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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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