Stuart D. Ryder
Yin-Sheng Sun
Michael C. B. Ashley
Michael G. Burton
Lori E. Allen
John W. V. Storey
School of Physics, University of New South Wales, Sydney 2052, Australia.
sun, mcba, mgb, lea, jwvs@newt.phys.unsw.edu.au
Current address: Joint Astronomy Centre, 660 N. A'Ohoku Place,
Hilo HI 96720, U.S.A.
sryder@jach.hawaii.edu
We describe the specifications, characteristics, calibration, and
analysis of data from the University of New South Wales Infrared
Fabry-Perot (UNSWIRF) etalon. UNSWIRF is a near-infrared tunable imaging
spectrometer, used primarily in conjunction with IRIS on the AAT, but
suitable for use as a visitor instrument at other telescopes. The
etalon delivers a resolving power in excess of 4000 (corresponding to
a velocity resolution
km
), and allows imaging of fields up
to 100'' in diameter on the AAT at any wavelength between 1.5 and
2.4
m for which suitable blocking filters are available.
Keywords: instrumentation: miscellaneous - methods: data analysis
infrared: ISM: lines
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