Calar Alto ALFA and the sodium laser guide star in astronomy

Author(s):  
David J. Butler ◽  
Richard I. Davies ◽  
Hayden Fews ◽  
Wolfgang K. P. Hackenberg ◽  
Sebastian Rabien ◽  
...  
2001 ◽  
Vol 205 ◽  
pp. 453-454
Author(s):  
T. Ott ◽  
R. Davies ◽  
S. Rabien

All 8-metre class telescopes will be equipped with adaptive optics systems in order to reach their highest angular resolutions. With the additional requirement for maximal sky coverage comes the mandatory use of a laser guide star. ALFA is an adaptive optics system using a sodium laser guide star, which is installed on the 3.5-m telescope at Calar Alto observatory. It has shown that it is possible to reach Strehl ratios better than 20% in the K-band. In this contribution we describe the design of the system, the observational trade-off necessary to use a laser guide star, and the performance that might be expected.


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

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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