Measurement of X-ray photon energy and arrival time using a silicon drift detector

[1]
Voges W, Aschenbach B, Boner T et al. ROSAT All-sky Survey Faint Source Catalogue. International Astronomical Union Circular, 2000, 7432[2] Sheikh S I, Pines J D. Journal of Guidance, Control, and Dynamics, 2006, 19: 49-63[3] Emadzadeh A A, Speye J L, Hadaegh F Y. A Parametric Study of Relative Navigation using Pulsars. Proceedings of ION 63rd Annual Meeting Cambridge, USA. 2007[4] Graven P H, Collins J T, Suneel I S et al. Spacecraft Aviation Using X-Ray Pulsars. 7th International ESA Conference on Guidance, Navigation Control Systems. County Kerry, Ireland, 2008[5] Wood K S, Determan J R, Ray P S et al. Using the Unconventional Stellar Aspect (USA) Experiment on ARGOS to Determine Atmospheric Parameters by X-ray Occultation. Proceedings of SPIE-The International Society for Optical Engineering. USA: SPIE, 2002[6] HU Hui-Jun, ZHAO Bao-Sheng. Acta Phys. Sin., 2012, 61(1): 1-7[7] ZHANG Fei, WANG Huan-Yu, PENG Wen-Xi et al. CPC (HEP NP), 2012, 36(2): 146-150[8] Lechner P, Eckbauer S, Hartmann R et al. Nuclear Instruments and Methods in Physics Research, 1996, 377: 346-351[9] Nouais D, Beole S, Bondila M et al. Nuclear Instruments and Methods in Physics Research, 2003, 501: 119-125[10] ZHENG Wei, SUN Shou-Ming. China Patent, ZL201010022035.7 2012 (in Chinese)