Closed-loop adaptive optic comparison between a Shack-Hartmann and a distorted-grating wavefront sensor

2004 ◽  
Author(s):  
Paul Harrison ◽  
Gavin R. G. Erry ◽  
Leonard J. Otten III ◽  
D. M. Cuevas ◽  
Lawrence D. Weaver
2004 ◽  
Author(s):  
Paul Harrison ◽  
Gavin R. G. Erry ◽  
Leonard J. Otten ◽  
Desirae M. Cuevas ◽  
Lawrence D. Weaver

2012 ◽  
Author(s):  
Shengqian Wang ◽  
Changhui Rao ◽  
Ang Zhang ◽  
Xuejun Zhang ◽  
Kai Wei ◽  
...  

1980 ◽  
Author(s):  
L. E. Schmutz ◽  
J. K. Bowker ◽  
J. Feinleib ◽  
S. N. Landon ◽  
S. J. Tubbs

Author(s):  
Alexis Kudryashov ◽  
Alex Alexandrov ◽  
Vadim Samarkin ◽  
Alexey Rukosuev ◽  
Pierre Galarneau

2012 ◽  
Vol 285 (12) ◽  
pp. 2814-2820
Author(s):  
Jianxin Wang ◽  
Fuzhong Bai ◽  
Yu Ning ◽  
Fei Li ◽  
Wenhan Jiang

2016 ◽  
Author(s):  
Shengqian Wang ◽  
Kai Wei ◽  
Wenjia Zheng ◽  
Changhui Rao

2013 ◽  
Vol 8 (S299) ◽  
pp. 34-35 ◽  
Author(s):  
Thayne Currie ◽  
Olivier Guyon ◽  
Frantz Martinache ◽  
Christophe Clergeon ◽  
Michael McElwain ◽  
...  

AbstractWe present new on-sky results for the Subaru Coronagraphic Extreme Adaptive Optics imager (SCExAO) verifying and quantifying the contrast gain enabled by key components: the closed-loop coronagraphic low-order wavefront sensor (CLOWFS) and focal plane wavefront control (“speckle nulling”). SCExAO will soon be coupled with a high-order, Pyramid wavefront sensor which will yield > 90% Strehl ratio and enable 106–107 contrast at small angular separations allowing us to image gas giant planets at solar system scales. Upcoming instruments like VAMPIRES, FIRST, and CHARIS will expand SCExAO's science capabilities.


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