Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

S. Abe; J. Abhir; A. Abhishek; F. Acero; A. Acharyya; R. Adam; A. Aguasca-Cabot; I. Agudo; I. Albanese; J. Alfaro; C. Alispach; R. Alves Batista; E. Amato; G. Ambrosi; D. Ambrosino; F. Ambrosino; L. Angel; C. Aramo; A. Arbet-Engels; C. Arcaro; C. Arena; T. T. H. Arnesen; K. Asano; H. Ashkar; C. Bakshi; C. Balazs; M. Balbo; A. Baquero Larriva; V. Barbosa Martins; J. A. Barrio; C. Bartolini; I. Batkovic; R. Batzofin; N. Bavdaz; J. Becerra Gonzalez; G. Beck; W. Benbow; E. Bernardini; M. G. Bernardini; J. Bernete; A. Berti; B. Bertucci; V. Beshley; P. Bhattacharjee; S. Bhattacharyya; C. Bigongiari; A. Biland; E. Bissaldi; M. Blana; O. Blanch; J. Blazek; C. Boisson; G. Bonnoli; Z. Bosnjak; E. Bottacini; M. Bottcher; E. Bronzini; G. Brunelli; J. Buces Saez; A. Bulgarelli; T. Bulik; L. Burmistrov; P. G. Calisse; A. Campoy-Ordaz; B. K. Cantlay; G. Capasso; A. Caproni; R. Capuzzo-Dolcetta; M. Cardillo; S. Caroff; A. Carosi; E. Carquin; S. Casanova; E. Cascone; F. Cassol; G. Castignani; F. Catalani; D. Cerasole; M. Cerruti; A. Cervino Cortinez; P. M. Chadwick; S. Chaty; A. W. Chen; Y. Chen; M. Chernyakova; A. Chiavassa; G. Chon; J. Chudoba; L. Chytka; G. M. Cicciari; A. Cifuentes Santos; C. H. Coimbra Araujo; J. L. Contreras; B. Cornejo; J. Cortina; A. Costa; G. Cotter; P. Cristofari; O. Cuevas; Z. Curtis-Ginsberg; A. D'Ai; G. D'Amico; F. D'Ammando; P. D'Avanzo; P. Da Vela; L. David; F. Dazzi; M. de Bony de Lavergne; V. De Caprio; E. M. de Gouveia Dal Pino; B. De Lotto; M. de Naurois; V. de Souza; L. del Peral; M. V. del Valle; C. Delgado; D. della Volpe; D. Depaoli; A. Dettlaff; L. Di Bella; T. Di Girolamo; A. Di Piano; F. Di Pierro; R. Di Tria; L. Di Venere; R. Dima; A. Dinesh; E. Do Souto Espineira; D. Dominis Prester; A. Donini; D. Dorner; J. Dorner; M. Doro; L. Ducci; V. V. Dwarkadas; J. Ebr; C. Eckner; K. Egberts; L. Eisenberger; D. Elsasser; G. Emery; C. Escanuela Nieves; P. Escarate; M. Escobar Godoy; J. Escudero Pedrosa; P. Esposito; D. Falceta-Goncalves; E. Fedorova; S. Fegan; K. Feijen; Q. Feng; G. Ferrand; E. Fiandrini; A. Fiasson; M. Filipovic; V. Fioretti; L. Foffano; G. Fontaine; F. Frias Garcia-Lago; Y. Fukazawa; Y. Fukui; G. Galanti; G. Galaz; S. Gallozzi; V. Gammaldi; S. Garcia Soto; M. Garczarczyk; C. Gasbarra; D. Gasparrini; M. Gaug; G. Ghirlanda; J. G. Giesbrecht Formiga Paiva; N. Giglietto; F. Giordano; M. Giroletti; R. Giuffrida; J-F. Glicenstein; P. Goldoni; J. M. Gonzalez; J. Goulart Coelho; T. Gradetzke; J. Granot; R. Grau; D. Green; J. G. Green; J. Grube; J. Hackfeld; D. Hadasch; A. Hahn; P. Hamal; W. Hanlon; S. Hara; V. M. Harvey; T. Hassan; K. Hayashi; B. Hess; L. Heckmann; N. Hiroshima; B. Hnatyk; R. Hnatyk; D. Horan; P. Horvath; D. Hrupec; S. Hussain; M. Iarlori; T. Inada; F. Incardona; S. Inoue; F. Iocco; A. Iuliano; Jahanvi; M. Jamrozy; P. Janecek; F. Jankowsky; C. Jarnot; I. Jaroschewski; P. Jean; V. Jilek; I. Jimenez Martinez; J. Jimenez Quiles; W. Jin; E. Joshi; J. Jurysek; V. Karas; H. Katagiri; J. Kataoka; S. Kaufmann; T. Keita; D. Kerszberg; M. Kherlakian; D. B. Kieda; R. Kissmann; T. Kleiner; Y. Kobayashi; K. Kohri; D. Kolar; N. Komin; A. Kong; K. Kosack; D. Kostunin; G. Kowal; H. Kubo; J. Kushida; A. La