Using ray-tracing simulations and simulation-based inference, the authors construct an AGN population that reproduces the cosmic X-ray background, number counts, and absorption properties, deriving an intrinsic Compton-thick fraction of 40±3%.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Radiative feedback from disk-reprocessed soft photons produces limit-cycle oscillations whose frequency and spectra match observed type-C QPOs in black-hole X-ray binaries for suitable coronal parameters.
citing papers explorer
-
Population synthesis of active galactic nuclei based on the radiation-regulated unification model
Using ray-tracing simulations and simulation-based inference, the authors construct an AGN population that reproduces the cosmic X-ray background, number counts, and absorption properties, deriving an intrinsic Compton-thick fraction of 40±3%.
-
Radiative feedbacks as drivers for quasi-periodic-oscillation activity in black-hole X-ray binaries
Radiative feedback from disk-reprocessed soft photons produces limit-cycle oscillations whose frequency and spectra match observed type-C QPOs in black-hole X-ray binaries for suitable coronal parameters.