Home ContactSitemap CAS中文
About Us
Brief Introduction
History
Directors
Organization
Research Groups
Scientific Progress
Seminars
Colloquia
CAS Members
Experts
Faculty
Research Fields
Center for Astro-geodynamics
Astrophysics Division
DRAST (Division of Radio Astronomy Science and Technology )
High Technology Laboratories

Location: Home>Research>Seminars
The demographics of broad line quasars
Author:
ArticleSource:
Update time: 2011-08-17
Close
Text Size: A A A
Print
Title: The demographics of broad line quasars
Speaker: Dr. Yue Shen (Clay Fellow)
Affiliation: Harvard-Smithsonian Center for Astrophysics (CfA) of the United States
Time:Aug, 17th, 2pm
Location:Middle conference room, 3rd floor
Abstract: The demographics of broad line quasars is one of the central topics in studying the cosmological evolution of supermassive black holes. This is traditionally studied in terms of the quasar luminosity function. Reverberation mapping studies of local AGNs have enabled us to estimate the masses of broad line quasars using virial mass estimators based on single-epoch spectroscopy, and thus it has become possible to study the evolution of the SMBH population in the 2-dimensional mass-luminosity plane. I will present some recent work on quasar demographics in the mass-luminosity plane, with BH masses estimated using virial mass estimators. I will highlight some caveats of these virial mass estimators in estimating BH masses, and present a forward modeling approach to determine the intrinsic distribution of quasars in the mass-luminosity plane.

Shanghai Astronomical Observatory, All Rights Reserved
80 Nandan Road, Shanghai 200030, China
Tel: +86-21-64386191 Email:shao@shao.ac.cn