Chinese Academy of Sciences
China
Shuang-Nan Zhang mostly deals with Astrophysics, Astronomy, Black hole, Dark energy and Cosmology. Galaxy, Luminosity, Accretion, Light curve and Quasar are among the areas of Astrophysics where the researcher is concentrating his efforts. His research in the fields of Rotating black hole overlaps with other disciplines such as Power law.
His work carried out in the field of Dark energy brings together such families of science as Gravitation, Classical mechanics and Attractor. Shuang-Nan Zhang has included themes like Singularity, Universe, Redshift and Quantum field theory in his Cosmology study. His work on Luminosity distance as part of general Redshift study is frequently connected to Interaction energy, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them.
Shuang-Nan Zhang focuses on Astrophysics, Astronomy, Gamma-ray burst, Black hole and Neutron star. His Astrophysics research focuses on Spectral line and how it relates to X-ray. His Gamma-ray burst research is multidisciplinary, relying on both Redshift, Polarization, Supernova, Gamma ray and Polar.
Shuang-Nan Zhang combines subjects such as Cosmology and Dark energy with his study of Redshift. His Neutron star research includes themes of Accretion, Magnetosphere, Magnetic field and Pulsar. His Quasar study integrates concerns from other disciplines, such as Radio galaxy and Blazar.
His main research concerns Astrophysics, Telescope, Gamma-ray burst, Detector and Satellite. His work investigates the relationship between Astrophysics and topics such as Spectral line that intersect with problems in Luminosity and Light curve. The Telescope study combines topics in areas such as Energy, Calibration and Sky.
He interconnects Gamma ray and Polar in the investigation of issues within Gamma-ray burst. The concepts of his Detector study are interwoven with issues in Pixel, X-ray telescope and Photon. Satellite is the subject of his research, which falls under Astronomy.
Shuang-Nan Zhang mainly investigates Astrophysics, Telescope, Detector, Gamma-ray burst and Sky. His studies in Neutron star, Black hole, Accretion, Pulsar and Accretion are all subfields of Astrophysics research. His study in Telescope is interdisciplinary in nature, drawing from both Orbit, Satellite, Calibration and Photon.
His work is dedicated to discovering how Photon, Field of view are connected with Astronomy, Scintillator and Omnidirectional antenna and other disciplines. Shuang-Nan Zhang does research in Astronomy, focusing on Gravitational wave specifically. Shuang-Nan Zhang works mostly in the field of Gamma-ray burst, limiting it down to topics relating to Polar and, in certain cases, Polarization and Polarimeter, as a part of the same area of interest.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Black Hole Spin in X-Ray Binaries: Observational Consequences
S. N. Zhang;S. N. Zhang;Wei Cui;Wan Chen;Wan Chen.
The Astrophysical Journal (1997)
Spectral Transitions in Cyg X-1 and Other Black Hole X-Ray Binaries
Ann A. Esin;Ramesh Narayan;Wei Cui;J. Eric Grove.
arXiv: Astrophysics (1997)
Spectral Transitions in Cygnus X-1 and Other Black Hole X-Ray Binaries
Ann A. Esin;Ramesh Narayan;Wei Cui;J. Eric Grove.
The Astrophysical Journal (1998)
Optical and Near-Infrared Observations of the Highly Reddened, Rapidly Expanding Type Ia Supernova 2006X in M100
Xiaofeng Wang;Xiaofeng Wang;Weidong Li;Alexei V. Filippenko;Kevin Krisciunas.
arXiv: Astrophysics (2007)
Temporal Properties of Cygnus X-1 during the Spectral Transitions
Wei Cui;S. N. Zhang;W. Focke;W. Focke;J. H. Swank.
The Astrophysical Journal (1997)
EVIDENCE FOR FRAME-DRAGGING AROUND SPINNING BLACK HOLES IN X-RAY BINARIES
Wei Cui;S. N. Zhang;S. N. Zhang;Wan Chen;Wan Chen.
The Astrophysical Journal (1998)
The 1996 Soft State Transition of Cygnus X-1
S.N. Zhang;S.N. Zhang;W. Cui;B.A. Harmon;W.S. Paciesas;W.S. Paciesas.
The Astrophysical Journal (1997)
Correlations between x-ray outbursts and relativistic ejections in the x-ray transient GRO J1655-40
B. A. Harmon;C. A. Wilson;S. N. Zhang;W. S. Paciesas.
Nature (1995)
Optical and Near-Infrared Observations of the Highly Reddened, Rapidly Expanding Type Ia Supernova SN 2006X in M100
Xiaofeng Wang;Xiaofeng Wang;Weidong Li;Alexei V. Filippenko;Kevin Krisciunas.
The Astrophysical Journal (2008)
The golden standard type ia supernova 2005cf: Observations from the ultraviolet to the near-infrared wavebands
X. Wang;X. Wang;W. Li;A. V. Filippenko;R. J. Foley;R. J. Foley.
The Astrophysical Journal (2009)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
Tsinghua University
Guangxi University
University of Tübingen
Institute of Space Sciences
École Normale Supérieure
Qingdao University of Science and Technology
Federal University of Toulouse Midi-Pyrénées
National Institute for Astrophysics
Chinese Academy of Sciences
Marshall Space Flight Center
University of Alberta
GlobalFoundries (Germany)
Spanish National Research Council
Hainan University
École Polytechnique Fédérale de Lausanne
Virginia Tech
University of Vermont
University of Clermont Auvergne
University of Arizona
St. Jude Children's Research Hospital
University of Dundee
Cornell University
Lamont-Doherty Earth Observatory
Washington University in St. Louis
Cardiff University
McMaster University