\begin{table}%T9
\caption{Fundamental parameters of targets in XEST (3): Photometry and spectroscopy [first ten entries].}
%\centerline
 {
\begin{tabular}{rlrrrrrrr}
\hline
\hline\\[-3.2mm]
XEST & Name & Spec$^a$  & Refs. & $A_{\rm V}^a$ & $A_{J}$  & $T_{\rm eff}^a$ &  $L_*^b$        & Refs.	\\
     &      &		 &	& (mag)        & (mag)   &  (K) 	   & ($L_{\odot})$     &	\\
\hline
27-115 &  HBC 352	    & G0	&   27      &	     0.87 &  0.25 &	   6030 &		0.740 &   27	       \\
27-000 &  HBC 353	    & G5	&   27      &	     0.97 &  0.28 &	   5770 &		0.500 &   27	       \\
06-005 &  HBC 358 AB	    & M2	&   27      &	     0.21 &  0.06 &	   3580 &		0.280 &   27	       \\
06-007 &  HBC 359	    & M2	&   27      &	     0.49 &  0.14 &	   3580 &		0.260 &   27	       \\
06-059 &  L1489 IRS	    & K4	&   59      &	    10.20 &   ... &	   4500 &		4.900 &   10, 59       \\
20-001 &  LkCa 1	    & M4	&    5      &	     0.00 &  0.00 &	   3270 &		0.380 &    5, 27       \\
20-005 &  Anon 1	    & M0	&    5      &	     1.32 &  1.03 &	   3850 &		2.600 &    5, 27       \\
20-000 &  IRAS 04108+2803 A & ...	&  ...      &	      ... &   ... &	    ... &		  ... &   ...	       \\
20-022 &  IRAS 04108+2803 B & ...	&  ...      &	      ... &   ... &	   3500 &		0.400 &   10	       \\
20-000 &  2M J04141188+28   & M6.25	&   33      &	      ... &  0.28 &	   2962 &		0.015 &   33	       \\
\hline
\end{tabular}}
\smallskip
$^a$ For multiples, first number or spectral type refers to primary, second to secondary component.\\
$^b$ For multiples, three numbers give primary/secondary/total system luminosity.\\
$^c$ Referring to $L_{\rm bol}$ as derived from integration of the optical and infrared spectrum.\\
\end{table}