Fig. 2.
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|Zmax| distribution of the Gaia RVS DR3 stars with [Fe/H] < −0.55 and Lz/Jtot > 0.95 (left). The red dashed line at |Zmax|=1.5 kpc correspond to the upper limit that we impose to avoid stars that reach very large distances from the Galactic plane. Eccentricities distribution of the our final thin disc selection: stars with Lz/Jtot > 0.95 and |Zmax|< 1.5 kpc (right).
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