The WISE view of the disc-torus connection in z~0.6 Active Galactic Nuclei
Giorgio Calderone, Tullia Sbarrato, Gabriele Ghisellini

TL;DR
This study analyzes a large sample of radio-quiet AGN at z~0.6 using WISE infrared data to investigate the disc-torus connection, revealing that the torus reprocesses about one-third to one-half of the accretion disc luminosity.
Contribution
It provides the largest IR-based analysis of the disc-torus connection in AGN at this redshift, quantifying the reprocessed luminosity fraction.
Findings
Torus reprocesses approximately 1/3 to 1/2 of the accretion disc luminosity.
Sample size of about 4000 AGN with IR detection across all four WISE bands.
Largest IR-based study of the disc-torus connection at z~0.6.
Abstract
We selected all radio-quiet AGN in the latest release of Sloan digital sky survey quasar catalog, with redshift in the range 0.56-0.73. About 4000 (~80%) of these have been detected in all four IR-bands of WISE (Wide-field Infrared Survey Explorer). This is the largest sample suitable to study the disc-torus connection. We find that the torus reprocesses on average ~1/3-1/2 of the accretion disc luminosity.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Star Formation Studies · Astronomy and Astrophysical Research
