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

the CTA Consortium and FIRESONG Team

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

the CTA Consortium and FIRESONG Team

AGH University of Krakow
Kyiv National Taras Shevchenko University
NASU - Main Astronomical Observatory
Durham University
University of Copenhagen
Laboratoire de Physique Nucléaire et de Hautes Energies
University of Turku
Georgia Institute of Technology
Tokai University
The University of Tokyo
University of Alabama
Université Côte d'Azur
Laboratoire Leprince-Ringuet
University of Barcelona
CSIC - Institute of Astrophysics of Andalusia
Pontificia Universidad Católica de Chile
Complutense University
Universidad Autónoma de Madrid
PSL Research University
Osservatorio Astrofisico Di Arcetri, Florence
Osservatorio Astronomico Roma
Scientific and Technological Research Council of Turkey
National Institute for Nuclear Physics
Laboratoire Univers et Particules de Montpellier
University of Groningen
Universidade de São Paulo
TU Dortmund University
University of Namibia
North West University
Monash University
University of Geneva
Universidad del Azuay
German Electron Synchrotron
Centro Brasileiro de Pesquisas Físicas
University of Padua
University of Potsdam
University of the Witwatersrand
Ruhr University Bochum
Harvard-Smithsonian Center for Astrophysics
CIEMAT
Max Planck Institute for Nuclear Physics
Max Planck Institute for Physics (Werner Heisenberg Institute)
NASU - Pidstryhach Institute for Applied Problems of Mechanics and Mathematics
Université Savoie Mont Blanc
University of Nova Gorica
University of Tübingen
Swiss Federal Institute of Technology Zurich
Polytechnic University of Bari
Institute for High Energy Physics
Czech Academy of Sciences
Sorbonne Université
Osservatorio Astronomico di Brera
University of Zagreb
Université Paris-Saclay
Adelaide University
Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
Dublin Institute for Advanced Studies
University of Udine
Armagh Observatory
University of New South Wales
Cherenkov Telescope Array Observatory
Autonomous University of Barcelona
Kasetsart University
National Astronomical Research Institute of Thailand
National Institute for Astrophysics
Universidade Cruzeiro do Sul
Lund University
Centre de Physique des Particules de Marseille
Osservatorio Astronomico di Capodimonte
University of Alcalá
University of Bari
APC - AstroParticule et Cosmologie
Dublin City University
University of Turin
Universidade Federal do Paraná
Osservatorio Astrofisico di Catania
Universidad de Valparaíso
University of Wisconsin-Madison
University of Bergen
University of Naples Federico II
Universidad Técnica Federico Santa Maria
University of Würzburg
Friedrich-Alexander University Erlangen-Nürnberg
The University of Chicago
LAPTH Laboratoire d'Annecy-Le-Vieux de Physique Theorique
University of California at Santa Cruz
University of Pavia
University of Manitoba
RIKEN
University of Perugia
Nagoya University
A. Alikhanian Yerevan Institute of Physics
Universidad Andrés Bello
Universidad Nacional Autónoma de México
Universidade Federal do Espírito Santo
Open University of Israel
George Washington University
University of Liverpool
King's College London
Yamagata University
Yamanashi Gakuin University
Université Paul Sabatier Toulouse III
University of Innsbruck
Joint Laboratory of Optics
Josip Juraj Strossmayer University of Osijek
Gran Sasso Science Institute
University of L'Aquila
University of Lodz
Jagiellonian University in Kraków
Heidelberg University
UJF-CNRS (UMR 5571)
University of Utah
Polish Academy of Sciences
High Energy Accelerator Research Organization, Institute of Particle and Nuclear Physics
University of Leicester
Western Sydney University
Université Bordeaux 1
University of Trieste
University of La Laguna
University of Jaén
University of Amsterdam
Homi Bhabha National Institute
University of Catania
University of Palermo
Comillas Pontifical University
Universidad de Chile
CSIC - Institute of Space Sciences
Institute of Nuclear Physics PAN
Konan University
Hiroshima University
Columbia University
Kitasato University
Kavli Institute for Particle Astrophysics and Cosmology
University of Białystok
Charles University
Ivan Franko National University of L'viv
University of California at Los Angeles
Tokushima University
University of Pisa
University of Rijeka
Ruder Boskovic Institute
Astronomical Observatory of Padua
University of Siena
University of Johannesburg
University of Oxford
Universidad Metropolitana de Ciencias de la Educación
Universidad de Concepción
University of Split
Observatoire de Sauverny
Humboldt University of Berlin
Nicolaus Copernicus University in Toruń
Cherenkov Telescope Array Observatory GGmbH
Warsaw University of Technology
Sun Yat-Sen University
Aoyama Gakuin University
Kyoto University
Port d'Informació Científica
Ibaraki University

Research output: Contribution to journal › Conference article › peer-review

1 Scopus citations

Abstract

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.

