Galaxies, The Big Bang & Dark Matter Stephen Perrenod, Ph.D. Interstellar Intergalactic! What is a Galaxy? Gravitationally bound system of: Stars Planets Gas Dust "Dark…

Slide 1 Slide 2  Acceleration of Universe  Background level  Evolution of expansion: H(a), w(a)  degeneracy: DE & MG  Perturbation level  Evolution…

Chapter 16: Other Galaxies WHAT DO YOU THINK? Do all galaxies have spiral arms? Are galaxies isolated objects? Are all other galaxies moving away from the Milky Way? You…

Jennifer Lotz Hubble Science Briefing Jan. 16, 2014 Exploring the Depths of the Universe Hubble is now observing galaxies 97% of the way back to the Big Bang, during the…

Large-scale Structure: Theory & Observations Josh Frieman Structure Formation & Evolution, Santiago, October 2002 The Structure Formation Cookbook 1. Initial Conditions:…

Observational Probes of Dark Energy Timothy McKay University of Michigan Department of Physics Observational cosmology: parameters (H0,0) => evolution (a(t), g(z,k))…

Evolution of structure in the Universe Galaxy Superclusters Detected in the MPF-Catalogue Using the FoF Method Elena Panko Nikolaev National University Input data PF catalogue…

Jennifer Lotz Hubble Science Briefing Jan. 16, 2014 Exploring the Depths of the Universe Hubble is now observing galaxies 97% of the way back to the Big Bang, during the…

Environmental Properties of a Sample of Starburst Galaxies Selected from the 2dFGRS Matt Owers (UNSW) Warrick Couch (UNSW) Chris Blake (UBC) Michael Pracy (UNSW) Kenji Bekki…

Acceleration of Universe Background level Evolution of expansion: H(a), w(a) degeneracy: DE & MG Perturbation level Evolution of inhomogeneity: G(a), G(a, k), Phi, Psi……