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The top documents tagged [deg fov]

EMU: Evolutionary Map of the Universe Ray Norris 13 September 2011
EMU: Evolutionary Map of the Universe Ray Norris 13 September 2011
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EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame
EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame
213 views
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
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
218 views
Observing Dark Energy SDSS, DES, WFMOS teams. Understanding Dark Energy No compelling theory, must be observational driven We can make progress on questions:
Observing Dark Energy SDSS, DES, WFMOS teams. Understanding Dark Energy No compelling theory, must be observational driven We can make progress on questions:
218 views
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
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
217 views
MC studies for a future gamma-ray array Stefan Funk, Jim Hinton & S. Digel Kavli Institute for Astroparticle Physics and Cosmology, Stanford University
MC studies for a future gamma-ray array Stefan Funk, Jim Hinton & S. Digel Kavli Institute for Astroparticle Physics and Cosmology, Stanford University
218 views
EMU: Redshifts for radio continuum surveys Ray Norris Taipan meeting December 2012
EMU: Redshifts for radio continuum surveys Ray Norris Taipan meeting December 2012
216 views
Ultimate wide field Imaging: The Large Synoptic Sky Survey Marek Kowalski Physikalisches Institut Universität Bonn
Ultimate wide field Imaging: The Large Synoptic Sky Survey Marek Kowalski Physikalisches Institut Universität Bonn
214 views
Odyssey II & III Caribou Xanthos. Typical coverage area: –500m X 500m @ altitude = 10% of desired range –25m spacing between 21 tracklines FULL coverage
Odyssey II & III Caribou Xanthos. Typical coverage area: –500m X 500m @ altitude = 10% of desired range –25m spacing between 21 tracklines FULL coverage
223 views
BRITE-Constellation Nov. 2010 BRITE Satellites Cubic form factor (20cm/side) with mass < 8kg Cubic form factor (20cm/side) with mass < 8kg Pre-deployed
BRITE-Constellation Nov. 2010 BRITE Satellites Cubic form factor (20cm/side) with mass < 8kg Cubic form factor (20cm/side) with mass < 8kg Pre-deployed
222 views
The Transient Universe: AY 250 Spring 2007 Extra Solar Planets Geoff Bower
The Transient Universe: AY 250 Spring 2007 Extra Solar Planets Geoff Bower
219 views
Observatory System of Systems LSST Internet 2 MSC NVO Mauna Kea Observatories Mauna Kea Observatories
Observatory System of Systems LSST Internet 2 MSC NVO Mauna Kea Observatories Mauna Kea Observatories
232 views