| Naslov: | Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events |
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| Avtorji: | ID Sergijenko, Olga (Avtor)
ID Bhattacharyya, Saptashwa (Avtor)
ID MARČUN, Barbara (Avtor)
ID Pérez Romero, Judit (Avtor)
ID Stanič, Samo (Avtor)
ID Vodeb, Veronika (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zaharijas, Gabrijela (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Živec, Miha (Avtor), et al. |
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| Datoteke: |  ICRC2021_975.pdf (1,15 MB)
MD5: 3BF7731672AAD1214511C0D9A3A2D91F
 https://pos.sissa.it/395/
https://pos.sissa.it/395/975
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| Jezik: | Angleški jezik |
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| Vrsta gradiva: | Delo ni kategorizirano |
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| Tipologija: | 1.08 - Objavljeni znanstveni prispevek na konferenci |
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| Organizacija: | UNG - Univerza v Novi Gorici
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| Opis: | 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 di˙use astrophysical neutrino flux measured by IceCube. We derive the detection probability for di˙erent zenith angles and geomagnetic field configurations. The di˙erence in detectability of sources between CTA-North and CTA-South for the average geomagnetic field is not substantial. We investigate the e˙ect of a higher night-sky background and the preliminary CTA Alpha layout on the detection probability. |
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| Ključne besede: | Cherenkov Telescope Array, VHE gamma-rays, neutrinos, Ice Cube, FIRESONG |
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| Status publikacije: | Objavljeno |
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| Leto izida: | 2021 |
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| PID: | 20.500.12556/RUNG-8436  |
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| COBISS.SI-ID: | 164940291 |
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| NUK URN: | URN:SI:UNG:REP:1PNKQDCZ |
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| Datum objave v RUNG: | 19.09.2023 |
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| Število ogledov: | 637 |
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| Število prenosov: | 7 |
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| Metapodatki: |     |
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| Vaša ocena: | Ocenjevanje je dovoljeno samo prijavljenim uporabnikom. |
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