Table D.1
Observations in Lupus and Upper Sco.
| Name | M* | Age | RCO, 90% |
|---|---|---|---|
| (M⊙) | (Myr) | (AU) | |
| Lupus | |||
| Sz 65 | 0.70 ± 0.16 |  |
172 ± 24 |
| Sz 68 | 2.13 ± 0.34 |  |
68 ± 6 |
| Sz 71 | 0.42 ± 0.11 |  |
218 ± 54 |
| Sz 73 | 0.82 ± 0.16 |  |
103 ± 9 |
| Sz 75 | 0.51 ± 0.14 |  |
194 ± 21 |
| Sz 76 | 0.25 ± 0.03 |  |
164 ± 6 |
| J15560210-3 655 282 | 0.46 ± 0.12 |  |
110 ± 3 |
| IM Lup | 1.10 ± 0.0 |  |
388 ± 84 |
| Sz 84 | 0.18 ± 0.03 |  |
146 ± 18 |
| Sz 129 | 0.80 ± 0.15 |  |
140 ± 12 |
| RY Lup | 1.47 ± 0.22 |  |
250 ± 63 |
| J16000236-4 222 145 | 0.24 ± 0.03 |  |
266 ± 45 |
| MY Lup | 1.02 ± 0.13 |  |
194 ± 39 |
| EX Lup | 0.56 ± 0.14 |  |
178 ± 12 |
| Sz 133 | 0.63 ± 0.05 |  |
238 ± 66 |
| Sz 91 | 0.47 ± 0.12 |  |
450 ± 80 |
| Sz 98 | 0.74 ± 0.20 |  |
358 ± 52 |
| Sz 100 | 0.18 ± 0.03 |  |
178 ± 12 |
| J16083070-3 828 268 | 1.81 ± 0.28 |  |
394 ± 100 |
| V1094 Sco | 0.47 ± 0.14 |  |
438 ± 112 |
| Sz 111 | 0.46 ± 0.12 |  |
462 ± 96 |
| Sz 123A | 0.46 ± 0.11 |  |
146 ± 12 |
| Upper Sco | |||
| J15534211-2 049 282 |  |
(5 − 11) |  |
| J16001844-2 230 114 |  |
(5 − 11) |  |
| J16020757-2 257 467 |  |
(5 − 11) |  |
| J16035767-2 031 055 |  |
(5 − 11) |  |
| J16035793-1 942 108 |  |
(5 − 11) |  |
| J16075796-2 040 087 |  |
(5 − 11) |  |
| J16082324-1 930 009 |  |
(5 − 11) |  |
| J16123916-1 859 284 |  |
(5 − 11) |  |
| J16142029-1 906 481 |  |
(5 − 11) |  |
Notes. Stellar parameters derived from observations presented in Alcalá et al. (2014, 2017) (For the stellar age estimation, see Andrews et al. 2018). Gas radii for Lupus from Ansdell et al. (2018). Stellar masses for Upper Sco taken from Barenfeld et al. (2016). For the stellar age, the 5–11 Myr stellar age of Upper Sco is used (see, e.g. Preibisch et al. 2002; Pecaut et al. 2012). For sources in Upper Sco RCO, 90% were calculated from the fit to the observed 12CO intensity in Barenfeld et al. (2017).
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