Table 2.
Residual multiplicative bias for the five tomographic bins.
| Tomographic bin | Bin | Median | RMS | m (with-z) | m (no-z) | m (FC17cor) |
|---|---|---|---|---|---|---|
| definition | label | magnitude | ellipticity | |||
| 0.1 < zB ≤ 0.3 | B1 | 22.34 | 0.264 | −0.013 ± 0.008 | −0.036 ± 0.003 | 0.021 ± 0.004 |
| 0.3 < zB ≤ 0.5 | B2 | 23.00 | 0.258 | −0.010 ± 0.006 | −0.028 ± 0.003 | 0.017 ± 0.004 |
| 0.5 < zB ≤ 0.7 | B3 | 23.71 | 0.274 | −0.011 ± 0.006 | −0.008 ± 0.003 | 0.023 ± 0.004 |
| 0.7 < zB ≤ 0.9 | B4 | 23.85 | 0.237 | +0.007 ± 0.006 | +0.006 ± 0.003 | 0.029 ± 0.004 |
| 0.9 < zB ≤ 1.2 | B5 | 24.06 | 0.237 | +0.006 ± 0.007 | +0.009 ± 0.003 | 0.045 ± 0.004 |
Notes. The bias values in the second column correspond to our fiducial calibration where we split the galaxy sample first into tomographic bins (with-z); for the m (no-z) results the bias as a function of size and S/N is determined before the split into tomographic bins; m (FC17cor) lists the results if the FC17 simulations had been analysed with the correct weight recalibration.
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