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Table D.2.

Best fitting values for ax and bx as defined in Eq. (28), fitted to KiDS-450 data.

u-band g-band r-band i-band
ax −3.5 −17 −37 −19
bx 5.5 23 47 23

Notes. In this equation the signal-to-noise of measured fluxes are written as a linear function of , where ϵ is the observed ellipticity of galaxies and is the PSF ellipticity in photometric band x = u,  g , r ,  i.

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