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Metal enrichment and evolution in four <i>z</i> &gt; 6.5 quasar sightlines observed with JWST/NIRSpec

Abstract:
We present JWST/NIRSpec R$\approx$2700 spectra of four high-redshift quasars: VDES J0020-3653 (z = 6.860), DELS J0411-0907(z = 6.825), UHS J0439+1634 (z = 6.519) and ULAS J1342+0928 (z = 7.535). The exquisite data quality, signal-to-noise ratio of 50-200, and large $0.86\!~\mu{\rm m}\le \lambda \le 5.5\!~\mu{\rm m}$ spectral coverage allows us to identify between 13 and 17 intervening and proximate metal absorption line systems in each quasar spectrum, with a total number of 61 absorption-line systems detected at $2.426$ and find: i) A continued increase of the low-ionization OI, CII, and SiII incidence, ii) Decreasing high-ionization CIV and SiIV incidence with a transition from predominantly high- to low-ionization at $z\approx6.0$, and iii) a constant MgII incidence across all redshifts. The observations support a change in the ionization state of the intergalactic medium in the EoR rather than a change in metallicity. The abundance ratio of [Si/O] in five $z>6$ absorption systems show enrichment signatures produced by low-mass Pop III pair instability supernovae, and possibly Pop III hypernovae. In the Gunn-Peterson troughs we detect transmission spikes where Ly$\alpha$ photons can escape. From 22 absorption systems at $z>5.7$, only a single low-ionization system out of 13 lies within 2000 km s$^{-1}$ from a spike, while four high-ionization systems out of nine lie within $\sim$2000 km s$^{-1}$ from a spike. This confirms that galaxies responsible for the heavy elements that are transported into the circumgalactic medium lie in predominantly in high-density, neutral environments, while lower density environments are ionized without being polluted by metals at $z\approx$ 6-7. [abridged]Comment: 50 pages including 30 pages of appendices. Submitted to A&
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1051/0004-6361/202347943
Publication website:
https://hal.science/hal-04776982v1/file/aa47943-23.pdf

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Role:
Author
ORCID:
0000-0001-8415-7547
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Role:
Author
ORCID:
0000-0002-6780-2441
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Role:
Author
ORCID:
0000-0002-4201-7367
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Author
ORCID:
0000-0001-7997-1640
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0002-8651-9879


Publisher:
EDP Sciences
Journal:
Astronomy & Astrophysics More from this journal
Volume:
680
Pages:
A82-A82
Publication date:
2023-10-19
Acceptance date:
2023-10-11
DOI:
EISSN:
1432-0746
ISSN:
0004-6361


Language:
English
Keywords:
Pubs id:
1599236
Local pid:
pubs:1599236
Source identifiers:
W4387770588
Deposit date:
2026-06-05
ARK identifier:
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