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6. Real-time turbulence profiling with a pair of laser guide star Shack-Hartmann wavefront sensors for wide-field adaptive optics systems on large to extremely large telescopes. Gilles L; Ellerbroek BL J Opt Soc Am A Opt Image Sci Vis; 2010 Nov; 27(11):A76-83. PubMed ID: 21045893 [TBL] [Abstract][Full Text] [Related]
7. Revisiting the comparison between the Shack-Hartmann and the pyramid wavefront sensors via the Fisher information matrix. Plantet C; Meimon S; Conan JM; Fusco T Opt Express; 2015 Nov; 23(22):28619-33. PubMed ID: 26561131 [TBL] [Abstract][Full Text] [Related]
8. Wavefront reconstruction for extremely large telescopes via CuRe with domain decomposition. Rosensteiner M J Opt Soc Am A Opt Image Sci Vis; 2012 Nov; 29(11):2328-36. PubMed ID: 23201793 [TBL] [Abstract][Full Text] [Related]