Barbera; N. La Palombara; B. Lacave; M. Lainez; A. Lamastra; J. Lapington; S. Lazarevic; J-P. Lenain; F. Leone; E. Leonora; G. Leto; E. Lindfors; S. Lombardi; F. Longo; R. Lopez-Coto; M. Lopez-Moya; A. Lopez-Oramas; J. Lozano Bahilo; P. L. Luque-Escamilla; E. Lyard; O. Macias; P. Majumdar; M. Makariev; D. Mandat; S. Mangano; A. Marchetti; M. Mariotti; S. Markoff; I. Marquez; G. Marsella; J. Marti; D. Martin Dominguez; M. Martinez; O. Martinez; G. Maurin; D. Mazin; D. Melkumyan; S. Menon; E. Mestre; D. M-A. Meyer; D. Miceli; M. Miceli; M. Michailidis; T. Miener; J. M. Miranda; R. Moderski; M. Molero; C. Molfese; E. Molina; K. Morik; A. Morselli; E. Moulin; A. L. Muller; K. Munari; T. Murach; A. Muraczewski; H. Muraishi; T. Nakamori; L. Nava; R. Nemmen; J. Niemiec; D. Nieto; M. Nievas Rosillo; M. Nikolajuk; L. Nikolic; K. Noda; D. Nosek; V. Novotny; S. Nozaki; A. Okumura; R. A. Ong; R. Orito; M. Orlandini; E. Orlando; S. Orlando; J. Otero-Santos; I. Oya; M. Ozlati Moghadam; A. Pagliaro; M. Palatiello; A. Pandey; G. Panebianco; D. Paneque; F. R. Pantaleo; J. M. Paredes; B. Patricelli; A. Pe'er; M. Pech; M. Pecimotika; M. Peresano; E. Peretti; J. Perez-Romero; G. Peron; F. Perrotta; M. Persic; O. Petruk; F. Pfeifle; E. Pietropaolo; M. Pihet; L. Pinchbeck; F. Pintore; G. Pirola; C. Pittori; F. Podobnik; M. Pohl; V. Pollet; G. Ponti; E. Prandini; G. Principe; M. Prouza; E. Pueschel; G. Puhlhofer; M. L. Pumo; M. Punch; A. Quirrenbach; S. Raino; R. Rando; S. Recchia; A. Reimer; O. Reimer; I. Reis; A. Reisenegger; W. Rhode; M. Ribo; C. Ricci; T. Richtler; J. Rico; L. Riitano; V. Rizi; E. Roache; G. Rodriguez Fernandez; J. J. Rodriguez-Vazquez; P. Romano; G. Romeo; J. Rosado; A. Rosales de Leon; A. Roy; I. Sadeh; L. Saha; T. Saito; M. Sanchez-Conde; P. Sangiorgi; H. Sano; R. Santos-Lima; V. Sapienza; S. Sarkar; F. G. Saturni; A. Scherer; F. Schiavone; P. Schipani; P. Schovanek; F. Schussler; M. Seglar Arroyo; O. Sergijenko; H. Siejkowski; A. Simongini; V. Sliusar; A. Slowikowska; I. Sofia; H. Sol; S. Spinello; A. Stamerra; S. Stanic; T. Starecki; R. Starling; L. Stawarz; T. Stolarczyk; Y. Suda; A. Sunny; T. Suomijarvi; R. Takeishi; S. J. Tanaka; F. Tavecchio; T. Tavernier; Y. Terada; M. Teshima; V. Testa; W. W. Tian; Y. Tian; L. Tibaldo; O. Tibolla; S. J. Tingay; C. J. Todero Peixoto; F. Tombesi; D. Tonev; F. Torradeflot; D. F. Torres; N. Tothill; G. Tovmassian; G. Tripodo; A. Trois; A. Tsiahina; A. Tutone; L. Vaclavek; M. Vacula; C. van Eldik; J. Vandenbroucke; V. Vassiliev; M. Vazquez Acosta; M. Vecchi; S. Vercellone; S. D. Vergani; I. Viale; A. Viana; A. Vigliano; J. Vignatti; C. F. Vigorito; J. Villanueva; E. Visentin; V. Voitsekhovskyi; S. Vorobiov; I. Vovk; T. Vuillaume; R. Walter; M. Wechakama; M. White; A. Wierzcholska; M. Will; F. Wohlleben; A. Wolter; F. Xotta; T. Yamamoto; R. Yamazaki; T. Yoshikoshi; M. Zacharias; G. Zaharijas; R. Zanmar Sanchez; D. Zavrtanik; M. Zavrtanik; A. Zech; V. I. Zhdanov; M. Zivec; J. Zuriaga-Puig; A. Colombo; CTAO Consortium

