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Optics Design and Verificatgion for the APEX Swedish Heterodyne Facility Instrument (SHeFI)

Nyström, Olle, 1979 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Lapkin, Igor, 1963 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Desmaris, Vincent, 1977 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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Dochev, Dimitar Milkov, 1981 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Ferm, Sven-Erik, 1961 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Fredrixon, Mathias, 1972 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Henke, Doug, 1974 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Meledin, Denis, 1974 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Monje, Raquel, 1979 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Strandberg, Magnus, 1975 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Sundin, Erik, 1979 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Vassilev, Vessen, 1969 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Belitsky, Victor, 1955 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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 (creator_code:org_t)
2009-05-01
2009
English.
In: Journal of Infrared, Millimeter, and Terahertz Waves. - : Springer Science and Business Media LLC. - 1866-6892 .- 1866-6906. ; 30:7, s. 746-761
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • In this paper, we present the design and verification of the optics of the Swedish Heterodyne Facility Instrument (SHeFI) receiver installed in the Atacama Pathfinder EXperiment (APEX) telescope during spring 2008. SHeFI is located in the Nasmyth instrumentation Cabin A (NCA). The receiver has been designed to have 6 frequency channels, of which four receiver channels have been built, and characterized: 211-275 GHz(Band 1), 275-370 GHz (Band 2), 385-500 GHz (Band 3), and 1250-1390 GHz (Band T2). Bands 1, 2, and T2 are installed at the telescope and are currently in operation. The optical design is driven by the requirement of frequency independent illumination of the secondary with -12 dB edge taper for each frequency channel and the limitation (beam clearance through the Nasmyth tube and the elevation encoder) imposed by the receiver position in the NCA. This paper describes the design approach, optimization, and verification of the optical system, coupling each individual receiving beam to the common optics of the telescope.

Subject headings

TEKNIK OCH TEKNOLOGIER  -- Annan teknik (hsv//swe)
ENGINEERING AND TECHNOLOGY  -- Other Engineering and Technologies (hsv//eng)
TEKNIK OCH TEKNOLOGIER  -- Annan teknik -- Övrig annan teknik (hsv//swe)
ENGINEERING AND TECHNOLOGY  -- Other Engineering and Technologies -- Other Engineering and Technologies not elsewhere specified (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

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