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Fig. 8.


Best-fitting PHOEBE2.0 model to our observational data. Top left panel: best-fitting eclipse model (in black) to the unaltered light curve (in blue) and the light curve with the pulsations removed (in orange). The red points correspond to the synthetic fluxes that were interpolated through to create the complete eclipse model. Top right panel: best-fitting Keplerian orbital fit to the primary (in blue) and secondary (in red) radial velocities. The residuals of the fit of the eclipse model and the radial velocities are displayed in the bottom left and bottom right panels respectively, with the same colour-coding as the top panels.

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