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.

Using nulling interferometry, LIFE will allow us to constrain the radius and effective temperature of (terrestrial) exoplanets

We discuss the impact of the quality of the data on the retrievals in Section 4.3 and the systematic effects for the retrieval runs in Section 4.4.

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.