Speaker
Maurizio Paolillo
(Istituto Nazionale di Astrofisica (INAF))
Description
We explore the dependence of Active Galactic Nuclei from the BH mass and luminosity for the ~30 supermassive BHs with mass estimates in the Chandra Deep Field south. With this dataset we can test wether the results are consistent with the models based on low-redshift AGNs, and validate the use of AGN variability to estimate the accretion history of SMBH as well as for future cosmological applications.
| Affiliation | Università di Napoli Federico II |
|---|---|
| Topic | Active Galactic Nuclei: accretion physics and evolution across cosmic time |
Primary authors
Prof.
Iossif Papadakis
(University of Crete)
Maurizio Paolillo
(Istituto Nazionale di Astrofisica (INAF))
