\hline
\multicolumn{8}{l}{\it M01k}\\[1mm]
\object{HD~11131}       & 5796$^c$&   70.5 $\pm$  1.9& 71.2&78.0&2.47 $\pm$ 0.06&2.46 $\pm$ 0.06&2.58 $\pm$ 0.10&2.38 $\pm$ 0.04&29$^c$&10.87\\
\object{HD~24916 A}     & 4600$^b$& $<$8.0 $\pm$  3.0&     &    &             &             &             &             &33    &1.08\\
\object{HD~26923}       & 5975$^c$&   88.0 $\pm$  2.1& 88.9&84.3&2.77 $\pm$ 0.07&2.72 $\pm$ 0.06&2.83 $\pm$ 0.09&2.69 $\pm$ 0.03&25$^c$&9.02\\
\object{HD~38393}       & 6310&       65.3 $\pm$  0.7& 63.5&58.5&2.87 $\pm$ 0.05&2.81 $\pm$ 0.04&2.96 $\pm$ 0.09&2.82 $\pm$ 0.03&17    &0.33\\
\object{HD~41593}       & 5278$^c$&   14.0 $\pm$  3.9& 15.8&    &1.17 $\pm$ 0.16&1.29 $\pm$ 0.15&1.20 $\pm$ 0.12&             &30$^c$&8.72\\
\object{HD~238087}      & 4350$^g$&$<$20.0 $\pm$  5.0&     &    &             &             &             &             &39&--\\
\object{HD~112196}      & 6110&      109.8 $\pm$  3.1&109.5&    &3.04 $\pm$ 0.06&2.94 $\pm$ 0.05&3.09 $\pm$ 0.09&             &28&11.17\\
\object{HD~152863 A}$^a$& 4980$^e$&$<$7.0 $\pm$  5.0&     &    &             &             &             &             &17&--0.37\\
\object{HD~155674 A}    & $\lesssim$4800 &$<$9.0 $\pm$  6.0&     &    &             &             &             &             &37&11.87\\
\object{HD~155674 B}    & 3900$^f$&$<$10.0 $\pm$  2.0&     &    &             &             &             &             &39&--\\
\object{HD~167389}      & 5895&       59.7 $\pm$  2.4& 59.2&58.8&2.48 $\pm$ 0.08&2.46 $\pm$ 0.07&2.50 $\pm$ 0.10&2.41 $\pm$ 0.04&21&4.70\\
\object{HD~184960}      & 6310&       60.5 $\pm$  1.9& 60.0&61.6&2.82 $\pm$ 0.04&2.76 $\pm$ 0.04&2.90 $\pm$ 0.08&2.78 $\pm$ 0.03&17&--0.02\\
\object{HD~205435}$^a$  & 5060$^g$&$<$15.0 $\pm$  5.0&     &    &             &             &             &             &20&--0.73\\
\hline
\multicolumn{8}{l}{\it M01k, K03k}\\[1mm]
%\hline
\object{HD~238224}      & 4350$^f$&$<$11.0 $\pm$  4.0&     &    &             &             &             &             &61&--\\
\hline
\multicolumn{8}{l}{\it M01k, K03k, K03f}\\[1mm]
%\hline
\object{HD~59747}       & 5094$^c$&   35.8 $\pm$  4.4& 38  &41.0&1.39 $\pm$ 0.12&1.53 $\pm$ 0.10&1.44 $\pm$ 0.16&1.16 $\pm$ 0.07&32$^c$&9.90\\
\object{HD~109647}      & 4980&       46.0 $\pm$  5.0& 44.2&25.0&1.37 $\pm$ 0.09&1.53 $\pm$ 0.08&1.36 $\pm$ 0.11&0.49 $\pm$ 0.15&34&11.65\\
\object{HD~110463}      & 4940&       21.8 $\pm$  2.6& 23.7&18.0&0.99 $\pm$ 0.11&1.17 $\pm$ 0.10&1.05 $\pm$ 0.11&0.31 $\pm$ 0.06&32&10.03\\
