The Astrophysical Journal Letters (Jan 2023)

Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ≃ 8–10

  • Pablo Arrabal Haro,
  • Mark Dickinson,
  • Steven L. Finkelstein,
  • Seiji Fujimoto,
  • Vital Fernández,
  • Jeyhan S. Kartaltepe,
  • Intae Jung,
  • Justin W. Cole,
  • Denis Burgarella,
  • Katherine Chworowsky,
  • Taylor A. Hutchison,
  • Alexa M. Morales,
  • Casey Papovich,
  • Raymond C. Simons,
  • Ricardo O. Amorín,
  • Bren E. Backhaus,
  • Micaela B. Bagley,
  • Laura Bisigello,
  • Antonello Calabrò,
  • Marco Castellano,
  • Nikko J. Cleri,
  • Romeel Davé,
  • Avishai Dekel,
  • Henry C. Ferguson,
  • Adriano Fontana,
  • Eric Gawiser,
  • Mauro Giavalisco,
  • Santosh Harish,
  • Nimish P. Hathi,
  • Michaela Hirschmann,
  • Benne W. Holwerda,
  • Marc Huertas-Company,
  • Anton M. Koekemoer,
  • Rebecca L. Larson,
  • Ray A. Lucas,
  • Bahram Mobasher,
  • Pablo G. Pérez-González,
  • Nor Pirzkal,
  • Caitlin Rose,
  • Paola Santini,
  • Jonathan R. Trump,
  • Alexander de la Vega,
  • Xin Wang,
  • Benjamin J. Weiner,
  • Stephen M. Wilkins,
  • Guang Yang,
  • L. Y. Aaron Yung,
  • Jorge A. Zavala

DOI
https://doi.org/10.3847/2041-8213/acdd54
Journal volume & issue
Vol. 951, no. 1
p. L22

Abstract

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We present JWST/NIRSpec prism spectroscopy of seven galaxies selected from Cosmic Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric redshifts z _phot > 8. We measure emission line redshifts of z = 7.65 and 8.64 for two galaxies. For two other sources without securely detected emission lines we measure $z={9.77}_{-0.29}^{+0.37}$ and ${10.01}_{-0.19}^{+0.14}$ by fitting model spectral templates to the prism data, from which we detect continuum breaks consistent with Ly α opacity from a mostly neutral intergalactic medium. The presence of strong breaks and the absence of strong emission lines give high confidence that these two galaxies have redshifts z > 9.6, but the redshift values derived from the breaks alone have large uncertainties given the low spectral resolution and relatively low S/N of the CEERS NIRSpec prism data. The two z ∼ 10 sources observed are relatively luminous ( M _UV 8 candidates with CEERS NIRSpec spectroscopy do not have secure redshifts, but the absence of emission lines in their spectra is consistent with redshifts z > 9.6. We find that z > 8 photometric redshifts are generally in agreement (within their uncertainties) with the spectroscopic values, but also that the photometric redshifts tend to be slightly overestimated (〈Δ z 〉 = 0.45 ± 0.11), suggesting that current templates do not fully describe the spectra of very-high- z sources. Overall, the spectroscopy solidifies photometric redshift evidence for a high spatial density of bright galaxies at z > 8 compared to theoretical model predictions, and further disfavors an accelerated decline in the integrated UV luminosity density at z > 8.

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