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This article has an erratum: [https://doi.org/10.1051/0004-6361/202038840e]


Fig. 11.

image

Observed and predicted smoothed apparent Hess diagram of the Gaia conic sample. Four rows (top to bottom) show the data and predictions of the standard, the MCMC1, and the MCMC2 models. The contributions of the thin and thick disk as well as of the halo are shown in three columns on the left. Values given there in parenthesis correspond to each component’s relative contribution to the total Hess diagram in terms of star counts. The fourth column shows the total Hess diagram, where the observed or modelled number of stars is given in parentheses. The last column displays the logarithmic χ2 calculated according to Eq. (28).

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