The Astrophysical Journal (Jan 2024)

The Web Epoch of Reionization Lyα Survey (WERLS). I. MOSFIRE Spectroscopy of z ∼ 7–8 Lyα 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,
  • Óscar A. Chávez Ortiz,
  • Sadie Coffin,
  • M. C. Cooper,
  • Nicole Drakos,
  • Andreas L. Faisst,
  • Maximilien Franco,
  • Seiji Fujimoto,
  • Steven Gillman,
  • Ghassem Gozaliasl,
  • Santosh Harish,
  • Taylor A. Hutchison,
  • Anton M. Koekemoer,
  • Vasily Kokorev,
  • Jitrapon Lertprasertpong,
  • Daizhong Liu,
  • Arianna S. Long,
  • Casey Papovich,
  • R. Michael Rich,
  • Brant E. Robertson,
  • Margherita Talia,
  • Brittany N. Vanderhoof,
  • John R. Weaver,
  • Katherine E. Whitaker,
  • Jorge A. Zavala

DOI
https://doi.org/10.3847/1538-4357/ad4c6c
Journal volume & issue
Vol. 970, no. 1
p. 50

Abstract

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We present the first results from the Web Epoch of Reionization Ly α Survey (WERLS), a spectroscopic survey of Ly α emission using Keck I/MOSFIRE and LRIS. WERLS targets bright ( J < 26) galaxy candidates with photometric redshifts of 5.5 ≲ z ≲ 8 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 z ∼ 7–8 Ly α emitters (LAEs; three secure and eight tentative candidates) detected in the first five nights of WERLS MOSFIRE data. We estimate our observed LAE yield is ∼13%, which 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 Ly α emission is unlikely for galaxies embedded in a neutral intergalactic medium. Our targets are selected to be UV-bright, and span a range of absolute UV magnitudes with −23.1 < M _UV < −19.8. With two LAEs detected at z = 7.68, we also consider the possibility of an ionized bubble at this redshift. Future synergistic Keck+JWST efforts will provide a powerful tool for pinpointing beacons of reionization and mapping the large-scale distribution of mass relative to the ionization state of the Universe.

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