Table D.2.
Stellar parameters used for the flux ratio estimation in visible-band (6040.35−6128.93 Å)
| Adopted stellar parameters | predicted observed flux | ||||
|---|---|---|---|---|---|
| Star | Teff | log g | R | ([M/H] = 0)a | ([M/H] = −0.5)b |
| (K) | (R⊙) | (erg/cm2/s/A) | (erg/cm2/s/A) | ||
| Ba | 4000 | 4.5 | 1.064 | 2.8660 × 10−13 | 3.0026 × 10−13 |
| Bb | 3700 | 4.5 | 0.942 | 1.2269 × 10−13 | 1.3758 × 10−13 |
Notes.
From theoretical flux obtained with the BT-Settl (CIFIST) model (Allard et al. 2013; Caffau et al. 2011) multiplied by the dilution factor Md.
Same as (a), but using the theoretical flux obtained with the BT-Settl (AGSS2009) model (Allard et al. 2013; Asplund et al. 2009).
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