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Table 1

Stellar parameters of the targets.

Target RA (J2000) Dec (J2000) SpT V d Teff L* AV M* Age
(h:m:s) (deg:m:s) (mag) (pc) (K) (LSun) (mag) (MSun) (Myr)
LkCa 15 04:39:17.79 +22:21:03.38 K5 12.0 157.2 ± 0.6 4800 1.11 ± 0.04 0.6 1.2 ± 0.1 6.3
                       
HD 34282 05:16:00.47 −09:48:35.39 B9.5 9.8 318.6 ± 2.2 9400 19.0 ± 1.8 0.6 1.9 ± 0.1 8.9
                       
HD 36112 05:30:27.52 +25:19:57.08 A8V 8.3 155.9 ± 0.8 8200 11.8 ± 0.5 0.2 1.8 ± 0.1 8.9
                       
CQ Tau 05:35:58.46 +24:44:54.08 F5IV 10.0 149.4 ± 1.3 6800 7.3 ± 0.6 0.4 1.4 ± 0.1 9.9
                       
Sz Cha 10:58:16.74 −77:17:17.18 K0 12.7 190.2 ± 0.9 4900 2.6 ± 0.2 1.5 1.5 ± 0.2 1.9
                       
TW Hya 11:01:51.90 −34:42:17.03 K6V 10.5 60.14 ± 0.05 4000 0.33 ± 0.02 0.0 0.8 ± 0.1 6.3
                       
HD 97048 11:08:03.31 −77:39:17.49 A0V 9.0 184.4 ± 0.8 10 400 44.2 ± 5.7 1.1 2.4 ± 0.2 3.9
                       
HD 100546 11:33:25.44 −70:11:41.23 A0V 6.3 108.1 ± 0.4 9800 31.6 ± 0.7 0.1 2.2 ± 0.2 5.0
                       
PDS 66 13:22:07.54 −69:38:12.21 K1V 10.4 97.9 ± 0.1 4600 1.26 ± 0.04 0.8 1.2 ± 0.2 3.1
                       
PDS 70 14:08:10.15 −41:23:52.57 K7IV 12.2 112.4 ± 0.2 4000 0.31 ± 0.02 0.0 0.8 ± 0.1 7.9
                       
HD 135344B 15:15:48.44 −37:09:16.02 F8V 8.7 135.0 ± 0.4 6400 6.9 ± 0.4 0.4 1.5 ± 0.1 8.9
                       
HD 139614 15:40:46.38 −42:29:53.53 A9V 8.2 133.6 ± 0.5 7800 7.0 ± 1.6 0.0 1.6 ± 0.1 12.2
                       
RX J1604.3-2130A 16:04:21.65 −21:30:28.54 K2 12.3 145.3 ± 0.6 4600 0.60 ± 0.03 1.1 1.0 ± 0.1 11.1
                       
RX J1615.3-3255 16:15:20.23 −32:55:05.09 K5 12.0 155.6 ± 0.6 4000 0.90 ± 0.02 0.6 0.6 ± 0.1 1.0
                       
HD 169142 18:24:29.77 −29:46:49.32 F1V 8.2 114.0 ± 0.8 7400 5.6 ± 1.2 0.0 1.5 ± 0.2 12.3
                       

Notes. Stellar parameters of the PPD hosts considered in this work. References for the stellar temperature and optical extinction can be found in Table F.1 of Garufi et al. (2018). Mass, luminosity and age have been derived here using Gaia EDR3 parallaxes (Gaia Collaboration 2021).

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