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Fig. 9.

image

Confidence intervals for the axisymmetric Vogelsberger model in (log10(M1 kpc, Rs) (after fixing c/a = 0.8) for a kinematic dataset with 105 stars and 9 × 9 kinematic bins. The Δχ2 = [2.3, 6.18, 11.8]-contours are in white, grey, and black, respectively. The best-fit model is indicated by the white cross, while the expectations are given by the green contour (identical to that shown in Fig. 6). The mass parameter is well constrained and models with Rs ≤ 2.0 kpc are strongly disfavoured, consistent with our expectations. The small panels on the right show the Δχ2 landscapes when only considering (top), (top-middle), (bottom-middle), or (bottom).

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