21 August 1998 UNSWIRF: the University of New South Wales infrared Fabry-Perot
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We describe an imaging Fabry-Perot instrument, and give examples of its astronomical applications. The salient features of the instrument are: wide wavelength coverage with a single etalon, operation near the focal plane in a converging beam, resolving power R approximately 4000, relatively easy portability to other telescopes.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Lori E. Allen, Lori E. Allen, Michael C. B. Ashley, Michael C. B. Ashley, Michael G. Burton, Michael G. Burton, Stuart D. Ryder, Stuart D. Ryder, John W. V. Storey, John W. V. Storey, Yinsheng Sun, Yinsheng Sun, } "UNSWIRF: the University of New South Wales infrared Fabry-Perot", Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); doi: 10.1117/12.317242; https://doi.org/10.1117/12.317242


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