Temperature curves from the retrievals including all the detected chemical species and orbital phase coverage. Left panel: median of the sampled temperature profiles with the 1σ interval. The dark blue line indicates the temperature profile computed using all the spectra outside the RV interval ±v_rotsini_*. We also measured the temperature profiles by running the retrieval on two subsets of the spectral time series. The T-p profile inferred from the spectra far from secondary eclipse is indicated in pink, while that inferred from the spectra close to eclipse is in light blue. Right panel: orbital phase intervals used to compute the different T-p profiles (orbital phases in the RV range ±v_rotsini_* in transparent dark blue).