Table 1
Selection criteria applied to our mock galaxies to emulate stellar-mass samples consistent with SES13 and for the two additional colour-selected samples RED and BLUE.
| Galaxy sample | Selectiona |
|---|---|
| SM1 | 0.5 ≤ M* < 1; i′ < 22.5 |
| SM2 | 1 ≤ M* < 2; i′ < 22.5 |
| SM3 | 2 ≤ M* < 4; i′ < 22.5 |
| SM4 | 4 ≤ M* < 8; i′ < 22.5 |
| SM5 | 8 ≤ M* < 16; i′ < 22.5 |
| SM6 | 16 ≤ M* < 32; i′ < 22.5 |
| RED | u − r > 1.93 z + 1.85; i′ < 22.5; |
| 0.5 ≤ M* < 32 | |
| BLUE | u − r ≤ 1.93 z + 1.85; i′ < 22.5; |
| 0.5 ≤ M* < 32 | |
| SOURCES | i′≤ 24.7; 0.65 ≤ zp < 1.2 |
Notes. The samples are further subdivided, as in SES13, into the two redshift bins, low-z (
) and high-z (
), by an emulated selection in photometric redshift zp. The redshiftdistributions of all samples are summarised by Fig. 1. The sample SOURCES is used as background sample for the mock lensing analysis. (a) M* refers to the stellar mass in units of 1010 M⊙; i′, u, r are apparent magnitudes as defined for CFHTLenS (Erben et al. 2013); z is the (cosmological) galaxy redshift; zp is a photometric redshift with errors similar to CFHTLenS
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