Fig. 15.
Dependence of brightness maximum orbital phase ϕ0 (top panel) and the amplitude A (bottom panel) of the sinusoidal fits on the superorbital phase. The solid blue lines correspond to the linear fit of the data, while the ±1σ and ±3σ confidence intervals are shown in dark and light blue. The red squares show the parameters from Table 3 of Paredes-Fortuny et al. (2015).
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