Paper
10 July 2014 VIRUS: assembly, testing and performance of 33,000 fibres for HETDEX
Andreas Kelz, Thomas Jahn, D. Haynes, G. J. Hill, H. Lee, J. D. Murphy, Justus Neumann, Harald Nicklas, M. Rutowska, C. Sandin, O. Streicher, S. Tuttle, M. Fabricius, S. M. Bauer, B. Vattiat, H. Anwand, R. Savage
Author Affiliations +
Abstract
VIRUS is the visible, integral-field replicable unit spectrograph for the Hobby-Eberly-Telescope (HET) consisting of 75 integral-field-units that feed 150 spectrographs. The full VIRUS instrument features over 33,000 fibres, each projecting to 1.5 arcseconds diameter on sky, deployed at the prime focus of the upgraded 10m HET. The assembly and acceptance testing for all IFUs includes microscopic surface quality inspections, astrometry of fibre positions, relative throughput measurements, focal-ratio-degradation evaluation, and system acceptance using a VIRUS reference spectrograph to verify the image quality, spectral transmission, stability, or to detect any stray light issues.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andreas Kelz, Thomas Jahn, D. Haynes, G. J. Hill, H. Lee, J. D. Murphy, Justus Neumann, Harald Nicklas, M. Rutowska, C. Sandin, O. Streicher, S. Tuttle, M. Fabricius, S. M. Bauer, B. Vattiat, H. Anwand, and R. Savage "VIRUS: assembly, testing and performance of 33,000 fibres for HETDEX", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914775 (10 July 2014); https://doi.org/10.1117/12.2056384
Lens.org Logo
CITATIONS
Cited by 5 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Spectrographs

Head

Polishing

Image quality

Surface finishing

Telescopes

Inspection

RELATED CONTENT

Optical design of MAAT an IFU for the GTC...
Proceedings of SPIE (August 29 2022)
The VIRUS data reduction pipeline
Proceedings of SPIE (June 30 2006)
The VIRMOS very wide integral field unit for the VLT...
Proceedings of SPIE (March 07 2003)
Performances of HARPS and FEROS fibers in La Silla ESO...
Proceedings of SPIE (September 30 2004)

Back to Top