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Fig. A.1.

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Simulation by our model of bulge components with radius smaller than (i.e. smaller than one pixel). These bulge components are at the end of the Euclid Flagship radii distribution (Fig. 1) outside the COSMOS training domain. As can be seen, our model is able to extrapolate from those cases. Because the object is not resolved, it is almost purely the VIS PSF.

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