Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events

Keyphrases

• Astrophysical Neutrinos 50%
• Astrophysical Sources 50%
• Cherenkov Telescope Array 100%
• Detection Probability 100%
• Field Configuration 50%
• Gamma Rays 100%
• Geomagnetic Field 100%
• IceCube 50%
• Neutrino Flux 50%
• Neutrino Targets 50%
• Neutrinos 100%
• Night Sky Background 50%
• Target of Opportunity 50%
• TeV gamma Rays 50%
• Zenith Angle 50%

Physics

• Gamma Radiation 100%
• Geomagnetism 100%
• Night Sky Brightness 50%