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

Abstract 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 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi>U</mml:mi> <mml:mo stretchy="false">)</mml:mo> </mml:math> = −1.9 ± 0.2, and an ionizing photon production efficiency <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>ξ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>ion</mml:mi> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>=</mml:mo> <mml:mn>25.2</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.2</mml:mn> <mml:mspace width="0.25em"/> </mml:math> 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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Journal
The Astrophysical Journal
Published
2024-09-01
DOI
https://doi.org/10.3847/1538-4357/ad5da8
Citations
65
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
21.22

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article

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

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65 citations
The Astrophysical Journal
Stellar, planetary, and galactic studies
21.22
article

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

Matilde Mingozzi, Pratika Dayal, Nimisha Kumari, Seiji Fujimoto, Colin Norman, Adam C. Carnall, Stephen M. Wilkins, Maruša Bradač, Massimo Ricotti, Lukas J. Furtak, Intae Jung, Rogier A. Windhorst, Vasily Kokorev, Tom Broadhurst, Rebecca L. Larson, Anton Vikaeus, Bethan L. James, Christopher J. Conselice, Erik Zackrisson, Brian Welch, Angela Adamo, Svea Hernández, Larry Bradley, Dan Coe, Jacqueline Antwi-Danso, Tiger Yu-Yang Hsiao, Marc Postman, Nor Pirzkal, Hyunbae Park, Xinfeng Xu, E. Vanzella, Megan Donahue, Gabriel Brammer, J. J. Eldridge, Jane R. Rigby, Taylor A. Hutchison, Adi Zitrin, J. M. Diego, Alaina Henry, Felipe Andrade-Santos, no-firstname Abdurro’uf
article en
65 citations

Abstract

Abstract 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 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi>U</mml:mi> <mml:mo stretchy="false">)</mml:mo> </mml:math> = −1.9 ± 0.2, and an ionizing photon production efficiency <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>ξ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>ion</mml:mi> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>=</mml:mo> <mml:mn>25.2</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.2</mml:mn> <mml:mspace width="0.25em"/> </mml:math> 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.

The Astrophysical JournalVol. 973(1)
Damien Foundation (BD)
National Science Foundation, National Aeronautics and Space Administration, Oak Ridge Associated Universities, Space Telescope Science Institute, Leverhulme Trust, European Commission, National Research Foundation, Rijksuniversiteit Groningen, Danmarks Grundforskningsfond, United States-Israel Binational Science Foundation, Swedish National Space Agency, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Ministero dell’Istruzione, dell’Università e della Ricerca, Javna Agencija za Raziskovalno Dejavnost RS, Vetenskapsrådet, Goddard Space Flight Center, Science and Technology Facilities Council
Openalex Percentile: Top 0%
Stellar, planetary, and galactic studies
21.22
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