The Swedish-ESO Submillimetre Telescope

Details The Swedish-ESO Submillimetre Telescope The Swedish-ESO Submillimetre Telescope

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987msngr..48....2b&link_type=abstract

ESO Messenger (ISSN 0722-6691), June 1987, p. 2-6.

Computer Science

Performance

7

European Space Agency, Radio Telescopes, Submillimeter Waves, Swedish Space Program, Telescopes, Atmospheric Attenuation, Automatic Control, Data Processing, Functional Design Specifications, User Requirements

Scientific paper

The Swedish-ESO Submillimeter Telescope (SEST) is designed to achieve a reflector profile accuracy of 50 microns rms giving good (coherent) performance down to wavelengths of less than about 0.8 mm (375 GHz). La Silla is an important site for SEST owing to its southern location and low atmospheric attenuation. SEST control and data analysis are discussed as well as its operations and scientific program.

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