Comparison of the P-T posterior of WISE 1738 with the nearest possible grid model (in terms of T_eff, log g, composition, etc) from Lacy & Burrows (2023) and Sonora Elf Owl (Mukherjee et al. 2024), for several clear and cloudy, and equilibrium and dis-equilibrium conditions. The pink regions are the estimated 1σ of the emission contribution functions for the MIRI probed photosphere (at the top) and the near-infrared probed photosphere (at the bottom). The equilibrium state water ice, ammonia, metal chloride and sulfide condensation curves are plotted along the profile in blue, purple, red, and green respectively for solar metallicity and C/O ratio.