Figure 1.
Angular coordinates of the 2M++ galaxies (purple), simulated SIBELIUS galaxies (yellow) and SNeIa (orange). The Coma cluster (Abell 1656) is indicated by a white cross. The SIBELIUS-DARK galaxies follow the distribution of observed galaxies in the real Universe on large scales.

Angular coordinates of the 2M++ galaxies (purple), simulated SIBELIUS galaxies (yellow) and SNeIa (orange). The Coma cluster (Abell 1656) is indicated by a white cross. The SIBELIUS-DARK galaxies follow the distribution of observed galaxies in the real Universe on large scales.

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