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JADES: Probing interstellar medium conditions at <i>z</i> ∼ 5.5–9.5 with ultra-deep JWST/NIRSpec spectroscopy

Abstract:
We present emission line ratios from a sample of 26 Lyman break galaxies from $z\sim5.5-9.5$ with $-17.05.5$ spectra. We find that the emission line ratios exhibited by these $z\sim5.5-9.5$ galaxies occupy clearly distinct regions of line-ratio space compared to typical z~0-3 galaxies, instead being more consistent with extreme populations of lower-redshift galaxies. This is best illustrated by the [OIII]/[OII] ratio, tracing interstellar medium (ISM) ionisation, in which we observe more than half of our sample to have [OIII]/[OII]>10. Our high signal-to-noise spectra reveal more than an order of magnitude of scatter in line ratios such as [OII]/H$\beta$ and [OIII]/[OII], indicating significant diversity in the ISM conditions within the sample. We find no convincing detections of [NII] in our sample, either in individual galaxies, or a stack of all G395M/F290LP spectra. The emission line ratios observed in our sample are generally consistent with galaxies with extremely high ionisation parameters (log $U\sim-1.5$), and a range of metallicities spanning from $\sim0.1\times Z_\odot$ to higher than $\sim0.3\times Z_\odot$, suggesting we are probing low-metallicity systems undergoing periods of rapid star-formation, driving strong radiation fields. These results highlight the value of deep observations in constraining the properties of individual galaxies, and hence probing diversity within galaxy population.Comment: 20 pages, 9 figures, submitted to Astronomy & Astrophysics, updated values in table
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1051/0004-6361/202346107
Publication website:
http://uhra.herts.ac.uk/bitstream/2299/27372/1/aa46107-23.pdf

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Role:
Author
ORCID:
0000-0002-0450-7306
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-5333-9970
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0002-8651-9879
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Role:
Author
ORCID:
0000-0003-2388-8172
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Role:
Author
ORCID:
0000-0002-6719-380X


Publisher:
EDP Sciences
Journal:
Astronomy & Astrophysics More from this journal
Volume:
677
Pages:
A115-A115
Publication date:
2023-07-28
Acceptance date:
2023-07-17
DOI:
EISSN:
1432-0746
ISSN:
0004-6361


Language:
English
Keywords:
Pubs id:
1541184
Local pid:
pubs:1541184
Source identifiers:
W4385369331
Deposit date:
2026-05-17
ARK identifier:
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