Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Tsinghua U. & IHEP
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS, Beijing, PR. China
Tsinghua Univ
Department of Physics, Tsinghua University
Tsinghua U & IHEP
High Energy Astrophys. Lab., IHEP, Beijing;
Tsinghua U. & Ihep
Tsinghua U. & IHEP, Beijing
Laboratory for Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Beijing, China for Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Beijing 100039, China
Chinese Academy of Science, Beijing, PRC
High Energy Astrophysics Lab., Institute of High Energy Physics, P.O. Box 918-3, 100039, Beijing, China
High Energy Astrophysics Lab., Institute of High Energy Physics, P.O. BOX 918-3, 100039, Beijing, China
Durham, University, Durham, England
THU / IHEP
UvA
Department of Physics and Center for Astrophysics, Tsinghua University, Beijing 100084, China; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China Department and Center for Astrophysics, Tsinghua University, Beijing 100084, PR China; Laboratory for Particle Astrophysics, Institute of High Energy Physics, CAS, Beijing 100039, PR China
Department of Physics and Center for Astrophysics, Tsinghua University, Beijing 100084, China; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; Department of Engineering Physics and Center for Astrophysics, Tsinghua University, Beijing 100084, China. of Engineering Physics, Department of Physics & Center for Astrophysics, Tsinghua University, Beijing, China; Particle Astrophysics Lab., Institute of H
A Direct Restoration Method for Spectral and Image Analysis
A Golden Standard Type Ia Supernova SN 2005cf: Observations from the Ultraviolet to the Near-Infrared Wavebands
A hard X-ray telescope and its observation of the Crab pulsar
A New Method to Determine the Distances of Variable Galactic X-Ray Sources
A Possible Glitch of Gamma-Ray Pulsar Geminga?
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