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Table B.1

12CO and 13CO fluxes and 3σ upper limits,distances (Gaia Collaboration 2018), stellar luminosity, and stellar mass (calculated using the evolutionary tracks by Baraffe et al. 2015; Alcalá et al. 2017) for the sources in the studied subsample of faint Lupus disks.

Source d L M
(mJy km s−1) (mJy km s−1) (pc) L M
Sz77 350.0 ±80.0 <69.0 155 0.59 1.09
Sz114 <85.2 <87.0 162 0.21 0.21
J16100133-3906449 <84.0 <90.0 193 0.19
J16080175-3912316 <81.9 <87.0 159 (b)
J16121120-3832197 <87.3 <90.0 159 (b)
Sz90 577.0 ± 88.0 (a) <87.0 160 0.42 1.03
J16104536-3854547 <87.0 <87.0 159 (b)
J16134410-3736462 <85.5 <84.0 159 0.04 0.15
Sz88A <83.4 <84.0 158 0.31 0.87
Sz106 <86.7 <90.0 162 0.06 0.59
J16085324-3914401 322.0 ± 67.0 (a) <87.0 168 0.21 0.38
J16101857-3836125 <85.5 <90.0 159 (b) 0.04 0.14
Sz123A <90.0 <90.0 159 0.13 0.65
J16002612-4153553 <84.6 <90.0 164 0.08 0.14
Sz95 <86.1 <87.0 158 0.26 0.40
Sz96 221.0 ± 55.0 <87.0 157 0.42 0.75
Sz117 <85.2 <87.0 159 0.28 0.35
J16000060-4221567 <85.2 <87.0 161 0.10 0.22
Sz131 367.0 ± 57.0 (a) <90.0 160 0.15 0.36
Sz72 240.0 ± 31.0 (a) <90.0 156 0.27 0.54
Sz123B <89.1 <84.0 159 0.03 0.45
Sz66 373.0 ± 84.0 <87.0 157 0.22 0.38
J16085529-3848481 <87.0 <87.0 158 0.05 0.08
Sz74 <66.0 <87.0 159 1.16
J16101307-3846165 <82.8 <87.0 159 (b)
Sz97 <83.7 <87.0 157 0.11 0.25
Sz99 <87.3 <87.0 159 0.05 0.23
Sz103 <84.3 <90.0 160 0.12 0.26
J16084940-3905393 <86.1 <87.0 159
Sz110 <88.5 <93.0 159 0.18 0.28
Sz113 <84.3 <90.0 163 0.04 0.17
Sz115 <85.8 <90.0 158 0.11 0.22
Sz88B <84.3 <87.0 159 0.07 0.21
J15592523-4235066 <87.0 <84.0 159 (b) 0.02 0.12
J16081497-3857145 343.0 ± 56.0 <87.0 158 0.01 0.09
J15445789-3423392 <85.5 <90.0 159 (b)
Sz104 <84.3 <87.0 166 0.07 0.17
Sz112 <84.3 <90.0 160 0.12 0.18
J16115979-3823383 <87.3 <84.0 159 (b)
J16073773-3921388 <86.1 <90.0 174
J16080017-3902595 <85.8 <87.0 159
J160828.1-391310 <86.4 <87.0 159 (b)
Sz108B <86.1 <87.0 169 0.11 0.1
J16085373-3914367 <88.5 <84.0 159 0.10
Sz81A <89.2 <87.0 160 0.25 0.26
J16101984-3836065 <85.8 <87.0 158 0.04 0.08
J16095628-3859518 83.0 ± 25.0 <90.0 157
J15430131-3409153 <207.0 <87.0 159 (b)
J15430227-3444059 <85.5 <87.0 159 (b)
J15450634-3417378 303.0 ± 64.0 (a) <87.0 154
J16075475-3915446 <84.6 <90.0 153
J160831.1-385600 <86.4 <87.0 159 (b)
J16085828-3907355 <87.0 <90.0 159 (b)
J16085834-3907491 <88.5 <87.0 159 (b)
J16091644-3904438 <92.4 <87.0 159 (b)
J160918.1-390453 <136.5 <84.0 159 (b)
J16092032-3904015 <28.7 <90.0 159 (b)
J16092317-3904074 <86.1 <90.0 159 (b)
J160934.2-391513 <86.7 <90.0 159 (b)
J16093928-3904316 <85.2 <90.0 159 (b)
J16102741-3902299 <87.6 <87.0 159 (b)
J16120445-3809589 <85.8 <87.0 159 (b)
V856Sco <85.2 <87.0 159 (b)

Notes. (a) By visual inspection of the spectra published by Ansdell et al. (2018), 12CO line seems partially absorbed by the cloud. (b) No distance has been measured by Gaia DR2 (Gaia Collaboration 2018). The distance is therefore calculated as the median of the Gaia DR2 distances measured for the other sources in this Lupus subsample.

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