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This article has been cited by the following article(s):
Evolution of the UV slope of galaxies at cosmic morning (z > 4): The properties of extremely blue galaxies
D. Dottorini, A. Calabrò, L. Pentericci, S. Mascia, M. Llerena, L. Napolitano, P. Santini, G. Roberts-Borsani, M. Castellano, R. Amorin, M. Dickinson, A. Fontana, N. Hathi, M. Hirschmann, A. M. Koekemoer, R. A. Lucas, E. Merlin, A. Morales, F. Pacucci, S. Wilkins, P. Arrabal Haro, M. Bagley, S. L. Finkelstein, J. Kartaltepe, C. Papovich and N. Pirzkal Astronomy & Astrophysics 698 A234 (2025) https://doi.org/10.1051/0004-6361/202453267
The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization