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

the CTA Consortium and the FIRESONG Team Collaboration

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

the CTA Consortium and the FIRESONG Team Collaboration

Physics

Kyiv National Taras Shevchenko University
Durham University
National Institute for Nuclear Physics
University of Naples Federico II
German Electron Synchrotron
Georgia Institute of Technology
Johannes Gutenberg University Mainz
Technical University of Munich
North West University
The University of Tokyo
Pontificia Universidad Católica de Chile
Université Paris-Saclay
Port d’Informació Científica
Monash University
Laboratoire Leprince-Ringuet
Columbia University
University of Oslo
Complutense University
Instituto de Astrofísica de Andalucía - CSIC
Campus UAB
Universidad Autónoma de Madrid
Dublin Institute for Advanced Studies
Universidad Nacional Autónoma de México
University of Geneva
University of L'Aquila
Universidade de São Paulo
PSL University
Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
Osservatorio Astrofisico Di Arcetri, Florence
University of Perugia
Argonne National Laboratory
Aix-Marseille Université
Osservatorio Astronomico Roma
Osservatorio Astrofisico di Catania
National Astronomical Research Institute of Thailand
University of La Laguna
Czech Academy of Sciences
Universidad Técnica Federico Santa Maria
Swiss Federal Institute of Technology Zurich
University of Manitoba
Université Montpellier 2
Centro Brasileiro de Pesquisas Físicas
Institute for High Energy Physics
University of Groningen
University of New South Wales
National Institute for Astrophysics
Université Savoie Mont Blanc
TU Dortmund University
University of Zagreb
University of Namibia
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
University of Hamburg
Max Planck Institute for Nuclear Physics
RIKEN
University of Padua
University of Jaén
Linnaeus University
University of the Witwatersrand
Ruhr University Bochum
University of Łódź
University of Siena
Harvard & Smithsonian
University of Turku
NASU - Pidstryhach Institute for Applied Problems of Mechanics and Mathematics
Bhabha Atomic Research Centre
University of Nova Gorica
University of Tübingen
Australian National University
University of California at Los Angeles
Polytechnic University of Bari
Astronomical Observatory of Padua
University of Palermo
University of Sydney
Sorbonne Université
University of Barcelona
Washington University St. Louis
Saha Institute of Nuclear Physics
Osservatorio Astronomico di Capodimonte
Université de Paris
Sofia University
IRAP
University of Minnesota
University of Warsaw
Armagh Observatory
Stanford University
Universidade Cruzeiro do Sul
Universidad de Valparaíso
Lund University
Cracow
University of Udine
Palacký University Olomouc
Max Planck Institute for Physics (Werner Heisenberg Institute)
Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
Dublin City University
University of Turin
Tata Institute of Fundamental Research
Oskar Klein Centre
Yale University
CIEMAT
University of Oxford
University of Southampton
University of Bergen
Western Sydney University
University of Adelaide
University of Rijeka
University of Würzburg
Universidade Federal do Paraná
University of Leicester
IPAG
National Centre for Nuclear Research
The University of Chicago
University of Potsdam
Iowa State University
Aristotle University of Thessaloniki
King's College London
Pennsylvania State University
National Technical University of Athens
University of Wisconsin-Madison
Purdue University
Institut d'Estudis Espacials de Catalunya
Nagoya University
Hiroshima University
Friedrich-Alexander University Erlangen-Nürnberg
University of California at Santa Cruz
University of Trieste
A. Alikhanian Yerevan Institute of Physics
University of Bari
University of Split
Universidad Andrés Bello
AGH University of Science and Technology
University of Liverpool
Yamagata University
Adler Planetarium
Yamanashi Gakuin University
Tokai University
University of Hertfordshire
Cherenkov Telescope Array Observatory
Tohoku University
Rikkyo University
University of Delaware
University of Innsbruck
University of Utah
Radboud University Nijmegen
Josip Juraj Strossmayer University of Osijek
Osaka University
Kyoto University
Jagiellonian University in Kraków
Heidelberg University
Department of Physics and Astronomy
University of Bath, Department of Physics
University of Iowa
University of Amsterdam
Ibaraki University
Waseda University
Nicolaus Copernicus University in Toruń
Saitama University
National University of Singapore
High Energy Accelerator Research Organization, Institute of Particle and Nuclear Physics
University of Sheffield
Universidade Federal do ABC
University of Catania
Humboldt University of Berlin
Texas Tech University
University of Zielona Gora
Bulgarian Academy of Sciences
University of Białystok
National and Kapodistrian University of Athens
Universidad de Chile
University of Miyazaki
Kitasato University
Universidad de Concepción
Charles University
Ivan Franko National University of L'viv
Tokushima University
Polish Academy of Sciences
Universidade Federal do Rio Grande do Norte
University College Dublin
Universidad Metropolitana de Ciencias de la Educación
Universidade Federal de São Carlos
University of Zurich
Aoyama Gakuin University
University of The Free State
Warsaw University of Technology
Ruder Boskovic Institute
Konan University
Kumamoto University
University of Pavia
Aalto University
Italian Space Agency
Université Côte d'Azur
University of Johannesburg

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

Abstract

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.

Original language	English
Article number	975
Journal	Proceedings of Science
Volume	395
Publication status	Published - 18 Mar 2022
Event	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Germany Duration: 12 Jul 2021 → 23 Jul 2021

ASJC Scopus subject areas

Multidisciplinary

Cite this

@article{6c3bd26d5cc24c6dafe959cc7df15e2a,

title = "Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events",

abstract = "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.",

author = "\{the CTA Consortium and the FIRESONG Team Collaboration\} and Olga Sergijenko and Brown, \{Anthony M.\} and Fiorillo, \{Damiano F.G.\} and \{de Le{\'o}n\}, \{Alberto Rosales\} and Konstancja Satalecka and Tung, \{Chun Fai\} and Ren{\'e} Reimann and Theo Glauch and Ignacio Taboada and H. Abdalla and H. Abe and S. Abe and A. Abusleme and F. Acero and A. Acharyya and \{Ac{\'i}n Portella\}, V. and K. Ackley and R. Adam and C. Adams and Adhikari, \{S. S.\} and I. Aguado-Ruesga and I. Agudo and R. Aguilera and A. Aguirre-Santaella and F. Aharonian and A. Alberdi and R. Alfaro and J. Alfaro and C. Alispach and R. Aloisio and \{Alves Batista\}, R. and Amans, \{J. P.\} and L. Amati and E. Amato and L. Ambrogi and G. Ambrosi and M. Ambrosio and R. Ammendola and J. Anderson and M. Anduze and Ang{\"u}ner, \{E. O.\} and Antonelli, \{L. A.\} and V. Antonuccio and P. Antoranz and R. Anutarawiramkul and \{Aragunde Gutierrez\}, J. and C. Aramo and A. Araudo and M. Araya and S. Razzaque",

note = "Publisher Copyright: {\textcopyright} 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); 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "English",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

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 - https://www.scopus.com/pages/publications/85145264074

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 -

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

Abstract

ASJC Scopus subject areas

Other files and links

Fingerprint

Cite this