A New Hope for AGN SED Fitting: X-Ray Spectral Analysis of 12MGS AGN with the C2PO-Torus Model

arXiv:2609.38350 · astro-ph.GA · Submitted 2026-09-29 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-29

Updated: 2026-09-29

Comments: Accepted for publication by MNRAS. 27 pages, 12 figures, 5 tables

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• AGN — 117× in this paper · explained in 1 episode
• Abundance — 11× in this paper · explained in 1 episode
• Chandra X-ray Center — 4× in this paper
• Calibration — 3× in this paper · explained in 7 episodes
• Active Galactic Nuclei (AGN) — 2× in this paper · explained in 1 episode
• Trace — 2× in this paper · explained in 2 episodes
• Computational Biology — 1× in this paper · explained in 2 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• InterUniversity Institute for Data Intensive Astronomy — 1× in this paper
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Society of PhotoOptical Instrumentation Engineers — 1× in this paper
• Southern African Large Telescope — 1× in this paper

Sources

• In-flight PSF calibration of the NuSTAR hard X-ray optics
• X-ray perspective of Narrow-line Seyfert 1 galaxies
• Data analysis recipes: Fitting a model to data
• 3D Radiative Transfer Modeling of Clumpy Dust Tori Around AGN
• Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS
• Chandra X-Ray Observatory (CXO):Overview
• Science with the X-ray Imaging and Spectroscopy Mission (XRISM)

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