The 2MIG isolated AGNs -- 4. Linking hot-dust reverberation to spectroscopically predicted BLR scales in IC 5287 and Mrk 845

arXiv:2609.35306 · astro-ph.GA, astro-ph.IM · Submitted 2026-09-28 · Read on arXiv

astro-ph.GA, astro-ph.IM

Submitted: 2026-09-28

Updated: 2026-09-28

Terminology

• AGN — 64× in this paper · explained in 1 episode
• Robustness — 19× in this paper · explained in 5 episodes
• Aperture — 11× in this paper · explained in 1 episode
• Calibration — 9× in this paper · explained in 7 episodes
• Consistency — 4× in this paper · explained in 3 episodes
• Core — 4× in this paper · explained in 2 episodes
• Velocity Dispersion — 4× in this paper · explained in 2 episodes
• Monte Carlo Analysis — 3× in this paper · explained in 2 episodes
• Aperture Photometry — 2× in this paper · explained in 1 episode
• Trace — 2× in this paper · explained in 2 episodes
• Sloan Digital Sky Survey — 1× in this paper

Sources

• The 2MIG isolated AGNs. 3. Optical--IR variability and dust reverberation in the NLSy1 galaxies Mrk~42 and Mrk~493
• Milky Way Near Twins (MWNeTs). I. A Hierarchical Framework for Identifying Candidate Evolutionary Counterparts of the Milky Way

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