The Astrophysical Journal (Jan 2023)

Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST

  • Hollis B. Akins,
  • Caitlin M. Casey,
  • Natalie Allen,
  • Micaela B. Bagley,
  • Mark Dickinson,
  • Steven L. Finkelstein,
  • Maximilien Franco,
  • Santosh Harish,
  • Pablo Arrabal Haro,
  • Olivier Ilbert,
  • Jeyhan S. Kartaltepe,
  • Anton M. Koekemoer,
  • Daizhong Liu,
  • Arianna S. Long,
  • Henry Joy McCracken,
  • Louise Paquereau,
  • Casey Papovich,
  • Nor Pirzkal,
  • Jason Rhodes,
  • Brant E. Robertson,
  • Marko Shuntov,
  • Sune Toft,
  • Guang Yang,
  • Guillermo Barro,
  • Laura Bisigello,
  • Véronique Buat,
  • Jaclyn B. Champagne,
  • Olivia Cooper,
  • Luca Costantin,
  • Alexander de la Vega,
  • Nicole E. Drakos,
  • Andreas Faisst,
  • Adriano Fontana,
  • Seiji Fujimoto,
  • Steven Gillman,
  • Carlos Gómez-Guijarro,
  • Ghassem Gozaliasl,
  • Nimish P. Hathi,
  • Christopher C. Hayward,
  • Michaela Hirschmann,
  • Benne W. Holwerda,
  • Shuowen Jin,
  • Dale D. Kocevski,
  • Vasily Kokorev,
  • Erini Lambrides,
  • Ray A. Lucas,
  • Georgios E. Magdis,
  • Benjamin Magnelli,
  • Jed McKinney,
  • Bahram Mobasher,
  • Pablo G. Pérez-González,
  • R. Michael Rich,
  • Lise-Marie Seillé,
  • Margherita Talia,
  • C. Megan Urry,
  • Francesco Valentino,
  • Katherine E. Whitaker,
  • L. Y. Aaron Yung,
  • Jorge Zavala,
  • the COSMOS-Web and CEERS teams

DOI
https://doi.org/10.3847/1538-4357/acef21
Journal volume & issue
Vol. 956, no. 1
p. 61

Abstract

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We present a search for extremely red, dust-obscured, z > 7 galaxies with JWST/NIRCam+MIRI imaging over the first 20 arcmin ^2 of publicly available Cycle 1 data from the COSMOS-Web, CEERS, and PRIMER surveys. Based on their red color in F277W−F444W (∼2.5 mag) and detection in MIRI/F770W (∼25 mag), we identify two galaxies, COS-z8M1 and CEERS-z7M1, that have best-fit photometric redshifts of $z={8.4}_{-0.4}^{+0.3}$ and ${7.6}_{-0.1}^{+0.1}$ , respectively. We perform spectral energy distribution fitting with a variety of codes (including bagpipes , prospector , beagle , and cigale ) and find a >95% probability that these indeed lie at z > 7. Both sources are compact ( R _eff ≲ 200 pc) and highly obscured ( A _V ∼ 1.5–2.5) and, at our best-fit redshift estimates, likely have strong [O iii ]+H β emission contributing to their 4.4 μ m photometry. We estimate stellar masses of ∼10 ^10 M _⊙ for both sources; by virtue of detection in MIRI at 7.7 μ m, these measurements are robust to the inclusion of bright emission lines, for example, from an active galactic nucleus. We identify a marginal (2.9 σ ) Atacama Large Millimeter/submillimeter Array detection at 2 mm within 0.″5 of COS-z8M1, which, if real, would suggest a remarkably high IR luminosity of ∼10 ^12 L _⊙ . These two galaxies, if confirmed at z ∼ 8, would be extreme in their stellar and dust masses and may be representative of a substantial population of highly dust-obscured galaxies at cosmic dawn.

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