Stuart D. Ryder , Yin-Sheng Sun , Michael C. B. Ashley , Michael G. Burton , Lori E. Allen , John W. V. Storey, PASA, 15 (2), 228
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file.
Next Section: Introduction
UNSWIRF: A Tunable Imaging Spectrometer for the Near-Infrared
Stuart D. Ryder
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, email@example.com
Current address: Joint Astronomy Centre, 660 N. A'Ohoku Place, Hilo HI 96720, U.S.A.
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
|HTML Section||Download Full Paper|
© Copyright Astronomical Society of Australia 1997