Disentangling accretion disk and dust emissions in the infrared spectrum of type 1 AGN
Antonio Hern\'an-Caballero, Evanthia Hatziminaoglou, Almudena, Alonso-Herrero, Silvia Mateos

TL;DR
This study models the infrared spectrum of type 1 AGN, disentangling accretion disk and dust emissions, revealing their uniformity and providing templates applicable to both quasars and Seyfert galaxies.
Contribution
It introduces a semi-empirical model that separates and characterizes the accretion disk and dust emissions in AGN spectra, creating universal templates for the 1-10um range.
Findings
Disk and dust components are remarkably uniform among quasars.
Differences in SEDs are mainly due to obscuration and luminosity ratios.
Templates successfully reproduce spectra of local Seyfert 1 galaxies.
Abstract
We use a semi-empirical model to reproduce the 0.1-10um spectral energy distribution (SED) of a sample of 85 luminous quasars. In the model, the continuum emission from the accretion disk as well as the nebular lines are represented by a single empirical template (disk), where differences in the optical spectral index are reproduced by varying the amount of extinction. The near- and mid-infrared emission of the AGN-heated dust is modelled as the combination of two black-bodies (dust). The model fitting shows that the disk and dust components are remarkably uniform among individual quasars, with differences in the observed SED largely accounted for by varying levels of obscuration in the disk as well as differences in the relative luminosity of the disk and dust components. By combining the disk-subtracted SEDs of the 85 quasars, we generate a template for the 1-10um emission of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
