Cosmological Evolution of the Duty Cycle of Quasars

Slides:



Advertisements
Similar presentations
Feedback Limits Rapid Growth Seed BHs at High Redshift Jianmin Wang, Yanmei Chen, Chen Hu Institute of High Energy Physics.
Advertisements

1 Black Holes in the Early Universe Accretion and Feedback Geoff Bicknell & Alex Wagner Research School of Astronomy & Astrophysics Australian National.
Probing the End of Reionization with High-redshift Quasars Xiaohui Fan University of Arizona Mar 18, 2005, Shanghai Collaborators: Becker, Gunn, Lupton,
Marianne Vestergaard Dark Cosmology Centre, Copenhagen First Galaxies, Quasars, and GRBs, June Determining Black Hole Masses in Distant Quasars.
COEVOLUTION OF SUPERMASSIVE BLACK HOLES AND THEIR HOST GALAXIES...OR: CHICKEN, EGG OR BOTH? Jari Kotilainen Tuorla Observatory, University of Turku, Finland.
UNCERTAINTIES ON THE BLACK HOLE MASSES AND CONSEQUENCES FOR THE EDDINGTON RATIOS Suzy Collin Observatoire de Paris-Meudon, France Collaborators: T. Kawaguchi.
Growth of massive black holes during radiatively inefficient accretion phases Xinwu Cao Shanghai Astronomical Observatory, CAS.
Molecular gas in the z~6 quasar host galaxies Ran Wang National Radio Astronomy Observatory Steward Observatory, University of Atrizona Collaborators:
AGN Eddington Ratio Distributions
Quasar Clustering from SDSS DR7: Dependencies on FIRST Radio Magnitudes Andria C. Schwortz, Sarah Eftekharzadeh, Adam D. Myers, Yue Shen Clustering is.
Star Formation in AGN hosts Li Shao & PACS Evolutionary Probe (PEP) group Hangzhou, China April 28, 2011 Evidence from Herschel PACS.
Super-Eddington Accretion: Models and Applications Jian-Min Wang Institute of High Energy Physics 2005, 4, 26.
Tidal Disruption from Supermassive Black Hole Binaries in Merging Galaxies: Before & After the Coalescence Shuo Li NAOC Collaborated with Rainer Spurzem,
Constraining Astronomical Populations with Truncated Data Sets Brandon C. Kelly (CfA, Hubble Fellow, 6/11/2015Brandon C. Kelly,
The relation among black holes, their host galaxies and AGN activity INAF ISTITUTO NAZIONALE DI ASTROFISICA NATIONAL INSTITUTE FOR ASTROPHYSICS Galaxies.
The fraction of obscured quasars Junxian Wang Center for Astrophysics University of Science and Technology of China Xi’an, China Collaborated with.
THE MODERATELY LARGE SCALE STRUCTURE OF QUASARS
A Unified, Merger-Driven Model of the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes, and Galaxy Spheroids Hopkins,
“ Testing the predictive power of semi-analytic models using the Sloan Digital Sky Survey” Juan Esteban González Birmingham, 24/06/08 Collaborators: Cedric.
ACCRETION MODELS FOR BLACK HOLE EVOLUTION Francesco Shankar In collaboration with: D. Weinberg J. Miralda-Escude’ L. Ferrarese A. Cavaliere S. Mathur CCAPP/OSU.
Advanced Methods for Studying Astronomical Populations: Inferring Distributions and Evolution of Derived (not Measured!) Quantities Brandon C. Kelly (CfA,
Forming and Feeding Super-massive Black Holes in the Young Universe Wolfgang J. Duschl Institut für Theoretische Astrophysik Universität Heidelberg.
1 The Fundamental Plane Relationship of Astrophysical Black Holes Ran Wang Supervisor: Xuebing Wu Peking University Ran Wang Supervisor: Xuebing Wu Peking.
Obscured AGN in the (z)COSMOS survey AGN9, Ferrara, May Angela Bongiorno Max-Planck-Institut für extraterrestrische Physik, Garching, GERMANY AND.
The Evolution of Quasars and Massive Black Holes “Quasar Hosts and the Black Hole-Spheroid Connection”: Dunlop 2004 “The Evolution of Quasars”: Osmer 2004.
Coevolution of black holes and galaxies at high redshift David M Alexander (Durham)
Gravitational Waves from Massive Black-Hole Binaries Stuart Wyithe (U. Melb) NGC 6420.
New Puzzles in Supermassive Black Hole Evolution Charles L. Steinhardt IPMU, University of Tokyo October 14, 2010 Steinhardt & Elvis 2010, MNRAS, 402,
The Black-Hole – Halo Mass Relation and High Redshift Quasars Stuart Wyithe Avi Loeb (The University of Melbourne) (Harvard University) Fan et al. (2001)
Populations of accreting X-ray sources in galaxies
A Tidal Disruption model for gamma-ray burst of GRB YE LU National Astronomical Observatories, Chinese Academy of Sciences June 22-27, 2008 Nanjing.
Black Hole Spin Properties of 130 AGN Ruth A. Daly Penn State University
Modeling the dependence of galaxy clustering on stellar mass and SEDs Lan Wang Collaborators: Guinevere Kauffmann (MPA) Cheng Li (MPA/SHAO, USTC) Gabriella.
Black Hole - Bulge Relation of High Redshift Quasars Xue-Bing Wu (Dept. of Astronomy, Peking University)
Spins of supermassive black holes in quasars and galaxies Jian-Min Wang ( 王建民 ) Institute of High Energy Physics Chinese Academy of Sciences, Beijing Dec.
HOW WHAT Conclusions Barausse E., 2012, MNRAS, 423, 2533 De Rosa G., Decarli R., Walter F.,Fan X., Jiang L., Kirk J., Pasquali A., Rix H. W., 2011, ApJ,
Discovery of a 12 Billion Solar Mass Black Hole at Redshift 6.3 and its Challenge to the Black Hole/Galaxy Coevolution at Cosmic Dawn Xue-Bing WU Kavli.
AGN feedback in action: constraints on the scaling relations between BH and galaxy at high redshift Andrea Merloni (EXC, MPE) A. Bongiorno (MPE), COSMOS.
Black hole accretion history of active galactic nuclei 曹新伍 中国科学院上海天文台.
Black Holes and the Evolution of Galaxies…. Summary Quasars and Evolution: the universe becomes interesting How we do it: things invisible to see. Demographics:
1 Baryon Acoustic Oscillations Prospects of Measuring Dark Energy Equation of State with LAMOST Xuelei Chen ( 陳學雷 ) National Astronomical Observatory of.
The Evolution of AGN Obscuration Ezequiel Treister (ESO) Meg Urry (Yale) Julian Krolik (JHU)
The dependence on redshift of quasar black hole masses from the SLOAN survey R. Decarli Università dell’Insubria, Como, Italy A. Treves Università dell’Insubria,
Evolution of Accretion Disks around Massive Black Holes: Constraints from the Demography of Active Galactic Nuclei Qingjuan Yu UC Berkeley April 21, 2006.
The History of Black Hole Accretion from X-ray Stacking Ezequiel Treister (IfA, Hawaii) Collaborators: Meg Urry, Priya Natarajan, Kevin Schawinski (Yale),
Quasar Surveys -- From Sloan to SNAP
Probing Dark Energy with Cosmological Observations Fan, Zuhui ( 范祖辉 ) Dept. of Astronomy Peking University.
Warm Dust in the Most Distant Quasars Ran Wang Department of Astronomy, Peking University, China.
Tools for computing the AGN feedback: radio-loudness and the kinetic luminosity function Gabriele Melini Fabio La Franca Fabrizio Fiore Active Galactic.
Active Galactic Nuclei Origin of correlations.
YOUR LOGO The FUS(FIRST-UKIDSS-SDSS) RED Quasar Survey Dohyeong Kim 서울대학교 천문학과 김도형
Jounal Club 04/04, Sunmyon Chon [1a]Gravitational Waves from the Remnants of the First Stars, T. Hartwig et al. [arXiv: ]arXiv: and.
High Redshift QUASAR Spectra as Probe of Reionization of IGM.
Percolation analysis for cosmic web with discrete points
Growth of SMBH studied through X-ray surveys
Cosmological evolution of supermassive black holes and AGN: a synthesis model for accretion and feedback Andrea Merloni Excellence Cluster Universe &
Signs of the Blandford & Znajek mechanism in GRB afterglow lightcurves
The cosmic spin of SMBHs from radio observations
Biases in Virial Black Hole Masses: an SDSS Perspective
Black Hole Candles for Expansion History of High-z Universe
Shuang-Nan Zhang, Yuan Liu, Jin Zhang Institute of High Energy Physics
On the Outliers of the Black Hole - Bulge Relation
The redshift dependence of the MBH-Mhost relation in quasars
Speaker: Longbiao Li Collaborators: Yongfeng Huang, Zhibin Zhang,
Modeling the dependence of galaxy clustering on stellar mass and SEDs
Demographics of SDSS Quasars in Two-Dimension
Radio-loud quasars in SDSS DR3
Galactic Astronomy 銀河物理学特論 I Lecture 3-3: Stellar mass function of galaxies Seminar: Perez-Gonzalez et al. 2008, ApJ, 675, 234 Lecture: 2012/01/16.
The 1/Vmax SMF for the high-redshift samples.
Presentation transcript:

