EMU: Evolutionary Map of the Universe Ray Norris 13 September 2011.
EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame.
Juhan Kim KIAS. 2 2 BigBOSS will enlarge redshift-space maps to 21 million objects 10X larger than SDSS + SDSS-II + BOSS Necessary for Stage IV dark energy.
Observing Dark Energy SDSS, DES, WFMOS teams. Understanding Dark Energy No compelling theory, must be observational driven We can make progress on questions:
Subaru AO in future. Outline Overview of AO systems at Mauna Kea and in the world. Ongoing plan of AOS at Subaru and Mauna Kea. What’s in future.
MC studies for a future gamma-ray array Stefan Funk, Jim Hinton & S. Digel Kavli Institute for Astroparticle Physics and Cosmology, Stanford University.
EMU: Redshifts for radio continuum surveys Ray Norris Taipan meeting December 2012.
Ultimate wide field Imaging: The Large Synoptic Sky Survey Marek Kowalski Physikalisches Institut Universität Bonn.
Odyssey II & III Caribou Xanthos. Typical coverage area: –500m X 500m @ altitude = 10% of desired range –25m spacing between 21 tracklines FULL coverage.
BRITE-Constellation Nov. 2010 BRITE Satellites Cubic form factor (20cm/side) with mass < 8kg Cubic form factor (20cm/side) with mass < 8kg Pre-deployed.
The Transient Universe: AY 250 Spring 2007 Extra Solar Planets Geoff Bower.
Observatory System of Systems LSST Internet 2 MSC NVO Mauna Kea Observatories Mauna Kea Observatories.