Translator Disclaimer
9 August 2016 Impact of optical distortions on fiber positioning in the dark energy spectroscopic instrument
Author Affiliations +
Abstract
The Dark Energy Spectroscopic Instrument, to be located at the prime focus of the Mayall telescope, includes a wide field corrector, a 5000 fiber positioner system, and a fiber view camera. The mapping of the sky to the focal plane, needed to position the fibers accurately, is described in detail. A major challenge is dealing with the large amount of distortion introduced by the optics (of order 10% scale change), including time-dependent non-axisymmetric distortions introduced by the atmospheric dispersion compensator. Solutions are presented to measure or mitigate these effects.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephen Kent, Michael Lampton, A. Peter Doel, David Brooks, Tim Miller, Robert Besuner, Joe Silber, Ming Liang, David Sprayberry, Charles Baltay, and David Rabinowitz "Impact of optical distortions on fiber positioning in the dark energy spectroscopic instrument", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99088F (9 August 2016); https://doi.org/10.1117/12.2232689
PROCEEDINGS
10 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Mosaic3 a red sensitive upgrade for the prime focus...
Proceedings of SPIE (August 09 2016)
Measuring system of fiber position of LAMOST
Proceedings of SPIE (September 29 2004)
Status of the Dark Energy Survey Camera (DECam) project
Proceedings of SPIE (September 24 2012)
T80Cam the wide field camera for the OAJ 83...
Proceedings of SPIE (September 24 2012)
Low-cost CCD cameras for amateur astronomy
Proceedings of SPIE (October 24 2003)

Back to Top