Table 1
Dynamical mass results.
| Sample | log(Mdyn) | nlens | ⟨ z ⟩ | ⟨ Mdyn ⟩ | flate |
|
αearly |
|
αlate |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
|
|
|||||||||
| D1 | [10.00,10.50] | 2011 | 0.08 | 1.96 | 0.44 |
|
|
|
|
| D2 | [10.50,11.00] | 4752 | 0.10 | 5.91 | 0.35 |
|
|
|
|
| D3 | [11.00,11.25] | 2762 | 0.13 | 13.2 | 0.25 |
|
|
|
|
| D4 | [11.25,11.50] | 2281 | 0.16 | 23.6 | 0.16 |
|
|
|
|
| D5 | [11.50,11.75] | 1715 | 0.22 | 41.7 | 0.07 |
|
|
|
|
| D6 | [11.75,12.00] | 935 | 0.32 | 72.5 | 0.05 |
|
|
|
|
| D7 | [12.00,12.50] | 380 | 0.39 | 137.4 | 0.07 |
|
|
|
|
Notes. (1) The dynamical mass range of the bin; (2) the number of lenses; (3) the mean redshift; (4) the mean dynamical mass in units of 1010 M⊙; (5) the fraction of late-type galaxies; (6) the best fit halo mass for the early-types in units of 1011 h-1 M⊙; (7) the best fit satellite fraction for the early-types; (8) the best fit halo mass for the late-types in units of 1011 h-1 M⊙; (9) the best fit satellite fraction for the late-types.
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