The Origin of the Universe and the Arrow of Time
Evolution of clustering in COSMOS: a progress report Luigi Guzzo (INAF, Milano) N. Scoville, O. Le Fevre, A. Pollo, B. Meneux, & COSMOS Team.
In collaboration with Christine Jones & Bill Forman Maxim Markevitch & John Zuhone A talk for the workshop “Diffuse Emission from Galaxy Clusters in the.
Reconstructing Gravity With Peculiar Velocties
Hydrogen 21cm Cosmology Tzu-Ching Chang (ASIAA) Ue-Li Pen, Kiyo Masui (CITA) Jeff Peterson, Kevin Bandura, Tabitha Voytek, Aravind Natarajan (CMU) Pat.
Evolution of a Powerful Radio Loud Quasar 3C186 and its Impact on the Cluster Environment at z=1 Aneta Siemiginowska Harvard-Smithsonian Center for Astrophysics.
Setting the rod straight: Baryon Acoustic Oscillations.
Particle Astrophysics & Cosmology SS 20081 Chapter 8 Structure Formation.
Dynamical Dark Energy. What is dynamical dark energy ?
Evolution of a Powerful Radio Loud Quasar 3C186 and its Impact on the Cluster Environment at z=1
Galaxy bias with Gaussian/non- Gaussian initial condition: a pedagogical introduction Donghui Jeong Texas Cosmology Center The University of Texas at Austin.
Baryon Acoustic Oscillations: A Robust and Precise Route to the Cosmological Distance Scale Daniel Eisenstein (University of Arizona) Michael Blanton,
