The Web Epoch of Reionization Lyman-$\alpha$ Survey (WERLS) I. MOSFIRE Spectroscopy of $\mathbf{z \sim 7-8}$ Lyman-$\alpha$ Emitters
Olivia R. Cooper, Caitlin M. Casey, Hollis B. Akins, Jake Magee,, Alfonso Melendez, Mia Fong, Stephanie M. Urbano Stawinski, Jeyhan S., Kartaltepe, Steven L. Finkelstein, Rebecca L. Larson, Intae Jung, Ash Bista,, Jaclyn B. Champagne, Oscar A. Chavez Ortiz, Sadie Coffin

TL;DR
This paper reports the first spectroscopic detections of Lyman-$eta$ emitters at redshifts 7-8 using Keck/MOSFIRE, providing insights into the ionization state of the early universe during the Epoch of Reionization.
Contribution
First spectroscopic survey of bright Lyman-$eta$ emitters at $z\,7-8$ using Keck/MOSFIRE, advancing understanding of reionization and galaxy evolution in the early universe.
Findings
Detected 11 Lyman-$eta$ emitters at $z\,7-8$
Observed LAE yield of approximately 13%
Evidence suggesting possible ionized bubble at $z=7.68$
Abstract
We present the first results from the Web Epoch of Reionization Lyman- Survey (WERLS), a spectroscopic survey of Lyman- emission using Keck I/MOSFIRE and LRIS. WERLS targets bright () galaxy candidates with photometric redshifts of selected from pre-JWST imaging embedded in the Epoch of Reionization (EoR) within three JWST deep fields: CEERS, PRIMER, and COSMOS-Web. Here, we report 11 Lyman- emitters (LAEs; 3 secure and 8 tentative candidates) detected in the first five nights of WERLS MOSFIRE data. We estimate our observed LAE yield is %, broadly consistent with expectations assuming some loss from redshift uncertainty, contamination from sky OH lines, and that the Universe is approximately half-ionized at this epoch, whereby observable Lyman- emission is unlikely for galaxies embedded in a neutral…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · CCD and CMOS Imaging Sensors
