High-sensitivity observations with the Infrared Space Observatory-Short Wavelength Spectrometer (ISO-SWS)

Dieter Lutz; Mattheus WM de Graauw

doi:10.1117/12.185834

14 September 1994 High-sensitivity observations with the Infrared Space Observatory Short Wavelength Spectrometer (ISO-SWS)

Dieter Lutz, Mattheus WM de Graauw

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Proceedings Volume 2268, Infrared Spaceborne Remote Sensing II; (1994) https://doi.org/10.1117/12.185834
Event: SPIE's 1994 International Symposium on Optics, Imaging, and Instrumentation, 1994, San Diego, CA, United States

Abstract

The ISO Short Wavelength Spectrometer will open the full 2.4-45 micrometers wavelength range for astronomical spectroscopy. At spectral resolving power approximately equals 1000, most sources detected by IRAS will be within reach. In addition, spectral resolving power approximately equals 30000 is provided for the 12-45 micrometers range. Examples of proposed observations illustrate the SWS capabilities.

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Dieter Lutz and Mattheus WM de Graauw "High-sensitivity observations with the Infrared Space Observatory Short Wavelength Spectrometer (ISO-SWS)", Proc. SPIE 2268, Infrared Spaceborne Remote Sensing II, (14 September 1994); https://doi.org/10.1117/12.185834

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KEYWORDS

Calibration

Spectroscopy

Spectral resolution

Galactic astronomy

Infrared radiation

Infrared spectroscopy

Sensors

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