Table 1.
Shifts in the shear multiplicative bias due to the faint galaxies.
| Fiducial | Radius | Background | |
|---|---|---|---|
| w/o clustering | |||
| ΔμSEx × 103 | −4.79 ± 0.30 | −5.71 ± 0.30 | −6.78 ± 0.26 |
| ΔμML × 103 | −3.14 ± 0.27 | −3.40 ± 0.26 | −3.69 ± 0.24 |
| ΔμKSB × 103 | −8.35 ± 0.21 | −9.03 ± 0.23 | −9.17 ± 0.23 |
Notes. The column headed “fiducial” corresponds to our standard analysis (Sect. 5.1), “radius” to the case where faint galaxy sizes are extrapolated from that of bright ones (Sect. 5.3), and “background” to the case without background subtraction (Sect. 5.4). Faint galaxies are included up to magnitude m = 29, except for the “radius” case where faint galaxies are included only up to magnitude m = 27, since the size extrapolation reaches zero for fainter objects.
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