Corrected reproduction of the insets of Figs. 4 and C1 of Demangeon et al. (2024): WASP-76 b occultation atmospheric retrievals for a model including the TiO and VO optical absorbers (left panel), including only VO (middle), and excluding both TiO and VO (right). The light blue, dark blue, and orange curves and their associated shaded areas show the retrieved spectra and 68% credible intervals when fitting the D1, D2, and D3 occultation observations, respectively (see the legend and notes in Table 1). The grey markers show the CHEOPS and TESS occultation measurements, although the fits are not constrained by these observations. The coloured square markers show the corrected model eclipse-depths integrated over the CHEOPS and TESS bands (see the passband response functions in grey at the bottom of the panels).