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A Status Report on the Thirty Meter Telescope Adaptive Optics Program

机译:三十米望远镜自适应光学程序的状态报告

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We provide an update on the recent development of the adaptive optics (AO) systems for the Thirty Meter Telescope (TMT) since mid-2011. 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 arcsec diameter fields with 50 per cent sky coverage at the galactic pole, as is required to support TMT science cases. The NFIRAOS and LGSF subsystems completed successful preliminary and conceptual design reviews, respectively, in the latter part of 2011. We also report on progress in AO component prototyping, control algorithm development, and system performance analysis, and conclude with an outline of some possible future AO systems for TMT.
机译:自2011年年中以来,我们提供了有关三十米望远镜(TMT)的自适应光学(AO)系统最新开发的最新信息。用于TMT的第一个轻型AO设施包括窄场红外AO系统(NFIRAOS)和相关的激光制导星空设施(LGSF)。这种60×60阶的激光导星(LGS)多共轭AO(MCAO)架构将在17、30 arcsec直径场的J,H和K波段提供均匀的,衍射受限的性能,并且在该区域的天空覆盖率为50%银河极,这是支持TMT科学案例所需的。 NFIRAOS和LGSF子系统分别在2011年下半年完成了成功的初步和概念设计审查。我们还报告了AO组件原型,控制算法开发和系统性能分析方面的进展,并总结了一些可能的未来用于TMT的AO系统。

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