Low-resolution imaging spectroscopy with SOFIA

Details Low-resolution imaging spectroscopy with SOFIA Low-resolution imaging spectroscopy with SOFIA

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3354..755k&link_type=abstract

Proc. SPIE Vol. 3354, p. 755-759, Infrared Astronomical Instrumentation, Albert M. Fowler; Ed.

Computer Science

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Scientific paper

LISA is the low resolution imaging spectrometer channel for SPICA. the proposed spectral-photometric-IR camera for the joint US and German stratospheric far IR observatory SOFIA. LISA will cover a spectral range from 40 micrometers to 220 micrometers at a spectral resolution (lambda) /(Delta) (lambda) approximately 22. It will record simultaneously individual diffraction limited spectra from several tens to several hundreds spatial positions of a rectangular field of view on the sky. A novel technical and optical solution will be presented for such an approach together with a brief discussion on the expected performance and possible astronomical applications.

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