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JWST NIRSpec spectroscopy of the triply lensed z = 10.17 galaxy MACS0647–JD
ID
Hsiao, Yu-Yang Tiger
(
Author
),
ID
Abdurro'uf
(
Author
),
ID
Coe, Dan
(
Author
),
ID
Larson, Rebecca L.
(
Author
),
ID
Jung, Intae
(
Author
),
ID
Bradač, Maruša
(
Author
)
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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] λλ1907, 1909, [O II] λ3727, [Ne III] λ3869, [Ne III] λ3968, Hδ λ4101, Hγ λ4340, and [O III] λ4363. 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) Ze, ionization parameter log(U) = −1.9 ± 0.2, and an ionizing photon production efficiency log 25.2 ± 0.2 erg-1 Hz. The spectrum has a softened Lyα break, evidence for a strong Lyα damping wing. The Lyα 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/Me) = 8.1 ± 0.3, including ∼6 × 10 7 Me in component A, most of which formed recently (within ∼20 Myr) with a star formation rate ∼ 2 ± 1 Me 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.
Language:
English
Keywords:
galaxies
,
high-redshift galaxies
,
early universe
,
strong gravitational lensing
,
galaxy spectroscopy
,
reionization
Work type:
Article
Typology:
1.01 - Original Scientific Article
Organization:
FMF - Faculty of Mathematics and Physics
Publication status:
Published
Publication version:
Version of Record
Year:
2024
Number of pages:
16 str.
Numbering:
Vol. 973, art. A8
PID:
20.500.12556/RUL-162192
UDC:
524.8
ISSN on article:
1538-4357
DOI:
10.3847/1538-4357/ad5da8
COBISS.SI-ID:
208089091
Publication date in RUL:
19.09.2024
Views:
171
Downloads:
33
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Record is a part of a journal
Title:
The Astrophysical journal
Shortened title:
Astrophys. j.
Publisher:
University of Chicago Press for the American Astronomical Society
ISSN:
1538-4357
COBISS.SI-ID:
515079705
Licences
License:
CC BY 4.0, Creative Commons Attribution 4.0 International
Link:
http://creativecommons.org/licenses/by/4.0/
Description:
This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.
Projects
Funder:
ARIS - Slovenian Research and Innovation Agency
Project number:
N1-0238-2022
Name:
Raziskave kozmične zore z James Webb vesoljskim teleskopom
Funder:
NSF - National Science Foundation
Project number:
2109066
Name:
NSF-BSF: Galaxies in the Reionization Era
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