What can we learn on the BLR from the smallest AGN? Or, how do the BLR properties change with luminosity, and what is it telling us? Specifically The BLR.
Romain G. Petrov, Lagrange Laboratory (OCA, UNS, CNRS), Nice, France with Suvendu Rakshit, Florentin Millour, Sebastian Hoënig, Anthony Meilland, Stephane.
The Distribution of DM in Galaxies Paolo Salucci (SISSA) TeVPa Paris,2010.
CDF Trigger System Veronica Sorin Michigan State University Silicon Workshop UCSB May 11,2006.
Z > 6 Surveys Represent the Current Frontier Motivation: - census of earliest galaxies (z=6, =0.95 Gyr) - contribution of SF to cosmic reionization -
Evolution of High-Redshift Quasars Xiaohui Fan University of Arizona Castel Gandolfo, Oct 2005 Collaborators: Strauss,Schneider,Richards, Hennawi,Gunn,Becker,White,Rix,Pentericci,
z > 6 Surveys Represent the Current Frontier
Dataset Based Physics Analysis
CDF Trigger System
Dec. 1-8, 2010
The Clustering of AGN Using Photometric Redshifts
The Clustering of AGN Using Photometric Redshifts Elias Koulouridis Antonis Georgakakis National Observatory of Athens.