doi:10.3847/1538-4357/ae658c

Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

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Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

S. Abe, J. Abhir, A. Abhishek, F. Acero, A. Acharyya, R. Adam, A. Aguasca-Cabot, I. Agudo, I. Albanese, J. Alfaro, …

The Astrophysical journal, 卷.1004(1), 頁.46

10/06/2026

DOI: https://doi.org/10.3847/1538-4357/ae658c

Web of Science ID: WOS:001788970100001

摘要

Astronomy & Astrophysics

Physical Sciences

Science & Technology

The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, the short gamma-ray burst GRB 170817A, heralded the birth of multimessenger astronomy. The detection of TeV emission from GRBs motivates follow-up observations with the Cherenkov Telescope Array Observatory (CTAO), which is ideal for detecting such signals due to its unprecedented sensitivity, rapid response, and wide-field survey capabilities. The aim of this work is to evaluate GeV-TeV GW follow-up strategies for CTAO using a multistep simulation pipeline and to estimate the expected rate of joint GW-GRB detections during observing run O5. Using a simulated sample of BNS systems with corresponding GW detections, gamma-ray emission is simulated through phenomenological prescriptions based on the observed population of short GRBs, including off-axis jet scenarios. CTAO observations are simulated to account for instrument response, sky tiling strategies, integration times, and varying observing conditions. Strategies with variable and constant integration times are investigated. We find that, via an optimized follow-up strategy, about 5% of simulated GW-associated short GRBs produce GeV-TeV radiation detectable by CTAO. Detectability is strongly influenced by the jet opening angle and viewing angle, suggesting that even rough estimates of the viewing angle in GW alerts could enhance targeting. This framework motivates future follow-ups of GW-detectable events, including neutron star-black hole mergers, and further supports the development of advanced strategies incorporating galaxy distributions and synergies with future detectors such as the Einstein Telescope.

