A solar metallicity galaxy at z > 7? Possible detection of the [N II] 122 mu m and [O III] 52 mu m lines
Journal article, 2023
galaxies:ISM
submillimetre:galaxies
galaxies:individual:(A1689-zD1)
ISM:abundances
galaxies:high-redshift
Author
Meghana Killi
University of Copenhagen
Darach Watson
University of Copenhagen
Seiji Fujimoto
University of Copenhagen
Hollis Akins
University of Texas
Kirsten Knudsen
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Johan Richard
Université de Lyon
Yuichi Harikane
University College London (UCL)
University of Tokyo
Dimitra Rigopoulou
European University Cyprus
University of Oxford
Francesca Rizzo
University of Copenhagen
Michele Ginolfi
University of Florence
Gergo Popping
European Southern Observatory Santiago
Vasily Kokorev
University of Copenhagen
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 521 2 2526-2534Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Probability Theory and Statistics
Fusion, Plasma and Space Physics
DOI
10.1093/mnras/stad687