Acta Optica Sinica, Volume. 22, Issue 7, 829(2002)
Noise Bias Compensation in the Iterative Shift-and-Add Method for Astronomical Image Reconstruction
[1] [1] Labeyrie A.Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Asrton. Astrophys., 1970, 6(1):85~87
[2] [2] Knox K T, Thompson B J. Recovery of images from atmospherically degraded short-exposure photographs. Astron. J., 1974, 193(1):L45~L48
[3] [3] Lohmann A W, Weigelt G, Wirnitzer B. Speckle masking in astronomy: Trible correlation theory and applications. Appl. Opt., 1983, 22(24):4028~4037
[4] [4] Liu Zhong, Qiu Yaohui, Lu Ruwei. Reconstruction of video images through turbulent atmosphere. Proc. SPIE, 1998, 3561:326~331
[6] [6] Bates R H T, Cady F M. Towards true imaging by wideband speckle interferometry. Opt. Commun., 1980, 32(3):365~369
[7] [7] Ribak E. Astronomical images by filtered weighted-shift-and-add technique. J. Opt. Soc. Am. (A), 1986, 3(12);2069~2076
[10] [10] Korff D. Analysis of a method for obtaining near-diffraction-limited information in the presence of atmospheric turbulence. J. Opt. Soc. Am., 1973,63(8):971~980
Get Citation
Copy Citation Text
[in Chinese], [in Chinese], [in Chinese], [in Chinese]. Noise Bias Compensation in the Iterative Shift-and-Add Method for Astronomical Image Reconstruction[J]. Acta Optica Sinica, 2002, 22(7): 829