Modeling highly aspherical optical surfaces using a new polynomial formalism into Zemax
S. Vivès(Laboratoire d’Astrophysique de Marseille), Marc Ferrari(Laboratoire d’Astrophysique de Marseille), D. Le Mignant(Laboratoire d’Astrophysique de Marseille), Jean-Gabriel Cuby(Centre National de la Recherche Scientifique), S. Pascal(Centre National de la Recherche Scientifique), A. Secroun(Centre de physique des particules de Marseille), Morgan Gray(Centre National de la Recherche Scientifique)
Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE
September 20, 2011
Cited by 6
Related Papers
The DESI Experiment Part I: Science,Targeting, and Survey Design
|arXiv (Cornell University)|2016|1.3k
The DESI Experiment Part II: Instrument Design
|arXiv (Cornell University)|2016|236
A complex multi-notch astronomical filter to suppress the bright infrared sky
|Nature Communications|2011|143
Spectroscopic confirmation of a galaxy at redshift z = 8.6
|Nature|2010|130
The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-<i>α</i>emitters from<i>z</i>= 2 to<i>z</i>= 6
|Astronomy and Astrophysics|2014|127