Characterizing the Average Interstellar Medium Conditions of Galaxies at Z ∼ 5.6–9 with Ultraviolet and Optical Nebular Lines
Weida Hu,Casey Papovich,Mark Dickinson,Robert Kennicutt,Lu Shen,Ricardo O. Amorin,Pablo Arrabal Haro,Micaela B. Bagley,Rachana Bhatawdekar,Nikko J. Cleri,Justin W. Cole,Avishai Dekel,Alexander de la Vega,Steven L. Finkelstein,Norman A. Grogin,Nimish P. Hathi,Michaela Hirschmann,Benne W. Holwerda,Taylor A. Hutchison,Intae Jung,Anton M. Koekemoer,Jeyhan S. Kartaltepe,Ray A. Lucas,Mario Llerena,S. Mascia,Bahram Mobasher,L. Napolitano,Jeffrey A. Newman,Laura Pentericci,Pablo G. Perez-Gonzalez,Jonathan R. Trump,Stephen M. Wilkins,L. Y. Aaron Yung The Astrophysical Journal（2024）
Key words
High-redshift galaxies,Galaxy chemical evolution,Emission line galaxies,Galaxy spectroscopy,Reionization
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