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Department of Electrical Engineering, University of Texas at Dallas
Yunnan Astrophysics Center, Yunnan University, Kunming 650091, China
Yunnan Observatory, National Astronomical Observatoires, Chinese Academy of Sciences, PO Box 110, Kunming 650011 China; United Laboratory of Optical Astronomy, Chinese Academy of Sciences; Yunnan Astrophysics Center, Yunnan University, Kunming 650091, China
National Astronomical Observatoires, Yunnan Observatory, Chinese Academy of Sciences, Kunming, Yunnan 650011, China; Yunnan Astrophysics Centre, Yunnan University, Kunming 650092, Chin; send offprint requests to
Yunnan Astrophysics Center, Yunnan University, Kunming, China.
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing, China; United Laboratory of Optical Astronomy, Chinese Academy of Sciences, Beijing, China; Yunnan Astrophysics Center, Yunnan University, Kunming 650091, China.
Physics Department, Yunnan University, Kunming 650091, China
National Astronomical Observatoires / Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, Chin; Graduate School of the Chinese Academy of Sciences, Beijing, China; Department of Physics, Yunnan University, Kunming 650091, China. Observatory, National Astronomical Observatoires, Chinese Academy of Sciences, Kunming 650011, China; Yunnan Astrophysics Center, Yunnan University, Kunming 650091, China.
Yunnan Observatory, National Astronomical Observatoires, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, Chin; Yunnan Astrophysics Center, Department of Physics, Yunnan University, 650091 Kunming, China; Graduate School of the Chinese Academy of Sciences.
CCD photometric studies of rapid variability in eight blazars
CCD photometry of five X-ray selected BL Lacertae objects
Correlation between Eddington Ratios and Broad-Line Luminosities in Flat-Spectrum Radio Quasars, BL Lacertae Objects, and Radio Galaxies
Masses, Dimensionless Kerr Parameters, and Emission Regions in GeV Gamma-Ray-loud Blazars
Periodicity Analysis of the Radio Curve of PKS 1510-089 and Implications for its Central Structure
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