Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic stars Article Swipe
Sandro Tacchella
,
William McClymont
,
Jan Scholtz
,
R. Maiolino
,
Xihan Ji
,
Natalia C. Villanueva
,
S. Charlot
,
Francesco D’Eugenio
,
Jakob M. Helton
,
Christina C. Williams
,
Joris Witstok
,
Rachana Bhatawdekar
,
Stefano Carniani
,
Jacopo Chevallard
,
Mirko Curti
,
Kevin Hainline
,
Zhiyuan Ji
,
Benjamin D. Johnson
,
Joel Leja
,
Yijia Li
,
Michael V. Maseda
,
Dávid Puskás
,
Marcia Rieke
,
Brant Robertson
,
Irene Shivaei
,
Maddie S. Silcock
,
Charlotte Simmonds
,
Hannah Übler
,
Christopher N. A. Willmer
,
Chris J. Willott
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staf718
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staf718
Understanding the sources that power nebular emission in high-redshift galaxies is fundamentally important not only for shedding light on to the drivers of reionization, but to constrain stellar populations and the growth of black holes. Here, we focus on an individual object, GS9422, a galaxy at $z_{\rm spec}=5.943$ with exquisite data from the JWST Advanced Deep Extragalactic Survey (JADES), JWST Extragalactic Medium-band Survey (JEMS), and First Reionization Epoch Spectroscopically Complete Observations (FRESCO) surveys, including 14-band JWST/NIRCam photometry and deep NIRSpec prism and grating spectroscopy. We map the continuum emission and nebular emission lines across the galaxy on 0.2-kpc scales. GS9422 has been claimed to have nebular-dominated continuum and an extreme stellar population with top-heavy initial mass function. We find clear evidence for different morphologies in the emission lines, the rest-ultraviolet and rest-optical continuum emission, demonstrating that the full continuum cannot be dominated by nebular emission. While multiple models reproduce the spectrum reasonably well, our preferred model with a type-2 active galactic nucleus (AGN) and local damped Ly$\alpha$ (DLA) clouds can explain both the spectrum and the wavelength-dependent morphology. The AGN powers the off-planar nebular emission, giving rise to the Balmer jump and the emission lines, including Ly$\alpha$, which therefore does not suffer DLA absorption. A central, young stellar component dominates the rest-UV emission and – together with the DLA clouds – leads to a spectral turn over. A disc-like, older stellar component explains the flattened morphology in the rest-optical continuum. We conclude that GS9422 is consistent with being a normal galaxy with an obscured, type-2 AGN – a simple scenario, without the need for exotic stellar populations.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/staf718
- https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staf718/63039547/staf718.pdf
- OA Status
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- Cited By
- 10
- References
- 137
- Related Works
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- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4410019022Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/staf718Digital Object Identifier
- Title
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Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic starsWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-04-30Full publication date if available
- Authors
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Sandro Tacchella, William McClymont, Jan Scholtz, R. Maiolino, Xihan Ji, Natalia C. Villanueva, S. Charlot, Francesco D’Eugenio, Jakob M. Helton, Christina C. Williams, Joris Witstok, Rachana Bhatawdekar, Stefano Carniani, Jacopo Chevallard, Mirko Curti, Kevin Hainline, Zhiyuan Ji, Benjamin D. Johnson, Joel Leja, Yijia Li, Michael V. Maseda, Dávid Puskás, Marcia Rieke, Brant Robertson, Irene Shivaei, Maddie S. Silcock, Charlotte Simmonds, Hannah Übler, Christopher N. A. Willmer, Chris J. WillottList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/staf718Publisher landing page
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staf718/63039547/staf718.pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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goldOpen access status per OpenAlex
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staf718/63039547/staf718.pdfDirect OA link when available
- Concepts
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10Total citation count in OpenAlex
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2025: 10Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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