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High-energy astronomy





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High-energy astronomy is the study of astronomical objects that release electromagnetic radiation of highly energetic wavelengths. It includes X-ray astronomy, gamma-ray astronomy, extreme UV astronomy, neutrino astronomy, and studies of cosmic rays. The physical study of these phenomena is referred to as high-energy astrophysics.[1]

Astronomical objects commonly studied in this field may include black holes, neutron stars, active galactic nuclei, supernovae, kilonovae, supernova remnants, and gamma-ray bursts.

Missions

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Some space and ground-based telescopes that have studied high energy astronomy include the following:[2]

  • AMS-02
  • AUGER
  • CALET
  • Chandra
  • Fermi
  • HAWC
  • H.E.S.S.
  • IceCube
  • INTEGRAL
  • MAGIC
  • NuSTAR
  • Proton
  • Swift
  • TA
  • XMM-Newton
  • VERITAS
  • References

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    1. ^ "Steve's Gamma Ray Burst Astronomy Site". highenergyastro.homestead.com. Archived from the original on 17 August 2011. Retrieved 22 January 2018.
  • ^ "HEASARC: Observatories". heasarc.gsfc.nasa.gov. Retrieved 22 January 2018.
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  • Retrieved from "https://en.wikipedia.org/w/index.php?title=High-energy_astronomy&oldid=1232019506"
     



    Last edited on 1 July 2024, at 14:12  





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    This page was last edited on 1 July 2024, at 14:12 (UTC).

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