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Proceedings Paper

The CCD imaging systems for LAMOST
Author(s): Sicheng Zou; Gang Wang
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Paper Abstract

The CCD imaging systems for the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) are being designed and built in the National Astronomical Observatories of China (NAOC). LAMOST is to be equipped with 16 low-resolution spectrographs (LRS) with a total 32 CCD cameras. Each CCD camera consists of a LN2 cooling system, a CCD controller and a large-format scientific-grade CCD with 4K*4K pixels, two output registers and four output amplifiers. The CCD controller enables low readout noise, photometric stability and software-selectable switching from single- to four- output amplifier readout modes. The whole 32 CCD cameras need to be communicated with several network-connected computers. The computer cluster allows synchronized processes of accumulation and readout of CCD systems and rapid, reliable data transfer from CCD cameras. We introduce the current design of above components as well as its performance. And the design schedule of the CCD imaging systems for LAMOST is reported.

Paper Details

Date Published: 29 June 2006
PDF: 8 pages
Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 626922 (29 June 2006); doi: 10.1117/12.669319
Show Author Affiliations
Sicheng Zou, National Astronomical Observatories (China)
Gang Wang, National Astronomical Observatories (China)


Published in SPIE Proceedings Vol. 6269:
Ground-based and Airborne Instrumentation for Astronomy
Ian S. McLean; Masanori Iye, Editor(s)

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