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Table 1

Dust masses and optical depths for a subsample of 28 Lupus disks.

Source Dust mass (M) τ
J16124373-3815031 9.82.5+20.1$\[9.8_{-2.5}^{+20.1}\]$ 0.86
Sz117 3.30.8+36.3$\[3.3_{-0.8}^{+36.3}\]$ 1.03
Sz110 6.40.0+92.6$\[6.4_{-0.0}^{+92.6}\]$ 0.75
J16134410-3736462 2.01.6+19.4$\[2.0_{-1.6}^{+19.4}\]$ 5.00
J16080017-3902595 1.50.4+2.1$\[1.5_{-0.4}^{+2.1}\]$ 1.40
Sz95 0.80.2+1.0$\[0.8_{-0.2}^{+1.0}\]$ 0.67
J16073773-3921388 0.60.1+0.2$\[0.6_{-0.1}^{+0.2}\]$ 0.31
J16085324-3914401 10.54.5+1030.6$\[10.5_{-4.5}^{+1030.6}\]$ 1.93
Sz97 1.70.6+176.7$\[1.7_{-0.6}^{+176.7}\]$ 1.56
Sz77 0.80.2+0.0$\[0.8_{-0.2}^{+0.0}\]$ 1.03
Sz106 0.40.1+2.4$\[0.4_{-0.1}^{+2.4}\]$ 0.54
V1192Sco 1.20.0+0.0$\[1.2_{-0.0}^{+0.0}\]$ 1.07
Sz81B 0.80.0+1.1$\[0.8_{-0.0}^{+1.1}\]$ 0.72
J15592523-4235066 0.30.0+0.6$\[0.3_{-0.0}^{+0.6}\]$ 1.07
Sz108B 14.93.9+961.3$\[14.9_{-3.9}^{+961.3}\]$ 0.87
J16092697-3836269 1.30.3+1.0$\[1.3_{-0.3}^{+1.0}\]$ 0.28
Sz72 17.812.6+47.3$\[17.8_{-12.6}^{+47.3}\]$ 4.63
Sz90 4.80.9+4.2$\[4.8_{-0.9}^{+4.2}\]$ 0.41
Sz96 0.50.1+0.4$\[0.5_{-0.1}^{+0.4}\]$ 0.31
Sz131 2.70.6+0.0$\[2.7_{-0.6}^{+0.0}\]$ 0.55
Sz66 5.40.0+2.0$\[5.4_{-0.0}^{+2.0}\]$ 0.56
Sz65 20.64.9+6.1$\[20.6_{-4.9}^{+6.1}\]$ 0.51
Sz76 3.40.8+0.0$\[3.4_{-0.8}^{+0.0}\]$ 0.23
Sz103 4.71.1+13.3$\[4.7_{-1.1}^{+13.3}\]$ 0.52
J16081497-3857145 10.72.8+6.3$\[10.7_{-2.8}^{+6.3}\]$ 0.51
Sz73 11.42.1+3.8$\[11.4_{-2.1}^{+3.8}\]$ 0.27
GQLup 20.90.0+9.1$\[20.9_{-0.0}^{+9.1}\]$ 0.87
RXJ1556.1-3655 26.36.5+15.7$\[26.3_{-6.5}^{+15.7}\]$ 0.69

Notes. These disks have radii <30 au, which fit within our model grid.

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