Computer Science – Performance
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982spie..332...65w&link_type=abstract
IN: International Conference on Advanced Technology Optical Telescopes, Tucson, AZ, March 11-13, 1982, Proceedings (A83-30976 13
Computer Science
Performance
High Resolution, Mirrors, Performance Tests, Reflecting Telescopes, Signal To Noise Ratios, Charge Coupled Devices, Fourier Transformation, Gratings (Spectra), Infrared Interferometers, Michelson Interferometers, Speckle Patterns, Spectral Resolution
Scientific paper
Attention is given to the design features and measured or projected performance of several astronomical research instruments which can be used with the Multiple Mirror Telescope (MMT). Among these, the high resolution Echelle spectrograph, the intermediate resolution spectrograph, and the IR photometer, have reached a stage of development and reliability at which any qualified astronomer, after receiving the requisite instruction, can apply for observational use of them. The optical speckle camera, Fourier transform spectrometers and IR Michelson interferometer incorporated by the MMT, however, are either very specialized or still undergoing development and testing.
Angel James Roger P.
Chaffee Frederic
Lebofsky Matt
Weymann Ray
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