Artigo Acesso aberto

TMT adaptive optics program status report

2012; SPIE; Volume: 8447; Linguagem: Inglês

10.1117/12.927046

ISSN

1996-756X

Autores

Brent L. Ellerbroek, Sean M. Adkins, David R. Andersen, Jenny Atwood, Arnaud Bastard, Yong Bo, Marc-André Boucher, Corinne Boyer, Peter Byrnes, Kris Caputa, Shanqiu Chen, Carlos Correia, Raphaël Cousty, Joeleff Fitzsimmons, Luc Gilles, James A. Gregory, Glen Herriot, Paul Hickson, Alexis Hill, John Pazder, Hubert Pagès, Thomas Pfrommer, В. А. Решетов, Scott Roberts, Jean-Christophe Sinquin, Matthias Schoeck, Malcolm J. Smith, Jean‐Pierre Véran, Lianqi Wang, Kai Wei, Ivan Wevers,

Tópico(s)

Astronomy and Astrophysical Research

Resumo

We provide an update on the development of the first light adaptive optics systems for the Thirty Meter Telescope (TMT) over the past two years. The first light AO facility for TMT consists of the Narrow Field Infra-Red AO System (NFIRAOS) and the associated Laser Guide Star Facility (LGSF). This order 60 × 60 laser guide star (LGS) multi-conjugate AO (MCAO) architecture will provide uniform, diffraction-limited performance in the J, H, and K bands over 17-30 arc sec diameter fields with 50 per cent sky coverage at the galactic pole, as is required to support TMT science cases. Both NFIRAOS and the LGSF have successfully completed design reviews during the last twelve months. We also report on recent progress in AO component prototyping, control algorithm development, and system performance analysis.

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