Values of the phase difference Δϕ between the primary and secondary eclipses as a function of time and ω inferred from the photometric light curves and the RVs. The pink filled symbol and the pink open symbols correspond to the data of the fits of the ASAS-3 photometry, and the TESS-12 and TESS-39 photometry, respectively. The solid blue line corresponds to our best-fit value of Δϕ inferred from the RVs, and the hatched cyan zone corresponds to the range of values according to the 1σ uncertainties on e.