Galaxy surveys: from controlling systematics to new physics Ofer Lahav (UCL) CLASH MACS1206 1.
Jim Ulvestad Division Director, AST October 13, 2011 Division of Astronomical Sciences.
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.
Answering Cosmological Questions with The Next Generation of Galaxy Surveys Will Percival (University of Portsmouth)
CCD Mosaics at CTIO and SOAR. Abstract: Mosaics based on 2K x 4K CCDs are briefly reviewed. An 8Kx8K mosaic of SITe002A CCDs is in use at the 4m Blanco.
Scientists Find Possible Birth of Tiniest Known Solar System ? Jeng-Lwen, Chiu Institute of Physics, NTHU 2005 / 12 / 15.
1 DESpec Outline Concept Technical Components –Optics –Fiber Positioner –Fibers & Spectrographs –CCD & RO Some discussion about choices that may be available.
DECam in Chile
DESpec: Key Science Goals Ofer Lahav University College London - DES and needs for spectroscopy per probe - The landscape of spectroscopic surveys - Improving.
I F A E ( I NSTITUT de F ÍSICA d’ A LTES E NERGIES) IN FIVE MINUTES
1 DECam in Chile Intro to Dark Energy Survey & DECam Project Status of arrivals in Chile Instrument checkout in Chile Schedule for first light.
The Dark Side of the Universe - I
