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

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00568934" target="_blank" >RIV/67985815:_____/22:00568934 - isvavai.cz</a>
Alternative codes found
RIV/68378271:_____/22:00567959 RIV/61989592:15310/22:73616621
Result on the web
<a href="https://pos.sissa.it/395/975/pdf" target="_blank" >https://pos.sissa.it/395/975/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0975" target="_blank" >10.22323/1.395.0975</a>

Result language
angličtina
Original language name
Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events
Original language description
We investigate the possibility of detection of the VHE gamma-ray counterparts to the neutrino astrophysical sources within the Neutrino Target of Opportunity (NToO) program of CTA using the populations simulated by the FIRESONG software to resemble the diffuse astrophysical neutrino flux measured by IceCube. We derive the detection probability for different zenith angles andngeomagnetic field configurations. The difference in detectability of sources between CTA-North and CTA-South for the average geomagnetic field is not substantial. We investigate the effect of a higher night-sky background and the preliminary CTA Alpha layout on the detection probability.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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