Sensitivity of the Cherenkov Telescope Array to the gamma-ray emission from neutrino sources detected by IceCube

the CTA Consortium and FIRESONG Team

פרסום מחקרי: פרסום בכתב עתמאמר מכנסביקורת עמיתים

תקציר

Gamma-ray observations of the astrophysical neutrino sources are fundamentally important for understanding the underlying neutrino production mechanism. We investigate the Cherenkov Telescope Array (CTA) ability to detect the very-high-energy (VHE) gamma-ray counterparts to the neutrino-emitting Active Galaxies. The CTA performance under different configurations and array layouts is computed based on the neutrino and gamma-ray simulations of steady and transient types of sources, assuming that the neutrino events are detected with the IceCube neutrino telescope. The CTA detection probability is calculated for both CTA sites taking into account the visibility constraints. We find that, under optimal observing conditions, CTA could observe the VHE gamma-ray emission from at least 3 neutrino events per year.

שפה מקוריתאנגלית
מספר המאמר1531
כתב עתProceedings of Science
כרך444
סטטוס פרסוםפורסם - 27 ספט׳ 2024
אירוע38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, יפן
משך הזמן: 26 יולי 20233 אוג׳ 2023

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