
Proceedings Paper
VIRUS instrument enclosuresFormat | Member Price | Non-Member Price |
---|---|---|
$17.00 | $21.00 |
Paper Abstract
The Visible Integral-Field Replicable Unit Spectrograph (VIRUS) instrument will be installed at the Hobby-Eberly
Telescope† in the near future. The instrument will be housed in two enclosures that are mounted adjacent to the
telescope, via the VIRUS Support Structure (VSS). We have designed the enclosures to support and protect the
instrument, to enable servicing of the instrument, and to cool the instrument appropriately while not adversely affecting
the dome environment. The system uses simple HVAC air handling techniques in conjunction with thermoelectric and
standard glycol heat exchangers to provide efficient heat removal. The enclosures also provide power and data transfer
to and from each VIRUS unit, liquid nitrogen cooling to the detectors, and environmental monitoring of the instrument
and dome environments. In this paper, we describe the design and fabrication of the VIRUS enclosures and their subsystems.
Paper Details
Date Published: 6 August 2014
PDF: 12 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91476U (6 August 2014); doi: 10.1117/12.2057040
Published in SPIE Proceedings Vol. 9147:
Ground-based and Airborne Instrumentation for Astronomy V
Suzanne K. Ramsay; Ian S. McLean; Hideki Takami, Editor(s)
PDF: 12 pages
Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91476U (6 August 2014); doi: 10.1117/12.2057040
Show Author Affiliations
T. Prochaska, Texas A&M Univ. (United States)
R. Allen, Texas A&M Univ. (United States)
N. Mondrik, Texas A&M Univ. (United States)
J. P. Rheault, Texas A&M Univ. (United States)
M. Sauseda, Texas A&M Univ. (United States)
E. Boster, Texas A&M Univ. (United States)
M. James, Texas A&M Univ. (United States)
M. Rodriguez-Patino, Texas A&M Univ. (United States)
G. Torres, Texas A&M Univ. (United States)
J. Ham, Texas A&M Univ. (United States)
R. Allen, Texas A&M Univ. (United States)
N. Mondrik, Texas A&M Univ. (United States)
J. P. Rheault, Texas A&M Univ. (United States)
M. Sauseda, Texas A&M Univ. (United States)
E. Boster, Texas A&M Univ. (United States)
M. James, Texas A&M Univ. (United States)
M. Rodriguez-Patino, Texas A&M Univ. (United States)
G. Torres, Texas A&M Univ. (United States)
J. Ham, Texas A&M Univ. (United States)
E. Cook, Texas A&M Univ. (United States)
D. Baker, Texas A&M Univ. (United States)
Darren L. DePoy, Texas A&M Univ. (United States)
Jennifer L. Marshall, Texas A&M Univ. (United States)
G. J. Hill, McDonald Observatory, The Univ. of Texas at Austin (United States)
The Univ. of Texas at Austin (United States)
D. Perry, McDonald Observatory, The Univ. of Texas at Austin (United States)
R. D. Savage, McDonald Observatory, The Univ. of Texas at Austin (United States)
J. M. Good, McDonald Observatory, The Univ. of Texas at Austin (United States)
Brian L. Vattiat, McDonald Observatory, The Univ. of Texas at Austin (United States)
D. Baker, Texas A&M Univ. (United States)
Darren L. DePoy, Texas A&M Univ. (United States)
Jennifer L. Marshall, Texas A&M Univ. (United States)
G. J. Hill, McDonald Observatory, The Univ. of Texas at Austin (United States)
The Univ. of Texas at Austin (United States)
D. Perry, McDonald Observatory, The Univ. of Texas at Austin (United States)
R. D. Savage, McDonald Observatory, The Univ. of Texas at Austin (United States)
J. M. Good, McDonald Observatory, The Univ. of Texas at Austin (United States)
Brian L. Vattiat, McDonald Observatory, The Univ. of Texas at Austin (United States)
Published in SPIE Proceedings Vol. 9147:
Ground-based and Airborne Instrumentation for Astronomy V
Suzanne K. Ramsay; Ian S. McLean; Hideki Takami, Editor(s)
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