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JADES Dark Horse: demonstrating high-multiplex observations with JWST /NIRSpec dense-shutter spectroscopy in the JADES Origins Field

Abstract:
We present James Web Space Telescope/NIRSpec dense-shutter spectroscopy (DSS). This novel observing strategy with the NIRSpec/multi-shutter assembly (MSA) deliberately permits a high number of controlled spectral overlaps to reach extreme multiplex while retaining the low background of slit spectroscopy. In a single configuration over the JADES Origins Field, we opened shutters on all faint ( mag) candidates, prioritizing emission-line science and rejecting only bright continuum sources. Using 33.6 and 35.8 ks on-source in G235M and G395M, we observed a single mask with 850 sources, obtaining spectroscopic redshifts for 540 galaxies over . The per-configuration target density in DSS mode is 4–5 higher than standard no- and low-overlap MSA strategies (<200 sources), with no loss in redshift precision or accuracy. Line-flux sensitivities are 30 per cent lower at fixed exposure time, matching the expected increase in background noise, but the gain in survey speed is 5 in our setup, more than justifying the penalty. The measured line sensitivity exceeds NIRCam slitless spectroscopy by at least ( in exposure time) at , demonstrating that DSS is a compelling method to gain deep, wide-band spectra for large samples. Crucially, NIRSpec/MSA could deliver even higher target allocation densities than those used here. We derive H α-based star-formation rates, gas-phase metallicities (including a large sample suitable for strong-line calibrations), and identify rare mini-quenched galaxies and broad-line AGN. DSS is immediately applicable wherever deep imaging enables robust pre-selection and astrometry, providing an efficient method to obtain large samples of faint emission-line galaxies, a compelling middle ground between the completeness of slitless surveys and the sensitivity and bandwidth of NIRSpec/MSA.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stag824

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ORCID:
0000-0003-2388-8172
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ORCID:
0000-0002-7524-374X
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ORCID:
0000-0002-2929-3121
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Author
ORCID:
0000-0002-4985-3819
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Author
ORCID:
0000-0002-6719-380X


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Funder identifier:
https://ror.org/0472cxd90
Grant:
789056
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Funder identifier:
https://ror.org/03wnrjx87
Grant:
101040227
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Funder identifier:
10.13039/501100004837
Grant:
RYC2023-044853-I
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Funder identifier:
10.13039/501100001691
Grant:
24KJ0202
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Funder identifier:
https://ror.org/00znyv691
Grant:
140


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
549
Issue:
2
Pages:
stag824
Article number:
stag824
Publication date:
2026-04-30
Acceptance date:
2026-04-02
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Source identifiers:
4079596
Deposit date:
2026-05-26
ARK identifier:
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