Title of article
Technology of the LSST focal plane
Author/Authors
O’Connor، نويسنده , , P. and Geary، نويسنده , , Claire J. and Gilmore، نويسنده , , K. and Oliver، نويسنده , , J. and Radeka، نويسنده , , Valeriy V. and Takacs، نويسنده , , P.، نويسنده ,
Pages
8
From page
902
To page
909
Abstract
The Large Synoptic Survey Telescope, now in the research and development phase, will undertake a wide angle, deep survey of the entire southern sky starting in 2014. The survey database will support a wide variety of astrophysical investigations, with particular emphasis on elucidating the nature of dark energy. To achieve its science goals, LSST will incorporate a silicon-based focal plane with unprecedented size (3 Gpixel), speed (2 s readout), and sensitivity (high QE over 350–1000 nm wavelength). The technologies to be used in the LSST camera are described, with an emphasis on the silicon sensors and readout electronics.
Journal title
Astroparticle Physics
Record number
2031301
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