Table 1.
Data properties per tomographic redshift bin.
| Bin | zB range |
 |
σϵ, i | Δz = zest − ztrue | m |
|---|---|---|---|---|---|
| 1 | 0.1 < zB ≤ 0.3 | 0.62 | 0.27 | 0.000 ± 0.0106 | −0.009 ± 0.019 |
| 2 | 0.3 < zB ≤ 0.5 | 1.18 | 0.26 | 0.002 ± 0.0113 | −0.011 ± 0.020 |
| 3 | 0.5 < zB ≤ 0.7 | 1.85 | 0.27 | 0.013 ± 0.0118 | −0.015 ± 0.017 |
| 4 | 0.7 < zB ≤ 0.9 | 1.26 | 0.25 | 0.011 ± 0.0087 | 0.002 ± 0.012 |
| 5 | 0.9 < zB ≤ 1.2 | 1.31 | 0.27 | −0.006 ± 0.0097 | 0.007 ± 0.010 |
Notes. We list the index of the redshift bin, followed by the range of best-fitting photometric redshifts, zB, that divide galaxies into redshift bins. In the third column we show the effective number density, neff, calculated with Aeff = 777.4 deg2. The values for the ellipticity dispersion per ellipticity component, σϵ, i, are presented in the fourth column. For explicit definitions of neff and σϵ, i see Appendix C of J20. The last two columns show the central values of calibration parameters, which are the shift in the mean of the redshift distributions, Δz, and the multiplicative shear bias, m, as well as their associated uncertainties. In the analysis the uncertainty on each of these calibration parameters is accounted for through their covariance matrices, since the values for the different tomographic bins are correlated.
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