Original language	English
Article number	1531
Journal	Proceedings of Science
Volume	444
State	Published - 27 Sep 2024
Externally published	Yes
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: 26 Jul 2023 → 3 Aug 2023

Bibliographical note

Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.

Cite this

@article{d653aab05aba429da497538ca687f32b,

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

abstract = "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.",

author = "\{the CTA Consortium and FIRESONG Team\} and Olga Sergijenko and Brown, \{Anthony M.\} and Damiano Fiorillo and \{de Le{\'o}n\}, \{Alberto Rosales\} and Konstancja Satalecka and Tung, \{Chun Fai\} and Ignacio Taboada and K. Abe and S. Abe and A. Acharyya and R. Adam and A. Aguasca-Cabot and I. Agudo and J. Alfaro and N. Alvarez-Crespo and \{Alves Batista\}, R. and Amans, \{J. P.\} and E. Amato and F. Ambrosino and Ang{\"u}ner, \{E. O.\} and Antonelli, \{L. A.\} and C. Aramo and C. Arcaro and L. Arrabito and K. Asano and J. Aschersleben and H. Ashkar and \{Augusto Stuani\}, L. and D. Baack and M. Backes and C. Balazs and M. Balbo and \{Baquero Larriva\}, A. and \{Barbosa Martins\}, V. and \{Barres de Almeida\}, U. and Barrio, \{J. A.\} and D. Bastieri and Batista, \{P. I.\} and I. Batkovic and R. Batzofin and J. Baxter and G. Beck and \{Becker Tjus\}, J. and L. Beiske and D. Belardinelli and W. Benbow and E. Bernardini and \{Bernete Medrano\}, J. and K. Bernl{\"o}hr and A. Pe{\textquoteright}er",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

language = "אנגלית",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

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TY - JOUR

T1 - Sensitivity of the Cherenkov Telescope Array to the gamma-ray emission from neutrino sources detected by IceCube

AU - the CTA Consortium and FIRESONG Team

AU - Sergijenko, Olga

AU - Brown, Anthony M.

AU - Fiorillo, Damiano

AU - de León, Alberto Rosales

AU - Satalecka, Konstancja

AU - Tung, Chun Fai

AU - Taboada, Ignacio

AU - Abe, K.

AU - Abe, S.

AU - Acharyya, A.

AU - Adam, R.

AU - Aguasca-Cabot, A.

AU - Agudo, I.

AU - Alfaro, J.

AU - Alvarez-Crespo, N.

AU - Alves Batista, R.

AU - Amans, J. P.

AU - Amato, E.

AU - Ambrosino, F.

AU - Angüner, E. O.

AU - Antonelli, L. A.

AU - Aramo, C.

AU - Arcaro, C.

AU - Arrabito, L.

AU - Asano, K.

AU - Aschersleben, J.

AU - Ashkar, H.

AU - Augusto Stuani, L.

AU - Baack, D.

AU - Backes, M.

AU - Balazs, C.

AU - Balbo, M.

AU - Baquero Larriva, A.

AU - Barbosa Martins, V.

AU - Barres de Almeida, U.

AU - Barrio, J. A.

AU - Bastieri, D.

AU - Batista, P. I.

AU - Batkovic, I.

AU - Batzofin, R.

AU - Baxter, J.

AU - Beck, G.

AU - Becker Tjus, J.

AU - Beiske, L.

AU - Belardinelli, D.

AU - Benbow, W.

AU - Bernardini, E.

AU - Bernete Medrano, J.

AU - Bernlöhr, K.

AU - Pe’er, A.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/85212307988

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.conferencearticle???

AN - SCOPUS:85212307988

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1531

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

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

Abstract

Bibliographical note

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