In this section we show the results from the retrievals on the grid of different input spectra (see Table 1) assuming the baseline parameters listed in Table 2.

We start by discussing the details of the input spectra that were used in this study (Section 2.1). We then discuss the updates on the Bayesian retrieval routin

Corner plots for the retrieval runs at the reference R and S/N are shown in this section. We grouped both the cloudy and the clear sky retrievals for each epoch

In Figures D.1 and D.2 we show the retrieved exoplanet parameters and abundances for the different scenarios with varying R and S/N values.