TY - JOUR
T1 - Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events
AU - the CTA Consortium and the FIRESONG Team Collaboration
AU - Sergijenko, Olga
AU - Brown, Anthony M.
AU - Fiorillo, Damiano F.G.
AU - de León, Alberto Rosales
AU - Satalecka, Konstancja
AU - Tung, Chun Fai
AU - Reimann, René
AU - Glauch, Theo
AU - Taboada, Ignacio
AU - Abdalla, H.
AU - Abe, H.
AU - Abe, S.
AU - Abusleme, A.
AU - Acero, F.
AU - Acharyya, A.
AU - Acín Portella, V.
AU - Ackley, K.
AU - Adam, R.
AU - Adams, C.
AU - Adhikari, S. S.
AU - Aguado-Ruesga, I.
AU - Agudo, I.
AU - Aguilera, R.
AU - Aguirre-Santaella, A.
AU - Aharonian, F.
AU - Alberdi, A.
AU - Alfaro, R.
AU - Alfaro, J.
AU - Alispach, C.
AU - Aloisio, R.
AU - Alves Batista, R.
AU - Amans, J. P.
AU - Amati, L.
AU - Amato, E.
AU - Ambrogi, L.
AU - Ambrosi, G.
AU - Ambrosio, M.
AU - Ammendola, R.
AU - Anderson, J.
AU - Anduze, M.
AU - Angüner, E. O.
AU - Antonelli, L. A.
AU - Antonuccio, V.
AU - Antoranz, P.
AU - Anutarawiramkul, R.
AU - Aragunde Gutierrez, J.
AU - Aramo, C.
AU - Araudo, A.
AU - Araya, M.
AU - Razzaque, S.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
PY - 2022/3/18
Y1 - 2022/3/18
N2 - 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 and geomagnetic 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.
AB - 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 and geomagnetic 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.
UR - http://www.scopus.com/inward/record.url?scp=85145264074&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85145264074
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 975
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -