Ly$\alpha$ emission in galaxies at $z\simeq5-6$: new insight from JWST into the statistical distributions of Ly$\alpha$ properties at the end of reionization

TL;DR

This study uses JWST and other data to analyze the statistical properties of Ly$ extalpha$ emission in galaxies at $z\simeq5-6$, providing insights into the end of reionization and predicting Ly$ extalpha$ characteristics at higher redshifts.

Contribution

It offers the first comprehensive statistical analysis of Ly$ extalpha$ properties in $z\simeq5-6$ galaxies, incorporating new JWST observations and comparing evolution across redshifts.

Findings

Large Ly$ extalpha$ escape fractions (>0.2) are common at $z\simeq5-6$.

Ly$ extalpha$ prevalence increases from $z\sim3$ to $z\sim6$, with slowed evolution between $z\sim5$ and $z\sim6$.

Significant evolution in Ly$ extalpha$ velocity profiles suggests residual HI influences Ly$ extalpha$ escape.

Abstract

JWST has recently sparked a new era of Ly$\alpha$ spectroscopy, delivering the first measurements of the Ly$\alpha$ escape fraction and velocity profile in typical galaxies at $z\simeq6-10$. These observations offer new prospects for insight into the earliest stages of reionization. But to realize this potential, we need robust models of Ly$\alpha$ properties in galaxies at $z\simeq5-6$ when the IGM is mostly ionized. Here we use new JWST observations from the JADES and FRESCO surveys combined with VLT/MUSE and Keck/DEIMOS data to characterize statistical distributions of Ly$\alpha$ velocity offsets, escape fractions, and EWs in $z\simeq5-6$ galaxies. We find that galaxies with large Ly$\alpha$ escape fractions (> 0.2) are common at $z\simeq5-6$, comprising 30 per cent of Lyman break selected samples. Comparing to literature studies, our census suggests that Ly$\alpha$ becomes more prevalent in the galaxy population toward higher redshift from $z\sim3$ to $z\sim6$, although we find that this evolution slows considerably between $z\sim5$ and $z\sim6$, consistent with modest attenuation from residual HI in the mostly ionized IGM at $z\simeq5-6$. We find significant evolution in Ly$\alpha$ velocity profiles between $z\simeq2-3$ and $z\simeq5-6$, likely reflecting the influence of resonant scattering from residual intergalactic HI on the escape of Ly$\alpha$ emission near line center. This effect will make it challenging to use Ly$\alpha$ peak offsets as a probe of Lyman continuum leakage at $z\simeq5-6$. We use our $z\simeq5-6$ Ly$\alpha$ distributions to make predictions for typical Ly$\alpha$ properties at $z\gtrsim8$ and discuss implications of a recently-discovered Ly$\alpha$ emitter at $z\simeq8.5$ with a small peak velocity offset (156 km s$^{-1}$).