Table 1: Source list of sources observed with the ATCA.
Source Cloud Agea Spectral Luminosityc Distanced When observede Other namesf
    (Myr) typeb ($L_\odot$) (pc)    
SY Cha Cha I 3-5 M0 0.35 $160 \pm 15$ 2005 IRAS 10557-7655, SZ 3,
              HBC 565, Cha T4
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
CS Cha Cha I 2-3 K4 1.3 $160 \pm 15$ 2003$^\dagger$; 2005 IRAS 11011-7717, SZ 9,
              HBC 569, Cha T11
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
KG 28 Cha I ... K7 1.1 $160 \pm 15$ 2005 SZ 22, Cha T29
Glass Ig Cha I 2-3 K4 1.3 $160 \pm 15$ 2005 IRAS 11068-7717, Cha T33, KG 39
KG 49 Cha I ... ... 15 $160 \pm 15$ 2005 IRAS 11072-7727, Cha IRN
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
XX Cha Cha I 10-40 M1 0.10 $160 \pm 15$ 2005 IRAS 11101-7603, SZ 39,
              HBC 586, Cha T49
T Cha Isolated >12.5 G2 1.3 66+19-12 2003$^\dagger$; 2005 IRAS 11547-7904, HBC 591
HT Luph Lup I 0.4-0.8 K2 6.0 $150 \pm 20$ 2003$^\dagger$; 2005 IRAS 15420-3408, SZ 68, HBC 248
GW Lup Lup I 1.3-3.2 M2 0.23 $150 \pm 20$ 2003$^\dagger$; 2005 IRAS 15435-3421, SZ 71, HBC 249
IM Lup Lup II 0.09-0.6 M0 1.3 $150 \pm 20$ 2003$^\dagger$; 2005 IRAS 15528-3747, SZ 82, HBC 605
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
HK Lup Lup III 0.7-1.4 M0 0.62 $200 \pm 20$ 2003 IRAS 16050-3857, SZ 98, HBC 616
a Ages adopted from Hughes et al. (1994), Lawson et al. (1996), and van den Ancker et al. (1998). b Spectral types adopted from Herbig & Kameswara Rao (1972), Gauvin & Strom (1992), Hughes et al. (1994), Alcala et al. (1995), van den Ancker et al. (1998), and Comerón et al. (1999). c Luminosities adopted from Hughes et al. (1994), Lawson et al. (1996), Chen et al. (1997), and van den Ancker et al. (1998). d Distances adopted from Whittet et al. (1997), van den Ancker et al. (1998), - Comerón (2006). e The observations marked with a $\dagger$ were not used in the analysis. f Catalogue names: KG = [KG2001] (Kenyon & Gómez 2001), IRAS = Infrared Astronomical Satellite, SZ = Southern Zwicky (Rodgers et al. 1978), HBC = Herbig+Bell Catalog (Herbig & Bell 1988), Cha T = Assoc Chamaeleon T (Henize & Mendoza 1973). g This source is a binary with a separation of $2\hbox{$.\!\!^{\prime\prime}$ }4$; the spectrum quoted is that of component A. h This source is a binary in 2MASS K-band images with a separation < $3\hbox{$^{\prime\prime}$ }$. The spectrum quoted includes both sources.

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