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Proceedings Paper

A 1.4 Meter Fourier Transform Spectrometer For Astronomical Observations
Author(s): D. N. B. Hall; Steve Ridgway; E. A. Bell; J. M. Yarborough
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Paper Abstract

The observational capability and instrumental details of a Fourier spectrometer intended for moderate to very high resolution (20 cm-1 to 0.005 cm-1) observations of astronomical sources in the visible and infrared (700-2800 cm-1 i.e., 0.36μm to l4μm) are described and a few initial spectra are shown to illustrate performance achieved to date. The instrument is unusual in that it can be maintained by a moderate level of non-specialist technical support and does not require the observer to be an instrumentalist familiar with the details of the spectrometer.

Paper Details

Date Published: 3 May 1979
PDF: 9 pages
Proc. SPIE 0172, Instrumentation in Astronomy III, (3 May 1979); doi: 10.1117/12.957074
Show Author Affiliations
D. N. B. Hall, Kitt Peak National Observatory (United States)
Steve Ridgway, Kitt Peak National Observatory (United States)
E. A. Bell, Kitt Peak National Observatory (United States)
J. M. Yarborough, Kitt Peak National Observatory (United States)


Published in SPIE Proceedings Vol. 0172:
Instrumentation in Astronomy III
David L. Crawford, Editor(s)

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