Bright z ∼ 9 Galaxies in Parallel: The Bright End of the Rest-frame UV Luminosity Function from HST Parallel Programs

The abundance of bright galaxies at z > 8 can provide key constraints on models of galaxy formation and evolution, as the predicted abundance varies greatly when different physical prescriptions for gas cooling and star formation are implemented. We present the results of a search for bright z ∼...

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Bibliographic Details
Main Authors: Micaela B. Bagley, Steven L. Finkelstein, Sofía Rojas-Ruiz, James Diekmann, Keely D. Finkelstein, Mimi Song, Casey Papovich, Rachel S. Somerville, Ivano Baronchelli, Y. Sophia Dai
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad09dc