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Table C.1.

Stellar observational data used in Fig. 9 and Fig. 10. The respective uncertainties are given when available. Missing data is represented by "—".

Name Age [Myr] M [M] R [R] P [d] BI [G] BV [G] BQU [G]
AU Mic 23 ± 11 0.50 ± 0.032 0.75 ± 0.032 4.86 ± 0.012 2310 ± 2001 881 2000 ± 2001
WW Psa 27 ± 73 0.19 ± 0.043 0.70 ± 0.133 2.37 ± 0.013 2750 ± 2503
TX Psa 27 ± 73 0.11 ± 0.033 0.52 ± 0.103 1.09 ± 0.013 2750 ± 2503
V1124 Oria 1.24 0.264 2.154 8.184 2090 ± 3404
V1123 Oria 0.84 0.354 2.594 7.644 2510 ± 4104
V1568 Oria 1.34 0.404 2.374 5.544 1420 ± 2304
Upp Sco 55b 55 0.105 0.525 2.90 ± 0.305 2300 ± 13005
TWA 9B 106 0.306 0.916 3.986 3100 ± 2006
TWA 8A 11 ± 57 0.45 ± 0.107 0.80 ± 0.207 4.58 ± 0.017 6000 ± 5007 7207
GJ 490B 35-3508 0.339 0.349 0.549 3200 ± 4009 6809
V2247 Opha 1.010 0.3510 2.0010 3.4010 2700 ± 10011 9010
TWA 7 17 ± 1012 0.62 ± 0.0312 0.80 ± 0.1012 5.00 ± 0.0112 2700 ± 20011 5012

Notes. aDespite the young age of those stars, they are identified as NTTS or weak accretors and thus, included in the list. bP calculated from vsini data.

References. (1) Kochukhov & Reiners (2020); (2) Plavchan et al. (2020); (3) Messina et al. (2017); (4) Yang & Johns-Krull (2011); (5) Reiners et al. (2009); (6) Yang et al. (2008); (7) Hill et al. (2019); (8) Klutsch et al. (2014); (9) Phan-Bao et al. (2009); (10) Donati et al. (2010); (11) Lavail et al. (2019), (12) Nicholson et al. (2021).

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