HESS observations of γ-ray bursts in 2003-2007

F. Aharonian; A. G. Akhperjanian; U. Barres De Almeida; A. R. Bazer-Bachi; B. Beheral; W. Benbow; K. Bernlöhr; C. Boisson; A. Bochow; V. Borrel; I. Braun; E. Brion; J. Brucker; P. Brun; R. Bühler; T. Bulik; I. Büsching; T. Boutelier; S. Carrigan; P. M. Chadwick; A. Charbonnier; R. C.G. Chaves; A. Cheesebrough; L. M. Chounet; A. C. Clapson; G. Coignet; M. Dalton; B. Degrange; C. Deil; H. J. Dickinson; A. Djannati-Ataï; W. Domainko; L. O.C. Drury; F. Dubois; G. Dubus; J. Dyks; M. Dyrda; K. Egberts; D. Emmanoulopoulos; P. Espigat; C. Farnier; F. Feinstein; A. Fiasson; A. Förster; G. Fontaine; M. Füßling; S. Gabici; Y. A. Gallant; L. Gérard; B. Giebels; J. F. Glicenstein; B. Glück; P. Goret; C. Hadjichristidis; D. Hauser; M. Hauser; S. Heinz; G. Heinzelmann; G. Henri; G. Hermann; J. A. Hinton; A. Hoffmann; W. Hofmann; M. Holleran; S. Hoppe; D. Horns; A. Jacholkowska; O. C. De Jager; I. Jung; K. Katarzyński; S. Kaufmann; E. Kendziorra; M. Kerschhaggl; D. Khangulyan; B. Khélifi; D. Keogh; Nu Komin; K. Kosack; G. Lamanna; J. P. Lenain; T. Lohse; V. Marandon; J. M. Martin; O. Martineau-Huynh; A. Marcowith; D. Maurin; T. J.L. McComb; M. C. Medina; R. Moderski; E. Moulin; M. Naumann-Godo; M. De Naurois; D. Nedbal; D. Nekrassov; J. Niemiec; S. J. Nolan; S. Ohm; J. F. Olive; E. De Oña Wilhelmi

doi:10.1051/0004-6361:200811072

HESS observations of γ-ray bursts in 2003-2007

F. Aharonian
, A. G. Akhperjanian
, U. Barres De Almeida
, A. R. Bazer-Bachi
, B. Beheral
, W. Benbow
, K. Bernlöhr
, C. Boisson
, A. Bochow
, V. Borrel
, I. Braun
, E. Brion
, J. Brucker
, P. Brun
, R. Bühler
, T. Bulik
, I. Büsching
, T. Boutelier
, S. Carrigan
, P. M. Chadwick

A. Charbonnier, R. C.G. Chaves, A. Cheesebrough, L. M. Chounet, A. C. Clapson, G. Coignet, M. Dalton, B. Degrange, C. Deil, H. J. Dickinson, A. Djannati-Ataï, W. Domainko, L. O.C. Drury, F. Dubois, G. Dubus, J. Dyks, M. Dyrda, K. Egberts, D. Emmanoulopoulos, P. Espigat, C. Farnier, F. Feinstein, A. Fiasson, A. Förster, G. Fontaine, M. Füßling, S. Gabici, Y. A. Gallant, L. Gérard, B. Giebels, J. F. Glicenstein, B. Glück, P. Goret, C. Hadjichristidis, D. Hauser, M. Hauser, S. Heinz, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, A. Hoffmann, W. Hofmann, M. Holleran, S. Hoppe, D. Horns, A. Jacholkowska, O. C. De Jager, I. Jung, K. Katarzyński, S. Kaufmann, E. Kendziorra, M. Kerschhaggl, D. Khangulyan, B. Khélifi, D. Keogh, Nu Komin, K. Kosack, G. Lamanna, J. P. Lenain, T. Lohse, V. Marandon, J. M. Martin, O. Martineau-Huynh, A. Marcowith, D. Maurin, T. J.L. McComb, M. C. Medina, R. Moderski, E. Moulin, M. Naumann-Godo, M. De Naurois, D. Nedbal, D. Nekrassov, J. Niemiec, S. J. Nolan, S. Ohm, J. F. Olive, E. De Oña Wilhelmi

