Fig. 4.
Inferred total matter density of data samples S1–S8, as a function of height with respect to the Galactic plane. The matter density is plotted for three different cases: when using the velocity information of all stellar objects, when using the velocity information of stellar objects with good radial velocity measurements only, and when using the velocity information of stellar objects in the mid-plane only. Also shown is the 1-σ band of the baryonic model (see Sect. 2.5).
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