Lyman Alpha Emitters and the 21cm Power Spectrum as Probes of Density-Ionization Correlation in the Epoch of Reionization
Michael Pagano, Adrian Liu

TL;DR
This study explores how observations of Lyman Alpha Emitters and the 21cm power spectrum can jointly constrain the morphology of the Epoch of Reionization, revealing the limitations and potential of current measurements.
Contribution
It introduces a parametrization of density-ionization correlation during reionization and demonstrates how combined LAE and 21cm data can constrain reionization models.
Findings
LAE observations alone cannot distinguish reionization models at 68% credibility.
Combining LAE data with 21cm measurements can rule out certain reionization scenarios at 99% credibility.
LAE clustering and number density provide complementary information for probing EoR morphology.
Abstract
Due to the large cross section of Ly photons with hydrogen, Lyman Alpha Emitters (LAEs) are sensitive to the presence of neutral hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR): the period in the Universe's history where neutral hydrogen in the IGM is ionized. The correlation of the ionized regions in the IGM with respect to the underlying intrinsic LAEs has a pronounced effect on the number of observed LAEs and their apparent clustering. As a result, observations of LAEs during the EoR can be used as a probe of the EoR morphology. Here we build on previous works where we parametrize the density-ionisation correlation during the EoR, and study how the observed number density and angular correlation function (ACF) of LAEs depends on this parametrization. Using Subaru measurements of the number density of LAEs and their ACF at z = 6.6, we place…
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