The Curious Case of Lyman Alpha Emitters: Growing Younger from z ~ 3 to z ~ 2?
Viviana Acquaviva, Carlos Vargas, Eric Gawiser, Lucia Guaita

TL;DR
This study compares the properties of Lyman Alpha Emitting galaxies at redshifts 3.1 and 2.1 using consistent analysis methods, revealing significant differences that challenge the idea of direct evolutionary connection between these galaxy populations.
Contribution
The paper applies a uniform SED fitting approach to two galaxy samples, providing clearer evidence that LAEs at different redshifts have distinct physical properties.
Findings
LAEs at z=3.1 are old (~1 Gyr) and metal-poor.
LAEs at z=2.1 are young (~50 Myr) and metal-rich.
Direct evolution from z=3.1 to z=2.1 LAEs is unlikely.
Abstract
Lyman Alpha Emitting (LAE) galaxies are thought to be progenitors of present-day L* galaxies. Clustering analyses have suggested that LAEs at z ~ 3 might evolve into LAEs at z ~ 2, but it is unclear whether the physical nature of these galaxies is compatible with this hypothesis. Several groups have investigated the properties of LAEs using spectral energy distribution (SED) fitting, but direct comparison of their results is complicated by inconsistencies in the treatment of the data and in the assumptions made in modeling the stellar populations, which are degenerate with the effects of galaxy evolution. By using the same data analysis pipeline and SED fitting software on two stacked samples of LAEs at z = 3.1 and z = 2.1, and by eliminating several systematic uncertainties that might cause a discrepancy, we determine that the physical properties of these two samples of galaxies are…
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