Results of the forward modeling of β Pic b using the most recent spectro/photometric observations of the planet (except CRIRES₊). From top to bottom: Exo-REM, ATMO, BT-Settl and Sonora. Top sub-panels: spectra (points) and photometry (squares) of β Pic b alongside a R_λ ∼ 4000 spectrum extracted using the best fit parameters for the inversion on all datasets. Observations have been re-normalized using the analytic scaling factors computed during the inversion. Bottom sub-panel: residuals for each fit. Dotted lines represent the ±σ (68%) confidence interval.