WASP-76 b retrieved spectra and temperature profiles. Same as Figure 4 but for the runs without TiO opacity (top panels) and without TiO nor VO opacity (bottom panels). The spectra and thermal profiles show the same behaviour as the runs including TiO and VO opacity, with the only significant difference that the D1 model does not show the TiO emission over the CHEOPS and TESS bands, therefore predicting much lower thermal emission (insets).