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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
X-ray AGN at intermediate redshifts live in dark matter halos of mass ~10^13 solar masses with no significant dependence on black hole mass, Eddington ratio or X-ray luminosity.
citing papers explorer
-
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.
-
Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
X-ray AGN at intermediate redshifts live in dark matter halos of mass ~10^13 solar masses with no significant dependence on black hole mass, Eddington ratio or X-ray luminosity.