Infrared Fourier spectrometer for airborne and ground-based astronomy

Details Infrared Fourier spectrometer for airborne and ground-based astronomy Infrared Fourier spectrometer for airborne and ground-based astronomy

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apopt..19.4138d&link_type=abstract

Applied Optics, vol. 19, Dec. 15, 1980, p. 4138-4155.

Physics

Optics

24

Astronomical Spectroscopy, Fourier Analysis, High Resolution, Infrared Spectrometers, Telescopes, Airborne Equipment, Cassegrain Optics, Ground Stations, Indium Antimonides, Infrared Detectors

Scientific paper

A unique high resolving power near-infrared, astronomical Fourier spectrometer has been constructed for use at both ground-based and airborne telescopes. Its capabilities include a limiting resolution of 0.01/cm and spectral coverage over the InSb detector sensitivity region (0.8-5.6 micron). The instrument is optimized for operation in environments inaccessible to other high-resolution Fourier spectrometers, namely, the Cassegrain focuses of conventional telescopes and the NASA Kuiper Airborne Observatory's 91-cm telescope. Details of the spectrometer are discussed, and various astronomical and laboratory spectra are presented.

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