Table 1.
Lens galaxy samples.
Survey | Colour | Stellar mass [M⊙] | N | σϵ |
---|---|---|---|---|
CFHTLenS | Red | 10 < log10M* < 10.5 | 61 569 | 0.35 |
CFHTLenS | Red | 10.5 < log10M* < 11 | 70 015 | 0.30 |
CFHTLenS | Red | log10M* > 11 | 19 624 | 0.23 |
CFHTLenS | Blue | 9.5 < log10M* < 10 | 125 968 | 0.38 |
CFHTLenS | Blue | 10 < log10M* < 10.5 | 69 175 | 0.36 |
CFHTLenS | Blue | log10M* > 10.5 | 25 195 | 0.30 |
RCSLenS | Red | 10 < log10M* < 10.5 | 84 380 | 0.34 |
RCSLenS | Red | 10.5 < log10M* < 11 | 60 248 | 0.29 |
RCSLenS | Red | log10M* > 11 | 7059 | 0.25 |
CS82 | Red | 10 < log10M* < 10.5 | 120 640 | 0.39 |
CS82 | Red | 10.5 < log10M* < 11 | 141 107 | 0.35 |
CS82 | Red | log10M* > 11 | 68 231 | 0.29 |
CS82 | Blue | 9.5 < log10M* < 10 | 294 854 | 0.37 |
CS82 | Blue | 10 < log10M* < 10.5 | 120 989 | 0.33 |
CS82 | Blue | log10M* > 10.5 | 25 528 | 0.27 |
KV450 | Red | 10 < log10M* < 10.5 | 178 394 | 0.33 |
KV450 | Red | 10.5 < log10M* < 11 | 190 479 | 0.30 |
KV450 | Red | log10M* > 11 | 32 543 | 0.30 |
KV450 | Blue | 9.5 < log10M* < 10 | 421 945 | 0.37 |
KV450 | Blue | 10 < log10M* < 10.5 | 182 514 | 0.31 |
KV450 | Blue | log10M* > 10.5 | 53 465 | 0.31 |
NGVSLenS | Red | 10 < log10M* < 10.5 | 66 637 | 0.37 |
NGVSLenS | Red | 10.5 < log10M* < 11 | 121 840 | 0.36 |
NGVSLenS | Red | log10M* > 11 | 85 231 | 0.31 |
NGVSLenS | Blue | 9.5 < log10M* < 10 | 277 549 | 0.41 |
NGVSLenS | Blue | 10 < log10M* < 10.5 | 262 997 | 0.39 |
NGVSLenS | Blue | log10M* > 10.5 | 150 760 | 0.33 |
Notes. Overview over the sub-sample of lens galaxies used: Column 2: Split between red and blue lenses using g − i colour for CS82 and the photometric type TBPZ from BPZ for the other surveys. Column 3: Stellar mass range. Column 4: Number of selected lenses in the redshift interval 0.4 ≤ zl < 0.6 for RCSLenS and 0.2 ≤ zl < 0.6 for the other surveys, where the CFHTLenS numbers are based on the fields that pass the systematics tests from Heymans et al. (2012, see Sect. 2.1). Column 5: Ellipticity dispersion of the selected lenses with 0.05 < |ϵg| < 0.95 combining both ellipticity components.
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