HWR Princeton, 2005 III. The Growth of Galaxy Disks and the Evolution of Galaxy Sizes Observed galaxies occupy a small fraction of possible structural.
“The Dark SDSS” Bob Nichol ICG, Portsmouth Special thanks to Masao Sako, David Weinberg, Andy Connolly, Albert Stebbins, Rob Crittenden, Daniel Eisenstein,
Redshift Evolution of the Correlation Function Peter Capak J. Blazek, D. Sanders, I. Szapudi, N. Scoville Kyoto, May 23, 2005.
FMOS Workshop, Jan. 2004 The Decline in Cosmic Star Formation: is Environment to blame? or Mapping the interaction of galaxies with their environment as.
“Observing Dark Energy” Bob Nichol ICG, Portsmouth Special thanks to Masao Sako, David Weinberg, Andy Connolly, Albert Stebbins, Rob Crittenden, Daniel.
Redshift Evolution Of The Morphology Density Relation
Metallicity Evolution of Active Galactic Nuclei
Quasar Clustering (A Dabbler’s Perspective) CCAPP AGN Workshop: Oct. 2, 2007
Center for Theoretical Physics University of Provence Marseille
Observational Probes of Dark Energy Timothy McKay University of Michigan Department of Physics Observational cosmology: parameters (H 0, 0 ) => evolution.
“The present and next generation of large galaxy surveys”
“The Dark SDSS”
