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Table A.3.

Stellar and disk masses for the transition disks used here.

Object RA Dec Dist [pc] Mdust [M] log acc Ref
J16083070 16:08:30.68 −38:28:27.22 156 34.45 −9.32 Alcalá et al. (2017)
RYLup 15:59:28.37 −40:21:51.58 159 72.84 −8.16 Alcalá et al. (2017)
Sz111 16:08:54.67 −39:37:43.49 158 46.97 −9.47 Alcalá et al. (2014)
Sz100 16:08:25.75 −39:06:01.64 137 10.74 −9.87 Alcalá et al. (2014)
Sz118 16:09:48.64 −39:11:17.24 164 17.77 −9.21 Alcalá et al. (2017)
Sz123A 16:10:51.57 −38:53:14.10 158 10.66 −9.21 Alcalá et al. (2014)
J15583692 15:58:36.90 −22:57:15.57 166 47.26 −7.80 Manara et al. (in prep.)
J16042165 16:04:21.64 −21:30:28.98 150 42.66 −10.51 Manara et al. (in prep.)
SzCha 10:58:16.71 −77:17:17.15 190 147.41 −7.65 Manara et al. (2014)
J10563044 10:56:30.31 −77:11:39.25 183 50.94 −9.22 Manara et al. (2016b)
DoAr44 16:31:33.46 −24:27:37.52 146 50.88 −8.12 Manara et al. (2014)
HD100546 11:33:25.36 −70:11:41.27 110 152.72 −6.84 Fairlamb et al. (2015)
HD135344B 15:15:48.42 −37:09:16.33 135 110.93 −7.33 Fairlamb et al. (2015)
LkCa15 04:39:17.80 +22:21:03.22 159 144.40 −8.31 Manara et al. (2014)
SR21 16:27:10.27 −24:19:13.01 138 82.29 −7.81 Manara et al. (2014)
SR24S 16:26:58.50 −24:45:37.20 115 82.48 −7.47 Natta et al. (2006)
Sz91 16:07:11.57 −39:03:47.85 159 11.31 −9.07 Alcalá et al. (2014)
TCha 11:57:13.28 −79:21:31.72 110 35.54 −8.40 Schisano et al. (2009)
HD34282 05:16:00.48 −09:48:35.42 311 344.39 −8.30 Fairlamb et al. (2015)
CIDA1 04:14:17.62 +28:06:09.28 136 7.46 −7.92 Pinilla et al. (2018)
CQTau 05:35:58.47 +24:44:53.70 163 105.71 < −7.94 Mendigutía et al. (2011)
HD142666 15:56:40.2 −22:01:39.5 148 80.79 < −8.27 Fairlamb et al. (2015)
RYTau 04:21:57.42 +28:26:35.13 130 75.03 −7.65 Mendigutía et al. (2011)
UXTauA 04:30:04.00 +18:13:49.18 140 30.16 −8.71 Rigliaco et al. (2015)
RXJ1615 16:15:20.23 −32:55:05.36 158 209.81 −8.49 Manara et al. (2014)
DMTau 04:33:48.75 +18:10:09.66 145 25.22 −8.02 Manara et al. (2014)
PDS70 14:08:10.15 −41:23:52.58 113 39.79 −10.26 Haffert et al. (2019)

Notes. References are for the stellar and accretion properties. All disk masses from Lupus are from Ansdell et al. (2016), that for PDS70 from Keppler et al. (2019), for DMTau from Kudo et al. (2018), the others from Pinilla et al. (2018).

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