Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants

CTA Consortium

Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants

CTA Consortium

University of Amsterdam
Division of Physics and Astronomy
RIKEN Cluster for Pioneering Research
North Carolina State University
University of Manitoba
Center for Astrophysics | Harvard & Smithsonian
University of Heidelberg
University of New South Wales at Australian Defence Force Academy
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
Astroparticule and Cosmol APC
INFN Roma Tor Vergata
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
Durham University
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
INAF Istituto di Radioastronomia
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
National University of Kyiv
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
University of Turku
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
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
INAF - Osservatorio Astronomico di Palermo G.S. Vaiana
University of California, Los Angeles
Tokushima University
College of Computing
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
Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture, University of Split
Observatoire de Sauverny
Humboldt-Universität zu Berlin
National Academy of Sciences of Ukraine
Agh University of Science and Technology Faculty of Computer Science
Academic Computer Centre CYFRONET AGH
Nicolaus Copernicus University
Cherenkov Telescope Array Observatory gGmbH
Warsaw University of Technology
Sun Yat-Sen University
Aoyama Gakuin University
Port d'Informació Científica
Ibaraki University

Résultats de recherche: Contribution à un journal › Article de conférence › Revue par des pairs

Résumé

Modern imaging atmospheric Cherenkov telescopes have extensively observed young nearby supernova remnants (SNRs), with ages of about 1000 years or less, in the very-high-energy (VHE) gamma-ray band. These efforts resulted in the detection of VHE emission from three young SNRs – Cassiopeia A, Tycho, and SN 1006 – and provided significant evidence for emission from the more distant Kepler’s SNR. However, many questions on the production of VHE gamma rays in these remnants remain unanswered. Using detailed physical models for Tycho’s SNR based on the CR-hydro-NEI code and physically motivated models for the other young nearby remnants, we simulated observations with the Cherenkov Telescope Array (CTA) of these gamma-ray sources. We highlight properties of these remnants accessible for investigation with future CTA observations and discuss which questions are expected to be answered.

langue originale	Anglais
Numéro d'article	824
journal	Proceedings of Science
Volume	444
état	Publié - 27 sept. 2024
Evénement	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japon Durée: 26 juil. 2023 → 3 août 2023

Contient cette citation

@article{3ace5b98809f4d2bbfe5eb18482caa53,

title = "Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants",

abstract = "Modern imaging atmospheric Cherenkov telescopes have extensively observed young nearby supernova remnants (SNRs), with ages of about 1000 years or less, in the very-high-energy (VHE) gamma-ray band. These efforts resulted in the detection of VHE emission from three young SNRs – Cassiopeia A, Tycho, and SN 1006 – and provided significant evidence for emission from the more distant Kepler{\textquoteright}s SNR. However, many questions on the production of VHE gamma rays in these remnants remain unanswered. Using detailed physical models for Tycho{\textquoteright}s SNR based on the CR-hydro-NEI code and physically motivated models for the other young nearby remnants, we simulated observations with the Cherenkov Telescope Array (CTA) of these gamma-ray sources. We highlight properties of these remnants accessible for investigation with future CTA observations and discuss which questions are expected to be answered.",

author = "\{CTA Consortium\} and Prokhorov, \{Dmitry A.\} and Lee, \{Shiu Hang\} and Shigehiro Nagataki and Jacco Vink and Ellison, \{Donald C.\} and Gilles Ferrand and Patnaude, \{Daniel J.\} and Roepke, \{Friedrich K.\} and Seitenzahl, \{Ivo R.\} and Slane, \{Patrick O.\} 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 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",

}

TY - JOUR

T1 - Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants

AU - CTA Consortium

AU - Prokhorov, Dmitry A.

AU - Lee, Shiu Hang

AU - Nagataki, Shigehiro

AU - Vink, Jacco

AU - Ellison, Donald C.

AU - Ferrand, Gilles

AU - Patnaude, Daniel J.

AU - Roepke, Friedrich K.

AU - Seitenzahl, Ivo R.

AU - Slane, Patrick O.

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 - Chaty, S.

AU - Fegan, S.

AU - Horan, D.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - Modern imaging atmospheric Cherenkov telescopes have extensively observed young nearby supernova remnants (SNRs), with ages of about 1000 years or less, in the very-high-energy (VHE) gamma-ray band. These efforts resulted in the detection of VHE emission from three young SNRs – Cassiopeia A, Tycho, and SN 1006 – and provided significant evidence for emission from the more distant Kepler’s SNR. However, many questions on the production of VHE gamma rays in these remnants remain unanswered. Using detailed physical models for Tycho’s SNR based on the CR-hydro-NEI code and physically motivated models for the other young nearby remnants, we simulated observations with the Cherenkov Telescope Array (CTA) of these gamma-ray sources. We highlight properties of these remnants accessible for investigation with future CTA observations and discuss which questions are expected to be answered.

AB - Modern imaging atmospheric Cherenkov telescopes have extensively observed young nearby supernova remnants (SNRs), with ages of about 1000 years or less, in the very-high-energy (VHE) gamma-ray band. These efforts resulted in the detection of VHE emission from three young SNRs – Cassiopeia A, Tycho, and SN 1006 – and provided significant evidence for emission from the more distant Kepler’s SNR. However, many questions on the production of VHE gamma rays in these remnants remain unanswered. Using detailed physical models for Tycho’s SNR based on the CR-hydro-NEI code and physically motivated models for the other young nearby remnants, we simulated observations with the Cherenkov Telescope Array (CTA) of these gamma-ray sources. We highlight properties of these remnants accessible for investigation with future CTA observations and discuss which questions are expected to be answered.

M3 - Conference article

AN - SCOPUS:85212258705

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 824

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants

Résumé

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