Imaging Fourier transform spectrometer for NGST

Details Imaging Fourier transform spectrometer for NGST Imaging Fourier transform spectrometer for NGST

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4013..706p&link_type=abstract

Proc. SPIE Vol. 4013, p. 706-714, UV, Optical, and IR Space Telescopes and Instruments, James B. Breckinridge; Peter Jakobsen; E

Computer Science

Scientific paper

An imaging FTS would be capable of carrying out many of the programs in the DRM, namely all those which require imaging and/or low spectral resolution wide field/multi-object spectroscopy. We review the DRM science areas, describing the relevance of an imaging FTS. Required instrumental capabilities are then derived from the science goals. Our compact camera and imaging FTS instrument design emphasizes simplicity with a single optical train covering a field 6 X 3 arcmin2, with a fixed spatial sampling of 0.03 arcsec/pixel on a 12 k X 6 k detector array.

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