Table 3
Derived parameters of WD 1856+534 b in the three high-cadence light curves and assuming a circular orbit.
Parameter | Sloan g | Sloan i | J |
---|---|---|---|
Rp (R⊙) | 0.104 ± 0.006 | 0.110 ± 0.007 | 0.111 ± 0.007 |
b | 8.3 ± 0.8 | 8.9 ± 0.9 | 9.0 ± 0.9 |
ub | 0.13 ± 0.10 | 0.23 ± 0.16 | 0.25 ± 0.20 |
uc | 0.08 ± 0.15 | 0.37 ± 0.30 | 0.24 ± 0.29 |
fout | 0.9994 ± 0.0004 | 1.0007 ± 0.0003 | 0.9992 ± 0.0007 |
Rp,fix (R⊙) (a) | 0.105975 ± 0.000014 | 0.105981 ± 0.000016 | 0.105974 ± 0.000039 |
Notes. (a) Radius of the secondary assuming b = 8.5 and RWD = 0.0123 R⊙ and with thequadratic limb darkening coefficients ub and uc fixed to thevalues given by Gianninas et al. (2013) for a DA WD with log g =8.0 dex and Teff = 5000 K. For the values of these coefficients in the J filter, we extrapolated the Gianninas et al. (2013) values using polynomial fits, obtaining ub = − 0.027 and uc = 0.353.
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