[1] G. Weigelt. Modified speckle inteferometr: Speckle masking. Opt. Commun., 1977, 21(1):55～59

[2] A. W. Lohmann, G. P. Weigelt, B. Wirnitzer. Speckle masking in astronomy trible correlation theory and application. Appl. Opt., 1983, 22(24):4028～4037

[3] H. Bartelt, A. W. Lohmann, B. Wirnitzer. Phase and amplitude recovery from bispectra. Appl. Opt., 1984, 23(18):3121～3129

[4] A. Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astron. Aatrophs., 1970, 6(1):85～87

[5] D. Korff. Analysis of a method for obtaiing near diffrection limited information in presence of atmospheric turbulence. J. Opt. Soc. Am., 1973, 63(8):971～980

[7] B. Wirnizer. Bispectra analysis at low light levels and astronomical speckle masking. J. Opt. Soc. Am. (A), 1985, 2(1):14～21

[8] E. Pehlemann, K. -H. Hofmann, G. Weigelt. Photon bias compensation in trible correlation imaging and observation of R136. Astron. Astrophys., 1992, 256(2):701～714

[9] J. R. Fienup. Space imaging through the turbulent atmosphere. Proc. Soc. Photo-Opt. Instrum. Eng., 1978, 149(1):72～76

[10] S. Ebstein. Stellar speckle interferometry energy spectrum recovery by convex projection. Appl. Opt., 1987, 26(8):1530～1536

[12] Sky catalogue 2000.0 Vol.2 Double Stars. Variable Stars and Nonstellar Objects. Edited by Alan Hirshfeld and Roger W. Sinnott, New York:Press Syndicate of the University of Cambridge, 1985