High-Redshift Quasars Probing Early Star Formation Matthias Dietrich The Ohio State University...

download High-Redshift Quasars Probing Early Star Formation Matthias Dietrich The Ohio State University Department…

If you can't read please download the document

description

Introduction Quasars are among the most luminous objects in the universe and have been detected to z > 6 Current generally accepted framework super-massive black hole accretion disk (+ corona) broad emission line region absorbing structure (torus) narrow emission line region jets (radio, optical, X-rays) outflows, disk winds The CCAPP Symposium 2009 – Columbus – October 14, 2009

Supermassive black hole formation at high redshift - … · High z Quasars: 14 ★Supermassive black holes of ~10 9 solar masses have been observed at z>6 (Venemans +15) ★The highest-redshift

Supermassive black hole formation at high redshift - … · High z Quasars: 14 ★Supermassive black holes of ~10 9 solar masses have been observed at z>6 (Venemans +15) ★The highest-redshift

Probing the End of Reionization with High-redshift Quasars Xiaohui Fan University of Arizona Mar 18, 2005, Shanghai Collaborators: Becker, Gunn, Lupton,

Probing the End of Reionization with High-redshift Quasars Xiaohui Fan University of Arizona Mar 18, 2005, Shanghai Collaborators: Becker, Gunn, Lupton,

High-redshift Quasars in Cosmological Simulationsbccp.berkeley.edu/beach_program/presentations12/DeGraf.pdf · Conclusions Simulation provides large statistical sample of quasars

High-redshift Quasars in Cosmological Simulationsbccp.berkeley.edu/beach_program/presentations12/DeGraf.pdf · Conclusions Simulation provides large statistical sample of quasars

Catalogue of Discordant Redshift Associations - isidore.co Halton-Catalogue of... · Arp, Halton C., 1927- ... (Arp, Atlas of Peculiar Galaxies No. 227). Quasars this radio bright

Catalogue of Discordant Redshift Associations - isidore.co Halton-Catalogue of... · Arp, Halton C., 1927- ... (Arp, Atlas of Peculiar Galaxies No. 227). Quasars this radio bright

Variabilityselected high-redshift quasars onSDSSStripe82which helps discriminating quasarsfrom variable stars, con-sists in parameters that describe the structure function. 2.1.Quasarandstarsamples

Variabilityselected high-redshift quasars onSDSSStripe82which helps discriminating quasarsfrom variable stars, con-sists in parameters that describe the structure function. 2.1.Quasarandstarsamples

Clustering of high-redshift(z>2.9) quasars from SDSS · 2007-05-23 · spectroscopic main quasar sample • Color selection of quasar targets (ugri color cube for z

Clustering of high-redshift(z>2.9) quasars from SDSS · 2007-05-23 · spectroscopic main quasar sample • Color selection of quasar targets (ugri color cube for z

Amazon Redshift - Cluster Management Guide · Amazon Redshift Cluster Management Guide Are You a First-Time Amazon Redshift User? What Is Amazon Redshift? Welcome to the Amazon Redshift

Amazon Redshift - Cluster Management Guide · Amazon Redshift Cluster Management Guide Are You a First-Time Amazon Redshift User? What Is Amazon Redshift? Welcome to the Amazon Redshift

Black holes, redshift and quasars - MSPmsp.warwick.ac.uk/~cpr/paradigm/quasars.pdfBlack holes, redshift and quasars 3 our model, because the observed radiation comes only from near

Black holes, redshift and quasars - MSPmsp.warwick.ac.uk/~cpr/paradigm/quasars.pdfBlack holes, redshift and quasars 3 our model, because the observed radiation comes only from near

CHARACTERIZING THE WARM-HOT INTERGALACTIC MEDIUM AT … · high redshift, along the lines of sight to five bright quasars observed with the Keck I telescope and HIRES spectro-graph.

CHARACTERIZING THE WARM-HOT INTERGALACTIC MEDIUM AT … · high redshift, along the lines of sight to five bright quasars observed with the Keck I telescope and HIRES spectro-graph.

The Black-Hole – Halo Mass Relation and High Redshift Quasars

The Black-Hole – Halo Mass Relation and High Redshift Quasars

High-Redshift, Radio-Loud Quasars - CORE · quasars, however, imply that radio is perhaps a better search wavelength for quasars, less prone to selection e ects than optical surveys.

High-Redshift, Radio-Loud Quasars - CORE · quasars, however, imply that radio is perhaps a better search wavelength for quasars, less prone to selection e ects than optical surveys.

Metallicity and Black Hole Masses of Redshift 6 Quasars Jaron Kurk (MPIA, D) The evening star (Mucha, 1902) The moon (Mucha, 1902) Fabian Walter, Dominik.

Metallicity and Black Hole Masses of Redshift 6 Quasars Jaron Kurk (MPIA, D) The evening star (Mucha, 1902) The moon (Mucha, 1902) Fabian Walter, Dominik.

Y-band Imaging of Extragalatic Fields and High redshift Quasars Changsu Choi 1, Myungshin Im 1 1 Center for the Exploration of the Origin of the Universe,

Y-band Imaging of Extragalatic Fields and High redshift Quasars Changsu Choi 1, Myungshin Im 1 1 Center for the Exploration of the Origin of the Universe,

High -Redshift Quasars and Galaxies at the Epoch of Cosmic Reionization

High -Redshift Quasars and Galaxies at the Epoch of Cosmic Reionization

REDSHIFT MEASUREMENT AND SPECTRAL CLASSIFICATION … · redshifts of galaxies, galaxy clusters, and quasars to map the three-dimensional distribution of matter. These observations

REDSHIFT MEASUREMENT AND SPECTRAL CLASSIFICATION … · redshifts of galaxies, galaxy clusters, and quasars to map the three-dimensional distribution of matter. These observations

sqlalchemy-redshift Documentation filesqlalchemy-redshift Documentation, Release 0.7.2 Amazon Redshift dialect for SQLAlchemy. Contents 1

sqlalchemy-redshift Documentation filesqlalchemy-redshift Documentation, Release 0.7.2 Amazon Redshift dialect for SQLAlchemy. Contents 1

The Highest-Redshift Quasars and the End of Cosmic Dark Ages Xiaohui Fan Collaborators: Strauss,Schneider,Richards, Hennawi,Gunn,Becker,White,Rix,Pentericci,

The Highest-Redshift Quasars and the End of Cosmic Dark Ages Xiaohui Fan Collaborators: Strauss,Schneider,Richards, Hennawi,Gunn,Becker,White,Rix,Pentericci,

Black Hole - Bulge Relation of High Redshift Quasars Xue-Bing Wu (Dept. of Astronomy, Peking University)

Black Hole - Bulge Relation of High Redshift Quasars Xue-Bing Wu (Dept. of Astronomy, Peking University)

Quasars Probing Quasars: Shedding (Quasar) Light on High Redshift Galaxies

Quasars Probing Quasars: Shedding (Quasar) Light on High Redshift Galaxies

The Black-Hole – Halo Mass Relation and High Redshift Quasars Stuart Wyithe Avi Loeb (The University of Melbourne) (Harvard University) Fan et al. (2001)

The Black-Hole – Halo Mass Relation and High Redshift Quasars Stuart Wyithe Avi Loeb (The University of Melbourne) (Harvard University) Fan et al. (2001)