Željko Ivezi?|S. M. Kahn|J. A. Tyson|Bob Abel|Emily Elizabeth Acosta|R. A. Allsman|David Alonso|Yusra AlSayyad|Scott F. Anderson|John Andrew|J. R. P. Angel|George Z. Angeli|R. Ansari|P. Antilogus|Constanza Araujo|Robert Armstrong|K. Arndt|P. Astier|É. Aubourg|Nicole Auza|T. S. Axelrod|Deborah Bard|J. Barr|A. Barrau|J. G. Bartlett|A. Bauer|Brian Bauman|S. Baumont|Ellen Bechtol|K. Bechtol|A. C. Becker|Jacek Becla|Cristina Beldica|Steve Bellavia|Federica Bianco|Rahul Biswas|G. Blanc|Jonathan Blazek|R. D. Blandford|J. S. Bloom|J. R. Bogart|Tim Bond|Michael T. Booth|A. W. Borgland|K. D. Borne|James Bosch|D. Boutigny|Craig A. Brackett|Andrew Bradshaw|W. N. Brandt|Michael E. Brown|James S. Bullock|P. R. Burchat|D. L. Burke|G. Cagnoli|D.R. Calabrese|Shawn Callahan|Alice Callen|Jeffrey L. Carlin|Erin L. Carlson|Srinivasan Chandrasekharan|Glenaver Charles-Emerson|S. R. Chesley|E. Cheu|Hsin?Fang Chiang|J. Chiang|Carol Chirino|Derek Chow|David R. Ciardi|Charles F. Claver|J. Cohen-Tanugi|Joseph J. Cockrum|Rebecca Coles|Andrew J. Connolly|K. H. Cook|Asantha Cooray|Kevin R. Covey|Chris Cribbs|Wei Cui|R. M. Cutri|Philip N. Daly|Scott F. Daniel|Felipe Daruich|Guillaume Daubard|Greg Daues|William A. Dawson|Francisco Delgado|A. Dellapenna|Robert de Peyster|M. de Val-Borro|S. W. Digel|Peter Doherty|R. Dubois|G. P. Dubois-Felsmann|Josef ?urech|Frossie Economou|T. F. Eifler|Michael Eracleous|Benjamin L. Emmons|A. Fausti Neto
LSST: From Science Drivers to Reference Design and Anticipated Data Products
University of Washington|Kavli Institute for Particle Astrophysics and Cosmology|Stanford University|SLAC National Accelerator Laboratory|Large Synoptic Survey Telescope Corporation|University of California, Davis|Olympic College|Large Synoptic Survey Telescope Corporation|Large Synoptic Survey Telescope Corporation|University of Oxford|Princeton University|University of Washington|Large Synoptic Survey Telescope Corporation|University of Arizona|GANIL|Laboratoire de Physique Nucléaire et de Hautes Énergies|Large Synoptic Survey Telescope Corporation|Princeton University|University of Oxford|Laboratoire de Physique Nucléaire et de Hautes Énergies|Astroparticle and Cosmology Laboratory|Large Synoptic Survey Telescope Corporation|University of Arizona|SLAC National Accelerator Laboratory|Large Synoptic Survey Telescope Corporation|Laboratory of Subatomic Physics and Cosmology|Astroparticle and Cosmology Laboratory|Large Synoptic Survey Telescope Corporation|Lawrence Livermore National Laboratory|Laboratoire de Physique Nucléaire et de Hautes Énergies|Large Synoptic Survey Telescope Corporation|University of Wisconsin–Madison|Large Synoptic Survey Telescope Corporation|University of Washington|SLAC National Accelerator Laboratory|University of Illinois Urbana-Champaign|Brookhaven National Laboratory|New York University|City University of New York|Stockholm University|GANIL|Délégation Paris 7|Université Paris Cité|The Ohio State University|École Polytechnique Fédérale de Lausanne|Kavli Institute for Particle Astrophysics and Cosmology|Stanford University|SLAC National Accelerator Laboratory|Kavli Institute for Particle Astrophysics and Cosmology|Stanford University|SLAC National Accelerator Laboratory|SLAC National Accelerator Laboratory|Large Synoptic Survey Telescope Corporation|SLAC National Accelerator Laboratory|George Mason University|Princeton University|Laboratoire d’Annecy de Physique des Particules|SLAC National Accelerator Laboratory|University of California, Davis|Pennsylvania State University|California Institute of Technology|University of California, Irvine|Kavli Institute for Particle Astrophysics and Cosmology|Stanford University|SLAC National Accelerator Laboratory|Kavli Institute for Particle Astrophysics and Cosmology|Stanford University|SLAC National Accelerator Laboratory|Laboratoire des Matériaux Avancés|Large Synoptic Survey Telescope Corporation|Large Synoptic Survey Telescope Corporation|SLAC National Accelerator Laboratory|Large Synoptic Survey Telescope Corporation|Large Synoptic Survey Telescope Corporation|University of Arizona|Large Synoptic Survey Telescope Corporation|Jet Propulsion Laboratory|University of Arizona|University of Illinois Urbana-Champaign|Kavli Institute for Particle Astrophysics and Cosmology|Stanford University|SLAC National Accelerator Laboratory|Large Synoptic Survey Telescope Corporation|SLAC National Accelerator Laboratory|Infrared Processing and Analysis Center|California Institute of Technology|Large Synoptic Survey Telescope Corporation|Laboratoire Univers et Particules de Montpellier|Large Synoptic Survey Telescope Corporation|The Ohio State University|University of Washington|University of California, Irvine|Western Washington University|University of Illinois Urbana-Champaign|Purdue University West Lafayette|Infrared Processing and Analysis Center|California Institute of Technology|University of Arizona|University of Washington|Large Synoptic Survey Telescope Corporation|Laboratoire de Physique Nucléaire et de Hautes Énergies|University of Illinois Urbana-Champaign|Lawrence Livermore National Laboratory|Large Synoptic Survey Telescope Corporation|Brookhaven National Laboratory|SLAC National Accelerator Laboratory|Princeton University|SLAC National Accelerator Laboratory|Harvard University|SLAC National Accelerator Laboratory|Infrared Processing and Analysis Center|California Institute of Technology|Czech Academy of Sciences, Astronomical Institute|Charles University|Large Synoptic Survey Telescope Corporation|University of Arizona|Pennsylvania State University|Large Synoptic Survey Telescope Corporation|Large Synoptic Survey Telescope Corporation
abstract describe ambitious survey currently planned optical large synoptic survey telescope lsst lsst design driven four main science themes probing dark energy dark matter taking inventory solar system exploring transient optical sky mapping milky way lsst large widefield groundbased system designed obtain repeated images covering sky visible cerro pachn northern chile telescope 84 65 effective primary mirror 96 deg 2 field view 32gigapixel camera six filters ugrizy covering wavelength range 3201050 nm project construction phase begin regular survey operations 2022 90 observing time devoted deepwidefast survey mode uniformly observe 18000 deg 2 region 800 times summed six bands anticipated 10 yr operations yield coadded map r 275 data result databases including 32 trillion observations 20 billion galaxies similar number stars serve majority primary science programs remaining 10 observing time allocated special projects deep fast time domain surveys whose details currently discussion illustrate lsst science drivers led choices system parameters describe expected data products characteristics