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A source-plane reassessment of the z=6--8 ultraviolet luminosity function behind Abell 2744: no requirement for additional faint-end curvature
We reassess the rest-frame ultraviolet luminosity function (UVLF) at $6\leq z<8$ behind Abell~2744 using public UNCOVER imaging, catalog photometry, and lens products. Observed sources use the released D032 aperture-to-total-corrected photometry; artificial sources use 0.32-arcsec forced apertures w
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