Target of Opportunity observations of flaring blazars with H.E.S.S.

H.E.S.S. Collaboration

Target of Opportunity observations of flaring blazars with H.E.S.S.

H.E.S.S. Collaboration

Astroparticule and Cosmol APC
LUTH - Laboratoire de l'Univers et de ses Theories
North-West University
Sorbonne Université
Landessternwarte Heidelberg
Dublin Institute for Advanced Studies
Max-Planck-Institut für Kernphysik
Yerevan State University
Université Paris-Saclay
University of Groningen
University of Namibia
Universität Hamburg
c/o DESY
Jagiellonian University
University of the Free State
University of Potsdam
Linnaeus University, Växjö
University of the Witwatersrand, Johannesburg
Humboldt-Universität zu Berlin
University of Tübingen
University of Oxford
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
University of Warsaw
Université Savoie Mont Blanc
Institute for Nuclear Physics
UMR 5797
University of Adelaide
Laboratoire Univers et Particules de Montpellier
Aix-Marseille Université
Ip Paris
University of Innsbruck
Nicolaus Copernicus University
Rikkyo University
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
University of Leicester
University of Amsterdam
Yerevan Physics Institute
Konan University
University of Tokyo
Riken

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

1 Citation (Scopus)

Résumé

Blazars are the most common class of TeV extragalactic emitters. In the framework of the AGN unified model, they are understood as AGNs with a relativistic jet pointing close the line of sight. They are characterized by extreme variability, observed to be as fast as minutes. These flares are usually observed at multiple wavelengths and their study require fast reaction and coordination among multiwavelength observatories. An important part of blazars observations with the H.E.S.S. array of Cherenkov telescopes is thus in the form of Target of Opportunity (ToO) observations. In this contribution the H.E.S.S. blazar ToO program is presented, with a focus on recent results.

langue originale	Anglais
Numéro d'article	924
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{156d06354b6f4f578f6fd11bb1120bbb,

title = "Target of Opportunity observations of flaring blazars with H.E.S.S.",

abstract = "Blazars are the most common class of TeV extragalactic emitters. In the framework of the AGN unified model, they are understood as AGNs with a relativistic jet pointing close the line of sight. They are characterized by extreme variability, observed to be as fast as minutes. These flares are usually observed at multiple wavelengths and their study require fast reaction and coordination among multiwavelength observatories. An important part of blazars observations with the H.E.S.S. array of Cherenkov telescopes is thus in the form of Target of Opportunity (ToO) observations. In this contribution the H.E.S.S. blazar ToO program is presented, with a focus on recent results.",

author = "\{H.E.S.S. Collaboration\} and M. Cerruti and C. Boisson and M. B{\"o}ttcher and O. Chibueze and I. Davids and A. Dmytriiev and G. Grolleron and F. Jankowsky and Lenain, \{J. P.\} and A. Luashvili and M. Zacharias and F. Aharonian and \{Ait Benkhali\}, F. and A. Alkan and J. Aschersleben and H. Ashkar and M. Backes and A. Baktash and \{Barbosa Martins\}, V. and A. Barnacka and J. Barnard and R. Batzofin and Y. Becherini and G. Beck and D. Berge and K. Bernl{\"o}hr and B. Bi and J. Bolmont and \{de Bony de Lavergne\}, M. and J. Borowska and M. Bouyahiaoui and F. Bradascio and M. Breuhaus and R. Brose and A. Brown and F. Brun and B. Bruno and T. Bulik and C. Burger-Scheidlin and T. Bylund and F. Cangemi and S. Caroff and S. Casanova and R. Cecil and J. Celic and P. Chambery and T. Chand and S. Chandra and A. Chen and S. Fegan",

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 - Target of Opportunity observations of flaring blazars with H.E.S.S.

AU - H.E.S.S. Collaboration

AU - Cerruti, M.

AU - Boisson, C.

AU - Böttcher, M.

AU - Chibueze, O.

AU - Davids, I.

AU - Dmytriiev, A.

AU - Grolleron, G.

AU - Jankowsky, F.

AU - Lenain, J. P.

AU - Luashvili, A.

AU - Zacharias, M.

AU - Aharonian, F.

AU - Ait Benkhali, F.

AU - Alkan, A.

AU - Aschersleben, J.

AU - Ashkar, H.

AU - Backes, M.

AU - Baktash, A.

AU - Barbosa Martins, V.

AU - Barnacka, A.

AU - Barnard, J.

AU - Batzofin, R.

AU - Becherini, Y.

AU - Beck, G.

AU - Berge, D.

AU - Bernlöhr, K.

AU - Bi, B.

AU - Bolmont, J.

AU - de Bony de Lavergne, M.

AU - Borowska, J.

AU - Bouyahiaoui, M.

AU - Bradascio, F.

AU - Breuhaus, M.

AU - Brose, R.

AU - Brown, A.

AU - Brun, F.

AU - Bruno, B.

AU - Bulik, T.

AU - Burger-Scheidlin, C.

AU - Bylund, T.

AU - Cangemi, F.

AU - Caroff, S.

AU - Casanova, S.

AU - Cecil, R.

AU - Celic, J.

AU - Chambery, P.

AU - Chand, T.

AU - Chandra, S.

AU - Chen, A.

AU - Fegan, S.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - Blazars are the most common class of TeV extragalactic emitters. In the framework of the AGN unified model, they are understood as AGNs with a relativistic jet pointing close the line of sight. They are characterized by extreme variability, observed to be as fast as minutes. These flares are usually observed at multiple wavelengths and their study require fast reaction and coordination among multiwavelength observatories. An important part of blazars observations with the H.E.S.S. array of Cherenkov telescopes is thus in the form of Target of Opportunity (ToO) observations. In this contribution the H.E.S.S. blazar ToO program is presented, with a focus on recent results.

AB - Blazars are the most common class of TeV extragalactic emitters. In the framework of the AGN unified model, they are understood as AGNs with a relativistic jet pointing close the line of sight. They are characterized by extreme variability, observed to be as fast as minutes. These flares are usually observed at multiple wavelengths and their study require fast reaction and coordination among multiwavelength observatories. An important part of blazars observations with the H.E.S.S. array of Cherenkov telescopes is thus in the form of Target of Opportunity (ToO) observations. In this contribution the H.E.S.S. blazar ToO program is presented, with a focus on recent results.

M3 - Conference article

AN - SCOPUS:85185581251

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 924

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Target of Opportunity observations of flaring blazars with H.E.S.S.

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