Yi-Zhong Fan mostly deals with Astrophysics, Gamma-ray burst, Astronomy, Afterglow and Light curve. His study in Astrophysics focuses on Neutron star, Kilonova, LIGO, Gravitational wave and Magnetar. His Gamma-ray burst research incorporates elements of Spectral line, GRB 080916C, Flare and Supernova.
His Astronomy study frequently draws connections to other fields, such as Gamma ray. His Afterglow research integrates issues from Light emission, Synchrotron, GRB 050709 and Kinetic energy. As a part of the same scientific study, Yi-Zhong Fan usually deals with the Light curve, concentrating on Astrophysical jet and frequently concerns with X-ray telescope, Swift Gamma-Ray Burst Mission and Telescope.
Yi-Zhong Fan mainly investigates Astrophysics, Gamma-ray burst, Astronomy, Afterglow and Neutron star. His study in Gamma ray, Light curve, Gravitational wave, Fermi Gamma-ray Space Telescope and Galaxy is carried out as part of his studies in Astrophysics. The various areas that Yi-Zhong Fan examines in his Gamma-ray burst study include Redshift, Telescope, Radius, Photon and Kilonova.
His work carried out in the field of Photon brings together such families of science as GRB 080916C, Synchrotron and Synchrotron radiation. His work in Afterglow covers topics such as Lorentz factor which are related to areas like Outflow. His work focuses on many connections between Neutron star and other disciplines, such as Equation of state, that overlap with his field of interest in Lambda.
His scientific interests lie mostly in Astrophysics, Neutron star, Dark matter, Gamma ray and Gravitational wave. In his study, Photon is strongly linked to Spectral line, which falls under the umbrella field of Astrophysics. Yi-Zhong Fan interconnects LIGO, Radius, Equation of state, Gravitation and Black hole in the investigation of issues within Neutron star.
His Dark matter research includes themes of Milky Way, Electron, Cosmic ray and Annihilation. His Gamma ray research includes elements of Scintillator, Detector, Supernova, Flare and Light curve. His research in Gamma-ray burst is mostly concerned with Afterglow.
The scientist’s investigation covers issues in Astrophysics, Neutron star, Dark matter, Cosmic ray and Gamma ray. His studies in Gamma-ray burst, Supernova, Fermi Gamma-ray Space Telescope, Galaxy and Blazar are all subfields of Astrophysics research. His study in Gamma-ray burst focuses on Afterglow in particular.
His study in Neutron star is interdisciplinary in nature, drawing from both Gravitational wave, LIGO, Radius and Equation of state. He combines subjects such as Physics beyond the Standard Model, Spectral line, Kinetic energy and Photon with his study of Dark matter. Cosmic ray is a primary field of his research addressed under Astronomy.
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.
Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors
J. Abadie;B. P. Abbott.
arXiv: High Energy Astrophysical Phenomena (2010)
Physical processes shaping GRB X-ray afterglow lightcurves: theoretical implications from the Swift XRT observations
Bing Zhang;Y. Z. Fan;Jaroslaw Dyks;Shiho Kobayashi.
arXiv: Astrophysics (2005)
Physical Processes Shaping Gamma-Ray Burst X-Ray Afterglow Light Curves: Theoretical Implications from the Swift X-Ray Telescope Observations
Bing Zhang;Y. Z. Fan;Y. Z. Fan;Jaroslaw Dyks;Shiho Kobayashi;Shiho Kobayashi.
The Astrophysical Journal (2006)
A gravitational wave observatory operating beyond the quantum shot-noise limit
J. Abadie;B. P. Abbott;R. Abbott;T. D. Abbott.
Nature Physics (2011)
Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
E. Pian;P. D'Avanzo;S. Benetti;M. Branchesi.
Nature (2017)
Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
G. Ambrosi;Q. An;R. Asfandiyarov.
Nature (2017)
A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. I. Spectral Components and Their Possible Physical Origins of LAT/GBM GRBs
Bin-Bin Zhang;Bing Zhang;En-Wei Liang;Yi-Zhong Fan.
arXiv: High Energy Astrophysical Phenomena (2010)
Late internal‐shock model for bright X‐ray flares in gamma‐ray burst afterglows and GRB 011121
Yi-Zhong Fan;Yi-Zhong Fan;D.M. Wei.
Monthly Notices of the Royal Astronomical Society: Letters (2005)
Localization and broadband follow-up of the gravitational-wave transient GW150914
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy.
The Astrophysical Journal (2016)
The X-ray afterglow flat segment in short GRB 051221A: Energy injection from a millisecond magnetar?
Yi-Zhong Fan;Yi-Zhong Fan;Dong Xu.
Monthly Notices of the Royal Astronomical Society: Letters (2006)
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:
University of Nevada, Las Vegas
University of Oregon
Max Planck Institute for Gravitational Physics
Max Planck Institute for Gravitational Physics
California Institute of Technology
Syracuse University
Revista de Chimie SRL
National Science Foundation
California Institute of Technology
University of Florida
Grenoble Alpes University
Xi'an Jiaotong University
McGill University
University of Siena
National Institute of Advanced Industrial Science and Technology
Peking University
University of Groningen
Imperial College London
University of California, Davis
Martin Luther University Halle-Wittenberg
University of Manchester
Cornell University
University of Milan
Emory University
Norwegian University of Life Sciences
University of Waikato