Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989irsa.rept..571w&link_type=abstract
In ESA, Infrared Spectroscopy in Astronomy p 571-573 (SEE N90-19084 11-89)
Astronomy and Astrophysics
Astronomy
Infrared Space Observatory (Iso), Infrared Spectrometers, Near Infrared Radiation, Spectral Resolution, Background Radiation, Continuous Radiation, Design Analysis, European Space Programs, Spectral Sensitivity
Scientific paper
The design, spectral coverage and sensitivity of Isophot-S, one of the four sub-experiments of Isophot, are described. Isophot-S is a low resolution near infrared spectrometer, designed to take full advantage of the Infrared Space Observatory (ISO) telescope with its low infrared background, wide field of view, and the complete absence of atmospheric attenuation. It consists of two grating spectrometers which cover the wavelength ranges 2.5 to 5 microns and 6 to 12 microns at resolutions of 0.04 microns and 0.09 microns respectively. The scientific capabilities of the equipment are underlined.
Chakaveh Sepideh
Garzon Francisco
Joseph Robert D.
Lemke Deitrich
Lutzow-Wentzky P.
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