Understand
The Advanced Gamma-ray Imaging System (AGIS) is a next-generation ground-based gamma-ray observatory being planned in the U.S.
- The anticipated sensitivity of AGIS is about one order of magnitude better than the sensitivity of current observatories, allowing it to measure gammaray emmission from a large number of Galactic and extra-galactic sources.
- We present here results of simulation studies of various possible designs for AGIS.
- The primary characteristics of the array performance - collecting area, angular resolution, background rejection, and sensitivity - are discussed.
Built on
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Hofmann, W. 2006, Proc. Cherenkov 2005 Workshop (Palaiseau); arXiv:astro-ph/0603076
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Maier, G. et al (VERITAS collaboration) 2007, Proc. 30th ICRC (Merida); arXiv:0709.4195
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Similar
Vassiliev, V., Fegan, S. & Brousseau 2007, Astroparticle Physics 28, 10
2007
Cited alongside, same era.
Vassiliev, V. & Fegan, S. 2007, Proc. 30th ICRC (Merida); arXiv:0708.2741
2007
Cited alongside, same era.
Acciari, V. et al (VERITAS collaboration) 2008, ApJ 679, 1427
2008
Cited alongside, same era.
Then
Bernlöhr, K. 2008, Astroparticle Physics 30, 149
2008
Later among the works it cites.
Holder, J. et al (VERITAS collaboration) 2008, AIPC, 1085, 657; arXiv:astro-ph/0810.0474
2008
Later among the works it cites.
Funk, S. & Hinton, J. 2009, arXiv:astro-ph/0901.2153
2009
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