A bias-controlled quasar sample of ~2000 objects demonstrates that the X-ray-to-UV luminosity relation remains constant from redshift 0.7 to 5.
2025b, MNRAS
2 Pith papers cite this work. Polarity classification is still indexing.
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A LambdaCDM black hole growth model predicts that observed high-redshift Little Red Dots are the luminous tip of a larger population undergoing super-Eddington accretion in nuclear bursts.
citing papers explorer
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The X-ray-to-UV relation does not evolve in homogeneous quasar samples
A bias-controlled quasar sample of ~2000 objects demonstrates that the X-ray-to-UV luminosity relation remains constant from redshift 0.7 to 5.
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Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots
A LambdaCDM black hole growth model predicts that observed high-redshift Little Red Dots are the luminous tip of a larger population undergoing super-Eddington accretion in nuclear bursts.