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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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.
Radiative cooling thins hot accretion disks around black holes, reduces wind power, and makes inflow-rate decrease depend more on MRI-driven turbulence than on winds as cooling strengthens.
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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Very High Energy Gamma Rays from Ultra Fast Outflows
Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.
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Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
Radiative cooling thins hot accretion disks around black holes, reduces wind power, and makes inflow-rate decrease depend more on MRI-driven turbulence than on winds as cooling strengthens.