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Table A.3.

Mean logarithmic density gradients, aI − I​V, of our models at a given collapse.

Model # aI aI​I aIII aI​V
e-10k 0.60 ± 0.22 2.39 ± 0.26 2.32 ± 0.07 3.44 ± 0.03
e-50k 1st 0.56 ± 0.21 2.41 ± 0.03 2.27 ± 0.03 3.36 ± 0.01
2nd 0.61 ± 0.15 2.37 ± 0.12 2.19 ± 0.02 3.35 ± 0.01
m-20k 1st 0.17 ± 0.21 2.09 ± 0.60 1.60 ± 0.10 3.96 ± 0.08
2nd 0.12 ± 0.24 2.07 ± 0.68 1.70 ± 0.09 3.89 ± 0.11
3rd 0.12 ± 0.24 2.22 ± 0.64 1.68 ± 0.08 3.80 ± 0.10
m-100k 1st 0.26 ± 0.31 1.76 ± 0.24 1.53 ± 0.18 3.97 ± 0.07
2nd 0.64 ± 0.25 1.88 ± 0.60 1.64 ± 0.10 3.85 ± 0.12
3rd 0.47 ± 0.16 1.95 ± 0.21 1.63 ± 0.06 3.61 ± 0.10

Notes. The fitted radii where the power law breaks, rI − I​II, shown in Table A.4. All numbers are given with their 1σ deviations calculated from the corresponding number of realisations.

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