Developing Engineering Model Cobra fiber positioners for the Subaru Telescope's Prime Focus Spectrometer
- Creators
- Fisher, Charles
- Morantz, Chaz
- Braun, David
- Seiffert, Michael
- Aghazarian, Hrand
- Partos, Eamon
- King, Matthew
- Hovland, Larry
- Schwochert, Mark
- Kaluzny, Joel
- Capocasale, Christopher
- Houck, Andrew
- Gross, Johannes
- Reiley, Dan
- Mao, Peter
- Riddle, Reed
- Bui, Khanh
- Henderson, David
- Haran, Todd
- Culhane, Rob
- Piazza, Daniele
- Walkama, Eric
Abstract
The Cobra fiber positioner is being developed by the California Institute of Technology (CIT) and the Jet Propulsion Laboratory (JPL) for the Prime Focus Spectrograph (PFS) instrument that will be installed at the Subaru Telescope on Mauna Kea, Hawaii. PFS is a fiber fed multi-object spectrometer that uses an array of Cobra fiber positioners to rapidly reconfigure 2394 optical fibers at the prime focus of the Subaru Telescope that are capable of positioning a fiber to within 5μm of a specified target location. A single Cobra fiber positioner measures 7.7mm in diameter and is 115mm tall. The Cobra fiber positioner uses two piezo-electric rotary motors to move a fiber optic anywhere in a 9.5mm diameter patrol area. In preparation for full-scale production of 2550 Cobra positioners an Engineering Model (EM) version was developed, built and tested to validate the design, reduce manufacturing costs, and improve system reliability. The EM leveraged the previously developed prototype versions of the Cobra fiber positioner. The requirements, design, assembly techniques, development testing, design qualification and performance evaluation of EM Cobra fiber positioners are described here. Also discussed is the use of the EM build and test campaign to validate the plans for full-scale production of 2550 Cobra fiber positioners scheduled to begin in late-2014.
Additional Information
© 2014 Society of Photo-Optical Instrumentation Engineers (SPIE). June 22, 2014. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Funding support was also provided by the Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo.Attached Files
Published - Fisher_2014p91511Y.pdf
Submitted - 1408.2833.pdf
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Additional details
- Eprint ID
- 58259
- DOI
- 10.1117/12.2054700
- Resolver ID
- CaltechAUTHORS:20150615-142629340
- NASA/JPL/Caltech
- Kavli Institute for the Physics and Mathematics of the Universe
- Created
-
2015-06-15Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 9151