Fig. 13.
Absolute Hess diagram of the full local sample (left column) as predicted by the MCMC1 and MCMC2 models (top to bottom). The black and white contours are added for comparison and show the distribution of stars in the data. The overplotted values give the total predicted number of stars in the sample and its relative difference to the observed number of stars. The right column shows the corresponding logarithmic χ2.
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