Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass
BibTeX Entry
@article{2026arXiv260602773Z,
author = {{Zhang}, Chenxuan and {Zhang}, Huanian and {Wu}, Qingwen and {Ho}, Luis C. and {Wang}, Jian-Min},
title = {{Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies},
year = {2026},
month = jun,
eid = {arXiv:2606.02773},
pages = {arXiv:2606.02773},
doi = {10.48550/arXiv.2606.02773},
archiveprefix = {arXiv},
eprint = {2606.02773},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260602773Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {abundance, black hole mass, clustering, host galaxy},
month_numeric = {6}
}
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