Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientist
Physics
High Energy Physics
High Energy Physics - Phenomenology
Scientist
Amsterdam
PKU
University of Illinois
GEPI, Observatoire de Paris
UMD, LHEA / GSFC
California Institute of Technology, Pasadena, California, USA
GEPI Observatoire de Paris Meudon
National Astronomical Observatories, Chinese Academy of Sciences;
Simon Fraser University
Laboratoire GEPI, Observatoire de Paris
UMCP, NASA / GSFC
Huazhong Normal University, Wuhan, P. R. China
University of Maryland
Univ. of Illinois
Institute of Space Science, National Central University, Jhongli, 320 Taiwan; Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA of Physics, Michigan Technological University, Houghton, MI 49931, USA Observatory, Kunming, People's Republic of China
Plasma and Space Science Center, National Cheng Kung University, Tainan, Taiwan; Central University, Chung-Li, Taiwan; of Space Science, National Central University, Jhongli, Taiwan; Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China
National Astronomical Observatoires / Yunnan Observatory, Chinese Academy of Sciences, Kunming, Yunnan, China United Laboratory of Optical Astronomy, Chinese Academy of Sciences, China
ASIAA, Taiwan
Astronomy Department, University of Maryland
Center for Imaging the Earth's Interior, Department of Physics, University of Colorado at Boulder, Boulder, CO 80309-03901, USA & GSFC
University of Maryland.
National Cheng Kung University, Plasma and Space Science Center, Tainan, 70101, Taiwan
Plasma and Space Science Center, Nation Cheng Kung University, No.1, University Road, Tainan, 70101, Taiwan
Yunnan Observatory, Chinese Academy of Sciences, Kunming, Yunnan Province, PR China; United Laboratory of Optical Astronomy, Chinese Academy of Sciences, PR China; Na
A "super" star cluster grown old: the most massive star cluster in the Local Group
A 3-D shear velocity model of the crust and uppermost mantle beneath the United States from ambient seismic noise
A forming disk at z~0.6: Collapse of a gaseous disk or major merger remnant?
A method to subtract the skylight for the multi-fiber instrument E-ELT/OPTIMOS-EVE
A Multiband Study of the Galaxy Populations of the First Four Sunyaev--Zeldovich Effect selected Galaxy Clusters
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