Fig. A.2.
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Upper panel: Multiplicative bias, defined as m ≡ (m1 + m2)/2 as a function of the input magnitude of galaxies for Euclid-like and different selections of seeings in LSST-like surveys. Lower panel: Multiplicative detection bias mdet with the input magnitude with galaxies are placed randomly, also defined as mdet ≡ (mdet, 1 + mdet, 2)/2.
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