Inferred reflectance and temperature maps for each planet, where the center of the map corresponds to the substellar point. The shading in the upper row corresponds to the single scattering albedo ω of the reflective region on the dayside. Cross validation prefers inhomogeneous models for each planet, so each dayside features a dark sub-stellar region bounded by sub-observer longitudes x₁ and x₂· The thermal emission maps in the second row are not uniform, but appear nearly uniform in this figure because the colormap spans the full range of dayside temperatures for all five planets.