Ratio maps of our diffuse emission reconstructions and the Fermi diffuse and isotropic emission templates for the M1 (top row) and M2 (bottom row) reconstructions. The maps show our diffuse reconstructions divided by the values predicted by the Fermi templates in selected energy bins on a logarithmic color scale. Numbers larger than 10⁰ indicate we have reconstructed more flux than the template predicts, and vice versa. Energy bins: 0.56–1.00 GeV (left), 10.0–17.8 GeV (middle), and 178–316 GeV (right).