Fig. 7

Angular distribution of the estimated parameters { ΩM,ΩΛ,H0 } k,cosmic_var at each pixel k after noise bias removal. The subsample of type Ia SNe in each pixel is used to estimate the value of the parameters { ΩM,ΩΛ,H0 } in that pixel, resulting in a map for each parameter. Subtracting the maps { ΩM,ΩΛ,H0 } k,shuffle_sn averaged over the different realizations, results in the corresponding unbiased maps. Operating the estimated maps results in the derived maps for Ωκ and q0. Subtracting the fiducial values, results in the corresponding difference maps. The fiducial values are
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