Fig. 5
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Structured data set to train the calibration NN with the MSB loss function (similar to Fig. 2 in Tewes et al. 2019). Each row corresponds to one case containing 2000 galaxies (i.e., 2000 columns), which differ only in the orientations sharing the same shear and PSF. 5000 cases (i.e., 5000 rows) in total are used to train the NN. Shape noise cancellation is adopted.
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