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

Open Access

Fig. A.1.

We use the velocity distribution given in Mao et al. (2013), with (v₀/v_esc, p)=(0.13, 0.78) and M_lens = 10^−2.2 M_⊙. Here the core size is $237_{- 32}^{+ 34}$ $237^{+34}_{-32}$ ( $2 . 37_{- 0.06}^{+ 0.06}$ $2.37^{+0.06}_{-0.06}$ in magnitude) and the $f_{MDMS} = 0 . 0096_{- 0.0005}^{+ 0.0006}$ $f_{\mathrm{MDMS}} = 0.0096^{+0.0006}_{-0.0005}$ . The one-sigma range still overlaps with the Gaussian cases.

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