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Postdispersion system for astronomical observations with Fourier transform spectrometers in the thermal infraredA 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.
Document ID
19890038975
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wiedermann, Guenter
(Max-Planck-Institut fuer extraterrestrische Physik Garching, Federal Republic of Germany, United States)
Jennings, D. E.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Hanel, R. H.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Kunde, V. G.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Moseley, S. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Applied Optics
Volume: 28
ISSN: 0003-6935
Subject Category
Instrumentation And Photography
Accession Number
89A26346
Distribution Limits
Public
Copyright
Other

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