Sub-mm direct photometry with large telescopes

Details Sub-mm direct photometry with large telescopes Sub-mm direct photometry with large telescopes

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..265k&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 265-270 (SEE N91-21986 13-89)

Mathematics

Logic

48

Bolometers, Photometry, Submillimeter Waves, Telescopes, Error Analysis, Meteorological Parameters, Photographic Measurement, Photometers, Technological Forecasting

Scientific paper

Bolometer systems used on largemm telescopes for carrying out sensitive continuum measurements are described. The MPIFR bolometer system on the IRAM 30 m MRT and the SEST (Swedish-ESO Submillimetre Telescope) telescope is given special attention. The characteristics of the bolometer are presented as that of representative example. Special observation procedures designed to account for variations in the limit surface of large telescopes due to gravity, temperature and wind are summarized. Performance figures and plans for future instrumentation are outlined.

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