Dark matter in the Milky Way: Measurements up to 3 kpc from the Galactic plane above the Sun

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Table 1.

Best fitting values for stellar disc components.

	Adjusted			Fixed
Component	parameters			parameters

	${\tilde{ρ}}_{0}$ $\tilde\rho_{0}$	${\tilde{σ}}_{R, 0}$ $\tilde{\sigma}_{R,0}$	${\tilde{σ}}_{z, 0}$ $\tilde{\sigma}_{z,0}$	${\tilde{H}}_{ρ}$ $\tilde{H}_{\rho}$	${\tilde{H}}_{σ_{R}}$ $\tilde{H}_{\sigma_R}$	${\tilde{H}}_{σ_{z}}$ $\tilde{H}_{\sigma_z}$
		km/s	km/s	kpc	kpc	kpc
1	3070 ± 31	51.4 ± 0.2	28.7 ± 0.1	2.9	21.5	6.1
2	17 119 ± 112	33.6 ± 0.8	16.6 ± 0.4	2.9	21.5	6.1
3	21 435 ± 272	32.3 ± 0.2	10.8 ± 0.1	4.2	62	5.8
4	23 635 ± 808	6.3 ± 0.2	7.1 ± 0.08	2.5	70	3.5

Notes. The remaining fitted parameters are the flattening of the dark halo potential, q_ϕ, and the solar velocity (see text).

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