Table 1:

Summary of the 3.3 mm ATCA observations.

Object				rms	Commentsb	Ref.	Other names
	(J2000)	(J2000)	(mJy)	(mJy)
AS 205A	16:11:31.4	-18:38:26.0	27.2	1.2	triple (1.5'', sb)	1	HBC 254
SR 4	16:25:56.1	-24:20:48.3	4.4	0.4			AS 206
GSS 26	16:26:10.3	-24:20:54.9	24.2	0.9
EL 20	16:26:18.9	-24:28:20.2	7.3	0.5			VSSG 1
LFAM 1	16:26:21.7	-24:22:50.8	17.5	0.6	flat spectrum	2
DoAr 24E	16:26:23.4	-24:21:00.7	8.3	0.4	binary (2.0'')	1	GSS 31
DoAr 25	16:26:23.7	-24:43:14.1	25.0	0.6			WSB 29
EL 24	16:26:24.1	-24:16:14.0	48.8	0.7			WSB 31
EL 27	16:26:45.0	-24:23:08.2	38.7	0.6			GSS 39
WL 18	16:26:49.0	-24:38:25.7	3.1	0.5	binary (3.6'')	3	GY 129
SR 24S	16:26:58.5	-24:45:37.1	26.6	0.8	flat spectrum, triple (5.2'', 0.2'')	2, 4, 5	HBC 262
SR 21	16:27:10.2	-24:19:12.9	4.2	0.4			EL 30
IRS 33a	16:27:14.5	-24:26:46.1	<1.2	0.4			GY 236
IRS 41	16:27:19.3	-24:28:44.4	6.2	1.2			WL 3
CRBR 85	16:27:24.7	-24:41:03.2	1.5	0.3	envelope	6
YLW 16c	16:27:26.5	-24:39:23.4	6.5	0.4			GY 262
GY 284a	16:27:30.8	-24:24:56.0	<1.2	0.4
IRS 49	16:27:38.3	-24:36:58.8	4.4	0.4			GY 308
DoAr 33	16:27:39.0	-23:58:19.1	3.7	0.3			WSB 53
WSB 52	16:27:39.5	-24:39:15.9	10.2	0.5			GY 314
IRS 51	16:27:39.8	-24:43:15.0	12.7	0.8	binary (1.6'')	3	GY 315
WSB 60	16:28:16.5	-24:36:58.0	15.3	0.5			YLW 58
SR 13	16:28:45.3	-24:28:19.2	10.0	0.6	binary (0.4'')	3	HBC 266
DoAr 44	16:31:33.5	-24:27:37.7	10.4	0.5			HBC 268
RNO 90	16:34:09.2	-15:48:16.9	7.6	0.5			HBC 649
Wa Oph 6	16:48:45.6	-14:16:36.0	10.3	0.4			HBC 653
AS 209	16:49:15.3	-14:22:08.6	17.5	0.5			HBC 270

Notes. ^(a) For this undetected source the (,) coordinates are from 2MASS (Cutri et al. 2003).
^(b) Reason why the source has not been considered in the analysis (see Sect. 3.1); enclosed in parenthesis there are the angular separation(s) between the stellar companions (``sb''= spectroscopic companion).

References. (1) McCabe et al. (2006); (2) Andrews & Williams (2007a); (3) Ratzka et al. (2005); (4) Reipurth & Zinnecker (1993); (5) Simon et al. (1995); (6) McClure et al. (2010).