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題名: Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
創作者：: S. Abe - The University of Tokyo
J. Abhir - Institute for Particle Physics and Astrophysics
A. Abhishek - University of Siena
F. Acero - Université Paris-Saclay
A. Acharyya - University of Alabama
R. Adam - Université Côte d'Azur
A. Aguasca-Cabot - Universitat de Barcelona
I. Agudo - Consejo Superior de Investigaciones Científicas
I. Albanese - University of Padua
J. Alfaro - Pontificia Universidad Católica de Chile
C. Alispach - University of Geneva
R. Alves Batista - Sorbonne Université
E. Amato - Arcetri Astrophysical Observatory
G. Ambrosi - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
D. Ambrosino - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
F. Ambrosino - Astronomical Observatory of Rome
L. Angel - Universidade Federal do Rio Grande do Norte
C. Aramo - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
A. Arbet-Engels - Max Planck Inst Phys & Astrophys, Boltzmannstr 8, D-85748 Garching, Germany
C. Arcaro - Istituto Nazionale di Fisica Nucleare, Sezione di Padova
C. Arena - Osservatorio Astrofisico di Catania
T. T. H. Arnesen - Universidad de La Laguna
K. Asano - The University of Tokyo
H. Ashkar - Institut Polytechnique de Paris
C. Bakshi - Saha Institute of Nuclear Physics
C. Balazs - Monash University
M. Balbo - University of Geneva
A. Baquero Larriva - UCM, IPARCOS, Inst Fis Particulas & Cosmos, E-28040 Madrid, Spain
V. Barbosa Martins - Ruhr University Bochum
J. A. Barrio - Universidad Complutense de Madrid
C. Bartolini - University of Trento
I. Batkovic - University of Padua
R. Batzofin - University of Potsdam
N. Bavdaz - University of Nova Gorica
J. Becerra Gonzalez - Consejo Superior de Investigaciones Científicas
G. Beck - University of the Witwatersrand
W. Benbow - Center for Astrophysics Harvard & Smithsonian
E. Bernardini - University of Padua
M. G. Bernardini - Brera Astronomical Observatory
J. Bernete - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
A. Berti - Max Planck Institute for Physics
B. Bertucci - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
V. Beshley - Pidstryhach Institute for Applied Problems of Mechanics and Mathematics
P. Bhattacharjee - University of Nova Gorica
S. Bhattacharyya - University of Nova Gorica
C. Bigongiari - Astronomical Observatory of Rome
A. Biland - Institute for Particle Physics and Astrophysics
E. Bissaldi - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
M. Blana - Pontificia Universidad Católica de Chile
O. Blanch - Institute for High Energy Physics
J. Blazek - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
C. Boisson - Université Paris Sciences et Lettres
G. Bonnoli - Brera Astronomical Observatory
Z. Bosnjak - University of Zagreb
E. Bottacini - University of Padua
M. Bottcher - North-West University
E. Bronzini - Osservatorio di Astrofisica e Scienza dello Spazio
G. Brunelli - Osservatorio di Astrofisica e Scienza dello Spazio
J. Buces Saez - UCM, IPARCOS, Inst Fis Particulas & Cosmos, E-28040 Madrid, Spain
A. Bulgarelli - Osservatorio di Astrofisica e Scienza dello Spazio
T. Bulik - University of Warsaw
L. Burmistrov - University of Geneva
P. G. Calisse - CTA Observatory
A. Campoy-Ordaz - Universitat Autònoma de Barcelona
B. K. Cantlay - National Astronomical Research Institute of Thailand
G. Capasso - Astronomical Observatory of Capodimonte
A. Caproni - Universidade Cidade de São Paulo
R. Capuzzo-Dolcetta - Astronomical Observatory of Rome
M. Cardillo - Institute for Space Astrophysics and Planetology
S. Caroff - Université Savoie Mont Blanc
A. Carosi - Astronomical Observatory of Rome
E. Carquin - Federico Santa María Technical University
S. Casanova - Max Planck Institute for Nuclear Physics
E. Cascone - Astronomical Observatory of Capodimonte
F. Cassol - Aix-Marseille Université
G. Castignani - Osservatorio di Astrofisica e Scienza dello Spazio
F. Catalani - Universidade de São Paulo
D. Cerasole - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
M. Cerruti - Université Paris Cité
A. Cervino Cortinez - Universidad Complutense de Madrid
P. M. Chadwick - Durham University
S. Chaty - Université Paris Cité
A. W. Chen - University of the Witwatersrand
Y. Chen - Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
M. Chernyakova - Dublin City University
A. Chiavassa - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
G. Chon - Max Planck Institute for Physics
J. Chudoba - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
L. Chytka - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
G. M. Cicciari - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
A. Cifuentes Santos - CIEMAT, Ave Complutense 40, Madrid 28040, Spain
C. H. Coimbra Araujo - Univ Fed Parana, Setor Palotina, Dept Engn & Exatas, Rua Pioneiro 2153, BR-85950000 Palotina, Parana, Brazil
