Paper
22 July 2016 Back-propagating the light of field stars to probe telescope mirrors aberrations
F. Soulez, F. Courbin, M. Unser
Author Affiliations +
Abstract
We propose a wavefront-based method to estimate the PSF over the whole field of view. This method estimate the aberrations of all the mirrors of the telescope using only field stars. In this proof of concept paper, we described the method and present some qualitative results.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
F. Soulez, F. Courbin, and M. Unser "Back-propagating the light of field stars to probe telescope mirrors aberrations", Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 991277 (22 July 2016); https://doi.org/10.1117/12.2232702
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Telescopes

Telescopes

Mirrors

Space telescopes

Space telescopes

Point spread functions

RELATED CONTENT

AIV procedure for a CHEOPS demonstration model
Proceedings of SPIE (August 28 2014)
The FLARE mission deep and wide field 1 5um...
Proceedings of SPIE (July 29 2016)
DUNE: the Dark Universe Explorer
Proceedings of SPIE (June 14 2006)

Back to Top