High-z LRDs and JWST AGN exhibit X-ray weakness consistent with local super-Eddington accreting SMBHs, supporting a link to highly accreting systems across cosmic time.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
AGN with black-hole masses above 10^8.5 solar masses may occupy halos ~0.4 dex more massive than matched control galaxies, though the difference remains consistent with uncertainties.
citing papers explorer
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The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes
High-z LRDs and JWST AGN exhibit X-ray weakness consistent with local super-Eddington accreting SMBHs, supporting a link to highly accreting systems across cosmic time.
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Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
AGN with black-hole masses above 10^8.5 solar masses may occupy halos ~0.4 dex more massive than matched control galaxies, though the difference remains consistent with uncertainties.