Table 3
Stellar mass results.
| Sample | log(M∗) | nlens | ⟨ z ⟩ | ⟨ M∗ ⟩ | flate |
|
αearly |
|
|
αlate |
|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | |
|
|
|||||||||||
| S1 | [10.00,10.50] | 3359 | 0.08 | 2.04 | 0.51 |
|
|
2.15 ± 0.004 |
|
|
2.04 ± 0.001 |
| S2 | [10.50,11.00] | 5870 | 0.11 | 6.03 | 0.28 |
|
|
7.66 ± 0.02 |
|
|
6.75 ± 0.01 |
| S3 | [11.00,11.25] | 2428 | 0.15 | 13.2 | 0.10 |
|
|
16.8 ± 0.1 |
|
|
14.4 ± 0.1 |
| S4 | [11.25,11.50] | 1631 | 0.20 | 24.0 | 0.05 |
|
|
40.3 ± 0.3 |
|
|
27.3 ± 0.4 |
| S5 | [11.50,11.75] | 1505 | 0.34 | 41.7 | 0.03 |
|
|
88.9 ± 1.1 |
|
|
71.0 ± 4.6 |
| S6 | [11.75,12.00] | 396 | 0.41 | 69.2 | 0.05 |
|
|
230 ± 6 |
|
|
- |
| S7 | [12.00,12.50] | 48 | 0.48 | 123 | 0.02 |
|
|
385 ± 28 | - | - | - |
Notes. (1) The stellar mass range of the bin; (2) the number of lenses; (3) the mean redshift; (4) the mean stellar 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 total stellar mass within r200 for the early-types in units of 1010 M⊙; (9) the best fit halo mass for the late-types in units of 1011 h-1 M⊙; (10) the best fit satellite fraction for the late-types; (11) the total stellar mass within r200 for the late-types in units of 1010 M⊙.
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