目次
Gamma-ray Astrophysics: Future and Prospects
Gamma-ray sky in 1973
Gamma-ray Sky in 1980
Gamma-ray Sky in 1996
Gamma-ray Sky in 2004?
Number of Sources vs. Time
Gamma-ray Sources in 1994
Gamma-ray Sources in 1996
Gamma-ray Sources in 1998
EGRET Source Catalog
Gamma-ray Sky above 300GeV
Technology in 1970’s - Satellite
Technology in 1980’s - Satellite
Technology in 1990’s - Satellite
Technology in 2000’s - Satellite
Comparison of Satellites
Technology in 1950’s - Ground
Technology in 1970’s - Ground
Technology in 1980’s -Imaging 1
Technology in 1980’s -Imaging 2
Imaging Technology in 1990’s
Technology in 2000’s - Stereo? 1
Technology in 2000’s - Stereo? 2
Stereo Project -1
Stereo Project -2
Stereo Project -3
Technology in 2000’s - Area?
Large Area Project -1
Large Area Project -2
Large Area Project -3
Comparison of techniques
Comparison of Telescopes
Future Sensitivities
Sensitivity -1
SNR - Where are protons?
Sensitivity -2
Crab unpulsed spectrum
Sensitivity -3
Wideband spectrum of AGN
Intergalactic absorption by IR
Spectrum cutoff for Blazars
Sensitivity -4
Energetic Universe
Non-thermal Universe
Conclusion
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