Fig. 7.

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Comparison between the predicted |zmax| distributions by the ES21 model (filled histograms) with APOGEE+astroNN stars (empty histograms) for the whole stellar sample introduced in Sect. 2 (left panels), for the high-α sequence (middle panels), and for the low-α sequence (right panels) normalised to the maximum number of stars in the bins of the distributions. In the first row we report ES21 predictions using the vertical action Jz reported in Eq. (3) without including any errors. In the second row, we report ES21 model results, adding a random error normally distributed around Jz with standard deviation σJz fixed at the values of σJz = 0.5 ⋅ Jz. Finally, in the last row the case with σJz = 1 ⋅ Jz is drawn. In each panel, the vertical solid green and dashed black lines indicate the median values of APOGEE stars and model predictions, respectively.
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