\begin{table}%T2
\caption{\label{tbl:hsnew}Analysis for eight stars from the HS survey, not included in
\citet{edelmann03}. }
\small%\centering
\par
\begin{tabular}{lclccc} 
\hline\hline\noalign{\smallskip}
Name & \mpg & Class & \teff & \logg & \logy \\
     & mag  &       & kK    & dex   & dex   \\
     \hline
     \multicolumn{6}{l}{Observed with CA/\twin} \\
\object{HS~1733+4540}         & 15.1 & sdOB & 37.5 & 5.6 & $-$3.0 \\
\object{HS~1909+7004}         & 15.4 & sdB  & 36.5 & 5.4 & $-$2.9 \\ 
\multicolumn{6}{l}{Spectra courtesy of \citet{YAS_PhD}} \\
\object{HS~0026+0439}\tablefootmark{1}     & 14.8 & sdB  & 36.7 & 5.8 & $-$3.0 \\
\object{HS~0042+0927}\tablefootmark{1}     & 16.0 & sdB  & 30.2 & 5.6 & $-$2.9 \\
\object{HS~2254+0640}\tablefootmark{1}     & 15.2 & sdB  & 29.1 & 5.6 & $-$2.7 \\
\object{HS~2320+0840}\tablefootmark{1,2} & 14.6 & sdB+ & 30.0 & 5.8 & $-$2.6 \\
\object{HS~2323+0459}\tablefootmark{1}     & 14.8 & sdB  & 29.3 & 5.4 & $-$2.8 \\
\object{HS~2334+0144}         & 15.5 & sdB  & 30.8 & 5.6 & $-$2.6 \\ 
\hline 
\end{tabular}
\tablefoot{\mpg\ gives the photographic magnitude from the HS survey plates,
``Class'' our spectroscopic classification, followed by the
effective temperature (\teff), surface gravity (\logg), and
atmospheric helium abundance ($\log y$~=~\lheh), from our model fits.
The sdB+ classification indicates a composite spectrum. The notes on
the names imply:
\tablefoottext{1}{Also found in the PG survey \citep{pgcat}.}\\
\tablefoottext{2}{Also found in the KUV survey \citep{kuv}.}}
\end{table}