Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
University of Adelaide
University of Adelaide, Australia
The University of Adelaide
Department of Physics and Mathematical Physics, University of Adelaide, Australia
U Adelaide
Department of Physics and Mathematical Physics, The University of Adelaide, Adelaide, Australia
Adelaide, University, Adelaide, Australia
Durham, University, Durham, England
Adelaide Univ., Australia.
Department of Physics and Mathematical Physics, University of Adelaide, SA 5005, Australia
Adelaide, University, Australia
National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.
Department of Phys. & Math. Phys., Adelaide Univ., SA, Australia
University of Adelaide, S.A., Australia
NASA, Goddard Space Flight Center, Laboratory for High Energy Astrophysics, Greenbelt, MD
Lab. for High Energy Astrophys., NASA / Goddard Space Flight Center, Greenbelt, MD, USA
Cosmo-Science Associates
Adelaide Univ., Australia
Department of Physics and Mathematical Physics, The University of Adelaide, Adelaide SA 5005, Australia
NASA, Goddard Space Flight Center, Laboratory for High Energy Astrophysics, Greenbelt; Maryland, University, College Park, MD
Maryland Univ., College Park
Department of Physics, School of Chemistry and Physics, University of Adelaide, SA 5005, Australia
NASA, Goddard Space Flight Center, Laboratory of High Energy Astrophysics, Greenbelt, Md; Durham, University, Durham, England
Department of Phys., Adelaide Univ., SA, Australia
Department of Phys., University of Adelaide, Adelaide, SA, Australia
University of Adelaide, Department of Physics & Math.Physics, Adelaide, SA 5005, Australia
NASA, Goddard Space Flight Center, Greenbelt, MD
Department of Physics and Mathematical Physics, University of Adelaide, Adelaide, South Australia 5000, Australia
Department of Physics, University of Durham, Durham, England
NASA, Go
"The Contribution of Active Galactic Nuclei to the Diffuse Gamma Ray Background"
A galactic component of the diffuse X-ray flux in the range 2-7 keV
A Hadronic Model for Gamma-Ray Loud Quasars
A lower limit of 50 microgauss for the magnetic field near the Galactic Centre
A new estimate of the extragalactic radio background and implications for ultra-high-energy gamma-ray propagation
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