Table 3
Parameters of the best-fit model.
| MS star mass | M* | 0.62 | ±0.05 | M⊙ |
| MS star radius | R* | 94% |  |
RRL |
| MS star temperature | T* | 4.5 | ±0.3 | kK |
| MS star luminosity (a) | L* | 0.18 |  |
L⊙ |
| WD mass | MWD | 0.725 |  |
M⊙ |
| WD radius | RWD | 0.019 |  |
R⊙ |
| WD temperature | TWD | 66.5 | ±3.5 | kK |
| WD star luminosity (b) | LWD | 5.2 | ±1.5 | L⊙ |
| Absorption efficiency (c) | η | 1.0 | ||
| System inclination | i | 40.2° | ±0.8° |
Notes. (a) The luminosity of the MS star is calculated from the mass and Roche Lobe radius, without taking into account other possible systematic effects. (b)The luminosity of the WD star is is constrained by the light curve amplitude. Thus error bars of the other parameters are not independent. (c) Adopted value.
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