Observing with the ISO Short-Wavelength Spectrometer.

Details Observing with the ISO Short-Wavelength Spectrometer. Observing with the ISO Short-Wavelength Spectrometer.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...315l..49d&link_type=abstract

Astronomy and Astrophysics, v.315, p.L49-L54

Astronomy and Astrophysics

Astrophysics

486

Instrumentation: Spectrographs, Methods: Data Analysis, Methods: Observational, Techniques: Spectroscopic, Infrared: General

Scientific paper

The Short-Wavelength Spectrometer (SWS) is one of the four instruments on-board ESA's Infrared Space Observatory (ISO), launched on November 17, 1995. The spectrometer covers the wavelength range of 2.38 to 45.2μm with a spectral resolution ranging from 1000 to 2000. By inserting Fabry-Perot filters the resolution can be enhanced by a factor 20 for the wavelength range from 11.4 to 44.5μm. An overview is given of the instrument, its in-orbit calibration, performance, observing modes and off-line processing software.

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