Unveiling the Dark Side of Ultraviolet/Optical Bright Galaxies: Optically Thick Dust Absorption

Over the past decades, a population of galaxies invisible in optical/near-infrared (NIR), but bright at longer wavelengths, have been identified through color selections. These so-called optically faint/dark galaxies are considered to be massive quiescent galaxies or highly dust-attenuated galaxies....

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Bibliographic Details
Main Authors:	Yingjie Cheng, Mauro Giavalisco, Bren E. Backhaus, Rachana Bhatawdekar, Nikko J. Cleri, Luca Costantin, Emanuele Daddi, Mark Dickinson, Steven L. Finkelstein, Michaela Hirschmann, Benne W. Holwerda, Anton M. Koekemoer, Ray A. Lucas, Fabio Pacucci, Pablo G. Pérez-González, Giulia Rodighiero, Lise-Marie Seillé, Katherine E. Whitaker, L. Y. Aaron Yung, Pablo Arrabal Haro, Micaela B. Bagley, Jeyhan S. Kartaltepe, Casey Papovich, Nor Pirzkal
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal
Subjects:	High-redshift galaxies James Webb Space Telescope Star formation Interstellar dust extinction Spectral energy distribution
Online Access:	https://doi.org/10.3847/1538-4357/ad9909
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Unveiling the Dark Side of Ultraviolet/Optical Bright Galaxies: Optically Thick Dust Absorption

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