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astro-ph.GA2026

Coronal gas excitation as a tracer of supermassive black hole mass: on the mid-IR coronal [Ne v] lines

J. S. Elford, A. Prieto, A. Rodríguez-Ardila

Coronal lines (CL) may be a reliable proxy of supermassive black hole (SMBH) masses in active galactic nuclei (AGN) because the production of these high ionisation potential (IP) l…

astro-ph.GA20261 cited

ReveaLLAGN 1: JWST Emission-Line Spectra Reveal Low-Luminosity AGN with UV-Deficient SEDs and Warm Molecular Gas

Kameron Goold, Anil Seth, Mallory Molina +20

We present near- and mid-infrared spectra of eight Low-Luminosity Active Galactic Nuclei (LLAGN), spanning nearly four orders of magnitude in black hole mass and Eddington ratio, o…

astro-ph.GA2025

Spatially resolved circumnuclear coronal emission in nearby Seyfert galaxies

S. Comerón, A. Prieto, P. Dabhade

Coronal lines are forbidden emission lines with a ionisation potential . They are linked to energetic phenomena triggered by AGNs in the circumnuclear medium…

astro-ph.GA2025

The size of the Coronal Line Region in Active Galactic Nuclei: a MUSE perspective

A. Rodríguez-Ardila, M. A. Fonseca-Faria, L. G. Dahmer-Hahn +3

We investigated by means of MUSE/VLT observations the true size of the coronal line region (CLR) in a local sample of nine active galactic nuclei known for displaying prominent cor…

astro-ph.GA2020

Coronal Line Forest AGN I: physical properties of the emission-line regions

F. C. Cerqueira-Campos, A. Rodríguez-Ardila, R. Riffell +3

Coronal-Line Forest Active Galactic Nuclei (CLiF AGN) are characterized by strong high-ionization lines, which contrast to what is found in most AGNs. Here, we carry out a multiwav…