The Astrophysical Journal (Jan 2023)

JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr after the Big Bang

  • Sandro Tacchella,
  • Daniel J. Eisenstein,
  • Kevin Hainline,
  • Benjamin D. Johnson,
  • William M. Baker,
  • Jakob M. Helton,
  • Brant Robertson,
  • Katherine A. Suess,
  • Zuyi Chen,
  • Erica Nelson,
  • Dávid Puskás,
  • Fengwu Sun,
  • Stacey Alberts,
  • Eiichi Egami,
  • Ryan Hausen,
  • George Rieke,
  • Marcia Rieke,
  • Irene Shivaei,
  • Christina C. Williams,
  • Christopher N. A. Willmer,
  • Andrew Bunker,
  • Alex J. Cameron,
  • Stefano Carniani,
  • Stephane Charlot,
  • Mirko Curti,
  • Emma Curtis-Lake,
  • Tobias J. Looser,
  • Roberto Maiolino,
  • Michael V. Maseda,
  • Tim Rawle,
  • Hans-Walter Rix,
  • Renske Smit,
  • Hannah Übler,
  • Chris Willott,
  • Joris Witstok,
  • Stefi Baum,
  • Rachana Bhatawdekar,
  • Kristan Boyett,
  • A. Lola Danhaive,
  • Anna de Graaff,
  • Ryan Endsley,
  • Zhiyuan Ji,
  • Jianwei Lyu,
  • Lester Sandles,
  • Aayush Saxena,
  • Jan Scholtz,
  • Michael W. Topping,
  • Lily Whitler

DOI
https://doi.org/10.3847/1538-4357/acdbc6
Journal volume & issue
Vol. 952, no. 1
p. 74

Abstract

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We present JWST NIRCam nine-band near-infrared imaging of the luminous z = 10.6 galaxy GN-z11 from the JWST Advanced Deep Extragalactic Survey of the GOODS-N field. We find a spectral energy distribution (SED) entirely consistent with the expected form of a high-redshift galaxy: a clear blue continuum from 1.5 to 4 μ m with a complete dropout in F115W. The core of GN-z11 is extremely compact in JWST imaging. We analyze the image with a two-component model, using a point source and a Sérsic profile that fits to a half-light radius of 200 pc and an index n = 0.9. We find a low-surface-brightness haze about 0.″4 to the northeast of the galaxy, which is most likely a foreground object but might be a more extended component of GN-z11. At a spectroscopic redshift of 10.60 (Bunker et al. 2023 ), the comparison of the NIRCam F410M and F444W images spans the Balmer jump. From population-synthesis modeling, here assuming no light from an active galactic nucleus, we reproduce the SED of GN-z11, finding a stellar mass of ∼10 ^9 M _⊙ , a star formation rate of ∼20 M _⊙ yr ^−1 , and a young stellar age of ∼20 Myr. Since massive galaxies at high redshift are likely to be highly clustered, we search for faint neighbors of GN-z11, finding nine galaxies out to ∼5 comoving Mpc transverse with photometric redshifts consistent with z = 10.6, and a tenth more tentative dropout only 3″ away. This is consistent with GN-z11 being hosted by a massive dark-matter halo (≈8 × 10 ^10 M _⊙ ), though lower halo masses cannot be ruled out.

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