Table 1
Stellar parameters of investigated targets (Group I from Kirchschlager et al. 2017).
| HD number | HIP number | Alternative name | d /pc | T★ /K | L★ /L⊙ | R★ /R⊙ | Spectral type |
|---|---|---|---|---|---|---|---|
| 10700 | 8102 | τ Cet | 3.7(a) | 5290(b) | 0.47(b) | 0.82(c) | G8 V (d) |
| 22484 | 16852 | 10 Tau | 13.9(a) | 5998(b) | 3.06(b) | 1.62(e) | F9IV-V (f) |
| 56537 | 35350 | λ Gem | 30.7(a) | 7932(b) | 27.39(b) | 2.78 (e) | A4IV (d) |
| 102647 | 57632 | β Leo | 11.0(g) | 8604(b) | 13.25(b) | 1.66(h) | A3 V (h) |
| 172167 | 91262 | α Lyr | 7.7(g) | 9620(i) | 37 (j) | 2.19 | A0V (k) |
| 177724 | 93747 | ζ Aql | 25.5(g) | 9078(b) | 36.56(b) | 2.45(e) | A0 IV-V(k) |
| 187642 | 97649 | α Aql | 5.1(g) | 7680(l) | 10.09 | 1.79(l) | A7V (k) |
| 203280 | 105199 | α Cep | 15.0(g) | 7510(m) | 18.1 (m) | 2.51 | A8 V (k) |
| 216956 | 113368 | α PsA | 7.7(g) | 8590(n) | 16.63(n) | 1.84(n) | A4 V (o) |
Notes. Stellar parameters are distance d, effective temperature T★, luminosity L★, and radius R★. The stellar radius of HD 172167 and HD 203280, and luminosity of HD 187642 were computed from 
(σsb is the Stefan–Boltzmann constant). We used interferometric measurements of the stellar radii where possible and used determinations based on stellar luminosity in the other cases (see Sect. 4.1.4 for a discussion of the stellar model).
References. (a)Gaia Collaboration (2021); (b)Boyajian et al. (2013); (c)Di Folco et al. (2004); (d)Keenan & McNeil (1989); (e)Boyajian et al. (2012); (ƒ)Gray & Garrison (1989); (g)van Leeuwen (2007); (h)van Belle & von Braun (2009); (i)Habing et al. (2001);(j)Aufdenberg et al. (2006a,b); (k)Gray et al. (2003); (l)van Belle et al. (2001); (m)Zhao et al. (2009); (n)Mamajek (2012); (o)Gray et al. (2006).
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