Table 2.
Posterior constraints derived from the best fitting to the ΔΣ measured around the galaxies from Blue Lens-1 and -2, Red Lens-1 and -2, and FLS by our halo model with responding reduced χ2 and p-value.
| Lens sample | log(M*/M⊙) | log(Mh/M⊙) | c | fsat |  |
p-value |
|---|---|---|---|---|---|---|
| Blue Lens-1 | 8.31 | 11.24 |
10.6 |
0.004 |
3.539 (1.644) | 0.003 (0.160) |
| Blue Lens-2 | 9.79 | 11.61 |
9.3 |
0.010 |
0.203 | 0.961 |
| Red Lens-1 | 10.01 | 11.84 |
10.9 |
0.128 |
1.253 | 0.281 |
| Red Lens-2 | 10.73 | 12.71 |
9.3 |
0.236 |
0.926 | 0.463 |
| FLS | 8.49 | 11.42 |
9.8 |
0.024 |
1.995 | 0.076 |
Notes. It presents the median of logarithmic stellar mass log(M*/M⊙), and the median parameter constraints: log(Mh/M⊙), c, fsat with statistical errors. The reduced χ2 and p-value in brackets indicate the model fit to the measurements without the outermost data point.
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