Table 1
Stellar properties, outer disc inclination, and dust cavity radius of the disc sample studied in this work.
| Object | d (pc) | Spectral type | Teff (K) | L(L⊙) | M* (M⊙) | i (°) | Classification | Dust cavity (au) | Ref.(a) |
|---|---|---|---|---|---|---|---|---|---|
| AA Tau | 137 | K7 | 4350 | 1.1 | 0.68 | 59 | TTS | 44 | 1 |
| AB Aur | 163 | A0 | 9520 | 65.1 | 2.56 | 23 | Herbig | 156 | 1 |
| CQ Tau | 163 | F2 | 6890 | 10.0 | 1.63 | 35 | Herbig | 50 | 1 |
| CS Cha | 176 | K2 | 4780 | 1.9 | 1.4 | 8 | TTS | 37 | 1 |
| DM Tau | 145 | M2 | 3580 | 0.2 | 0.39 | 35 | TTS | 25 | 1 |
| DoAr 44 | 146 | K2 | 4780 | 1.9 | 1.4 | 20 | TTS | 40 | 1 |
| GG Tau | 140 | K7+M0 | 4060 | 1.6 | 0.66 | 36 | TTS | 224 | 1 |
| GM Aur | 160 | K5 | 4350 | 1.0 | 1.01 | 53 | TTS | 40 | 1 |
| HD 100453 | 104 | F0 | 7200 | 6.2 | 1.47 | 30 | Herbig | 30 | 1 |
| HD 100546 | 110 | A0 | 9520 | 25.0 | 2.13 | 42 | Herbig | 27 | 1 |
| HD 135344B | 136 | F5 | 6440 | 6.7 | 1.51 | 12 | Herbig | 52 | 1 |
| HD 139614 | 134 | A9 | 7750 | 6.0 | 1.57 | 18 | Herbig | – | |
| HD 142527 | 157 | F6+M5/M6 | 6360 | 9.9 | 1.69+0.26 | 27 | Herbig | 185 | 1,3 |
| HD 169142 | 114 | A5 | 8200 | 8.0 | 1.65 | 12 | Herbig | 26 | 1 |
| HD 34282 | 312 | A0 | 9520 | 10.8 | 2.11 | 59 | Herbig | 87 | 1 |
| HD 97048 | 185 | A0 | 9520 | 30.0 | 2.17 | 41 | Herbig | 63 | 1 |
| HP Cha | 160 | K7 | 4060 | 2.4 | 0.95 | 37 | TTS | 50 | 1 |
| IP Tau | 131 | M0 | 3850 | 0.6 | 0.54 | 45 | TTS | 25 | 1 |
| IRS 48 | 134 | A0 | 9520 | 17.8 | 1.96 | 50 | Herbig | 83 | 1 |
| J1604.3-2130 | 150 | K3 | 4780 | 0.7 | 1.1 | 6 | TTS | 87 | 1 |
| LkCa 15 | 159 | K2 | 4730 | 1.3 | 1.32 | 55 | TTS | 76 | 1 |
| MWC 758 | 160 | A7 | 7850 | 14.0 | 1.77 | 21 | Herbig | 62 | 1 |
| PDS 70 | 113 | K7 | 4060 | 0.3 | 0.8 | 52 | TTS | 74 | 1 |
| PDS 99 | 155 | K6 | 4205 | 1.1 | 0.88 | 55 | TTS | 56 | 1 |
| RXJ1615.3-3255 | 156 | K7 | 4100 | 0.6 | 0.73 | 47 | TTS | – | |
| RXJ1852.3-3700 | 146 | K2 | 4780 | 0.6 | 1.05 | 30 | TTS | 49 | 1 |
| RY Lup | 159 | K2 | 4780 | 1.9 | 1.4 | 67 | TTS | 69 | 1 |
| RY Tau | 175 | G2 | 5860 | 15.0 | 2.25 | 65 | TTS | 27 | 1 |
| SR 21 | 138 | G4 | 5770 | 11.0 | 2.12 | 16 | TTS | 56 | 1 |
| Sz 91 | 159 | M1 | 3850 | 0.2 | 0.54 | 45 | TTS | 86 | 1 |
| SZ Cha | 190 | K2 | 5100 | 1.7 | 1.45 | 47 | TTS | – | |
| T Cha | 107 | G8 | 5570 | 1.3 | 1.12 | 73 | TTS | 34 | 1 |
| TW Hya | 60 | K7 | 4205 | 0.3 | 0.81 | 7 | TTS | 2 | 1 |
| UX Tau A | 140 | G8 | 5570 | 2.5 | 1.4 | 40 | TTS | 31 | 1 |
| V1247 Ori | 400 | F0 | 7200 | 15.0 | 1.82 | 30 | Herbig | 64 | 1 |
| V4046 Sgr | 72 | K7+K5 | 4060 | 0.5 | 0.9+0.85 | 34 | TTS | 31 | 1,4 |
Notes. (a)Unless indicated otherwise, data for spectral type, distance, effective temperature, stellar luminosity, stellar mass and disc inclination are taken from (1) Francis & van der Marel (2020) where all original references for the spectral type can be found. The distances are according to Gaia Collaboration (2018). (2) Bohn et al. (2022), (3) Claudi et al. (2019), (4) Rosenfeld et al. (2012). The radius of the dust cavity was determined by Francis & van der Marel (2020).
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