Bulgeless Evolution And the Rise of Discs (BEARD) - III. A numerical simulation view of satellites around Milky-Way analogues

Open Access

Table 4.

Scale measurements of the satellite radial distributions.

	log₁₀c_300kpc	d_half [kpc]
BD	0.25 ± 0.05	$165_{- 71}^{+ 33}$ $Mathematical equation: $ 165_{-71}^{+33} $$
CS	0.48 ± 0.06	$146_{- 58}^{+ 50}$ $Mathematical equation: $ 146_{-58}^{+50} $$
BL	0.79 ± 0.05	$118_{- 45}^{+ 50}$ $Mathematical equation: $ 118_{-45}^{+50} $$

MW	1.2 ± 0.5	(49, 84)

Notes. From left to right: base 10 log concentration in a 300 kpc aperture and the distance enclosing half of the satellites. The reported errors in the two columns are of different nature: for the concentration we report the standard error of the fit, while the errors of d_half indicate the 68% CI due to halo-to-halo variance, except for the MW, that we simply report the distance of the 2nd and 4th satellites.

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