The Astrophysical Journal (Jan 2024)

CEERS: Diversity of Lyα Emitters during the Epoch of Reionization

  • Intae Jung,
  • Steven L. Finkelstein,
  • Pablo Arrabal Haro,
  • Mark Dickinson,
  • Henry C. Ferguson,
  • Taylor A. Hutchison,
  • Jeyhan S. Kartaltepe,
  • Rebecca L. Larson,
  • Raymond C. Simons,
  • Casey Papovich,
  • Hyunbae Park,
  • Laura Pentericci,
  • Jonathan R. Trump,
  • Ricardo O. Amorín,
  • Bren E. Backhaus,
  • Micaela B. Bagley,
  • Caitlin M. Casey,
  • Yingjie Cheng,
  • Nikko J. Cleri,
  • M. C. Cooper,
  • Olivia R. Cooper,
  • Jonathan P. Gardner,
  • Eric Gawiser,
  • Andrea Grazian,
  • Nimish P. Hathi,
  • Michaela Hirschmann,
  • Anton M. Koekemoer,
  • Ray A. Lucas,
  • Bahram Mobasher,
  • Nor Pirzkal,
  • Swara Ravindranath,
  • Amber N. Straughn,
  • L. Y. Aaron Yung,
  • Alexander de la Vega

DOI
https://doi.org/10.3847/1538-4357/ad3913
Journal volume & issue
Vol. 967, no. 1
p. 73

Abstract

Read online

We analyze rest-frame ultraviolet to optical spectra of three z ≃ 7.47–7.75 galaxies whose Ly α emission lines were previously detected with Keck/MOSFIRE observations, using the JWST/NIRSpec observations from the Cosmic Evolution Early Release Science survey. From NIRSpec data, we confirm the systemic redshifts of these Ly α emitters, and emission-line ratio diagnostics indicate these galaxies were highly ionized and metal-poor. We investigate Ly α line properties, including the line flux, velocity offset, and spatial extent. For the one galaxy where we have both NIRSpec and MOSFIRE measurements, we find a significant offset in their flux measurements (∼1.3–5× greater in MOSFIRE) and a marginal difference in the velocity shifts. The simplest interpretation is that the Ly α emission is extended and not entirely encompassed by the NIRSpec slit. The cross-dispersion profiles in NIRSpec reveal that Ly α in one galaxy is significantly more extended than the nonresonant emission lines. We also compute the expected sizes of ionized bubbles that can be generated by the Ly α sources and discuss viable scenarios for the creation of sizable ionized bubbles (>1 physical Mpc). The source with the highest-ionization condition is possibly capable of ionizing its own bubble, while the other two do not appear to be capable of ionizing such a large region, but require additional sources of ionizing photons. Therefore, the fact that we detect Ly α from these galaxies suggests diverse scenarios for the escape of Ly α during the epoch of reionization. High-spectral-resolution spectra with JWST/NIRSpec will be extremely useful for constraining the physics of patchy reionization.

Keywords