The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes
BibTeX Entry
@article{2026arXiv260310162T,
author = {{Tortosa}, A. and {Ricci}, C. and {Du}, P. and {Venturi}, G. and {Ho}, L. C. and {Li}, R. and {Wang}, J.-M. and {Berton}, M.},
title = {{The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies, High Energy Astrophysical Phenomena},
year = {2026},
month = mar,
eid = {arXiv:2603.10162},
pages = {arXiv:2603.10162},
archiveprefix = {arXiv},
eprint = {2603.10162},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260310162T},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {agn-dominated, jwst, sed, super-eddington, x-ray},
month_numeric = {3}
}
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