Cosmological Evolution of the Duty Cycle of Quasars Yan-Mei Chen Collaborator: Jian-Min Wang, Fan Zhang Institute of High Energy Physics, CAS, China 21 Oct 2006

Outline Motivation The definition of duty cycle Black hole mass function Results

Background Continuity equation: Luminosity function Quasars’ duty cycle Ref: Marconi et al., 2004, MNRAS, 351, 169 Small & Blandford, 1992, MNRAS, 259, 725

Motivation During entire evolution, how many times and how many black holes are triggered ? What is the trigger mechanism and why do quasars switch off ? Constant Eddington ratio ? (Vestergaard, 2004, ApJ, 601, 676)

Duty cycle: episodic activity (Kharb et al., 2006) BH birth active dormant a single episodic phase today (1)For a single BH, ; (2)In statistic, duty cycle can be defined as the fraction of active BHs to their total number

Duty cycle: episodic activity Definition: where

Duty cycle The mass-averaged duty cycle: Soltan Argument (1982):

Sample Sample: SDSS DR3 (Richards et al. 2006) Total: 10, 979 Redshift: z<2.1 Estimation of BH mass (Mclure & Dunlop, 2004, MNRAS, 352, 1390)

Mass distribution Total: triple power law Mass function in each redshift z-bin

consistent with history of SFR density Main results: δ ∈ (10-3 , 1) strong evolution consistent with history of SFR density Open questions: how to explain the relation between δ and SFR density? feedback? duty cycle beyond z=2.1? how does duty cycle depend on BH mass? (Pablo G. Perez-Gonzalez et al., 2005, ApJ, 630, 82)

Thank You !