scholarly journals UNSWIRF: A Tunable Imaging Spectrometer for the Near-Infrared

1998 ◽  
Vol 15 (2) ◽  
pp. 228-239 ◽  
Author(s):  
Stuart D. Ryder ◽  
Yin-Sheng Sun ◽  
Michael C. B. Ashley ◽  
Michael G. Burton ◽  
Lori E. Allen ◽  
...  

AbstractWe 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 ∼75 km s−1), and allows imaging of fields up to 100″ in diameter on the AAT at any wavelength between 1·5 and 2·4 μm for which suitable blocking filters are available.


1997 ◽  
Vol 180 ◽  
pp. 205-205
Author(s):  
L. E. Allen ◽  
M.C.B. Ashley ◽  
S. D. Ryder ◽  
J.W.V. Storey ◽  
Y-S. Sun ◽  
...  

Near-infrared (1-3μm) emission lines of molecular and ionized hydrogen are excellent tools for investigating the morphology, energetics and kinematics of planetary nebulae, especially those PNe which contain large amounts of dust and are thus obscured at shorter wavelengths. The southern planetary nebula NGC 3132 was imaged with UNSWIRF (University of New South Wales Infrared Fabry-Perot) and IRIS on the 3.9m AAT Images in the H2 v=1-0 S(1) and H2 v=2-1 S(1) lines at 2.12μm and 2.25μm, and in Hii Brγ at 2.16μm are presented.



1998 ◽  
Author(s):  
Lori E. Allen ◽  
Michael C. B. Ashley ◽  
Michael G. Burton ◽  
Stuart D. Ryder ◽  
John W. V. Storey ◽  
...  


1994 ◽  
Vol 128 (4) ◽  
pp. 447-454 ◽  
Author(s):  
Melissa M. Monfries ◽  
Norman F. Kafer


Sign in / Sign up

Export Citation Format

Share Document