Bright z~9 Galaxies in Parallel: The Bright End of the Rest-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=9-10...

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Veröffentlicht in:	arXiv.org 2022-05
Hauptverfasser:	Bagley, Micaela B, Finkelstein, Steven L, Rojas-Ruiz, Sofía, Diekmann, James, Finkelstein, Keely D, Song, Mimi, Papovich, Casey, Somerville, Rachel S, Baronchelli, Ivano, Dai, Y Sophia
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Completeness Constraint modelling Contamination Galactic evolution Galaxies Gas cooling Hubble Space Telescope Infrared imaging Infrared telescopes Ionization Luminosity Parallel programming Space telescopes Star & galaxy formation Star formation
Online-Zugang:	Volltext
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