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Fig. 3

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Mock data for Auriga 23. The blue dots are disc stars that we excluded, i.e. stars with λz > 0.8 or stars with λz > 0.5 and Z/Z > 0.5. The black dots are taken as halo stars and kept in our sample. We divided the data into 7 × 6 bins in rgc versus θ with the intervals of rgc = [5, 8, 12, 16, 22, 30, 40, 50] kpc, θ = [0, 10, 20, 30, 40, 55, 90°]; here, we only show three columns to illustrate the data.

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