Design of a Next Generation High-Energy Gamma-ray telescope

Details Design of a Next Generation High-Energy Gamma-ray telescope Design of a Next Generation High-Energy Gamma-ray telescope

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..587..848h&link_type=abstract

GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP Conference Proceedings, Volume 587, pp. 848-852 (2001).

Astronomy and Astrophysics

Astrophysics

1

X- And Gamma-Ray Telescopes And Instrumentation, Image Processing, Gamma-Ray, Spaceborne And Space Research Instruments, Apparatus, And Components

Scientific paper

The Next Generation High-Energy Gamma-ray (NGHEG) mission is a recommended priority for a new mission after GLAST. One of the science goals of the NGHEG mission, mapping our Galaxy, clouds, supernova remnants, and nearby galaxies for cosmic ray sources at arcminute resolution, places stringent requirements on the design of the track imager. We examine the design requirements of a track imager for a gamma-ray telescope capable of arc-minute imaging. .

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