Max-Planck-Institut für Kernphysik
Dublin Institute for Advanced Studies
Yerevan Physics Institute
Department of Physics
Durham University
CNRS
Landessternwarte Heidelberg
Institut für Physik
Humboldt-Universität zu Berlin
LUTH - Laboratoire de l'Univers et de ses Theories
Universite Paris-Saclay
Physikalisches Institut
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
Unit for Space Physics
North-West University
LPNHE
Universités Paris VI and VII
Université Paris-Sud
Astroparticule and Cosmol APC
Institute for Nuclear Physics
Laboratoire Univers et Particules de Montpellier
Institut für Experimentalphysik
Universität Hamburg
School of Physics and Astronomy
University of Leeds
Institut für Astronomie und Astrophysik
University of Tübingen
Toruń Centre for Astronomy
Nicolaus Copernicus University
Charles University
European Associated Laboratory for Gamma-Ray Astronomy
CNRS and MPG

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

59 Citations (Scopus)

Résumé

Aims. Very-high-energy (VHE; ≳100 GeV) γ-rays are expected from γ-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the energetics and properties of GRBs. Methods. GRBs have been one of the prime targets for the HESS experiment, which makes use of four Imaging Atmospheric Cherenkov Telescopes (IACTs) to detect VHE γ-rays. Dedicated observations of 32 GRB positions were made in the years 2003-2007 and a search for VHE γ-ray counterparts of these GRBs was made. Depending on the visibility and observing conditions, the observations mostly start minutes to hours after the burst and typically last two hours.Results. Results from observations of 22 GRB positions are presented. Evidence of a VHE signal was found neither in observations of any individual GRBs nor from stacking data from subsets of GRBs with higher expected VHE flux according to a model-independent ranking scheme. Upper limits for the VHE γ-ray flux from the GRB positions were derived. For those GRBs with measured redshifts, differential upper limits at the energy threshold after correcting for absorption due to extra-galactic background light are also presented.

langue originale	Anglais
Pages (de - à)	505-512
Nombre de pages	8
journal	Astronomy and Astrophysics
Volume	495
Numéro de publication	2
Les DOIs	https://doi.org/10.1051/0004-6361:200811072
état	Publié - 1 févr. 2009
Modification externe	Oui

Accès au document

10.1051/0004-6361:200811072

Contient cette citation

Aharonian, F., Akhperjanian, A. G., De Almeida, U. B., Bazer-Bachi, A. R., Beheral, B., Benbow, W., Bernlöhr, K., Boisson, C., Bochow, A., Borrel, V., Braun, I., Brion, E., Brucker, J., Brun, P., Bühler, R., Bulik, T., Büsching, I., Boutelier, T., Carrigan, S., ... De Oña Wilhelmi, E. (2009). HESS observations of γ-ray bursts in 2003-2007. Astronomy and Astrophysics, 495(2), 505-512. https://doi.org/10.1051/0004-6361:200811072

@article{f014cb2406d145b9ad9f58c5afdc8fdd,

title = "HESS observations of γ-ray bursts in 2003-2007",

abstract = "Aims. Very-high-energy (VHE; ≳100 GeV) γ-rays are expected from γ-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the energetics and properties of GRBs. Methods. GRBs have been one of the prime targets for the HESS experiment, which makes use of four Imaging Atmospheric Cherenkov Telescopes (IACTs) to detect VHE γ-rays. Dedicated observations of 32 GRB positions were made in the years 2003-2007 and a search for VHE γ-ray counterparts of these GRBs was made. Depending on the visibility and observing conditions, the observations mostly start minutes to hours after the burst and typically last two hours.Results. Results from observations of 22 GRB positions are presented. Evidence of a VHE signal was found neither in observations of any individual GRBs nor from stacking data from subsets of GRBs with higher expected VHE flux according to a model-independent ranking scheme. Upper limits for the VHE γ-ray flux from the GRB positions were derived. For those GRBs with measured redshifts, differential upper limits at the energy threshold after correcting for absorption due to extra-galactic background light are also presented.",

