Postdispersion system for astronomical observations with Fourier transform spectrometers in the thermal infrared

Details Postdispersion system for astronomical observations with Fourier transform spectrometers in the thermal infrared Postdispersion system for astronomical observations with Fourier transform spectrometers in the thermal infrared

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apopt..28..139w&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 28, Jan. 1, 1989, p. 139-145.

Astronomy and Astrophysics

Astronomy

13

Astronomical Observatories, Fourier Transformation, Infrared Astronomy, Infrared Spectra, Thermal Radiation, High Resolution, Spectral Bands, Spectral Resolution, Voyager 2 Spacecraft

Scientific paper

A postdispersion system for astronomical observations with Fourier transform spectrometers in the thermal infrared has been developed which improves the sensitivity of radiation noise limited observations by reducing the spectral range incident on the detector. Special attention is given to the first-generation blocked impurity band detector. Planetary, solar, and stellar observations are reported.

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