Table 5: Parameters of the dark matter halos. The first column labels the models. The mass-to-light ratio M/LR and the dark matter fraction are calculated for two radii ( $7.5~{\rm kpc} \simeq R_{{\rm eff}}$ and $30~\rm kpc$is the radius within which the GCs used in the analysis are found). From the NFW parameters of our model halos, we calculate the virial radius, the virial mass, and the concentration parameter ${{(c_{\rm {vir}}= {R}_{{\rm vir}}/r_{{\rm dark}})}}$ using the definitions of Bullock et al. (2001). Then we give the total mass within 30 kpc, the mass-to-light ratios (R-band), and the dark matter fraction within 30 kpc and 7.5 kpc (effective radius). Note that the virial quantities were calculated for the dark halos without adding the stellar component. Thus, the virial masses presented below are lower limits.
# $\beta$ $r_{{\rm dark}}$ $\varrho_{{\rm dark},0}$ rms ${R}_{{\rm vir}}$ ${M}_{{\rm vir}}$ $c_{{\rm vir}}$ ${M}_{{\rm < 30~kpc}}$ M/LR $\frac{M_{{\rm dark}}}{M_{{\rm total}}}$ M/LR $\frac{M_{{\rm dark}}}{M_{{\rm total}}}$
    [kpc] $[{M}_{\odot}~{\rm pc}^{-3}]$ $[{\rm km~s}^{-1}] $ [kpc] [ $10^{12}~{M}_{\odot}$] $\quad$ $ [10^{11}~{M}_{\odot}]$ $(r=30~\rm {kpc})$ $(r=7.5~\rm {kpc})$
  M/LR= 6.8, $\sigma_{{\rm los}}(27~\rm kpc) = 121~\rm {km~s}^{-1}$ (cf. Fig. 13, left panels)
1 -2.0 5 0.12 23 207 0.52 41.4 5.5 10.9 0.37 9.6 0.29
2 -0.5 10 0.033 20 255 0.96 25.5 5.5 12.0 0.43 9.4 0.27
3 0 40 0.003 21 395 3.6 9.9 6.6 13.1 0.48 8.4 0.19
4 0.5 120 0.00075 26 655 16.6 5.5 7.2 14.3 0.52 8.2 0.17
5 1.0 240 0.00050 46 1100 77.9 4.57 9.2 18.3 0.63 8.7 0.22
  M/LR= 4.3, $\sigma_{{\rm los}}(27~\rm kpc) = 121~\rm {km~s}^{-1}$ (cf. Fig. 14, left panels)
6 - 2.0 5 0.195 22 248 0.90 49.6 5.5 10.9 0.61 8.9 0.52
7 - 0.5 5 0.230 20 264 1.01 52.8 6.1 12.1 0.64 9.7 0.56
8 0 20 0.0135 20 358 2.7 17.9 5.3 10.6 0.59 5.9 0.27
9 0.5 120 0.00100 25 743 24.1 6.2 7.2 14.3 0.70 6.2 0.30
10 1.0 120 0.00145 45 870 39.0 7.3 9.4 18.7 0.77 7.0 0.37
  M/LR= 6.8, $\sigma_{{\rm los}}(27~\rm kpc) = 227~\rm {km~s}^{-1}$ (cf. Fig. 13, right panels)
11 - 2.0 120 0.0012 18 803 30.5 6.7 9.4 18.7 0.64 9.0 0.25
12 - 0.5 80 0.0019 25 650 16.0 8.1 9.0 26.7 0.75 10.5 0.35
13 0.0 120 0.0011 32 773 27.2 6.4 9.0 17.7 0.62 8.8 0.23
14 0.5 120 0.0012 47 803 30.5 6.7 9.5 18.7 0.64 9.0 0.25
  M/LR= 4.3, $\sigma_{{\rm los}}(27~\rm kpc) = 227~\rm {km~s}^{-1}$ (cf. Fig. 14, right panels)
15 - 2.0 80 0.0023 16 703 20.4 8.8 9.0 18.0 0.76 7.1 0.39
16 - 0.5 120 0.0011 24 774 27.3 6.5 7.7 15.2 0.72 6.3 0.32
17 0.0 120 0.00135 27 845 35.4 7.0 9.0 17.7 0.76 6.8 0.37
18 0.5 120 0.0014 42 858 37.0 7.15 9.2 18.2 0.76 6.9 0.38

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