Table B.2:

Complete results of ATCA observations at 3 and 7 mm.

Obs. date	Effective	Target source	Continuum fluxa		rmsb	Gaussian size	RAa	Deca
	wavelength		(P)	(G)		(arcsec)	(J2000)	(J2000)
	(mm)		(mJy)		(mJy/bm)
20080712	3.18	HBC 556	<3.7c		1.2	-	8 10 31.3	-36 01 46.5
		HBC 557	<3.2c		1.1	-	8 12 47.4	-36 19 18.0
		HBC 559	<3.3c		1.1	-	8 13 56.4	-36 08 02.1
20080713	6.83	HBC 556	<0.7c		0.2	-	8 10 31.6	-36 01 46.5
		HBC 557	<0.4c		0.1	-	8 12 47.7	-36 19 18.0
		HBC 559	<0.6c		0.2	-	8 13 56.8	-36 08 02.1
20080728	6.85	HBC 559	<0.3c		0.1	-	8 13 56.8	-36 08 02.1
20080729	3.18	HBC 559	<4.3c		1.4	-	8 13 51.0	-36 08 02.1
		SZ Cha	<3.0c		1.0	-	10 58 10.0	-77 17 17.6
		Sz 32	<2.9c		1.0	-	11 09 48.0	-76 34 26.0
20080730	3.18	SZ Cha	3.4	5.8	0.5		10 58 16.6	-77 17 17.0
20080801	6.85	Sz 111	<0.6c		0.2	-	16 08 53.8	-39 37 43.1
		RY Lup	<0.6c		0.2	-	15 59 27.5	-40 21 51.2
		RX J1615.3-3255	<0.5c		0.2	-	16 15 19.4	-32 55 05.0
		VV CrA	3.4	3.4	0.2	(unresolved)	19 03 06.8	-37 12 49.3
		S CrA	3.7	5.4	0.2		19 01 08.6	-36 57 20.3
		DG CrA	<0.6c		0.2	-	19 01 54.4	-37 23 40.5
20080802	3.18	SZ Cha	<2.9c		1.0	-	10 58 15.5	-77 17 17.6
		Sz 111	5.7	-e	0.7	-	16 08 54.6	-39 37 53.3
		RY Lup	<2.3c		0.8	-	15 59 28.0	-40 21 51.2
		RX J1615.3-3255	6.8	-d	0.6	-	16 15 20.2	-32 55 05.6
		VV CrA a	31.0	-e	1.2	-e	19 03 06.8	-37 12 49.8
		VV CrA b	25.1 uniform	-e		-e	19 03 06.9	-37 12 48.3
		S CrA	22.0	-d	1.1	-	19 01 08.6	-36 57 20.2
		DG CrA	<3.0c		1.0	-	19 01 54.9	-37 23 40.5
20080803	3.18	MY Lup	8.7	-d	0.4	-	16 00 44.5	-41 55 31.2
		VV CrA a	23.0	-e	1.9	-e	19 03 06.8	-37 12 49.9
		VV CrA b	21.9	-e		-e	19 03 06.9	-37 12 48.4
		S CrA	24.9	-d	1.9	-	19 01 08.6	-36 57 20.6
		DG CrA	<4.3c		1.4	-	19 01 54.9	-37 23 40.5
20080804	3.18	Sz 65	3.4	-d	0.4	-	15 39 27.7	-34 46 17.6
		Sz 66	2.2	-d		-	15 39 28.2	-34 46 17.9
20080805	6.65	MY Lup	1.3	2.9	0.1		16 00 44.6	-41 55 31.5
		IM Lup	2.2	2.2	0.2	(unresolved)	15 56 09.2	-37 56 06.0

Notes. ^(a) Continuum flux and position are from fits in the (u, v) plane. For sources that were detected at 3, both the point-source flux (P) and the integrated flux for a Gaussian (G) are shown. For sources that were not detected, the coordinates of the phase centre are quoted.
^(b) Calculated from the cleaned image.
^(c) Quoted value is 3 upper limit.
^(d) No circular Gaussian could be fit to the source in the (u, v) plane.
^(e) The two components could not be separated with circular Gaussian fits in the (u, v) plane. One circular Gaussian was fitted to the binary, yielding a flux of 69.5 mJy and a size of 2.56  0.21 arcsec on 2 August 2008 and a flux of 44.2 mJy and a size of 2.28  0.38 arcsec on 3 August 2008.