\begin{table}%t1
 \caption{Source list of sources observed with the ATCA.}
 \label{tab: source list}
 \small%\centerline
{
  \begin{tabular}{llcclcll}
   \hline
   \hline
 & & & & & & & \\[-8pt]
   Source                       	& Cloud		& Age$^{a}$	& Spectral 		& Luminosity$^{c}$ 	& Distance$^{d}$	& When observed$^{e}$ 		& Other names$^{f}$				\\
                                	&		& (Myr)			& type$^{b}$     & ($L_\odot$)			& (pc)  		& 	        			&							\\
   \hline
   \object{SY Cha}              	& Cha I		& 3--5			& M0       		& 0.35				& $160 \pm 15$		& 2005					& IRAS 10557-7655, SZ 3, \\
   					& 		&			&			&				&			&					& HBC 565, Cha T4		\\
   \object{CR Cha}              	& Cha I		& 1--2			& K0, K2       		& 2.8				& $160 \pm 15$		& 2003$^\dagger$; 2005			& IRAS 10578-7645, SZ 6, \\
   					&		&			&			&				&			&					& HBC 244, Cha T8		\\
   \object{CS Cha}              	& Cha I		& 2--3			& K4      		& 1.3				& $160 \pm 15$		& 2003$^\dagger$; 2005			& IRAS 11011-7717, SZ 9, \\
   					&		&			&			&				&			&					& HBC 569, Cha T11		\\
   \object{DI Cha}              	& Cha I		& 3--4			& G1, G2      		& 8.9				& $160 \pm 15$		& 2005            			& IRAS 11059-7721, SZ 19, \\
   					&		&			&			&				&			&					& HBC 245, Cha T26, KG 6	\\
   \object{KG 28}               	& Cha I		& ...			& K7			& 1.1      			& $160 \pm 15$		& 2005             			& SZ 22, Cha T29					\\
   \object{Glass I}$^{g}$	& Cha I		& 2--3			& K4 			& 1.3				& $160 \pm 15$		& 2005					& IRAS 11068-7717, Cha T33, KG 39	\\
   \object{KG 49}               	& Cha I		& ...			& ...		     	& 15				& $160 \pm 15$		& 2005  				& IRAS 11072-7727, Cha IRN				\\
   \object{WW Cha}              	& Cha I		& 0.4--0.8		& K5       		& 2.2				& $160 \pm 15$		& 2003$^\dagger$; 2005  		& IRAS 11083-7618, SZ 34, \\
	&		&			&			&				&			&					& HBC 580, Cha T44		\\
   \object{XX Cha}              	& Cha I		& 10--40		& M1       		& 0.10				& $160 \pm 15$		& 2005              			& IRAS 11101-7603, SZ 39, \\
   					&		&			&			&				&			&					& HBC 586, Cha T49		\\
   \object{T Cha}               	& Isolated	& $>$$12.5$		& G2       		& 1.3				& $66^{+19}_{-12}$     	& 2003$^\dagger$; 2005              	& IRAS 11547-7904, HBC 591				\\
   \object{HT Lup}$^{h}$		& Lup I		& 0.4--0.8		& K2       		& 6.0				& $150 \pm 20$		& 2003$^\dagger$; 2005			& IRAS 15420-3408, SZ 68, HBC 248			\\
   \object{GW Lup}              	& Lup I		& 1.3--3.2		& M2       		& 0.23				& $150 \pm 20$		& 2003$^\dagger$; 2005	        	& IRAS 15435-3421, SZ 71, HBC 249			\\
   \object{IM Lup}              	& Lup II	& 0.09--0.6		& M0       		& 1.3				& $150 \pm 20$		& 2003$^\dagger$; 2005     		& IRAS 15528-3747, SZ 82, HBC 605			\\
   \object{RU Lup}              	& Lup II	& 0.04--0.5		& K7-M0    		& 2.1				& $150 \pm 20$		& 2003$^\dagger$; 2005	        	& IRAS 15534-3740, SZ 83, HBC 251			\\
   \object{HK Lup}              	& Lup III	& 0.7--1.4		& M0       		& 0.62				& $200 \pm 20$		& 2003	        			& IRAS 16050-3857, SZ 98, HBC 616			\\
   \hline
  \end{tabular}}
 \medskip
$^{a}$ Ages adopted from \citet{hughes:1994}, \citet{lawson:1996}, and \citet{vandenancker:1998}.
$^{b}$ Spectral types adopted from \citet{herbig:1972}, \citet{gauvin:1992}, \citet{hughes:1994}, \citet{alcala:1995}, \citet{vandenancker:1998}, and \citet{comeron:1999}.
$^{c}$ Luminosities adopted from \citet{hughes:1994}, \citet{lawson:1996}, \citet{chen:1997}, and \citet{vandenancker:1998}.
$^{d}$ Distances adopted from \citet{whittet:1997}, \citet{vandenancker:1998}, \and \citet{comeron:2006}.
$^{e}$ The observations marked with a~$\dagger$ were not used in the analysis.
$^{f}$ Catalogue names: KG~= [KG2001] \citep{kenyon:2001}, IRAS~= Infrared Astronomical Satellite, SZ~= Southern Zwicky \citep{rodgers:1978}, HBC~= Herbig+Bell Catalog \citep{herbig:1988}, Cha~T~= Assoc Chamaeleon~T \citep{henize:1973}.
$^{g}$ This source is a binary with a separation of $2\farcs4$; the spectrum quoted is that of component~A.
$^{h}$ This source is a binary in 2MASS $K$-band images with a~separation $<$$3\arcsec$. The spectrum quoted includes both sources.
\end{table}