On The Origins Of Oxygen: ALMA And JWST Characterise The Multi-phase, Metal-enriched, Star-bursting Medium Within A ‘Normal’ z>11 Galaxy

The unexpectedly high abundance of galaxies at z>11 revealed by JWST has sparked a debate on the nature of early galaxies and the physical mechanisms regulating their formation.
The Atacama Large Millimeter/submillimeter Array (ALMA) has begun to provide vital insights on their gas and dust content, but so far only for extreme ‘blue monsters’. Here we present new, deep ALMA observations of JADES-GS-z11-0, a more typical (sub-L∗) z>11 galaxy that bridges the discovery space of JWST and the Hubble Space Telescope.
These data confirm the presence of the [O III] 88 μm line at 4.5σ significance, precisely at the redshift of several faint emission lines previously seen with JWST/NIRSpec, while the underlying dust continuum remains undetected (Fν<9.0μJy), implying an obscured star formation rate (SFR) of SFRIR≲6M⊙yr−1 and dust mass of Mdust≲1.0×106M⊙ (all 3σ).
The accurate ALMA redshift of z[O III]=11.1221±0.0006 (≳5× refined over NIRSpec) helps confirm that redshifts measured purely from the Lyman-α break, even spectroscopically, should properly take into account the effects of potential damped Lyman-α absorption (DLA) systems to avoid systematic overestimates of up to Δz≈0.5. The [O III] 88 μm luminosity of L[O III]=(1.0±0.3)×108L⊙, meanwhile, agrees well with the scaling relation for local metal-poor dwarfs given the SFR measured by NIRCam, NIRSpec, and MIRI.
The spatially resolved MIRI and ALMA emission also underscores that JADES-GS-z11-0 is likely to consist of two low-mass components that are undergoing strong bursts of star formation yet are already pre-enriched in oxygen (~30% solar), only 400 Myr after the Big Bang.
Joris Witstok, Renske Smit, William M. Baker, Pierluigi Rinaldi, Kevin N. Hainline, Hiddo S. B. Algera, Santiago Arribas, Tom J. L. C. Bakx, Andrew J. Bunker, Stefano Carniani, Stéphane Charlot, Jacopo Chevallard, Mirko Curti, Emma Curtis-Lake, Daniel J. Eisenstein, Kasper E. Heintz, Jakob M. Helton, Gareth C. Jones, Roberto Maiolino, Michael V. Maseda, Pablo G. Pérez-González, Clara L. Pollock, Brant E. Robertson, Aayush Saxena, Jan Scholtz, Irene Shivaei, Fengwu Sun, Sandro Tacchella, Hannah Übler, Darach Watson, Chris J. Willott, Zihao Wu
Comments: 22 pages, 9 figures, 4 tables. Submitted to the Open Journal of Astrophysics
Subjects: Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2507.22888 [astro-ph.GA] (or arXiv:2507.22888v1 [astro-ph.GA] for this version)
https://doi.org/10.48550/arXiv.2507.22888
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From: Joris Witstok
[v1] Wed, 30 Jul 2025 17:59:56 UTC (3,925 KB)
https://arxiv.org/abs/2507.22888
Astrobiology, Astronomy, Astrochemistry,