Paper
21 September 2011 BigBOSS: enabling widefield cosmology on the Mayall Telescope
Author Affiliations +
Abstract
BigBOSS is a proposed DOE-NSF Stage IV ground-based dark energy experiment designed to study baryon acoustic oscillations (BAO) and the growth of large scale structure with a 14,000 square degree survey of the redshifts of galaxies and quasi-stellar objects. The project involves modification of existing facilities operated by the National Optical Astronomy Observatory (NOAO). Design and systems engineering of a preliminary 3 degree field of view refractive corrector, atmospheric dispersion corrector (ADC), and 5000 actuator fiber positioning system are presented.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael J. Sholl, Chris Bebek, Robert Besuner, Arjun Dey, Jerry Edelstein, Patrick Jelinsky, Michael L. Lampton, Michael E. Levi, Ming Liang, Paul Perry, Natalie Roe, and David Schlegel "BigBOSS: enabling widefield cosmology on the Mayall Telescope", Proc. SPIE 8127, Optical Modeling and Performance Predictions V, 81270D (21 September 2011); https://doi.org/10.1117/12.894381
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Galactic astronomy

Prisms

Spectrometers

Silica

Actuators

Astronomical imaging

RELATED CONTENT

Fibre system of DESI
Proceedings of SPIE (July 24 2014)
The Dark Energy Spectroscopic Instrument (DESI)
Proceedings of SPIE (July 18 2014)
Optical design of a Coudé Train for a stable and...
Proceedings of SPIE (November 18 2013)
An all-silica three element wide-field corrector for GMT
Proceedings of SPIE (August 08 2016)
Grism manufacturing by low temperature mineral bonding
Proceedings of SPIE (September 25 2017)
BigBOSS: a stage IV dark energy redshift survey
Proceedings of SPIE (September 24 2012)

Back to Top