Table A.1: Summary of the shear measurement pipeline.
Source Detection hfindpeaks
PSF: 2D polynomial model 2nd order fit of $e^\star (r_{\rm g})$, $P^{\rm sm\star}(r_{\rm g})$ and $P^{\rm sh\star}(r_{\rm g})$
Galaxy radius size $r_{\rm g}$ from hfindpeaks
Quadrupole, $P^{\rm sm}$ and $P^{\rm sh}$ estimate Interpolation (seeing $< r_{\rm g} < 1.2 \times$ seeing), $\theta_{\rm {max}}=4r_{\rm g}$ and $\Delta \theta = 0.5 \ \rm pixel$
  Approx ( $r_{\rm g} \geq 1.2 \ \times$ seeing ), $\theta_{\rm max}={\rm Int [}4r_{\rm g} {\rm ]}$ and $\Delta \theta = 1 \ \rm pixel$
$P_\gamma$ correction Fit in $(r_{\rm g}, mag)$ to $\rm {Tr}(P_\gamma)/2$
Weight Hoekstra et al. (2002b)
Ellipticity cut $\gamma^2 < 1.0$
Size cut $r_{\rm h} > 1.05 \ r_{\rm h}^\star$ and $1.75 \ {\rm pixel} < r_{\rm g} < 6.75 \ \rm pixel$
Significance cut $\nu > 8$
$P_\gamma$ cut $0 < \rm {Tr}P_\gamma/2 < 2$
Close pairs $\vert d\vert < 10 \ \rm pixel$ removed


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