Galaxy groups Michael Balogh Department of Physics and Astronomy University of Waterloo.
Candels the correlation_between_galaxy_morphology_and_star_formation_activity_at_z2
Astro 10-Lecture 13: Quiz 1. T/F We are near the center of our Galaxy 2.Cepheid variable stars can be used as distance indicators because a) They all have.
Steve Strom – The Galaxy Evolution Years (1976-1984) Pioneered instrumental and observing techniques to measure the right kind of stuff for galaxies.
UCSC - August, 2004 Large-Scale Structure in the DEEP2 Galaxy Redshift Survey Jeffrey Newman Lawrence Berkeley National Laboratory And The DEEP2 Team.
Congresso del Dipartimento di Fisica Highlights in Physics 2005
Properties of Galaxies at High- redshift in the UDS : Environmental Dependence Seong-Kook Lee, M. IM & J.-W. Kim CEOU@SNU / Feb. 15, 2013.
DEEP SURVEYS: Galaxy formation and evolution
Large-Scale Structure in the DEEP2 Galaxy Redshift Survey
Are galaxies still evolving strongly? Christopher J. Miller
Properties of Galaxies at High- redshift in the UDS : Environmental Dependence
