Observational Signatures of Lyman Alpha Emission from Early Galaxy Formation
Mark Dijkstra (MPA)

TL;DR
This paper discusses how Lyman Alpha emission from early galaxies can be used to probe the Epoch of Reionization, emphasizing the importance of understanding scattering effects and observational strategies to interpret high-redshift galaxy data.
Contribution
It highlights the role of galactic outflows and scattering in interpreting Lyman Alpha signals and outlines necessary steps to improve understanding of early galaxy observations.
Findings
Scattering through galactic outflows can transmit >5% of Lya radiation through a neutral IGM.
Lyman Alpha emission is a key spectral feature for studying high-redshift galaxies.
Understanding IGM effects is crucial for interpreting LAE observations during reionization.
Abstract
The next generation of telescopes aim to directly observe the first generation of galaxies that initiated the reionization process in our Universe. The Lyman Alpha (Lya) emission line is robustly predicted to be the most prominent intrinsic spectral feature of these galaxies, making it an ideal target to search for and study high-redshift galaxies. I briefly discuss why Lya emitting galaxies (LAEs) provide a good probe of the intergalactic medium (IGM) during the Epoch of Reionization (EoR). I argue that if we wish to fully exploit LAEs as a probe of the EoR, it is important to understand what drives their observed redshift evolution after reionization is completed. One important uncertainty in interpreting existing LAE observations relates to the impact of the ionized IGM on Lya photons emitted by galaxies, which is strongly connected to the effects of scattering through HI in galactic…
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