A faint z=5.66 galaxy with high ionizing efficiency (log xi_ion = 25.49), low metallicity, and high Lyman-alpha escape fraction is characterized via JWST spectroscopy.
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Using lensed JWST data behind Abell S1063, the UVLF at z~6-11 is fit with gradual quadratic turnover, yielding no evidence for turnover to M_UV=-13.5 at z=6, exclusion limits on turnover models, and lower bounds showing faint galaxies contribute >50% of UV luminosity density and ~64% of ionizing pho
citing papers explorer
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Chasing Cosmic Reionization: An Extremely Faint Highly Magnified Source at $z=5.66$ with high $\xi_{\rm ion}$
A faint z=5.66 galaxy with high ionizing efficiency (log xi_ion = 25.49), low metallicity, and high Lyman-alpha escape fraction is characterized via JWST spectroscopy.
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Tilting at the Turnover: Modeling the Faint-End of the UV Luminosity Function Behind Abell s1063 with JWST
Using lensed JWST data behind Abell S1063, the UVLF at z~6-11 is fit with gradual quadratic turnover, yielding no evidence for turnover to M_UV=-13.5 at z=6, exclusion limits on turnover models, and lower bounds showing faint galaxies contribute >50% of UV luminosity density and ~64% of ionizing pho