Table 2.
Results of the Bayesian analysis.
| Test | 2.5 perc. | Median | 97.5 perc. |
|---|---|---|---|
| (kpc) | (kpc) | (kpc) | |
| Full sample | 1.4 | 4.2 | 7.8 |
| R′/kpc < 30 | 1.3 | 3.9 | 7.7 |
| 30 < R′/kpc < 50 | 1.3 | 5.5 | 11.5 |
| R′/kpc > 50 | 1.3 | 6.9 | 11.7 |
| PSZ1 G311.65−18.48 | 1.4 | 4.8 | 10.8 |
| RCS2 032727−132623 | 2.1 | 6.2 | 11.5 |
| SGAS J1226+2152 | 1.2 | 4.2 | 8.8 |
| Free σ | 1.3 | 4.5 | 8 |
| 4 × 4 binning | 1.8 | 5.7 | 10.6 |
Notes. 2.5 percentile, median, and 97.5 percentile of the posterior distribution of Clength for the fiducial analysis of the whole sample (Sect. 4.1), the tests performed on different bins of projected distance (Sect. 4.2.1) and on the three individual galaxy halos (Sect. 4.2.2), and the tests where we introduced the intrinsic scatter σ as an additional free parameter and where we used a 4 × 4 binning in the data (see Sect. 5.4).
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