Restrictions placed on the vMR as a function of cloud deck altitude for the post-eclipse observations. The injection-recovery tests presented here rule out the models in light brown. Additionally, we highlight the models in dark brown which, due to the saturation of a large number of the spectral lines, have an average contrast ratio more than three sigma below the contrast of LTT-9779 b at these wavelengths measured by JWST NIRISS/SOSS data. To compare these restrictions to more complex models, we also plot the EU_VMRS for metallicities ranging from 0.1 times solar to 1000 times solar as a function of the altitude of the cloud deck for the original (T.1, circles) and modified (T.2, crosses) temperature profiles for the western dayside.