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 Science and Technology Faculty of Computer Science
National University of Kyiv
National Academy of Sciences of Ukraine
Durham University
Niels Bohr Institutet
Universités Paris VI and VII
University of Turku
College of Computing
Tokai University
University of Tokyo
University of Alabama
Université Côte d’Azur
Ip Paris
University of Barcelona
Instituto de Astrofísica de Andalucía-CSIC
Pontificia Universidad Católica de Chile
IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos)
Universidad Autónoma de Madrid
GEPI - Galaxies, Etoiles, Physique, Instrumentation
Osservatorio Astrofisico Di Arcetri
Osservatorio Astronomico di Roma
Sceintific and Technological Research Council of Turkey
INFN Sezione di Napoli
INFN
Laboratoire Univers et Particules de Montpellier
University of Groningen
University of São Paulo
University of Dortmund
University of Namibia
North-West University
Monash University
Université de Genève
Universidad del Azuay
c/o DESY
Centro Brasileiro de Pesquisas Fisicas
University of Padova
University of Potsdam
University of the Witwatersrand, Johannesburg
Ruhr-University Bochum
INFN Roma Tor Vergata
Center for Astrophysics | Harvard & Smithsonian
Astroparticule and Cosmol APC
Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)
Max-Planck-Institut für Kernphysik
Max-Planck-Institut für Physik
Pidstryhach Institute for Applied Problems in Mechanics and Mathematics NASU
Université Savoie Mont Blanc
University of Nova Gorica
University of Tübingen
ETH Zurich
Politecnico di Bari
INFN Sezione di Bari
The Barcelona Institute of Science and Technology
Institute of Physics of the Czech Academy of Sciences
Sorbonne Université
INAF
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
University of Zagreb, Faculty of Electrical Engineering and Computing
Université Paris-Saclay
University of Adelaide
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
Dublin Institute for Advanced Studies
and Physics University of Udine
University of Geneva
Armagh Observatory
University of New South Wales
CEA/UVSQ/CNRS
Cherenkov Telescope Array Observatory
University of São Paulo
Kasetsart University
National Astronomical Research Institute of Thailand
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
Universidade Cruzeiro do Sul
Lund Observatory
Aix-Marseille Université
Osservatorio Astronomico di Capodimonte
Universidad de Alcalá
Università degli studi di Bari Aldo Moro
Dublin City University
INFN Sezione di Torino
University of Turin
Universidade Federal Do Paraná - Setor Palotina
INAF Osservatorio Astrofisico di Catania
Universidad de Valparaíso
University of Wisconsin-Madison
University of Bergen
Istituto di Astrofisica e Planetologia Spaziali (IAPS)
University of Naples Federico II
Universidad Técnica Federico Santa María
University of Würzburg
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
University of Chicago
Chemin de Bellevue
University of California at Santa Cruz
Scuola Universitaria Superiore IUSS di Pavia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
University of Manitoba
RIKEN (The Institute of Physical and Chemical Research)
Sezione di Roma
University of Perugia
Nagoya University
Yerevan Physics Institute
INFN Sezione di Catania
Universidad Andres Bello
Universidad Nacional Autónoma de México
Universidade Federal do Espírito Santo
The Open University of Israel
George Washington University
University of Liverpool
King's College London
Yamagata University
Yamanashi-Gakuin University
IRAP/CNRS
University of Innsbruck
Joint Laboratory of Optics
Josip Juraj Strossmayer University of Osijek
Gran Sasso Science Institute
Laboratori Nazionali del Gran Sasso
Università Dell'Aquila
University of Lodz
Jagiellonian University
Landessternwarte Heidelberg
Université Grenoble Alpes
of Sciences
University of Utah
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
KEK (High Energy Accelerator Research Organization)
University of Leicester
Western Sydney University
UMR 5797
University of Trieste
Research Unit; CIBERNED and Universidad de La Laguna
University of Jaen
University of Amsterdam
An OCC of Homi Bhabha National Institute
Università degli Studi di Catania
University of Palermo
Complutense University
Universidad Pontificia Comillas — ICAI
University of Chile
Campus UAB
Institute for Nuclear Physics
Konan University
Hiroshima University
Columbia University
Kitasato University
Kavli Institute for Particle Astrophysics and Cosmology
University of Białystok
Charles University
National University of Lviv
University of California, Los Angeles
Tokushima University
University of Pisa
University of Rijeka
Ruđer Bošković Institute
INAF Osservatorio Astronomico di Padova
University of Siena
University of Johannesburg
University of Oxford
Universidad Metropolitana de Ciencias de la Educación
Universidad de Concepción
University of New South Wales at Australian Defence Force Academy
Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture, University of Split
Observatoire de Sauverny
Humboldt-Universität zu Berlin
Academic Computer Centre CYFRONET AGH
Nicolaus Copernicus University
Cherenkov Telescope Array Observatory gGmbH
Warsaw University of Technology
Sun Yat-Sen University
Aoyama Gakuin University
Division of Physics and Astronomy
Port d'Informació Científica
Ibaraki University

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

1 Citation (Scopus)

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
Publication status	Published - 27 Sept 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: 26 Jul 2023 → 3 Aug 2023

Cite this

@article{26b6643482b7411d8c385b7b010057b2,

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 S. Chaty and S. Fegan and D. Horan",

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 = "English",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

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 - Chaty, S.

AU - Fegan, S.

AU - Horan, D.

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.

M3 - Conference article

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

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