J. L. Contreras - Universidad Complutense de Madrid
B. Cornejo - Université Paris-Saclay
J. Cortina - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
A. Costa - Osservatorio Astrofisico di Catania
G. Cotter - University of Oxford
P. Cristofari - Université Paris Sciences et Lettres
O. Cuevas - University of Valparaíso
Z. Curtis-Ginsberg - University of Wisconsin System
A. D'Ai - INAF, Ist Astrofis Spaziale & Fis Cosm Palermo, Via Ugo La Malfa 153, I-90146 Palermo, Italy
G. D'Amico - Universidade Aberta
F. D'Ammando - Istituto di Radioastronomia di Bologna
P. D'Avanzo - Brera Astronomical Observatory
P. Da Vela - Osservatorio di Astrofisica e Scienza dello Spazio
L. David - Deutsches Elektronen-Synchrotron DESY
F. Dazzi - National Institute for Astrophysics
M. de Bony de Lavergne - Aix-Marseille Université
V. De Caprio - Astronomical Observatory of Capodimonte
E. M. de Gouveia Dal Pino - Universidade de São Paulo
B. De Lotto - University of Udine
M. de Naurois - Institut Polytechnique de Paris
V. de Souza - Universidade de São Paulo
L. del Peral - Universidad de Alcalá
M. V. del Valle - Universidade de São Paulo
C. Delgado - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
D. della Volpe - University of Geneva
D. Depaoli - CTA Observatory
A. Dettlaff - Max Planck Institute for Physics
L. Di Bella - TU Dortmund University
T. Di Girolamo - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
A. Di Piano - Osservatorio di Astrofisica e Scienza dello Spazio
F. Di Pierro - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
R. Di Tria - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
L. Di Venere - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
R. Dima - University of Padua
A. Dinesh - Universidad Complutense de Madrid
E. Do Souto Espineira - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
D. Dominis Prester - University of Rijeka
A. Donini - Astronomical Observatory of Rome
D. Dorner - University of Würzburg
J. Dorner - Ruhr University Bochum
M. Doro - University of Padua
L. Ducci - University of Tübingen
V. V. Dwarkadas - University of Chicago
J. Ebr - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
C. Eckner - University of Nova Gorica
K. Egberts - University of Potsdam
L. Eisenberger - University of Würzburg
D. Elsasser - TU Dortmund University
G. Emery - Consejo Superior de Investigaciones Científicas
C. Escanuela Nieves - Max Planck Institute for Nuclear Physics
P. Escarate - Pontificia Universidad Católica de Valparaíso
M. Escobar Godoy - Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, 1156 High St, Santa Cruz, CA 95064 USA
J. Escudero Pedrosa - Smithsonian Institution
P. Esposito - Istituto Universitario di Studi Superiori di Pavia
D. Falceta-Goncalves - Universidade de São Paulo
E. Fedorova - Taras Shevchenko National University of Kyiv
S. Fegan - Institut Polytechnique de Paris
K. Feijen - Université Paris Cité
Q. Feng - University of Utah
G. Ferrand - RIKEN
E. Fiandrini - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
A. Fiasson - Université Savoie Mont Blanc
M. Filipovic - Western Sydney University
V. Fioretti - Osservatorio di Astrofisica e Scienza dello Spazio
L. Foffano - Institute for Space Astrophysics and Planetology
G. Fontaine - Institut Polytechnique de Paris
F. Frias Garcia-Lago - Universidad de La Laguna
Y. Fukazawa - Hiroshima University
Y. Fukui - Nagoya University
G. Galanti - Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano
G. Galaz - Pontificia Universidad Católica de Chile
S. Gallozzi - Astronomical Observatory of Rome
V. Gammaldi - Universidad San Pablo CEU
S. Garcia Soto - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
M. Garczarczyk - Deutsches Elektronen-Synchrotron DESY
C. Gasbarra - Astronomical Observatory of Rome
D. Gasparrini - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
M. Gaug - Universitat Autònoma de Barcelona
G. Ghirlanda - Brera Astronomical Observatory
J. G. Giesbrecht Formiga Paiva - Centro Brasileiro de Pesquisas Físicas
N. Giglietto - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
F. Giordano - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
M. Giroletti - Istituto di Radioastronomia di Bologna
R. Giuffrida - Université Paris-Saclay
J-F. Glicenstein - Université Paris-Saclay
P. Goldoni - Université Paris Cité
J. M. Gonzalez - Universidad Andrés Bello
J. Goulart Coelho - Univ Fed Espirito Santo, Nucleo Astrofis & Cosmol Cosmo Ufes, Ave Fernando Ferrari 514, BR-29065910 Vitoria, ES, Brazil
T. Gradetzke - TU Dortmund University
J. Granot - George Washington University
R. Grau - The University of Tokyo
D. Green - CTA Observatory
J. G. Green - Max Planck Institute for Physics
J. Grube - King's College London
J. Hackfeld - TU Dortmund University
D. Hadasch - Institute of Space Sciences
A. Hahn - Max Planck Institute for Physics
