Evolution of clustering in COSMOS: a progress report Luigi Guzzo (INAF, Milano) N. Scoville, O. Le Fevre, A. Pollo, B. Meneux, & COSMOS Team.
Galaxy Mergers: major/minor wet/dry Hans-Walter Rix MPIA, Heidelberg … which galaxies are most shaped by mergers? … when do mergers matter for the SFR?
R. Chris Smith, C. Aguilera, K. Krisciunas, N. B. Suntzeff (NOAO/CTIO), A. Becker, R. Covarrubias, A. Miceli, G. Miknaitis, A. Rest, C. Stubbs (U. Washington),
Tom Theuns Institute for Computational Cosmology, Durham, UK Department of Physics, Antwerp, Belgium Munich 2005 Reionization And the thermal history of.
Searching for Supernovae
Jeroen Stil Department of Physics & Astronomy University of Calgary Stacking of Radio Surveys.
Astronomy, Astrophysics & Cosmology at the University of Nottingham.
Black Holes and the Fundamental Correlations Karl Gebhardt (UT Austin, MPE/USM)
Epoch of Reionization Tomography with the CSO Wide-field C+ spectral mapping and correlation with HI Matt Bradford CSO NSF visit: October 12, 2011 CSO.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 9; February 10 2014.
GRBs as Probes of First Light and the Reionization History of the Universe D. Q. Lamb (U. Chicago) Conference on First Light and Reionization Irvine, CA,
Meaning of deceleration parameter flat model q 0 tells you if the Universe is accelerating in its global expansion rate, or decelerating. Flat, matter.
