Presentation + Paper
6 July 2018 VIRUS: status and performance of the massively replicated fiber integral field spectrograph for the upgraded Hobby-Eberly Telescope
Gary J. Hill, Andreas Kelz, Hanshin Lee, Phillip MacQueen, Trent W. Peterson, Jason Ramsey, Brian L. Vattiat, D. L. DePoy, Niv Drory, Karl Gebhardt, John M. Good, Thomas Jahn, Herman Kriel, J. L. Marshall, Sarah E. Tuttle, Greg Zeimann, Edmundo Balderrama, Randy Bryant, Brent Buetow, Taylor S. Chonis, George Damm, Maximilian H. Fabricius, Daniel Farrow, James R. Fowler, Cynthia Froning, Dionne M. Haynes, Briana L. Indahl, Jerry Martin, Francesco Montesano, Emily Mrozinski, Harald Nicklas, Eva Noyola, Stephen Odewahn, Andrew Peterson, Travis Prochaska, Sergey Rostopchin, Matthew Shetrone, Greg Smith, Jan M. Snigula, Renny Spencer, Amy Westfall, Taft Armandroff, Ralf Bender, Gavin Dalton, Matthias Steinmetz
Author Affiliations +
Abstract
The Visible Integral-field Replicable Unit Spectrograph (VIRUS) consists of 156 identical spectrographs (arrayed as 78 pairs, each with a pair of spectrographs) fed by 35,000 fibers, each 1.5 arcsec diameter, at the focus of the upgraded 10 m Hobby-Eberly Telescope (HET). VIRUS has a fixed bandpass of 350-550 nm and resolving power R~750. The fibers are grouped into 78 integral field units, each with 448 fibers and 20 m average length. VIRUS is the first example of large-scale replication applied to optical astronomy and is capable of surveying large areas of sky, spectrally. The VIRUS concept offers significant savings of engineering effort and cost when compared to traditional instruments. The main motivator for VIRUS is to map the evolution of dark energy for the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), using 0.8M Lyman-alpha emitting galaxies as tracers. The VIRUS array has been undergoing staged deployment starting in late 2015. Currently, more than half of the array has been populated and the HETDEX survey started in 2017 December. It will provide a powerful new facility instrument for the HET, well suited to the survey niche of the telescope, and will open up large spectroscopic surveys of the emission line universe for the first time. We will review the current state of production, lessons learned in sustaining volume production, characterization, deployment, and commissioning of this massive instrument.
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gary J. Hill, Andreas Kelz, Hanshin Lee, Phillip MacQueen, Trent W. Peterson, Jason Ramsey, Brian L. Vattiat, D. L. DePoy, Niv Drory, Karl Gebhardt, John M. Good, Thomas Jahn, Herman Kriel, J. L. Marshall, Sarah E. Tuttle, Greg Zeimann, Edmundo Balderrama, Randy Bryant, Brent Buetow, Taylor S. Chonis, George Damm, Maximilian H. Fabricius, Daniel Farrow, James R. Fowler, Cynthia Froning, Dionne M. Haynes, Briana L. Indahl, Jerry Martin, Francesco Montesano, Emily Mrozinski, Harald Nicklas, Eva Noyola, Stephen Odewahn, Andrew Peterson, Travis Prochaska, Sergey Rostopchin, Matthew Shetrone, Greg Smith, Jan M. Snigula, Renny Spencer, Amy Westfall, Taft Armandroff, Ralf Bender, Gavin Dalton, and Matthias Steinmetz "VIRUS: status and performance of the massively replicated fiber integral field spectrograph for the upgraded Hobby-Eberly Telescope", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107021K (6 July 2018); https://doi.org/10.1117/12.2314280
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CITATIONS
Cited by 7 scholarly publications.
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KEYWORDS
Spectrographs

Telescopes

Cameras

Charge-coupled devices

Sensors

Image quality

Mirrors

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