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Table 1

Stellar parameters and adopted values for the StarSim simulations for ϵ Eri and TZ Ari.

Parameter Literature Ref. StarSim value Literature Ref. StarSim value
Name ϵ Eri TZ Ari (Gl 83.1)
Spectral type K2.0 V (1) HARPS K5 mask M5.0 V (2) CARMENES M5 mask
α 03:32:54.79 (3) 02:00:14.16 (3)
δ −09:27:29.41 (3) +13:02:38.66 (3)
µα (mas yr−1) −974.76±0.16 (3) 1096.46 ±0.07 (3)
µδ (mas yr−1) 20.88±0.12 (3) −1771.53±0.06 (3)
d (pc) 3.2198±0.0014 (3) 4.4696±0.0014 (3)
G (mag) 3.4658±0.0014 (3) 10.6811±0.0008 (3)
L (L) 0.32±0.05 (4) 0.00254±0.00002 (5)
age (Myr) 400–800 (6) >750 (7)
M (M) 0.82±0.05 (4) 0.815–0.825 0.140–0.160 (5) 0.150±0.010
R (R) 0.74±0.01 (4) 0.73–0.75 0.164±0.005 (5) 0.163–0.165
Teff (K) 5076±30 (8) 4900–5300 3154±54 (9) 2950–3350
Prot (days) 11.2 (10) 11.1–11.3 1.96±0.07 (11) 1.9–2
i (deg) 69.57.6+5.6Mathematical equation: $69.5_{ - 7.6}^{ + 5.6}$ (12) 70–90 <28 (7) 20–28
log g (dex) 4.30±0.08 (13) 4.5 5.01±0.06 (9) 5
Tcon(K)Mathematical equation: ${{\rm{T}}_{{\rm{con}}}^ * ({\rm{K}})}$ 1080±670 (14) 200–1000 536±318 (14) 200–1000
CBMathematical equation: ${{\rm{T}}_{{\rm{con}}}^ * ({\rm{K}})}$ ∼0.3 (15) 0.1–0.5 −0.2–0.2

Notes. (1) Keenan & McNeil (1989); (2) Lépine et al. (2013); (3) Brown et al. (2021); (4) Baines & Armstrong (2011); (5) Schweitzer et al. (2019); (6) Mamajek & Hillenbrand (2008); (7) Quirrenbach et al. (2022); (8) Heiter et al. (2015); (9) Passegger et al. (2019); (10) Fröhlich (2007); (11) this work; (12) Giguere et al. (2016); (13) Gonzalez et al. (2010); (14) Herbst et al. (2021); (15) Liebing et al. (2021). Tcon is the spot temperature difference with respect to the photosphere; CBMathematical equation: ${{\rm{T}}_{{\rm{con}}}^ * ({\rm{K}})}$ the convective blueshift in solar units.

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