[1] SHEIKH I S. The use of variable celestial X-ray sources for spacecraft navigation［D］. Maryland: University of Maryland, 2005.

[2] ZACHARY T, ROUMMEL F, REBECCA M. This is SPIRAL-TAP: sparse poisson intensity reconstruction algorithms-theory and practice［J］. IEEE Transactions on Image Processing, 2012, 21(36): 1084-1096.

[3] CHARLES C, RASSON J. Wavelet denoising of Poisson-distributed data and applications［J］. Computational Statistics & Data Analysis, 2003(43): 139-148.

[4] ANSCOMBE F. The transformation of Poisson, binomial and negative binomial data［J］. Biometrika, 1948, 35: 246-254.

[5] FISZ M. The limiting distribution of a function of two independent variables and its statistical application［J］. Colloquium Mathematicum, 1955, 3: 138-146.

[6] 高国荣,刘艳萍,潘琼. 基于小波域可导阈值函数与自适应阈值的脉冲星信号消噪［J］. 物理学报, 2012, 61(13): 139701.

    GAO Guo-Rong, LIU Yan-Ping, PAN Qiong. A differentiable thresholding function and an adaptive threshold selection technique for pulsar signal denoising［J］. Acta Physics Sinica, 2012, 61(13): 139701.

[7] KOLACZYK E. Bayesian multi-scale models for poisson processes［J］. Journal of the American Statistical Association, 1999, 94(447): 920-933.

[8] PIOTR F, NASON G. A wavelet-Fisz algorithm for Poisson intensity estimation［J］. Journal of Computational and Graphical Statistics, 2003, 13(3): 621-638.

[9] PIOTR F. Haar-Fisz methodology for interpretable estimation of large, sparse, time-varying volatility matrices［C］. Hernando: Universite Catholique de Louvain, 2011.

[10] 苏哲,许录平,王婷. X射线脉冲星导航半物理仿真实验系统研究［J］. 物理学报, 2011, 60(11): 119701.

    SU Zhe, XU Lu-ping, WANG Ting. X-ray pulsar-based navigation semi-physical simulation experiment system［J］. Acta Physics Sinica, 2011, 60(11): 119701.

[11] 盛立志, 赵宝升, 周峰, 等. X射线脉冲星导航探测器性能研究［J］. 光子学报, 2013, 42(9): 1071-1076.

    SHENG Li-zhi, ZHAO Bao-sheng, ZHOU Feng, et al. Performance of the detection system for X-ray pulsar based navigation［J］. Acta Photonica Sinica, 2013, 42(9): 1071-1076.

[12] SHEIKH I, GOLSHAN A, PINES D. Absolute and relative position determination using variable celestial X-ray sources［C］. Advances in the Astronautical Sciences, 2007, 128: 855-874.

[13] MARKKU M, ALESSANDRO F. Optimal inversion of the generalized anscombe transformation for poisson-gaussian noise［J］. IEEE Transactions on Image Processing, 2013, 22(1): 91-103.

[14] DONOHO D, JOHSTONE I. Ideal spatial adaption by wavelet shrinkage［J］. Biometrika, 1994, 81: 425-455.

[15] NASON G. Wavelet shrinkage using cross-validation［J］. Journal of the Royal Statistical Society B, 1996, 58: 463-479.

[16] BARANIUK R. Optimal tree approximation with wavelets［C］. SPIE, 1999, 3813: 206-214.