Table 1:

Source sample.

Source	RA	Dec	Dist.	Lum.	Ref.a	Notesc
	(h m s)	(d m s)	(pc)	( )
	[J2000]	[J2000]
Chamaeleon I
Ced 110 IRS 4	11 06 47.0	-77 22 32.4	150e	1	1,2,3	ISO-Cha 84
Ced 110 IRS 6	11 07 09.6	-77 23 04.3	150	0.6	1,3	ISO-Cha 92
Cha IRS 6a	11 07 09.9	-77 23 06.3	150	0.8	4	ISO-Cha 92+
Cha IRN	11 08 37.1	-77 43 51.0	150	5	3	ISO-Cha 150
Cha INa 2	11 09 36.6	-76 33 39.0	150	0.6	5
Corona australis
RCrA IRS 5	19 01 48.0	-36 57 21.6	170e	2	6,14	SMM 5
HH 100b	19 01 50.7	-36 58 10	170	15	6,14	SMM 3
RCrA IRS 7A	19 01 55.2	-36 57 21.0	170	3.3d	7,14	SMA 2, SMM 1C
RCrA IRS 7B	19 01 56.2	-36 57 27.0	170	17d	7,14	SMA 1, SMM 1B
RCrA TS 3.5	19 02 07.1	-36 53 26.2	170	-
CrA IRAS 32	19 02 58.7	-37 07 34.5	170	3.4	14	ISO-CrA 182, SMM 8
Isolated
HH 46	08 25 43.8	-51 00 35.6	450f	16	8,9,10	BHR 36
IRAS 07178-4429	07 19 21.8	-44 34 55.1	-	-	10,11	CG1/BHR 17
IRAS 12496-7650	12 53 17.2	-77 07 10.6	200g	50	12	DK Cha, Cham II
IRAS 13546-3941	13 57 42.2	-39 56 21.0	550h	-	10,11	CG12/BHR 92
IRAS 15398-3359	15 43 01.3	-34 09 15.0	130i	0.92	2,13	B228, Lupus

^a References: 1. Luhman et al. (2008); 2. Froebrich (2005); 3. Persi et al. (2000); 4. Persi et al. (2001); 5. Persi et al. (1999); 6. Nisini et al. (2005); 7. Groppi et al. (2007); 8. Noriega-Crespo et al. (2004); 9. Velusamy et al. (2007); 10. Bourke et al. (1995); 11. Santos et al. (1998); 12. van Kempen et al. (2006); 13. Evans et al. (2005); 14. Nutter et al. (2005); ^b observations of HH 100 were erronously pointed at coordinates: RA 19h01m49.1s, Dec -36d58m16.0s. See text for further discussion; ^c other names and cloud location; ^d the luminosities of the two RCrA IRS 7 sources are not well determined, due to confusion of the total integrated flux at far-IR wavelengths. The total luminosity of both sources (20 ) was used in the characterisation; ^e Knude & Høg (1998); ^f Heathcote et al. (1996); ^g Hughes & Hartigan (1992); ^h Maheswar et al. (2004); ⁱ Murphy et al. (1986).