MCMC fits to accretion disk SEDs of 23 high-z blazars give black hole masses of 10^8-10^10 solar masses and Eddington ratios 0.04-1, showing that ignoring IGM attenuation overestimates masses with larger bias at higher redshift.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
verdicts
UNVERDICTED 3representative citing papers
Euclid identifies 16 massive compact galaxies with V-shaped SEDs at z>4, half as old as the universe at their redshift, mostly distinct from known AGN.
AGN obscuration classifications mismatch in ~30% of cases, with broad-line X-ray-absorbed and narrow-line X-ray-unabsorbed populations showing distinct gas-to-dust ratios and host properties, indicating obscuration arises from both orientation and multi-scale distributions.
citing papers explorer
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Black-hole mass estimation through accretion disk spectral fitting for high-redshift blazars
MCMC fits to accretion disk SEDs of 23 high-z blazars give black hole masses of 10^8-10^10 solar masses and Eddington ratios 0.04-1, showing that ignoring IGM attenuation overestimates masses with larger bias at higher redshift.
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Euclid: Scaled-up little red dots and other sources with v-shaped spectral energy distributions at z>4
Euclid identifies 16 massive compact galaxies with V-shaped SEDs at z>4, half as old as the universe at their redshift, mostly distinct from known AGN.
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AGN obscuration in optical and X-rays: Host properties and the interplay of nuclear and galactic gas and dust in a combined SDSS-XMM sample
AGN obscuration classifications mismatch in ~30% of cases, with broad-line X-ray-absorbed and narrow-line X-ray-unabsorbed populations showing distinct gas-to-dust ratios and host properties, indicating obscuration arises from both orientation and multi-scale distributions.