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Table F.2

Results of the interferometric model fitting.

# Name Rsub (au) Ftot (Jy) q rhl (au) χ2 qgap Rin (au) rhl, gap (au)
1 SVS 13A1 0.066 20.0 0.78
2 LkHα 330 0.20 0.29 1.1
3 RY Tau 0.30 34.4
4 T Tau N 0.21 0.78
5 T Tau S 0.23 46.7 8.4
6 DG Tau 0.097 3.3
7 Haro 6-10N 0.033 6.8 0.47
8 Haro 6-10S 0.16 4.1
10 HL Tau 0.047 0.00
12 LkCa 15 0.072 0.22
13 DR Tau 0.14 4.2
14 UY Aur B 0.034 0.00
15 UY Aur A 0.057 0.01
16 GM Aur 0.057 0.10
17 AB Aur 0.55 7.7
18 SU Aur 0.21 0.00
19 MWC 480 0.32 0.55
20 UX Ori 0.22 12.1 4.0
21 CO Ori 0.54 3.3 5.0
22 GW Ori 0.61 27.8 35.6
23 MWC 758 0.30 0.71 0.86
24 NY Ori 0.14 0.00
25 CQ Tau 0.18 0.00
26 V1247 Ori 0.27 1.3 0.09
27 V883 Ori 2.3 0.72 1.3
28 MWC 120 1.0 0.00
29 FU Ori 0.99 0.82
30 V1647 Ori 0.42 23.8 18.0
31 V900 Mon 1.4 0.00
32 Z CMa 3.9 7.2
33 V646 Pup 1.4 0.00
34 HD 72106 0.42 19.1 12.2
35 CR Cha 0.15 1.4 1.7
36 TW Hya 0.043 2.4 0.98
37 DI Cha 0.28 4.1 0.20
38 Glass I 0.12 2.6 4.3
39 Sz 32 0.25 4.3
40 WW Cha 0.17 0.93
41 CV Cha 0.19 10.8
42 DX Cha 0.47 1.9 1.7
43 DK Cha 0.58 18.4 1.0
44 HD 135344B 0.23 5.2
45 HD 139614 0.21 3.2 0.64
46 HD 141569 0.33 0.02
47 HD 142527 0.32 15.3 9.5
48 RU Lup 0.095 1.1 0.73
49 HD 143006 0.16 0.00
50 EX Lup 0.047 58.7
51 HD 144432 0.45 2.0 0.64
52 V856 Sco 0.67 4.7
53 AS 205 N 0.16 0.31
54 AS 205 S 0.097 0.26 0.20
55 DoAr 20 0.079 0.99
57 HBC 639 0.16 0.32 0.49
59 Elias 24 0.16 4.8 3.7
61 SR 24S 0.099 0.00
62 Elias 29 0.44 0.00
63 SR 21A 0.27 0.06 0.01
64 IRS 42 0.14 0.04
65 IRS 48 0.24 0.00
66 V2129 Oph 0.12 0.00
67 Haro 1-16 0.076 0.94
68 V346 Nor 0.29 18.7
69 HD 150193 0.66 23.1 25.8
70 AS 209 0.10 1.4
71 AK Sco 0.19 1.7
72 HD 163296 0.40 6.1
73 HD 169142 0.20 0.09 0.07
74 VV Ser 0.53 0.17 0.20
75 SVS20N 0.26 19.2 10.2
76 SVS20S 2.9 75.3
77 S CrA S 0.073 0.00
78 S CrA N 0.11 21.9
79 T CrA 0.11 0.00
80 VV CrA NE 0.12 4.0
81 VV CrA SW 0.075 2.5 1.2
82 HD 179218 1.2 31.0 16.3

Notes. The fit parameters Ftot, q, and rhl belong to the continuous disk model. The parameters qgap, Rin, and rhl, gap belong to the gapped disk model. We indicate χ2 values for both models.

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