Characterizing the Average Interstellar Medium Conditions of Galaxies at z ∼ 5.6–9 with Ultraviolet and Optical Nebular Lines

Characterizing the Average Interstellar Medium Conditions of Galaxies at z ∼ 5.6–9 with Ultraviolet and Optical Nebular Lines

Ultraviolet (UV; rest-frame ∼1200–2000 Å) spectra provide a wealth of diagnostics to characterize fundamental galaxy properties, such as their chemical enrichment, the nature of their stellar populations, and their amount of Lyman-continuum (LyC) radiation. In this work, we leverage publicly release...

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Bibliographic Details
Main Authors: Weida Hu, Casey Papovich, Mark Dickinson, Robert Kennicutt, Lu Shen, Ricardo O. Amorín, 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. Pérez-González, Jonathan R. Trump, Stephen M. Wilkins, L. Y. Aaron Yung
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
High-redshift galaxies
Galaxy chemical evolution
Emission line galaxies
Galaxy spectroscopy
Reionization
Online Access:https://doi.org/10.3847/1538-4357/ad5015

Internet

https://doi.org/10.3847/1538-4357/ad5015

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