Future Hard X-ray Missions to study non-thermal universe

Details Future Hard X-ray Missions to study non-thermal universe Future Hard X-ray Missions to study non-thermal universe

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..199t&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

1

X-Ray Sources, X-Ray Bursts, Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation, Gamma-Ray, X-Ray

Scientific paper

The hard X-ray and γ-ray bands are important frequency windows for exploring the energetic universe. It is in these energy bands that the non-thermal emission becomes dominant. In order to study the ``non-thermal universe'', characterized by accelerated high energy particles, we need an advanced mission which has orders of magnitude better sensitivity than any previous or current mission.

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