Flux density in W m⁻² µm⁻¹ of the best models using ATMO (plain lines) and Exo-REM (dashed lines) fitting the near-IR (colored squares) and mid-IR (black circles) photometric data points for the four planets. The light color lines correspond to the fit of the near-IR data alone. The top four subpanels are for the photometrically calibrated files, and the bottom four are relative to contrast measurements with a reduced number of near-IR data points.