Faculty
Name: Gu Minfeng
Position: Professor
Phone: 021-34775314
E-mail: gumf@shao.ac.cn
Postal Code: 200030
Mailing Address: 80 Nandan Road, Shanghai

Resume:

   Gu Minfengwas born in Jiangsu province, PRC, 1974. In 1995, he received his BS degree in the Department of Astronomy, Nanjing University. Then, he joined Shanghai Astronomical Observatory (SHAO), CAS.  After obtaining a Ph.D. degree in 2002 from SHAO, he worked inKorea Astronomy and Space Science Institute as a postdoctoral fellow (2002-2003).In 2010, he visited University of California, Santa Barbara as a visiting scholar (2010 – 2011). Since 2011, he became a research professor in SHAO.His current research interest is active galactic nuclei, and he has published over 40 SCI papers.   

  Selected publications: 

  1Gu, MinfengThe evolution of the dusty torus covering factor in quasarsAstrophysical Journal, 2013, 773, 176 

  2Gu, M. F.; Li, S. -L.The ultraviolet/optical variability of steep-spectrum radio quasars: the change in accretion rate?Astronomy & Astrophysics, 2013, 554, A51 

  3Gu, Minfeng; Chen, YongjunThe compact radio structure of radio-loud narrow line Seyfert 1 galaxiesAstronomical Journal, 2010, 139, 2612 

  4Gu, Minfeng; Cao, XinwuThe anti-correlation between the hard X-ray photon index and the Eddington ratio in low-luminosity active galactic nucleiMonthly Notices of the Royal Astronomical Society, 2009, 399, 349-356 

  5Gu, Minfeng; Cao, Xinwu; Jiang, D. R.The bulk kinetic power of radio jets in active galactic nucleiMonthly Notices of the Royal Astronomical Society, 2009, 396, 984 

  6Wu, Qingwen; Gu, MinfengThe X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sourcesAstrophysical Journal, 2008, 682, 212 

  7Gu, M.F.; Lee, C.U.; Pak, S.; Yim, H.S.; Fletcher, A.B.Multi-colour optical monitoring of eight red blazarsAstronomy & Astrophysics, 2006, 450, 39 

  8Gu, M.F.; Cao, X.W.; Jiang, D.R.On the masses of black holes in radio-loud quasarsMonthly Notices of the Royal Astronomical Society, 2001, 327, 1111