Computer Science – Networking and Internet Architecture
Scientist
Computer Science
Networking and Internet Architecture
Scientist
CUHK
CfA
University of Utah
The Tibet AS gamma Collaboration
The Tibet ASgamma Collaboration
CFA
School of Earth and Space Sciences, Peking University, Peking University, Beijing, 100871 China of Plasma Physics, CAS, PO Box 1126, Hefei, Anh 230031 China
National Astronomical Observatoires, CAS;, Graduate University of the CAS
Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA
Key Laboratory of Particle Astrophysics, Inst. of High Energy Physics, Chinese Acad. of Sciences, Beijing 100049, China
University of California, Davis
Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan
National Astronomic Observatoires, Chinese Academy of Sciences, Beijing 100012, China; and Graduate School, Chinese Academy of Sciences, Beijing 100049, China
Center for Astrophysics, Harvard University
Harvard-Smithsonian Center for Astrophysics
Polytechnic University, Farmingdale, NY, US
Harvard / CfA
Weber Research Inst., Polytechnic Univ., Farmingdale, NY, US
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan
SAO
Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan
Key Laboratory of Solar Activities, National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China; LESIA, UMR CNRS 8109, Observatoire de Paris, Meudon 92195, France of Earth Science, China University of Geosciences, Lumo Rd, Wuhan 430074, China
The Isermann Department of Chemical Engineering, Rensselaer Polytechnic Institute, Troy, New York 12180
Smithsonian Astrophysical Observatory
Institute of Plasma Physics, CAS, Hefei Anhui, 230031 China
Faculty of Earth Sciences, China University of Geosciences, Wuhan, China Key Laboratory of Basic Plasma Physics, School of Science, University of Science and
86 Herschel sources SED model parameters (Rowan-Robinson+, 2010)
A 1.1mm AzTEC Survey Tracing Accelerated Galaxy Formation Towards a Protocluster at z 3.8
A 32-GHz Microstrip Array Antenna for Microspacecraft Application
A 32-GHz Phased Array Transmit Feed for Spacecraft Telecommunications
A generation mechanism for the downshifted peak in stimulated electromagnetic emission spectrum
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