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Home All issues Volume 663 (July 2022) A&A, 663 (2022) A72 Full HTML
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Table 3.

Success rate, S, of our method in recovering the axis ratio, qz, of the DM halo of an axisymmetric Galactic potential from the distribution of the magnitudes of the azimuthal velocities, D|vϑ|, of an observed sample of HVSs.

qz 1.4 (a) 1.3 1.2 1.1 1.0 0.9 0.8 0.7 (a)
S 88.9% 92.6% 96.6% 99.2% 98.4% 97.4% 97.2% 96.6%

Notes.

(a)

To properly compute the success rate of recovering the shape of DM halos with qz = 1.4 and qz = 0.7, we also generated reference sets of nt = 5000 HVS mock catalogs for DM halos of qz = 1.5 and qz = 0.6, respectively.

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