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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.GA2026★ 1 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…