\begin{table}%t3
%%\centering

\par
\caption{\label{table:3}Parameters deduced using the photometric temperatures and the gravities calculated using the Hipparcos parallax. Errors in $\log~{g}_{\rm Tphot}$ are from the ionisation balance using WIDTH6, whilst those in $\log ~{g}_{\rm Hipp}$ are from the errors in the Hipparcos parallax. The error in $\log ~{g}_{\rm Tphot}$ comes about from the statistical error in making sure the the abundance from different ionisation states is the same, ionisation balance.}
\small \begin{tabular} {l c c c c c c}
\hline\hline\noalign{\smallskip}
Star name& No. of \ion{Fe}{i} &$\textit{T}_{\rm phot}$ (K)	&	$\log ~{g}_{\rm Tphot}$	& [Fe/H]&	$\xi$\big(km~s$^{-1}$\big)	&	$\log~{g}_{\rm Hipp}$	\\
 &lines measured & & & & & \\
 \hline\noalign{\smallskip}
BD-13$^{\circ}$ 3442	& 86 &6210 	&	$3.77 \pm 0.04$	&	$-2.72$	&	1.30	& ...	\\
BD+20$^{\circ}$ 2030	&	98 &6200 	&	$3.985 \pm 0.04$	&	$-2.62$	&	1.20	&	...	\\
BD+24$^{\circ}$ 1676	& 96 &6170 	&	$3.68 \pm 0.04$	&	$-2.60$	&	1.40	&	...	\\
BD+26$^{\circ}$ 2621	&	107 &6150 	&	$3.88 \pm 0.10$	&	$-2.69$	&	1.20	&	$4.28 \pm 0.31$	\\
BD+26$^{\circ}$ 3578	&	126 &6150 	&	$3.72 \pm 0.08$	&	$-2.39$	&	1.35	&	$3.94 \pm 0.30$	\\
BD+3$^{\circ}$ 740	&	94 &6240 	&	$3.68 \pm 0.12$	&	$-2.77$	&	1.50	&	$4.18 \pm 0.21$	\\
BD+9$^{\circ}$ 2190	&	146 &6250 	&	$3.68 \pm 0.10$	&	$-2.84$	&	1.50	&	...	\\
CD-24$^{\circ}$ 17~504	&	69 &6070 	&	$3.57 \pm 0.30$	&	$-3.35$	&	1.30	& ...	\\
CD-33$^{\circ}$ 1173	&	126 &6250 	&	$3.87 \pm 0.10$	&	$-3.04$	&	1.50	&	$4.33 \pm 0.27$	\\
CD-35$^{\circ}$ 14~849	&	 69 &6060 	&	$3.92 \pm 0.07$	&	$-2.44$	&	1.20	&	$4.44 \pm 0.25$	\\
CD-71$^{\circ}$ 1234	&	127 &6190 	&	$3.90 \pm 0.07$	&	$-2.54$	&	1.50	&	…	\\
G64-12&	59 &	6220 	&	$4.05 \pm 0.08$	&	$-3.40$	&	1.40	& ...	\\
G64-37&	71 &	6240 	&	$4.29 \pm 0.04$	&	$-3.24$	&	1.30	& ...	\\
LP635-14&	163 &	6270 		&$3.90 \pm 0.10$	&	$-2.49$	&	1.50	& ...	\\
LP815-43&	157 &	6340 		&$3.78 \pm 0.12$	&	$-2.74$	&	1.40	&	...	\\
HD 84937	& 164	&6160 		&$3.66 \pm 0.10$	&	$-2.32$	&	1.30	&	$3.98\pm 0.12$	\\
%\hline\hline
HD 140283	&	124 &5750 	&	$3.40 \pm 0.04$	&	$-2.53$	&	1.50	&	$3.73 \pm 0.12$	\\
HD 74000	&	84 &6040 	&	$3.77 \pm 0.03$	&	$-2.19$	&	1.20	&	$4.03 \pm 0.18$	\\
\hline
Sensitivity to +100 K in $\textit{T}_{\rm phot}$&  &+0.15& & &  &$\pm$0.04\\
\hline
\end{tabular}
\end{table}