Lyman-alpha Emitters in Ionized Bubbles: Constraining the Environment and Ionized Fraction
A.C. Trapp, Steven R. Furlanetto, Frederick B. Davies

TL;DR
This paper introduces a Bayesian framework to analyze high-redshift Lyman-alpha emitter associations, allowing for better inference of the ionized fraction and density fields during reionization, with application to a notable LAE cluster.
Contribution
It develops the first comprehensive Bayesian method combining reionization modeling, Poisson noise, and density estimation for high-z LAE associations.
Findings
LAE association likely a 2.5-sigma over-density
Estimated global ionized fraction Q = 0.60 (+0.08,-0.09)
Poisson noise significantly affects density inferences
Abstract
Lyman-alpha emitters (LAEs) are excellent probes of the reionization process, as they must be surrounded by large ionized bubbles in order to be visible during the reionization era. Large ionized regions are thought to correspond to over-dense regions and may be protoclusters, making them interesting test-beds for early massive structures. Close associations containing several LAEs are often assumed to mark over-dense, ionized bubbles. Here, we develop the first framework to quantify the ionization and density fields of high-z galaxy associations. We explore the interplay between (i) the large-scale density of a survey field, (ii) Poisson noise due to the small number density of bright sources at high redshifts (z~7), and (iii) the effects of the ionized fraction on the observation of LAEs. We use Bayesian statistics, a simple model of reionization, and a Monte-Carlo simulation to…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Radio Astronomy Observations and Technology
