Table 2
Parameters and fit quality of the maximum likelihood DC14 and coreNFW models for the good galaxies in our sample.
| DC14 | cNFW | ||||||||
|
|
|||||||||
| Galaxy | log10 (Mvir) | c | log10 (M∗) |
|
log10 (Mvir) | c | log10 (M∗) | r c |
|
| (M⊙) | (M⊙) | (M⊙) | (M⊙) | (kpc) | |||||
|
|
|||||||||
| UGC 8508 | 9.83 |
30.84 |
6.86 |
0.42 | 9.85 |
25.43 |
6.86 |
1.09 | 0.61 |
| CVnIdwA | 9.57 |
16.84 |
6.68 |
0.34 | 9.84 |
13.39 |
7.04 |
3.12 | 0.41 |
| NGC 3741 | 10.43 |
15.52 |
7.35 |
0.18 | 10.55 |
9.88 |
7.35 |
0.60 | 1.23 |
| NGC 3741* | 10.35 |
16.75 |
7.35 |
4.06 |
0.19 | ||||
| WLM | 10.07 |
20.94 |
7.00 |
0.73 | 10.39 |
13.07 |
7.43 |
2.33 | 0.62 |
| DDO 154 | 10.30 |
20.29 |
7.53 |
0.61 | 10.14 |
46.23 |
7.53 |
6.14 | 0.86 |
| DDO 126 | 10.04 |
19.50 |
7.36 |
0.17 | 10.33 |
11.91 |
7.78 |
3.1 | 0.40 |
| DDO 87 | 10.30 |
21.74 |
7.71 |
0.24 | 10.74 |
13.96 |
8.02 |
5.88 | 1.24 |
| UGCA 442 | 10.53 |
18.99 |
8.05 |
0.65 | 10.59 |
14.00 |
8.05 |
3.34 | 0.63 |
| DDO 168 | 10.66 |
18.89 |
8.03 |
1.61 | 10.51 |
16.51 |
7.81 |
2.73 | 2.2 |
| DDO 52 | 10.32 |
20.07 |
7.78 |
0.20 | 10.64 |
11.42 |
8.20 |
3.99 | 0.30 |
| NGC 3109 | 10.86 |
16.96 |
8.22 |
0.13 | 10.83 |
14.57 |
8.22 |
4.73 | 0.23 |
| NGC 2366 | 10.57 |
17.00 |
8.02 |
0.93 | 10.57 |
16.03 |
8.03 |
5.07 | 1.25 |
| UGC 7603 | 10.60 |
19.48 |
8.50 |
0.43 | 10.81 |
13.06 |
8.53 |
2.17 | 0.58 |
|
|
|||||||||
| IC 2574 | 11.15 |
9.63 |
8.83 |
0.20 | |||||
| NGC 2976 | 11.11 |
23.69 |
8.99 |
0.43 | |||||
| M33 | 11.48 |
9.53 |
9.81 |
1.47 | |||||
| NGC 2403 | 11.61 |
12.57 |
9.83 |
0.56 | |||||
| NGC 3621 | 11.85 |
6.66 |
10.23 |
0.56 | |||||
| NGC 3198 | 11.88 |
4.00 |
10.44 |
1.04 | |||||
| NGC 5055 | 11.96 |
9.59 |
10.63 |
0.68 | |||||
Notes. Column 1 gives the galaxy name. Columns 2–5 represent the halo mass, halo concentration, stellar mass, and reduced chi-squared of the best-fit DC14 model. Columns 6–10 give the halo mass, halo concentration, stellar mass, dark matter core radius, and reduced chi-squared of the best-fit coreNFW model.
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