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

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Table 3.

Luminosity function fit parameters.

	α	M^knee [mag]	${log}_{10} \frac{ϕ}{[{kpc}^{- 3} h]}$ $Mathematical equation: $ \log_{10}\frac{\phi}{[\mathrm{kpc}^{-3}\ h]} $$
BD	−1.28 ± 0.01	−22.0 ± 0.3	−5.49 ± 0.07
CS	−1.27 ± 0.02	−21.8 ± 0.4	−5.77 ± 0.10
BL	−1.35 ± 0.02	−21.9 ± 0.6	−6.01 ± 0.14

Notes. From left to right: faint end luminosity slope (α), knee of the LF (M^knee), and normalisation (ϕ). Values indicate the mean and 1σ scatter. In the case of the CS the reported value (and error) indicates the average of the maximum a posteriori estimates (and standard deviation) of the 1000 different realisations.

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