Left: The fe model used in our analysis, generated with petitRADTRANS (P. Mollière et al. 2019), as described in Section 4. The full GHOST wavelength is shown; however, we note that we used only a subset of this wavelength range (corresponding to the “usable” range of 383–1000 nm; V. M. Kalari et al. 2024) in our analysis, shown in blue. Right: the two-point T–P profile used to generate the model, using the best-fit parameters from the high-resolution-only retrieval of D. Cont et al. (2024) and the planetary parameters listed in Table 1.