Fangjun Lu，male, born in 1969. Ph.D. in 1996 from IHEP. Worked at Max-Planck-Institute for Extraterrestrische Physik as a visiting scholar from 1998 to 1999 and at the University of Massachusetts as a senior research associate from 2001 to 2002. Research staff of IHEP since 2002 . Areas of Research: High Energy Astrophysics Achievement and Experience:
Works on observational high energy astrophysics, including image reconstruction, X-ray emission properties of supernova remnants, and the X-ray emission of pulsars and pulsar wind nebulae. Discovered the “Bulls-eye” pulsar and the fine structure of its X-ray nebula, found strong observational evidence to support the single degenerate origin of the Tycho’s supernova remnant, and gave results which were released as important discoveries by NASA and/or its Chandra Science Center. The deputy general designer of the Hard X-ray Modulation Telescope, China’s first astronomical satellite. Leads the development of all the payloads, which will enter the flight model phase in a few months.