# Ly$\alpha$ profile, dust, and prediction of Ly$\alpha$ escape fraction in Green Pea Galaxies

## TL;DR

This study analyzes Ly$ extalpha$ escape in 43 Green Pea galaxies, revealing correlations with dust, metallicity, and kinematic features, and develops a predictive model for Ly$ extalpha$ escape fraction useful for high-redshift galaxy observations.

## Contribution

It provides the largest sample analysis of Green Pea galaxies' Ly$ extalpha$ profiles, establishing new correlations and a predictive empirical relation for Ly$ extalpha$ escape fraction.

## Key findings

- Approximately 2/3 of Green Peas are strong Ly$ extalpha$ emitters.
- Ly$ extalpha$ escape fraction correlates with dust, metallicity, and [OIII]/[OII] ratio.
- An empirical linear relation predicts Ly$ extalpha$ escape fraction with about 0.3 dex accuracy.

## Abstract

We studied Lyman-$\alpha$ (Ly$\alpha$) escape in a statistical sample of 43 Green Peas with HST/COS Ly$\alpha$ spectra. Green Peas are nearby star-forming galaxies with strong [OIII]$\lambda$5007 emission lines. Our sample is four times larger than the previous sample and covers a much more complete range of Green Pea properties. We found that about 2/3 of Green Peas are strong Ly$\alpha$ line emitters with rest-frame Ly$\alpha$ equivalent width $>20$ \AA. The Ly$\alpha$ profiles of Green Peas are diverse. The Ly$\alpha$ escape fraction, defined as the ratio of observed Ly$\alpha$ flux to intrinsic Ly$\alpha$ flux, shows anti-correlations with a few Ly$\alpha$ kinematic features -- both the blue peak and red peak velocities, the peak separations, and FWHM of the red portion of the Ly$\alpha$ profile. Using properties measured from SDSS optical spectra, we found many correlations -- Ly$\alpha$ escape fraction generally increases at lower dust reddening, lower metallicity, lower stellar mass, and higher [OIII]/[OII] ratio. We fit their Ly$\alpha$ profiles with the HI shell radiative transfer model and found Ly$\alpha$ escape fraction anti-correlates with the best-fit $N_{HI}$. Finally, we fit an empirical linear relation to predict Ly$\alpha$ escape fraction from the dust extinction and Ly$\alpha$ red peak velocity. The standard deviation of this relation is about 0.3 dex. This relation can be used to isolate the effect of IGM scatterings from Ly$\alpha$ escape and to probe the IGM optical depth along the line of sight of each $z>7$ Ly$\alpha$ emission line galaxy in the JWST era.