23 June 2006 Overview of the Large Synoptic Survey Telescope project
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LSST will be a large, wide-field groundbased telescope designed to obtain sequential images of the entire visible sky every few nights. The optical design involves a 3-mirror system with an 8.4 m primary, which feeds three refractive correcting elements inside a camera, providing a 10 square degree field of view sampled by a 3 Gpixel focal plane array. The total effective system throughput, AΩ = 319 m2 deg2, is nearly two orders of magnitude larger than that of any existing facility. The survey will yield contiguous overlapping imaging of 20,000 square degrees of sky in 6 optical bands covering the wavelength regime 320-1060 nm.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Donald W. Sweeney, Donald W. Sweeney, "Overview of the Large Synoptic Survey Telescope project", Proc. SPIE 6267, Ground-based and Airborne Telescopes, 626706 (23 June 2006); doi: 10.1117/12.668217; https://doi.org/10.1117/12.668217


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