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Table 3:

Fluxes from point-source fits in the (u, v) plane obtained from interferometric data and single-dish 1.20-1.27 mm SEST fluxes.

Source
1.3 mma 3.2 mmb 6.8 mm SEST 1.20-1.27 mmc
  Flux rms Flux rms Flux rms Flux rms
  (mJy) (mJy/bm) (mJy) (mJy/bm) (mJy) (mJy/bm) (mJy) (mJy)

HBC 556
-- -- <3.7d 1.2 <0.7d 0.22 -- --
HBC 557 -- -- <3.2d 1.1 <0.6d 0.18 -- --
HBC 559 -- -- <2.9d 1.0 <0.3d 0.09 -- --
SZ Cha -- -- 2.3 0.4 -- -- 77.5 20.3
Sz 32 -- -- <2.9d 1.0 0.77 0.14 93.1 20.8
IK Lup 28 2.8 3.4 0.4 -- -- 56 10
Sz 66 <8d 2.8 2.2 0.4 -- -- 47 12
HM Lup <10d 3.4 -- -- -- -- <45d 15
Sz 73 a 16 2.9 -- -- -- -- 26 8
Sz 73 b 16 2.9 -- -- -- -- -- --
HN Lup 15 3.0 -- -- -- -- <51d 17
Sz 76 12 3.3 -- -- -- -- <45d 15
Sz 77 <10d 3.2 -- -- -- -- <45d 15
IM Lup 188 4.3 8.9 1.3 2.2 0.16 260 9
RY Lup 78 4.9 2.8 0.7 <0.6d 0.21 -- --
MY Lup 56 3.4 8.7 0.4 <0.6d 0.20 -- --
EX Lup 19 3.9 -- -- -- -- -- --
Sz 91 <13d 4.3 -- -- -- -- <27d 9
Sz 96 <13d 4.2 -- -- -- -- <45d 15
Sz 102 <11d 3.8 -- -- -- -- <30d 10
Sz 111 49 4.8 5.7 0.7 <0.6d 0.19 -- --
SSTc2d J161029.57-392214.7 <13d 4.4 -- -- -- -- -- --
SSTc2d J161159.81-382338.5 <13d 4.2 -- -- -- -- -- --
RX J1615.3-3255 132 3.9 6.7 0.6 <0.5d 0.17 -- --

EC 82
<15.7d 5.2 <2.9d 1.0 <0.5d 0.2 -- --
EC 90 95.7 10.4 11.5 1.2 <1.0d 0.3 -- --
EC 97 <23.3d 7.8 -- -- <0.6d 0.2 -- --
SSTc2d J182900.88+002931.5 26.4 4.9 3.4 0.5 <0.7d 0.2 -- --
IRAS 18268-0025 <15.6d 5.2 <1.9d 0.6 -- -- -- --
CoKu Ser-G3 <17.1d 5.7 <1.8d 0.6 <1.2d 0.4 -- --
SSTc2d J182858.08+001724.4 <24.6d 8.2 <1.9d 0.6 -- -- -- --
VV Ser <14.8d 4.9 <1.8d 0.6 <0.7d 0.2 -- --
SSTc2d J182850.20+000949.7 <22.8d 7.6 <1.9d 0.6 <0.6d 0.2 -- --
SSTc2d J182944.10+003356.1 <15.0d 5.0 <1.7d 0.6 -- -- -- --
SSTc2d J182936.19+004216.7 <8.7d 2.9 <2.9d 1.0 -- -- -- --
GSC 00446-00153 90.8 3.5 6.8 1.0 -- -- -- --
VV CrA 376 4.5 26.8 1.1 8.3 0.25 469, 584 21
S CrA 303 3.2 24.9 1.0 3.7 0.20 290 --
DG CrA <6.6 2.2 <2.5d 0.8 <0.5d 0.16 -- --

Notes. (a) 1 mm band observations are at 1.33 mm (SMA, Lupus and CARMA, Serpens) and at 1.35 mm (SMA, Corona Australis).
(b) 3 mm band observations are at 3.17 mm (ATCA, Lupus and Corona Australis) and at 3.15 mm (CARMA, Serpens).
(c) SEST fluxes are from Nürnberger et al. (1997, Lupus), Henning et al. (1993, Chamaeleon), and Henning et al. (1994, Corona Australis), with an adopted centre frequency of 236 GHz (1.27 mm). The values in italic are from Chini et al. (2003), with an adopted centre frequency of 250 GHz (1.20 mm). (d) Quoted value is 3$\sigma$ upper limit.


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