Table B.1.

Best light curve solution of Hen 2−428.

Fixed parameters:
q (=M2/M1) 0.64
A1 (a) 1.0
A2 (a) 1.0
g1 (b) 1.0
g2 (b) 1.0
x1(B) (c) 0.25
x1(i) (c) 0.17
x1(c) (c) 0.20
x2(B) (c) 0.25
x2(i) (c) 0.17
x2(c) (c) 0.20

Adjusted parameters:

i [°] 63.59 ± 0.54
Teff(1) [K] 40179 ± 370
Teff(2) [K] 40356 ± 175
δ1 (d) 0.02174 ± 0.0052
δ2 (d) 0.0033 ± 0.0021
(e) 0.5837 ± 0.0068
(e) 0.5842 ± 0.0068
(e) 0.5939 ± 0.0168
Ω1 (f) 2.965 ± 0.017
Ω2 (f) 2.965 ± 0.017
l3(B) (g) 0.0079 ± 0.0043
l3(i) (g) 0.0279 ± 0.0066
l3(c) (g) 0.2046 ± 0.0312

Roche radii (h):

r1(mean) [a] 0.4472 ± 0.0041
r1(pole) [a] 0.4121 ± 0.0030
r1(point) [a] −1.0000
r1(side) [a] 0.4407 ± 0.0039
r1(back) [a] 0.4806 ± 0.0056
r2(mean) [a] 0.3809 ± 0.0042
r2(pole) [a] 0.3465 ± 0.0028
r2(point) [a] −1.0000
r2(side) [a] 0.3676 ± 0.0036
r2(back) [a] 0.4212 ± 0.0067

Notes.

(a)

Bolometric albedo.

(b)

Gravitational darkening exponent.

(c)

Linear limb darkening coefficient; taken from Claret & Bloemen (2011).

(d)

Radiation pressure parameter, see Drechsel et al. (1995).

(e)

Relative luminosity; L2 is not independently adjusted, but recomputed from r2 and Teff(2).

(f)

Roche potentials.

(g)

Fraction of third light at maximum.

(h)

Fractional Roche radii in units of separation of mass centers.

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