Are There Local Analogs of Lyman Break Galaxies? James D. Lowenthal (Smith College/FCAD) R. Nick Durham (Smith College) Brian Lyons (Amherst College) David.
Interpreting stellar populations in a cosmological context rachel somerville MPIA with thanks to the GOODS & GEMS teams, S. Faber, B. Allgood, J. Primack,
Relativistic collapse and explosion of rotating supermassive stars with thermonuclear effects
Where will supersymmetric dark matter first be seen? Liang Gao National observatories of China, CAS.
How Do Galaxies Get Their Gas? astro-ph/0407095 Dušan Kereš University of Massachusetts Collaborators: Neal Katz, Umass David Weinberg, Ohio-State Romeel.
Cool gas in the distant Universe Epoch of galaxy assembly (z~1 to 5) Massive galaxy formation: imaging hyper-starbursts Main sequence galaxies: gas.
Pop III IMF Michael L. Norman Laboratory for Computational Astrophysics UC San Diego (with thanks to Andrea Ferrara & Mario Livio)
Statistical Properties of Radio Galaxies in the local Universe Yen-Ting Lin Princeton University Pontificia Universidad Católica de Chile Yue Shen, Michael.
Bi-modality and Do w n s i z i n g Avishai Dekel HU Jerusalem Bernard ’ s Cosmic Stories, Valencia, June 2006 Origin of E vs S Galaxies.
Lecture 3: The Highest Redshift Quasars: Early Black Hole Evolution and the End of Reionization Xiaohui Fan AGN Summer School, USTC May 25, 2007 Background:
Cosmological Constraints from the maxBCG Cluster Sample
The influence of baryons on the matter distribution and shape of dark matter halos