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Table 2

Best-fit disc morphologies and dust disc radii for all studied discs.

Disc name R68% [AU] R95% [AU] i [] PA [] Morphology/Model description
This Study Previous
SSTc2d J162823.3-242241 60 62 (a) 92 68.46 66.23 Inner cavity
MHO 2 49 37 (c) 66 45.54 106.25 Inner cavity
2MASS J04154278+2909597 50 39 (b) 69 33.21 174.94 Inner cavity
SSTc2d J163952.9-241931 43 31 (a) 58 81.41 106.31 Inner cavity
SU Aur 23 50 (c) 42 42.64 117.88 Inner cavity + one shoulder
HD 139614 44 67 (d) 87 0.46 −14.91 Inner cavity + one ring + one shoulder
SSTc2d J162718.4-243915 52 35 (a) 76 69.93 53.88 Inner Gaussian profile + one ring
2MASS J11160287-7624533 81 39 (e) 121 82.29 133.57 Inner Gaussian profile + one ring
2MASS J11104959-7717517 48 31 (e) 88 49.28 62.32 Inner Gaussian profile + one ring + one shoulder
SSTc2d J162145.1-234232 81 36 (a) 124 72.88 174.93 Inner Gaussian profile + one ring + one shoulder
2MASS J11094742-7726290 92 72 (e) 140 51.43 27.82 Inner Gaussian profile + two rings + one shoulder
RX J1556.1-3655 33 42 (f) 57 49.79 56.74 Inner Gaussian profile + three rings
Haro 6-37 B 98 34 (c) 150 27.95 179.98 Inner Gaussian profile + one shoulder
CY Tau 47 48 (b) 75 15.34 160.21 Inner Gaussian profile + one shoulder
MHO 1 48 26 (c) 78 39.40 83.98 Inner Gaussian profile + one shoulder
2MASS J11004022-7619280 48 36 (e) 89 16.74 −3.23 Inner Gaussian profile + two shoulders
2MASS J11111083-7641574 98 68 (e) 140 79.49 141.81 Inner Gaussian profile + two shoulders
SSTc2d J162652.0-243039 21 51 (a) 38 39.31 96.32 Compact
SSTc2d J162738.3-235732 21 <14 (a) 34 38.63 92.78 Compact
2MASS J16075796-2040087 16 <34 (g) 29 56.55 10.48 Compact
IT Tau A 21 <32 (c) 30 63.80 51.24 Compact
IT Tau B 21 <32 (c) 36 51.89 62.63 Compact
Haro 6-37 A 17 13 (c) 23 57.38 −4.48 Compact
SSTc2d J162546.6-242336 89 48 (a) 128 80.88 112.90 Highly inclined
SZ 133 59 104 (f) 87 77.18 126.10 Highly inclined

Notes. Disc morphologies and geometries were derived using Galario. Effective dust radii (R68% and R95%) were obtained using the curve-of-growth method; upper limits are indicated by ‘<’. Inclination and position angle were derived from MCMC fitting. References: (a) Cieza et al. (2019), (b) Tripathi et al. (2017), (c) Akeson et al. (2019), (d) Vioque et al. (2018), (e) Pascucci et al. (2016), (f) Ansdell et al. (2018), and (g) Barenfeld et al. (2016).

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