\object{HD~115043}      & 5850&       94.0 $\pm$  6.0& 84.0&101&2.70 $\pm$ 0.08&2.66 $\pm$ 0.06&2.78 $\pm$ 0.11&2.61 $\pm$ 0.08&27&9.48\\
\hline
\multicolumn{8}{l}{\it K03k, K03f}\\[1mm]
%\hline
\object{HD~28495}       & 5465&       69.0 $\pm$  2.4& 72.8&71.5&2.14 $\pm$ 0.09&2.18 $\pm$ 0.07&2.21 $\pm$ 0.08&1.86 $\pm$ 0.05&42&20.43\\
\object{HD~39587}       & 5920$^c$&  103.6 $\pm$  4.4&104.7&102.8&2.83 $\pm$ 0.08&2.77 $\pm$ 0.07&2.91 $\pm$ 0.10&2.74 $\pm$ 0.02&28$^c$&11.14\\
\object{HD~71974 A}     & 5570&       68.0 $\pm$  4.0& 66.7&    &             &             &             &             &32&12.90\\
\object{HD~95650}       & 3634$^d$&$<$45.0 $\pm$  5.0&     &    &             &             &             &             &73&--\\
\object{HD~109011}      & 5000&       29.0 $\pm$  6.0& 25.9&23.4&1.19 $\pm$ 0.16&1.35 $\pm$ 0.14&1.22 $\pm$ 0.20&0.55 $\pm$ 0.04&36&12.54\\ 
\object{HD~171746 A}    & 6100&       84.9 $\pm$  3.5& 83.3&    &2.85 $\pm$ 0.08&2.79 $\pm$ 0.07&2.90 $\pm$ 0.10&             &17&10.34\\
\object{HD~171746 B}    & 6040&       50.0 $\pm$  5.0& 45.3&    &2.51 $\pm$ 0.09&2.48 $\pm$ 0.08&2.51 $\pm$ 0.11&             &27&7.26\\
\hline
\end{tabular}}
\medskip
\par
{(2)} Effective temperature is adopted from Table~\ref{tab:uma_mem_par} if available, or from other sources as indicated in the footnotes to the table.   {(3)} Equivalent width $W^{{\rm int}}_{\rm Li}$ of Li~I$~{\lambda}6707.8~{\AA}$ from direct integration of the observed profile.   {(4)} Equivalent width $W^{{\rm fit}}_{\rm Li}$ from fitting with synthetic line profiles.   {(5)}~Equivalent width $W^{{\rm KS05}}_{\rm Li}$ according to \citet{KS05}.   {(6)} Li abundance $\log N^{\rm cog}_{\rm LTE}({\rm Li})$ using $W^{{\rm int}}_{\rm Li}$ by interpolation of the curves of growth of \citet{Soderblom93a}. {(7)} After application of the non-LTE corrections of \citet{Carlsson94} ($\log N^{\rm cog}_{\rm NLTE}({\rm Li})$).   {(8)} Li abundance $\log N^{\rm fit}_{\rm LTE}({\rm Li})$ derived by fitting a synthetic profile to the observed feature.   {(9)} Li abundance $\log N^{\rm KS05}_{\rm LTE}({\rm Li})$ according to \citet{KS05}.   {(10)} Relative infilling of the core of H$\alpha$ measured according to \citetalias{Fuhrmann04}.   {(11)} Chromospheric flux $F_{\rm H\alpha}$ measured according to \citet{Lyra05}.\\
$^a$ {Giant.}
$^b$ {From \citet{Koenig06}.}
$^c$ {From \citetalias{Fuhrmann04}.}
$^d$ {From \citet{Alonso96}.}
$^e$ {From \citet{deLaverny03}.}
$^f$ {Converted from spectral type with the calibration from \citet{KH95}.}
$^g$ {From \citet{McWilliam90}.}
\vspace*{-1mm}
\end{table}