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获奖名称:极端环境下天文仪器驱动系统非线性干扰补偿与潜隐故障无缝自愈技术及其应用。
获奖名称:中国小望远镜阵列CSTAR。
近日,国家天文台张彦霞研究员、赵永恒研究员和北京大学吴学兵教授基于中国郭守敬望远镜(LAMOST)和美国斯隆数字巡天(SDSS)的光谱数据,结合欧洲航天局的X射线牛顿天文望远镜(XMM-Newton)数据、广域红外巡天探测器(WISE)数据及SDSS可见光测光数据,通过交叉证认方法获取了具有不同波段信息的多个已知样本。基于此,研究人员通过机器学习方法构建了适合不同波段样本的最优分类器,为X射线牛顿...
获奖名称:LAMOST的核心创新和关键技术。
获奖名称:“大天区面积多目标光纤光谱天文望远镜”(LAMOST)工程研究集体。
The Thirty Meter Telescope is comprised of thirty five individual sub-systems which include optical systems, instruments, adaptive optics systems, controls, mechanical systems, supporting software a...
Thermal performances of the Thirty Meter Telescope (TMT) structure were evaluated by finite element thermal models. The thermal models consist of the telescope optical assembly systems, instruments,...
In a previous study we had presented a summary of the TMT Aero-Thermal modeling effort to support thermal seeing and dynamic loading estimates. In this paper a summary of the current status of Compu...
The merit function routine (MFR) is implemented in the National Research Council Canada Integrated Modeling (NRCIM) toolset and based in the MATLAB numerical computing environment. It links ANSYS fi...
The principal dynamic disturbances acting on a telescope segmented primary mirror are unsteady wind pressure (turbulence) and narrowband vibration from rotating equipment. Understanding these disturb...
Core components of systems engineering are the proper understanding of the top level system requirements, their allocation to the subsystems, and then the verification of the system built against th...
Wind buffeting of large telescopes.
We evaluate how well the performance of the Thirty Meter Telescope (TMT) can be maintained against thermally induced errors during a night of observation. We first demonstrate that using look-u...
The Normalized Point Source Sensitivity (PSSN) has previously been defined and analyzed as an On-Axis seeing-limited telescope performance metric. In this paper, we expand the scope of the PSSN...
Interaction Matrix Uncertainty in Active (and Adaptive) Optics.

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