Fig. 5.
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Top: Half-light ratio in the JWST/F444W filter vs. redshift for the sample of extended v-shape objects by Kocevski et al. (2025). The horizontal solid line indicate the HE band FWHM, scaled assuming a Gaussian function. Bottom: Fraction of extended v-shape objects that is expected to be unresolved in the HE band as a function ofredshift.
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