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Proceedings Paper

PARSEC: the laser for the VLT
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Paper Abstract

8m class telescopes offer an extremely powerful tool for astronomical research. The light collecting power is enormous and with the combination of adaptive optics and laser guide stars astronomy will make a big step forward in knowledge in almost any field. For the creation of artificial laser-based guide stars that make use of the sodium layer in the earth atmosphere, very powerful lasers at 589nm are necessary. We introduce here the PARSEC laser that will be installed at the UT4 telescope of the VLT, in Chile. This laser will emit cw radiation at more then 10W output power and offers a scalability in power for future multi guide star systems.

Paper Details

Date Published: 4 February 2002
PDF: 11 pages
Proc. SPIE 4494, Adaptive Optics Systems and Technology II, (4 February 2002); doi: 10.1117/12.454807
Show Author Affiliations
Sebastian Rabien, Max-Planck-Institut fuer Extraterrestriche Physik (Germany)
Richard I. Davies, Max-Planck-Institut fuer Extraterrestriche Physik (Germany)
Thomas Ott, Max-Planck-Institut fuer Extraterrestriche Physik (Germany)
Stefan Hippler, Max-Planck-Institut fuer Astronomie (Germany)
Ulrich Neumann, Max-Planck-Institut fuer Astronomie (United States)


Published in SPIE Proceedings Vol. 4494:
Adaptive Optics Systems and Technology II
Robert K. Tyson; Domenico Bonaccini; Michael C. Roggemann, Editor(s)

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