scholarly journals Photon return on-sky test for “by-product” Rayleigh plume of sodium laser guide star

2021 ◽  
pp. 127515
Author(s):  
Jian Huang ◽  
Lu Feng ◽  
Kai Jin ◽  
Min Li ◽  
Gongchang Wang
2003 ◽  
Vol 20 (10) ◽  
pp. 2093 ◽  
Author(s):  
Jean-Paul Pique ◽  
Sébastien Farinotti

2010 ◽  
Vol 511 ◽  
pp. A31 ◽  
Author(s):  
N. Moussaoui ◽  
B. R. Clemesha ◽  
R. Holzlöhner ◽  
D. M. Simonich ◽  
D. Bonaccini Calia ◽  
...  

1989 ◽  
Author(s):  
Chester S. Gardner ◽  
Byron M. Welsh ◽  
Laird A. Thompson

1999 ◽  
Author(s):  
David J. Butler ◽  
Richard I. Davies ◽  
Hayden Fews ◽  
Wolfgang K. P. Hackenberg ◽  
Sebastian Rabien ◽  
...  

2015 ◽  
Author(s):  
Feng Wang ◽  
Wei Zhang ◽  
Tianjiang Chen ◽  
Wenchao Zhou ◽  
Hong Yan

2014 ◽  
Vol 3 (3) ◽  
Author(s):  
Domenico Bonaccini Calia ◽  
Wolfgang Hackenberg ◽  
Ronald Holzlöhner ◽  
Steffan Lewis ◽  
Thomas Pfrommer

AbstractGround-based optical telescopes, in particular large ones, require adaptive optics to overcome the atmospheric seeing limit due to turbulence. Correcting the distorted wavefront necessitates bright stars in the field of view. The sky coverage can be greatly increased by using artificial sodium laser guide stars in addition to natural guide stars. We describe the underlying physics and technical considerations relevant to such systems before discussing the design of the four-laser guide star facility (4LGSF) which is currently under development for the ESO Very Large Telescope (VLT) on Cerro Paranal, Chile. The focus is upon the justification of the requirements and their technical solution.


1997 ◽  
Author(s):  
Andreas Quirrenbach ◽  
Wolfgang K. P. Hackenberg ◽  
Hans-Christoph Holstenberg ◽  
Norbert Wilnhammer

2015 ◽  
Author(s):  
Lu Feng ◽  
Edward Kibblewhite ◽  
Kai Jin ◽  
Suijian Xue ◽  
Zhixia Shen ◽  
...  

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