Figure 7
In the top panels, we show how the metrics, ,  and Qdn, for submissions change as the galaxy model changes; the colour scale labels the logarithm of Qdn. The galaxy models are: uniform bulge-to-disc ratio, each galaxy has, randomly sampled from the range [0.3, 0.95] with no offset (Uni.), a 50 per cent bulge-to-disc ratio = 0.5 with no offset (50/50.) and a 50 per cent bulge-to-disc ratio = 0.5 with a bulge-to-disc centroid offset (w/O). In the lower panels, we show the PSF size and ellipticity contributions α and β. In the bottom left-hand panel, we show the key that labels each method.

In the top panels, we show how the metrics, formula, formula and Qdn, for submissions change as the galaxy model changes; the colour scale labels the logarithm of Qdn. The galaxy models are: uniform bulge-to-disc ratio, each galaxy has, randomly sampled from the range [0.3, 0.95] with no offset (Uni.), a 50 per cent bulge-to-disc ratio = 0.5 with no offset (50/50.) and a 50 per cent bulge-to-disc ratio = 0.5 with a bulge-to-disc centroid offset (w/O). In the lower panels, we show the PSF size and ellipticity contributions α and β. In the bottom left-hand panel, we show the key that labels each method.

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