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Fig. E.2
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Distribution of mean PSF FWHM sizes (in arcsec) as reported by ESO for each paw-print observation of the KiDS fields. Binning is made is steps of {δRA, δDec} = {0.25/cos (Dec), 0.25} deg, as the spacing between adjacent chips in the paw-print is ~ 0.2 deg.
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