MétaCan
Menu
← Back to cohort
Record W4416719759 · doi:10.1093/mnras/staf2107

JADES: carbon-enhanced, nitrogen-normal compact galaxy at z = 11.2

2025· article· en· W4416719759 on OpenAlexaff
Jan Scholtz, Maddie S. Silcock, Emma Curtis-Lake, R. Maiolino, Stefano Carniani, Francesco D’Eugenio, Xihan Ji, P. Jakobsen, Kevin Hainline, Santiago Arribas, William Baker, Rachana Bhatawdekar, A. J. Bunker, S. Charlot, Jacopo Chevallard, Mirko Curti, Daniel J. Eisenstein, Yuki Isobe, Gareth C. Jones, Eleonora Parlanti, Pablo G. Pérez‐González, Pierluigi Rinaldi, Brant Robertson, Sandro Tacchella, Hannah Übler, Christina C. Williams, Chris J. Willott, Joris Witstok

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsHerzberg Institute of Astrophysics
FundersH2020 European Research CouncilAgencia Estatal de InvestigaciónJapan Society for the Promotion of ScienceMinisterio de Ciencia e InnovaciónEuropean CommissionScience and Technology Facilities CouncilNational Research FoundationUK Research and InnovationSpace Telescope Science InstituteDanmarks GrundforskningsfondUniversity of ArizonaUniversity of California, Santa CruzNational Aeronautics and Space AdministrationVillum FondenNational Science Foundation
KeywordsGalaxyMetallicityStarsActive galactic nucleusInterstellar mediumUniverseEquivalent widthRADIUSInteracting galaxy

Abstract

fetched live from OpenAlex

ABSTRACT Over the past few years James Webb Space Telescope (JWST) has been a major workhorse in detecting and constraining the metal enrichment of the first galaxies in the early Universe and finding the source of the ionization of their interstellar medium. In this work, we present new deep JWST/NIRSpec spectroscopy of GS-z11-1, a galaxy at z = 11.28, in which we report the detection of multiple rest-frame UV and optical emission lines: CIII]$\lambda \lambda$1907,09, CIV]$\lambda \lambda$1548,51, [OII]$\lambda \lambda$3726,29, [NeIII]$\lambda$3869, H$\gamma$ and tentative evidence for HeII$\lambda$1640. The ionization properties of GS-z11-1 are consistent with star formation, with potential contribution from an active galactic nucleus (AGN). We estimate a galaxy stellar mass of log($\rm{M_{\star }}$/M$_{\odot }$) = 7.8$\, \pm\, $0.2 and log(SFR/(M$_{\odot }$ yr$^{-1}$)) = 0.32$\, \pm \,$0.11 for the fiducial SF-only models. We measured C/O from the SED modelling of C/O = 1.20$\pm 0.15 \times$ solar. This is one of the highest C/O abundances at z $\, > \, $ 10, and it is consistent with either PopII and PopIII enrichment paths. Despite this source being extremely compact, with a half-light radius of 73 $\, \pm \,$ 10 pc, we see no increased equivalent width of NIV] and NIII] emission lines as seen in some other compact sources at similar redshifts, a potential signature of second-generation stars in GCs. Overall, this galaxy exhibits low metallicity and high ionization parameter consistent with intense star-formation or AGN activity in the early Universe, possibly observed before the enrichment by the second generation of stars in proto-globular clusters in the core of the galaxy.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.007
Threshold uncertainty score0.013

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0040.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.005
GPT teacher head0.200
Teacher spread0.195 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations3
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→