Table 1
Power law parameters.
| σ mod | a mod | b mod |
| [km s-1] | [km s-1] | [km s-1] |
| 180 < σmod < 300 | 44 ± 48 | 141 ± 54 |
| 100 < σmod < 400 | 93 ± 25 | 80 ± 25 |
| σ spec | a spec | b spec |
| [km s-1] | [km s-1] | [km s-1] |
| 180 < σspec < 300 | 176 ± 43 | −5 ± 50 |
| 100 < σspec < 400 | 129 ± 21 | 45 ± 23 |
| log (M∗) | a stel | b stel |
|
[km s-1] | [km s-1] |
| 10.8 < log (M∗) < 11.5 | 134 ± 36 | 179 ± 8 |
| 10.5 < log (M∗) < 12.0 | 118 ± 22 | 178 ± 6 |
Notes. Best-fit power law slope ax and offset bx that describe the relation between galaxy property x (“mod”, “spec”, and “stel” for model velocity dispersion, spectroscopic velocity dispersion, and stellar mass, respectively) and the lensing velocity dispersion for lens galaxies in the range that is indicated in the first column. Details of the fitting are described in the text.
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