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4 August 2010The Large Synoptic Survey Telescope preliminary design overview
The Large Synoptic Survey Telescope (LSST) Project is a public-private partnership that is well into the
design and development of the complete observatory system to conduct a wide fast deep survey and to
process and serve the data. The telescope has a 3-mirror wide field optical system with an 8.4 meter
primary, 3.4 meter secondary, and 5 meter tertiary mirror. The reflective optics feed three refractive
elements and a 64 cm 3.2 gigapixel camera. The LSST data management system will reduce, transport,
alert and archive the roughly 15 terabytes of data produced nightly, and will serve the raw and catalog data
accumulating at an average of 7 petabytes per year to the community without any proprietary period. The
project has completed several data challenges designed to prototype and test the data management system
to significant pre-construction levels. The project continues to attract institutional partners and has acquired
non-federal funding sufficient to construct the primary mirror, already in progress at the University of
Arizona, build the secondary mirror substrate, completed by Corning, and fund detector prototype efforts,
several that have been tested on the sky. A focus of the project is systems engineering, risk reduction
through prototyping and major efforts in image simulation and operation simulations. The project has
submitted a proposal for construction to the National Science Foundation Major Research Equipment and
Facilities Construction (MREFC) program and has prepared project advocacy papers for the National
Research Council's Astronomy 2010 Decadal Survey. The project is preparing for a 2012 construction
funding authorization.
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V. L. Krabbendam, D. Sweeney, "The Large Synoptic Survey Telescope preliminary design overview," Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 77330D (4 August 2010); https://doi.org/10.1117/12.857942