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Table D.1.

Best fit parameters.

aZ γZ fZ aK γK fK
[pc] [pc]
GC 1 67.2 0.66 0.03 28.9 0.27 0.03
GC 2 58.1 0.93 0.03 27.3 0.57 0.02
GC 3 175.6 0.94 0.13 101.0 0.94 0.13
GC 4 92.0 0.92 0.05 46.1 0.82 0.04
GC 5 119.8 1.03 0.06 66.7 0.96 0.06

Notes. Best likelihood parameters from our mass profile fits for each simulated globular cluster at z = 0. The first three columns yield the fits when using a Zhao (1996)αβγ model with fixed α = 2 and β = 5 (as in the classic Plummer model) for better convergence, while the last three columns yield the fits when adopting a Kazantzidis et al. (2004) model. Each three columns display the scale radius a, inner slope γ and mass fraction f relative to the first dark matter shell explained in Section 4.2.2, defined as M•, 1. For details, see Eqs. 5 and 6.

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