The density profile of Milky Way dark matter halo constrained from the OGLE microlensing sky map

Open Access

Fig. A.3.

We use ρ_aniso defined in Eq. (A.6) to rerun the MCMC with α as an additional parameter. Here, M_lens = 10^−2.2 M_⊙. The core size is $252_{- 30}^{+ 30}$ $252^{+30}_{-30}$ ( $2 . 40_{- 0.05}^{+ 0.05}$ $2.40^{+0.05}_{-0.05}$ in magnitude), $f_{MDMS} = 0 . 0050_{- 0.0003}^{+ 0.0003}$ $f_{\mathrm{MDMS}} = 0.0050^{+0.0003}_{-0.0003}$ , and $α = - 0 . 008_{- 0.002}^{+ 0.002}$ $\alpha = -0.008^{+0.002}_{-0.002}$ . This is still within the one-sigma range shown in the main body of our paper.

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