P. Hamal - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
W. Hanlon - Center for Astrophysics Harvard & Smithsonian
S. Hara - Yamanashi Gakuin University
V. M. Harvey - The University of Adelaide
T. Hassan - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
K. Hayashi - The University of Tokyo
B. Hess - University of Tübingen
L. Heckmann - Université Paris Cité
N. Hiroshima - Yokohama National University
B. Hnatyk - Taras Shevchenko National University of Kyiv
R. Hnatyk - Taras Shevchenko National University of Kyiv
D. Horan - Institut Polytechnique de Paris
P. Horvath - Palacký University Olomouc
D. Hrupec - University of Osijek
S. Hussain - University of Nova Gorica
M. Iarlori - University of L'Aquila
T. Inada - Kyushu University
F. Incardona - Osservatorio Astrofisico di Catania
S. Inoue - Chiba University
F. Iocco - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
A. Iuliano - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
Jahanvi - INFN, Sez Trieste, Via Sci 208, I-33100 Udine, Italy
M. Jamrozy - Jagiellonian University
P. Janecek - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
F. Jankowsky - Heidelberg University
C. Jarnot - Université de Toulouse
I. Jaroschewski - Université Paris-Saclay
P. Jean - Université de Toulouse
V. Jilek - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
I. Jimenez Martinez - Max Planck Institute for Physics
J. Jimenez Quiles - Institute for High Energy Physics
W. Jin - Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
E. Joshi - Deutsches Elektronen-Synchrotron DESY
J. Jurysek - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
V. Karas - Czech Academy of Sciences, Astronomical Institute
H. Katagiri - Ibaraki University
J. Kataoka - Waseda University
S. Kaufmann - Durham University
T. Keita - Université Paris-Saclay
D. Kerszberg - Sorbonne Université
M. Kherlakian - Ruhr University Bochum
D. B. Kieda - University of Utah
R. Kissmann - Universität Innsbruck
T. Kleiner - Deutsches Elektronen-Synchrotron DESY
Y. Kobayashi - Chiba University
K. Kohri - National Astronomical Observatory of Japan
D. Kolar - University of Nova Gorica
N. Komin - University of the Witwatersrand
A. Kong - Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwa No Ha, Kashiwa, Chiba 2778582, Japan
K. Kosack - Université Paris-Saclay
D. Kostunin - Deutsches Elektronen-Synchrotron DESY
G. Kowal - Universidade de São Paulo
H. Kubo - The University of Tokyo
J. Kushida - Tokai University
A. La Barbera - Istituto di Astrofisica Spaziale e Fisica cosmica di Palermo
N. La Palombara - Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano
B. Lacave - University of Geneva
M. Lainez - Universidad Complutense de Madrid
A. Lamastra - Astronomical Observatory of Rome
J. Lapington - University of Leicester
S. Lazarevic - Western Sydney University
J-P. Lenain - Sorbonne Université
F. Leone - University of Catania
E. Leonora - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
G. Leto - Osservatorio Astrofisico di Catania
E. Lindfors - University of Turku
S. Lombardi - Astronomical Observatory of Rome
F. Longo - University of Trieste
R. Lopez-Coto - Consejo Superior de Investigaciones Científicas
M. Lopez-Moya - Universidad Complutense de Madrid
A. Lopez-Oramas - Universidad de La Laguna
J. Lozano Bahilo - Universidad de Alcalá
P. L. Luque-Escamilla - Universidad de Jaén
E. Lyard - University of Geneva
O. Macias - University of Amsterdam
P. Majumdar - Saha Institute of Nuclear Physics
M. Makariev - Institute for Nuclear Research and Nuclear Energy
D. Mandat - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
S. Mangano - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
A. Marchetti - Brera Astronomical Observatory
M. Mariotti - University of Padua
S. Markoff - University of Amsterdam
I. Marquez - Consejo Superior de Investigaciones Científicas
G. Marsella - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
J. Marti - Universidad de Jaén
D. Martin Dominguez - Universidad Complutense de Madrid
M. Martinez - Institute for High Energy Physics
O. Martinez - Universidad Complutense de Madrid
G. Maurin - Université Savoie Mont Blanc
D. Mazin - Max Planck Institute for Physics
D. Melkumyan - Deutsches Elektronen-Synchrotron DESY
S. Menon - University of Rome Tor Vergata
E. Mestre - Universidade Aberta
D. M-A. Meyer - Institute of Space Sciences
D. Miceli - Istituto Nazionale di Fisica Nucleare, Sezione di Padova
M. Miceli - Osservatorio Astronomico di Palermo
M. Michailidis - Stanford University
T. Miener - University of Geneva
J. M. Miranda - Universidad Complutense de Madrid
R. Moderski - Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ulica Bartycka 18, PL-00716 Warsaw, Poland
M. Molero - CIEMAT, Ave Complutense 40, Madrid 28040, Spain
C. Molfese - National Institute for Astrophysics
E. Molina - Universidad de La Laguna
