Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots
BibTeX Entry
@article{2025arXiv250603244P,
author = {{Pacucci}, Fabio and {Loeb}, Abraham},
title = {{Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena},
year = {2025},
month = jun,
eid = {arXiv:2506.03244},
pages = {arXiv:2506.03244},
archiveprefix = {arXiv},
eprint = {2506.03244},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250603244P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {clustering, early universe, jwst, morphology, theory},
month_numeric = {6}
}
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