IRS: the Infrared Spectrograph on SIRTF

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dc.creatorHouck, J.
dc.creatorvan Cleve, J.
dc.creatorBrandl, B.
dc.creatorCharmandaris, V.
dc.creatorDevost, D.
dc.creatorUchida, K.
dc.date2000-03-15
dc.date.accessioned2026-07-07T01:52:45Z
dc.date.available2026-07-07T01:52:45Z
dc.descriptionThe Infrared Spectrograph (IRS)is one of the three instruments on board the Space Infrared Telescope Facility (SIRTF) to be launched in December 2001. The IRS will provide high resolution spectra R~600 from 10--37microns and low resolution spectra R~60 from 5.3--40microns Its high sensitivity and ``spectral mapping-mode'' make it a powerful instrument for observing both faint point-like and extended sources.
dc.description3 pages, 7 figures. To appear in the Proceedings of ``ISO beyond the Peaks'', Villafranca del Castillo, Spain 2-4 February 2000 (ESA SP-456, 2000). Higher resolution color images available at http://www.astro.cornell.edu/SIRTF
dc.identifierhttps://arxiv.org/abs/astro-ph/0003226
dc.identifierhttp://arxiv.org/abs/astro-ph/0003226
dc.identifierAstrophys.Space Sci. 277 (2001) 97-97
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/729
dc.subjectAstrophysics
dc.titleIRS: the Infrared Spectrograph on SIRTF
dc.typetext

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