Chris Churchill New Mexico State - Galaxies form in the cosmic web - They accrete IGM gas, form stars, and deposit energy/metals back into IGM - Extended.
G. Murante – INAF OATo P. Monaco – Univ. Ts M. Calabrese – SISSA Ts G. De Lucia - INAF OATs S. Borgani – Univ. Ts K. Dolag – Obs..Munchen Heidelberg, May.
X-ray and Radio AGN in Coma Cluster Progenitors Quyen Nguyen Hart University of Colorado at Boulder, Center for Astrophysics and Space Astronomy Collaborators.
Numerical issues in SPH simulations of disk galaxy formation Tobias Kaufmann, Lucio Mayer, Ben Moore, Joachim Stadel University of Zürich Institute for.
Dark Halos of Fossil Groups and Clusters Observations and Simulations Ali Dariush, Trevor Ponman Graham Smith University of Birmingham, UK Frazer Pearce.
RUDRANI KAR CHOWDHURY PRESIDENCY UNIVERSITY M.Sc thesis advisor Suchetana Chatterjee X-ray Surface Brightness Profiles of Galaxy Groups from Cosmological.
A.Kravtsov (U.Chicago) D. Ceverino (NMSU) O. Valenzuela (U.Washington) G. Rhee (UNLV) F. Governato, T.Quinn, G.Stinson (U.Washington) J.Wadsley (McMaster,
SAN DIEGO SUPERCOMPUTER CENTER at the UNIVERSITY OF CALIFORNIA, SAN DIEGO TeraGrid Coordination Meeting June 10, 2010 TeraGrid Forum Meeting June 16, 2010.
Ugo BeccianiHPC - Virtual Obs. - Grid1 Cosmology & Astrophysical Software Technology (Theory, Simulations and VO-Data Exploration) Ugo Becciani, V. Antonuccio,
Galaxies…. + On the largest scales… they trace the cosmic structure as the “living fossils” of the earliest density fluctuations of the universe They are.
Galaxy Color Matching in Catalogs
Kravtsov (U.Chicago) D. Ceverino (NMSU)