Reference : Status of the ARGOS project
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/213821
Status of the ARGOS project
English
Rabien, S. [Max-Planck-Institut für extraterrestrische Physik > > > >]
Barl, L. [> >]
Beckmann, U. [> >]
Bonaglia, M. [> >]
Borelli, J. L. [> >]
Brynnel, J. [> >]
Buschkamp, P. [> >]
Busoni, L. [> >]
Christou, J. [> >]
Connot, C. [> >]
Davies, R. [> >]
Deysenroth, M. [> >]
Esposito, S. [> >]
Gässler, W. [> >]
Gemperlein, H. [> >]
Hart, M. [> >]
Kulas, M. [> >]
Lefebvre, M. []
Lehmitz, M. [> >]
Mazzoni, T. [> >]
Nussbaum, E. [> >]
Orban De Xivry, Gilles mailto [Max-Planck-Institut für extraterrestrische Physik > > > >]
Peter, D. [> >]
Quirrenbach, A. [> >]
Raab, W. [> >]
Rahmer, G. [> >]
Storm, J. [> >]
Ziegleder, J. [> >]
2014
Adaptive Optics Systems IV
Proceedings of SPIE, volume 9148
No
International
SPIE Astronomical Telescopes and Instrumentation 2014
Sunday - Friday 22 - 27 June 2014
[en] ARGOS is the Laser Guide Star and Wavefront sensing facility for the Large Binocular Telescope. With first laser light on sky in 2013, the system is currently undergoing commissioning at the telescope. We present the overall status and design, as well as first results on sky. Aiming for a wide field ground layer correction, ARGOS is designed as a multi- Rayleigh beacon adaptive optics system. A total of six powerful pulsed lasers are creating the laser guide stars in constellations above each of the LBTs primary mirrors. With a range gated detection in the wavefront sensors, and the adaptive correction by the deformable secondary's, we expect ARGOS to enhance the image quality over a large range of seeing conditions. With the two wide field imaging and spectroscopic instruments LUCI1 and LUCI2 as receivers, a wide range of scientific programs will benefit from ARGOS. With an increased resolution, higher encircled energy, both imaging and MOS spectroscopy will be boosted in signal to noise by a large amount. Apart from the wide field correction ARGOS delivers in its ground layer mode, we already foresee the implementation of a hybrid Sodium with Rayleigh beacon combination for a diffraction limited AO performance.
Researchers
http://hdl.handle.net/2268/213821
10.1117/12.2055932
Copyright 2014 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.

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