Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. VII. Testing Disk-Corona Diagnostics with eROSITA
astro-ph.GA, astro-ph.HE
Submitted: 2026-10-07
Updated: 2026-10-07
Comments: 17 pages, 9 figures. Accepted for publication in MNRAS
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- Using Faded Changing-Look Quasars to Unveil the Spectral Energy Distribution Evolution of Low-Luminosity Active Galactic Nuclei
- A New Record Census of Dwarf AGN and a Bimodal M BH - M Scaling Relation with DESI DR1
- The Einstein Probe Mission
- Science objectives of the Einstein Probe mission
- 22 Newly Identified Repeating Changing-look AGNs and Evidence for Extreme Broad-line Region Breathing
Related papers
- Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
- Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
- Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
- Deriving volume density profiles of filaments from observed surface densities
- Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
- MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies