Inside the Perimeter Winter2011
Dark energy workshop Copenhagen Aug. 2007. Why the SNLS ? Questions to be addressed: -Can the intrinsic scatter in the Hubble diagram be further reduced?
Clusters, Galaxies and the COSMOS J Berian James (IfA Edinburgh), John Peacock, Alexis Finoguenov, Henry Joy McCracken & Gigi Guzzo for the COSMOS collaboration.
The National Science Foundation The Dark Energy Survey J. Frieman, M. Becker, J. Carlstrom, M. Gladders, W. Hu, R. Kessler, B. Koester, A. Kravtsov, for.
The Stellar Populations, Mass-to-Light Ratios and Dark Matter in Spiral Galaxies Roelof S. de Jong Steward Observatory Eric Bell Rob Kennicutt Rob Swaters.
1 Galaxies at Cosmic Dawn Revealed in the First Year of the Hubble Frontier Fields Initiative Dr. Gabriel Brammer (ESA/AURA, STScI) Hubble Science Briefing.
Cosmic shear results from CFHTLS Henk Hoekstra Ludo van Waerbeke Catherine Heymans Mike Hudson Laura Parker Yannick Mellier Liping Fu Elisabetta Semboloni.
Galaxy bias with Gaussian/non- Gaussian initial condition: a pedagogical introduction Donghui Jeong Texas Cosmology Center The University of Texas at Austin.
Lensing of supernovae by galaxies and galaxy clusters
Frontier Science Enabled by a Giant Segmented Mirror Telescope Rolf-Peter Kudritzki 1 for the GSMT Science Working Group 1 Chair, GSMT Science Working.
Frontier Science Enabled by a Giant Segmented Mirror Telescope
What you need to know about large scale structure Licia Verde University of Pennsylvania lverde.