The Astrophysical Journal (Jan 2024)

JWST NIRSpec Spectroscopy of the Triply Lensed z = 10.17 Galaxy MACS0647–JD

  • Tiger Yu-Yang Hsiao,
  • Abdurro’uf,
  • Dan Coe,
  • Rebecca L. Larson,
  • Intae Jung,
  • Matilde Mingozzi,
  • Pratika Dayal,
  • Nimisha Kumari,
  • Vasily Kokorev,
  • Anton Vikaeus,
  • Gabriel Brammer,
  • Lukas J. Furtak,
  • Angela Adamo,
  • Felipe Andrade-Santos,
  • Jacqueline Antwi-Danso,
  • Maruša Bradač,
  • Larry D. Bradley,
  • Tom Broadhurst,
  • Adam C. Carnall,
  • Christopher J. Conselice,
  • Jose M. Diego,
  • Megan Donahue,
  • Jan J. Eldridge,
  • Seiji Fujimoto,
  • Alaina Henry,
  • Svea Hernandez,
  • Taylor A. Hutchison,
  • Bethan L. James,
  • Colin Norman,
  • Hyunbae Park,
  • Norbert Pirzkal,
  • Marc Postman,
  • Massimo Ricotti,
  • Jane R. Rigby,
  • Eros Vanzella,
  • Brian Welch,
  • Stephen M. Wilkins,
  • Rogier A. Windhorst,
  • Xinfeng Xu,
  • Erik Zackrisson,
  • Adi Zitrin

DOI
https://doi.org/10.3847/1538-4357/ad5da8
Journal volume & issue
Vol. 973, no. 1
p. 8

Abstract

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We present JWST/NIRSpec prism spectroscopy of MACS0647−JD, a triply lensed z ∼ 11 candidate discovered in Hubble Space Telescope imaging and spatially resolved by JWST imaging into two components, A and B. Spectroscopy of component A yields a spectroscopic redshift z = 10.17 based on seven detected emission lines: C iii ] λ λ 1907, 1909, [O ii ] λ 3727, [Ne iii ] λ 3869, [Ne iii ] λ 3968, H δ λ 4101, H γ λ 4340, and [O iii ] λ 4363. These are the second-most distant detections of these emission lines to date, in a galaxy observed just 460 million years after the Big Bang. Based on observed and extrapolated line flux ratios we derive a gas-phase metallicity 12 + log(O/H) ∼ 7.5–8.0, or Z ∼ (0.06–0.2) Z _⊙ , ionization parameter $\mathrm{log}(U)$ = −1.9 ± 0.2, and an ionizing photon production efficiency $\mathrm{log}({\xi }_{\mathrm{ion}})=25.2\pm 0.2\,$ erg ^−1 Hz. The spectrum has a softened Ly α break, evidence for a strong Ly α damping wing. The Ly α damping wing also suppresses the F150W photometry, explaining the slightly overestimated photometric redshift z = 10.6 ± 0.3. MACS0647−JD has a stellar mass log( M / M _⊙ ) = 8.1 ± 0.3, including ∼6 × 10 ^7 M _⊙ in component A, most of which formed recently (within ∼20 Myr) with a star formation rate ∼ 2 ± 1 M _⊙ yr ^−1 , all within an effective radius 70 ± 24 pc. Spectroscopy of a fainter companion galaxy C separated by a distance of ∼ 3 kpc reveals a Lyman break consistent with z ∼ 10.17. MACS0647−JD is likely the most distant galaxy merger known.

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