Selecting Supernovae for Cosmology Cosmic Co-Motion, Courant Cove, September 2010 Troels Haugbølle [email protected] Niels Bohr International Academy – University.
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?
Ben Moore, Institute for Theoretical Physics, University of Zurich +Oscar Agertz, Roman Teyssier+ Galaxy formation: is the end in sight? Obergurgl, December.
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.
Cosmological constraints from models of galaxy clustering Abstract Given a dark matter distribution, the halo occupation distribution (HOD) provides a.
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