Table 1.
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Summary of source galaxy catalogue. |$z^{\rm {PZ}}_1-z^{\rm {PZ}}_2$| is the range of photometric redshifts of the given tomographic bin (Myles et al. 2021), neff is the effective number density of source galaxies in units of |$\rm {gal}/\rm {arcmin}^{2}$|⁠, and σe is uncertainty in the measurement of one component of the shape (Amon et al. 2022). |$\bar{R}_1$| and |$\bar{R}_2$| are the average METACALIBRATION responses for two galaxy ellipticity components (Gatti et al. 2021).

Redshift binBin-1Bin-2Bin-3Bin-4
|$z^{\rm {PZ}}_1-z^{\rm {PZ}}_2$|0.0–0.360.36–0.630.63–0.870.87–2.0
neff1.4761.4791.4841.461
σe0.2430.2620.2590.310
|$\bar{R}_1$|0.7670.7260.7010.629
|$\bar{R}_2$|0.7690.7270.7020.630
Redshift binBin-1Bin-2Bin-3Bin-4
|$z^{\rm {PZ}}_1-z^{\rm {PZ}}_2$|0.0–0.360.36–0.630.63–0.870.87–2.0
neff1.4761.4791.4841.461
σe0.2430.2620.2590.310
|$\bar{R}_1$|0.7670.7260.7010.629
|$\bar{R}_2$|0.7690.7270.7020.630
Table 1.
Open in new tab

Summary of source galaxy catalogue. |$z^{\rm {PZ}}_1-z^{\rm {PZ}}_2$| is the range of photometric redshifts of the given tomographic bin (Myles et al. 2021), neff is the effective number density of source galaxies in units of |$\rm {gal}/\rm {arcmin}^{2}$|⁠, and σe is uncertainty in the measurement of one component of the shape (Amon et al. 2022). |$\bar{R}_1$| and |$\bar{R}_2$| are the average METACALIBRATION responses for two galaxy ellipticity components (Gatti et al. 2021).

Redshift binBin-1Bin-2Bin-3Bin-4
|$z^{\rm {PZ}}_1-z^{\rm {PZ}}_2$|0.0–0.360.36–0.630.63–0.870.87–2.0
neff1.4761.4791.4841.461
σe0.2430.2620.2590.310
|$\bar{R}_1$|0.7670.7260.7010.629
|$\bar{R}_2$|0.7690.7270.7020.630
Redshift binBin-1Bin-2Bin-3Bin-4
|$z^{\rm {PZ}}_1-z^{\rm {PZ}}_2$|0.0–0.360.36–0.630.63–0.870.87–2.0
neff1.4761.4791.4841.461
σe0.2430.2620.2590.310
|$\bar{R}_1$|0.7670.7260.7010.629
|$\bar{R}_2$|0.7690.7270.7020.630
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