Share Email Print

Proceedings Paper

Status of the ARGOS ground layer adaptive optics system
Author(s): Wolfgang Gässler; Sebastian Rabien; Simone Esposito; Michael Lloyd-Hart; Lothar Barl; Udo Beckmann; Thomas Bluemchen; Marco Bonaglia; José Luis Borelli; Guido Brusa; Joar Brynnel; Peter Buschkamp; Lorenzo Busoni; Luca Carbonaro; Claus Connot; Richard Davies; Matthias Deysenroth; Olivier Durney; Richard Green; Hans Gemperlein; Victor Gasho; Marcus Haug; Pete Hubbard; Sebastian Ihle; Martin Kulas; Reinhard Lederer; Jason Lewis; Christina Loose; Michael Lehmitz; Jamison Noenickx; Edmund Nussbaum; Gilles Orban de Xivry; Diethard Peter; Andreas Quirrenbach; Matt Rademacher; Walfried Raab; Jesper Storm; Christian Schwab; Vidhya Vaitheeswaran; Julian Ziegleder
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

ARGOS the Advanced Rayleigh guided Ground layer adaptive Optics System for the LBT (Large Binocular Telescope) is built by a German-Italian-American consortium. It will be a seeing reducer correcting the turbulence in the lower atmosphere over a field of 2' radius. In such way we expect to improve the spatial resolution over the seeing of about a factor of two and more and to increase the throughput for spectroscopy accordingly. In its initial implementation, ARGOS will feed the two near-infrared spectrograph and imager - LUCI I and LUCI II. The system consist of six Rayleigh lasers - three per eye of the LBT. The lasers are launched from the back of the adaptive secondary mirror of the LBT. ARGOS has one wavefront sensor unit per primary mirror of the LBT, each of the units with three Shack-Hartmann sensors, which are imaged on one detector. In 2010 and 2011, we already mounted parts of the instrument at the telescope to provide an environment for the main sub-systems. The commissioning of the instrument will start in 2012 in a staged approach. We will give an overview of ARGOS and its goals and report about the status and new challenges we encountered during the building phase. Finally we will give an outlook of the upcoming work, how we will operate it and further possibilities the system enables by design.

Paper Details

Date Published: 13 September 2012
PDF: 10 pages
Proc. SPIE 8447, Adaptive Optics Systems III, 844702 (13 September 2012); doi: 10.1117/12.926167
Show Author Affiliations
Wolfgang Gässler, Max-Planck-Institut für Astronomie (Germany)
Sebastian Rabien, Max-Planck-Institut für extraterrestrische Physik (Germany)
Simone Esposito, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Michael Lloyd-Hart, The Univ. of Arizona (United States)
Lothar Barl, Max-Planck-Institut für extraterrestrische Physik (Germany)
Udo Beckmann, Max-Planck-Institut für Radioastronomie (Germany)
Thomas Bluemchen, Max-Planck-Institut für Astronomie (Germany)
Marco Bonaglia, INAF - Osservatorio Astrofisico di Arcetri (Italy)
José Luis Borelli, Max-Planck-Institut für Astronomie (Germany)
Guido Brusa, Large Binocular Telescope Observatory (United States)
Joar Brynnel, Large Binocular Telescope Observatory (United States)
Peter Buschkamp, Max-Planck-Institut für extraterrestrische Physik (Germany)
Lorenzo Busoni, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Luca Carbonaro, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Claus Connot, Max-Planck-Institut für Radioastronomie (Germany)
Richard Davies, Max-Planck-Institut für Radioastronomie (Germany)
Matthias Deysenroth, Max-Planck-Institut für Radioastronomie (Germany)
Olivier Durney, The Univ. of Arizona (United States)
Richard Green, Large Binocular Telescope Observatory (United States)
Hans Gemperlein, Max-Planck-Institut für extraterrestrische Physik (Germany)
Victor Gasho, The Univ. of Arizona (United States)
Marcus Haug, Max-Planck-Institut für extraterrestrische Physik (Germany)
Pete Hubbard, The Univ. of Arizona (United States)
Sebastian Ihle, PNSensor GmbH (Germany)
Martin Kulas, Max-Planck-Institut für Astronomie (Germany)
Reinhard Lederer, Max-Planck-Institut für extraterrestrische Physik (Germany)
Jason Lewis, The Univ. of Arizona (United States)
Christina Loose, Max-Planck-Institut für extraterrestrische Physik (Germany)
Michael Lehmitz, Max-Planck-Institut für Astronomie (Germany)
Jamison Noenickx, The Univ. of Arizona (United States)
Edmund Nussbaum, Max-Planck-Institut für Radioastronomie (Germany)
Gilles Orban de Xivry, Max-Planck-Institut für extraterrestrische Physik (Germany)
Diethard Peter, Max-Planck-Institut für Astronomie (Germany)
Andreas Quirrenbach, Landessternwarte Heidelberg (Germany)
Matt Rademacher, The Univ. of Arizona (United States)
Walfried Raab, Max-Planck-Institut für extraterrestrische Physik (Germany)
Jesper Storm, Leibniz-Institut für Astrophysik Potsdam (Germany)
Christian Schwab, Landessternwarte Heidelberg (Germany)
Vidhya Vaitheeswaran, The Univ. of Arizona (United States)
Julian Ziegleder, Max-Planck-Institut für extraterrestrische Physik (Germany)

Published in SPIE Proceedings Vol. 8447:
Adaptive Optics Systems III
Brent L. Ellerbroek; Enrico Marchetti; Jean-Pierre Véran, Editor(s)

© SPIE. Terms of Use
Back to Top