• Acta Optica Sinica
  • Vol. 40, Issue 14, 1411005 (2020)
Jingjing Yang1、2、3、***, Shuai Wang1、2、**, Lianghua Wen1、2、4, Ping Yang1、2, Wei Yang1、2, Chunlin Guan1、2, and Bing Xu1、2、*
Author Affiliations
  • 1Key Laboratory of Adaptive Optics, Chinese Academy of Sciences, Chengdu, Sichuan 610209, China
  • 2Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, Sichuan 610209, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China
  • 4School of Physics and Electronic Engineering, Yibin University, Yibin, Sichuan 644600, China
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    DOI: 10.3788/AOS202040.1411005 Cite this Article Set citation alerts
    Jingjing Yang, Shuai Wang, Lianghua Wen, Ping Yang, Wei Yang, Chunlin Guan, Bing Xu. Faint-Object Imaging of Diffractive Telescopes Based on Image Restoration[J]. Acta Optica Sinica, 2020, 40(14): 1411005 Copy Citation Text show less
    Flow chart of ABM3D algorithm
    Fig. 1. Flow chart of ABM3D algorithm
    Resolution board and simulated MTF curve. (a) Original image; (b) simulated MTF curve
    Fig. 2. Resolution board and simulated MTF curve. (a) Original image; (b) simulated MTF curve
    Comparison of simulation restoration results of resolution boards. (a) Raw images; (b) restored images by Awn algorithm; (c) restored images by ABM3D algorithm
    Fig. 3. Comparison of simulation restoration results of resolution boards. (a) Raw images; (b) restored images by Awn algorithm; (c) restored images by ABM3D algorithm
    Parameter results for images with and without restoration under different noise levels. (a) PSNR; (b) SSIM
    Fig. 4. Parameter results for images with and without restoration under different noise levels. (a) PSNR; (b) SSIM
    Experimental setup and light path diagram of diffractive telescope imaging system
    Fig. 5. Experimental setup and light path diagram of diffractive telescope imaging system
    MTFs of diffractive telescope imaging system
    Fig. 6. MTFs of diffractive telescope imaging system
    Comparison of experimental restoration results of resolution boards. (a) Output images; (b) restored images by Awn algorithm; (c) restored images by ABM3D algorithm
    Fig. 7. Comparison of experimental restoration results of resolution boards. (a) Output images; (b) restored images by Awn algorithm; (c) restored images by ABM3D algorithm
    Pixel traces. (a) σ=0.02; (b) σ=0.04
    Fig. 8. Pixel traces. (a) σ=0.02; (b) σ=0.04
    Jingjing Yang, Shuai Wang, Lianghua Wen, Ping Yang, Wei Yang, Chunlin Guan, Bing Xu. Faint-Object Imaging of Diffractive Telescopes Based on Image Restoration[J]. Acta Optica Sinica, 2020, 40(14): 1411005
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