The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?
Scuola Normale Superiore · University of Cambridge · +17 more institutions
Abstract
JADES-GS-z14-0 is the most distant spectroscopically confirmed galaxy yet, at z ≳14. With a UV magnitude of –20.81, it is one of the most luminous galaxies at cosmic dawn and its half-light radius of 260 pc means that stars dominate the observed UV emission. We report the Atacama Large Millimeter/submillimeter Array (ALMA) detection of [O III ]88 μm line emission with a significance of 6.67 σ and at a frequency of 223.524 GHz, corresponding to a redshift of 14.1796±0.0007, which is consistent with the candidate C III ] line detected in the NIRSpec spectrum. At this spectroscopic redshift, the Lyman- α break identified with NIRSpec requires a damped Lyman- α absorber with a column density of log( N HI /cm −2 )…
Citation impact
- FWCI
- 43.49
- Percentile
- 100%
- References
- 96
Authors
28Topics & keywords
- Physics
- Astrophysics
- Reionization
- Galaxy
- Redshift
- Metallicity
- Submillimeter Array
- Quasar
- Affordable and clean energy
Funding
- NSNational Science FoundationAwards: AST 1828315, 1828315
- UOUniversity of California, Santa CruzAward: 1828315
- URUK Research and InnovationAward: 101040227
- NRNational Radio Astronomy Observatory
- ECEuropean CommissionAwards: 789056, 695671, 101040227
- NRNational Research Foundation
- DGDanmarks Grundforskningsfond
- NSNational Science Council
- INIsaac Newton Trust
- NANational Astronomical Observatory of Japan
- SAScience and Technology Facilities CouncilAwards: NAS5-02015, 695671
- NINational Institutes of Natural Sciences