K. Morik - TU Dortmund University
A. Morselli - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
E. Moulin - Université Paris-Saclay
A. L. Muller - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
K. Munari - Osservatorio Astrofisico di Catania
T. Murach - Deutsches Elektronen-Synchrotron DESY
A. Muraczewski - Nicolaus Copernicus Astronomical Center
H. Muraishi - Kitasato University
T. Nakamori - Yamagata University
L. Nava - Brera Astronomical Observatory
R. Nemmen - Universidade de São Paulo
J. Niemiec - Institute of Nuclear Physics, Polish Academy of Sciences
D. Nieto - Universidad Complutense de Madrid
M. Nievas Rosillo - Universidad de La Laguna
M. Nikolajuk - Univ Bialystok, Fac Phys, Ul K Ciolkowskiego 1L, PL-15245 Bialystok, Poland
L. Nikolic - University of Siena
K. Noda - Chiba University
D. Nosek - Charles University
V. Novotny - Charles University
S. Nozaki - The University of Tokyo
A. Okumura - Nagoya University
R. A. Ong - Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
R. Orito - Tokushima University
M. Orlandini - Osservatorio di Astrofisica e Scienza dello Spazio
E. Orlando - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
S. Orlando - Osservatorio Astronomico di Palermo
J. Otero-Santos - INFN Sezione di Padova
I. Oya - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
M. Ozlati Moghadam - University of Potsdam
A. Pagliaro - Istituto di Astrofisica Spaziale e Fisica cosmica di Palermo
M. Palatiello - Astronomical Observatory of Rome
A. Pandey - University of Utah
G. Panebianco - Osservatorio di Astrofisica e Scienza dello Spazio
D. Paneque - Max Planck Institute for Physics
F. R. Pantaleo - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
J. M. Paredes - Universitat de Barcelona
B. Patricelli - University of Pisa
A. Pe'er - Max Planck Inst Phys & Astrophys, Boltzmannstr 8, D-85748 Garching, Germany
M. Pech - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
M. Pecimotika - Institute for High Energy Physics
M. Peresano - Max Planck Institute for Physics
E. Peretti - Université Paris Cité
J. Perez-Romero - University of Nova Gorica
G. Peron - Arcetri Astrophysical Observatory
F. Perrotta - Astronomical Observatory of Capodimonte
M. Persic - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
O. Petruk - Osservatorio Astronomico di Palermo
F. Pfeifle - University of Würzburg
E. Pietropaolo - University of L'Aquila
M. Pihet - Consejo Superior de Investigaciones Científicas
L. Pinchbeck - Monash University
F. Pintore - Istituto di Astrofisica Spaziale e Fisica cosmica di Palermo
G. Pirola - Max Planck Institute for Physics
C. Pittori - Astronomical Observatory of Rome
F. Podobnik - University of Geneva
M. Pohl - University of Potsdam
V. Pollet - Université Savoie Mont Blanc
G. Ponti - Brera Astronomical Observatory
E. Prandini - University of Padua
G. Principe - University of Trieste
M. Prouza - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
E. Pueschel - Ruhr University Bochum
G. Puhlhofer - University of Tübingen
M. L. Pumo - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
M. Punch - Université Paris Cité
A. Quirrenbach - Heidelberg University
S. Raino - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
R. Rando - University of Padua
S. Recchia - Arcetri Astrophysical Observatory
A. Reimer - Universität Innsbruck
O. Reimer - Universität Innsbruck
I. Reis - Universidade de São Paulo
A. Reisenegger - Pontificia Universidad Católica de Chile
W. Rhode - TU Dortmund University
M. Ribo - Universitat de Barcelona
C. Ricci - University of Geneva
T. Richtler - University of Concepción
J. Rico - Institute for High Energy Physics
L. Riitano - University of Wisconsin System
V. Rizi - University of L'Aquila
E. Roache - Center for Astrophysics Harvard & Smithsonian
G. Rodriguez Fernandez - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
J. J. Rodriguez-Vazquez - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
P. Romano - Brera Astronomical Observatory
G. Romeo - Osservatorio Astrofisico di Catania
J. Rosado - Universidad Complutense de Madrid
A. Rosales de Leon - University of Łódź
A. Roy - Hiroshima University
I. Sadeh - Deutsches Elektronen-Synchrotron DESY
L. Saha - Center for Astrophysics Harvard & Smithsonian
T. Saito - The University of Tokyo
M. Sanchez-Conde - Universidad Autónoma de Madrid
P. Sangiorgi - Istituto di Astrofisica Spaziale e Fisica cosmica di Palermo
H. Sano - Gifu University
R. Santos-Lima - Universidade de São Paulo
V. Sapienza - Osservatorio Astronomico di Palermo
S. Sarkar - University of Oxford
F. G. Saturni - Astronomical Observatory of Rome
A. Scherer - Universidad de Santiago de Chile
F. Schiavone - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
P. Schipani - Astronomical Observatory of Capodimonte
P. Schovanek - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
