中国科学院南京天文光学技术研究所机构知识库(NIAOT OpenIR): Home

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A VIPA spectrograph with ultra-high spectral res.. [期刊论文,2025-12]
Calibration approach of non-modulated pyramid wa.. [期刊论文,2025-12]
Automated High-Precision Recognition of Solar Fi.. [期刊论文,2025-12]
Cooling air flow field in the primary mirror tem.. [期刊论文,2025-12]
Low-loss and broadband arbitrary ratios 1 × 2 p.. [期刊论文,2025-12]
Current sensor unanticipated fault detection and.. [期刊论文,2025-12]
Satellite impact on astronomical observations ba.. [期刊论文,2025-12]
Efficient full-aperture mirror polishing method .. [期刊论文,2025-12]
Artificial Intelligence in Astronomical Optical .. [期刊论文,2025-12]
Fuzzy Proportional Integral Derivative control o.. [期刊论文,2025-12]

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1. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope.. [WOS:1547]

2. Active Optics in LAMOST [WOS:134]

3. Enabling low amounts of YAG：Ce3+ to convert blue into white .. [WOS:31]

4. A Coronagraph Based on Stepped-Transmission Filters [WOS:23]

5. A Transmission-Filter Coronagraph: Design and Test [WOS:19]

6. Calculations for the Pre-Calibration of LAMOST Active Optics [WOS:16]

7. Simulation and fabrication of the atmospheric turbulence phas.. [WOS:15]

8. SPECKLE NOISE SUBTRACTION AND SUPPRESSION WITH ADAPTIVE OPTIC.. [WOS:14]

9. Atmospheric dispersion corrector for the Large Sky Area Multi.. [WOS:13]

10. Stochastic parallel gradient descent based adaptive optics us.. [WOS:13]

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