in 1999-2004, Fu-Guo Xie got his undergraduate eduation University of Science and Technology of China (USTC), and majored in astronomy. He then got his graduate eduation in Shanghai Astronomical Observatory (SHAO) of Chinese Academy of Sciences (CAS). From 2009, he worked in SHAO as a faculty member, and he is now the associated director and full professor of the astrophysics division. Moreover, from 2009 to 2011, Fu-Guo was also a post-doc in Kavli Institute for Astronomy and Astrophysics of Peking University (KIAA-PKU). 

1-- Xie*, F. G., Yuan*, F., 2012, MNRAS, 427, 1580. Radiative efficiency of hot accretion flows

2-- Yang, Q. X., Xie*, F. G., Yuan*, F. et al., 2015, MNRAS, 447, 1692. Correlation between the photon index and X-ray luminosity of black hole X-ray binaries and active galactic nuclei: observations and interpretation

3-- Xie*, F. G., Yuan*, F., Ho, L. C., 2017, ApJ, 844, 42. Radiative Heating in the Kinetic Mode of AGN Feedback.

4-- Xie*, F. G., Yuan*, F., 2016, MNRAS, 456, 4377. Interpreting the radio/X-ray correlation of black hole binaries based on the accretion-jet model

5-- Yan*, Z., Xie*, F. G., Zhang, W., 2020, ApJL, 889, L18. Coronal Properties of Black Hole X-ray Binaries in the Hard State as Seen by NuSTAR and Swift

代表性论文（英文）：

1-- Xie*, F. G., Yuan*, F., 2012, MNRAS, 427, 1580. Radiative efficiency of hot accretion flows

2-- Yang, Q. X., Xie*, F. G., Yuan*, F. et al., 2015, MNRAS, 447, 1692. Correlation between the photon index and X-ray luminosity of black hole X-ray binaries and active galactic nuclei: observations and interpretation

3-- Xie*, F. G., Yuan*, F., Ho, L. C., 2017, ApJ, 844, 42. Radiative Heating in the Kinetic Mode of AGN Feedback.

4-- Xie*, F. G., Yuan*, F., 2016, MNRAS, 456, 4377. Interpreting the radio/X-ray correlation of black hole binaries based on the accretion-jet model

5-- Yan*, Z., Xie*, F. G., Zhang, W., 2020, ApJL, 889, L18. Coronal Properties of Black Hole X-ray Binaries in the Hard State as Seen by NuSTAR and Swift