F. Schussler - Université Paris-Saclay
M. Seglar Arroyo - Institute for High Energy Physics
O. Sergijenko - National Academy of Sciences of Ukraine
H. Siejkowski - Akademickie Centrum Komputerowe Cyfronet AGH
A. Simongini - University of Rome Tor Vergata
V. Sliusar - University of Geneva
A. Slowikowska - Nicolaus Copernicus University
I. Sofia - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
H. Sol - Université Paris Sciences et Lettres
S. Spinello - Osservatorio Astrofisico di Catania
A. Stamerra - Astronomical Observatory of Rome
S. Stanic - University of Nova Gorica
T. Starecki - Warsaw University of Technology
R. Starling - University of Leicester
L. Stawarz - Jagiellonian University
T. Stolarczyk - Université Paris-Saclay
Y. Suda - Hiroshima University
A. Sunny - University of Rome Tor Vergata
T. Suomijarvi - Université Paris-Saclay
R. Takeishi - The University of Tokyo
S. J. Tanaka - Aoyama Gakuin University
F. Tavecchio - Brera Astronomical Observatory
T. Tavernier - FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
Y. Terada - Saitama University
M. Teshima - Max Planck Institute for Physics
V. Testa - Astronomical Observatory of Rome
W. W. Tian - Sun Yat-sen University
Y. Tian - Deutsches Elektronen-Synchrotron DESY
L. Tibaldo - Université de Toulouse
O. Tibolla - Durham University
S. J. Tingay - Curtin University
C. J. Todero Peixoto - Universidade de São Paulo
F. Tombesi - University of Rome Tor Vergata
D. Tonev - Institute for Nuclear Research and Nuclear Energy
F. Torradeflot - Port d'Informació Científica
D. F. Torres - Institute of Space Sciences
N. Tothill - Western Sydney University
G. Tovmassian - Universidad Nacional Autónoma de México
G. Tripodo - University of Palermo
A. Trois - Osservatorio Astronomico di Cagliari
A. Tsiahina - Université de Toulouse
A. Tutone - Istituto di Astrofisica Spaziale e Fisica cosmica di Palermo
L. Vaclavek - Palacký University Olomouc
M. Vacula - Palacký University Olomouc
C. van Eldik - Friedrich-Alexander-Universität Erlangen-Nürnberg
J. Vandenbroucke - University of Wisconsin System
V. Vassiliev - Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
M. Vazquez Acosta - Universidad de La Laguna
M. Vecchi - University of Groningen
S. Vercellone - Brera Astronomical Observatory
S. D. Vergani - Université Paris Sciences et Lettres
I. Viale - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
A. Viana - Universidade de São Paulo
A. Vigliano - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
J. Vignatti - Federico Santa María Technical University
C. F. Vigorito - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
J. Villanueva - University of Valparaíso
E. Visentin - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
V. Voitsekhovskyi - University of Amsterdam
S. Vorobiov - University of Nova Gorica
I. Vovk - The University of Tokyo
T. Vuillaume - Université Savoie Mont Blanc
R. Walter - University of Geneva
M. Wechakama - National Astronomical Research Institute of Thailand
M. White - The University of Adelaide
A. Wierzcholska - Institute of Nuclear Physics, Polish Academy of Sciences
M. Will - CTA Observatory
F. Wohlleben - Max Planck Institute for Nuclear Physics
A. Wolter - Brera Astronomical Observatory
F. Xotta - University of Nova Gorica
T. Yamamoto - Konan University
R. Yamazaki - Aoyama Gakuin University
T. Yoshikoshi - The University of Tokyo
M. Zacharias - Heidelberg University
G. Zaharijas - University of Nova Gorica
R. Zanmar Sanchez - Astronomical Observatory of Capodimonte
D. Zavrtanik - University of Nova Gorica
M. Zavrtanik - University of Nova Gorica
A. Zech - Université Paris Sciences et Lettres
V. I. Zhdanov - Taras Shevchenko National University of Kyiv
M. Zivec - University of Nova Gorica
J. Zuriaga-Puig - Universidad Autónoma de Madrid
A. Colombo - National Institute for Astrophysics
CTAO Consortium
出版者: IOP Publishing Ltd
總頁數: 26
補助款備註: Max Planck Society State Secretariat for Education, Research and Innovation (SERI) Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq); Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ) U.S. Department of Energy; United States Department of Energy (DOE) Faculty of Electrical Engineering and Computing, Croatia ANR, Regional Council Ile de France; Agence Nationale de la Recherche (ANR); Association Nationale de la Recherche et de la Technologie (ANRT) Department of Atomic Energy, Department of Science and Technology, India ESFRI-2017-IAC-12; ESFRI-2020-01-IAC-12 / "Programa Operativo de Crecimiento Inteligente" FEDER INAF; Istituto Nazionale Astrofisica (INAF) Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)
學術資源類型: 期刊文章
出版日期: 10/06/2026
出版資訊: The Astrophysical journal, 卷.1004(1), 頁.46
語言: 英語

Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

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