Table 1
Protoplanetary disks from Lupus modeled in this study.
| Object | α | δ | Lupus | Distance | SpT | Teff | AV | L⋆ | M⋆ | Notes |
|---|---|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | cloud | [pc] | [K] | [mag] | [L⊙] | [M⊙] | |||
| BDs from this survey | ||||||||||
| J154518.5-342125 | 15:45:18.53 | − 34:21:24.8 | I | 152 ± 4 | M6.5 | 2935 | 0.0 | 0.04 | 0.09 ± 0.02 | 1 |
| SONYC-Lup3-7 | 16:08:59.53 | − 38:56:27.6 | III | 150 ± 6 | M8.5 | 2600 | 0.0 | 0.01 | 0.02 ± 0.01 | 1, 4 |
| Lup706 | 16:08:37.30 | − 39:23:10.8 | III | 158.5 | M7.5 | 2795 | 0.0 | 0.002 | 0.05 ± 0.01 | 1, 3, 5 |
| AKC2006-18 | 15:41:40.82 | − 33:45:19.0 | I | 149 ± 8 | M6.5 | 2935 | 0.0 | 0.01 | 0.07 ± 0.02 | 1 |
| SONYC-Lup3-10 | 16:09:13.43 | − 38:58:04.9 | III | 158.5 | M8.8 | 2650 | 1.5 | 0.003 | 0.03 ± 0.01 | 2, 3 |
| BDs from Lupus disks survey (Ansdell et al. 2016) | ||||||||||
| Lup818s | 16:09:56.29 | − 38:59:51.7 | III | 157 ± 3 | M6 | 2990 | 0.0 | 0.02 | 0.09 ± 0.02 | 1 |
| J161019.8-383607 | 16:10:19.84 | − 38:36:06.8 | III | 159 ± 3 | M6.5 | 2935 | 0.0 | 0.04 | 0.09 ± 0.02 | 1 |
| J160855.3-384848 | 16:08:55.29 | − 38:48:48.1 | III | 158 ± 3 | M6.5 | 2935 | 0.0 | 0.05 | 0.09 ± 0.02 | 1 |
| Lup607 | 16:08:28.10 | − 39:13:10.0 | III | 175 ± 6 | M6.5 | 2935 | 0.0 | 0.05 | 0.10 ± 0.02 | 1 |
| Disks from Lupus completion survey | ||||||||||
| Sz102 | 16:08:29.71 | − 39:03:11.0 | III | 158.5 | K2 | 4900 | 0.7 | 0.01 | – | 1, 3, 5, 6 |
| V1094 Sco | 16:08:36.18 | − 39:23:02.5 | III | 154 ± 1 | K6 | 4205 | 1.7 | 1.15 | 0.86 ± 0.18 | 1 |
| GQ Lup | 15:49:12.10 | − 35:39:05.1 | I | 152 ± 1 | K6 | 4205 | 0.7 | 1.48 | 0.85 ± 0.17 | 1 |
| Sz76 | 15:49:30.74 | − 35:49:51.4 | I | 160 ± 1 | M4 | 3270 | 0.2 | 0.18 | 0.23 ± 0.04 | 1 |
| Sz77 | 15:51:46.96 | − 35:56:44.1 | I | 155 ± 1 | K7 | 4060 | 0.0 | 0.59 | 0.75 ± 0.15 | 1 |
| RXJ1556.1–3655 | 15:56:02.10 | − 36:55:28.3 | II | 158 ± 1 | M1 | 3705 | 1.0 | 0.26 | 0.5 ± 0.14 | 1 |
| EX Lup | 16:03:05.49 | − 40:18:25.4 | III | 158 ± 1 | M0 | 3850 | 1.1 | 0.76 | 0.56 ± 0.13 | 1 |
| Observed objects rejected from being members of Lupus | ||||||||||
| IRAS 15567–4141 | 16:00:07.42 | − 41:49:48.4 | – | – | – | – | – | - | − | 7 |
| J160034.4-422540 | 16:00:34.40 | − 42:25:38.6 | – | – | – | – | – | – | − | 7 |
Notes. (1) Stellar properties from Alcalá et al. (2014, 2017) and adjusted to the new Gaia DR2 parallaxes. (2) Stellar properties from Mužić et al. (2014), and adjusted to the Gaia DR2 parallaxes. (3) Gaia parallax unknown, mean distance of Lupus region considered. (4) Two sets of stellar properties (Alcalá et al. 2017; Mužić et al. 2014). (5) Subluminous object (see Alcalá et al. 2014, 2017). (6) No estimation of the stellar mass since it falls below the zero-age main sequence in the HR diagram (see Alcalá et al. 2017). (7) Categorized as background sources (Frasca et al. 2017; Alcalá et al. 2017).
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