Fig. I.1.
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Non-weighted luminosity size relation evaluated at different redshifts is shown above. The y-axis shows the UV 1500 Å sizes in kpc and the x-axis shows luminosity at the same wavelength. The green scatter shows our sample of galaxies analysed with radiative transfer for curves of growth sizes using circular apertures whereas the yellow scatter shows the sizes for non-parametric Pixel Method as presented in FLARES IV.
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