keywords = "Gamma rays: bursts, Gamma rays: observations",

author = "F. Aharonian and Akhperjanian, \{A. G.\} and \{De Almeida\}, \{U. Barres\} and Bazer-Bachi, \{A. R.\} and B. Beheral and W. Benbow and K. Bernl{\"o}hr and C. Boisson and A. Bochow and V. Borrel and I. Braun and E. Brion and J. Brucker and P. Brun and R. B{\"u}hler and T. Bulik and I. B{\"u}sching and T. Boutelier and S. Carrigan and Chadwick, \{P. M.\} and A. Charbonnier and Chaves, \{R. C.G.\} and A. Cheesebrough and Chounet, \{L. M.\} and Clapson, \{A. C.\} and G. Coignet and M. Dalton and B. Degrange and C. Deil and Dickinson, \{H. J.\} and A. Djannati-Ata{\"i} and W. Domainko and Drury, \{L. O.C.\} and F. Dubois and G. Dubus and J. Dyks and M. Dyrda and K. Egberts and D. Emmanoulopoulos and P. Espigat and C. Farnier and F. Feinstein and A. Fiasson and A. F{\"o}rster and G. Fontaine and M. F{\"u}{\ss}ling and S. Gabici and Gallant, \{Y. A.\} and L. G{\'e}rard and B. Giebels and Glicenstein, \{J. F.\} and B. Gl{\"u}ck and P. Goret and C. Hadjichristidis and D. Hauser and M. Hauser and S. Heinz and G. Heinzelmann and G. Henri and G. Hermann and Hinton, \{J. A.\} and A. Hoffmann and W. Hofmann and M. Holleran and S. Hoppe and D. Horns and A. Jacholkowska and \{De Jager\}, \{O. C.\} and I. Jung and K. Katarzy{\'n}ski and S. Kaufmann and E. Kendziorra and M. Kerschhaggl and D. Khangulyan and B. Kh{\'e}lifi and D. Keogh and Nu Komin and K. Kosack and G. Lamanna and Lenain, \{J. P.\} and T. Lohse and V. Marandon and Martin, \{J. M.\} and O. Martineau-Huynh and A. Marcowith and D. Maurin and McComb, \{T. J.L.\} and Medina, \{M. C.\} and R. Moderski and E. Moulin and M. Naumann-Godo and \{De Naurois\}, M. and D. Nedbal and D. Nekrassov and J. Niemiec and Nolan, \{S. J.\} and S. Ohm and Olive, \{J. F.\} and \{De O{\~n}a Wilhelmi\}, E.",

year = "2009",

month = feb,

day = "1",

doi = "10.1051/0004-6361:200811072",

language = "English",

volume = "495",

pages = "505--512",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "2",

}

Aharonian, F, Akhperjanian, AG, De Almeida, UB, Bazer-Bachi, AR, Beheral, B, Benbow, W, Bernlöhr, K, Boisson, C, Bochow, A, Borrel, V, Braun, I, Brion, E, Brucker, J, Brun, P, Bühler, R, Bulik, T, Büsching, I, Boutelier, T, Carrigan, S, Chadwick, PM, Charbonnier, A, Chaves, RCG, Cheesebrough, A, Chounet, LM, Clapson, AC, Coignet, G, Dalton, M, Degrange, B, Deil, C, Dickinson, HJ, Djannati-Ataï, A, Domainko, W, Drury, LOC, Dubois, F, Dubus, G, Dyks, J, Dyrda, M, Egberts, K, Emmanoulopoulos, D, Espigat, P, Farnier, C, Feinstein, F, Fiasson, A, Förster, A, Fontaine, G, Füßling, M, Gabici, S, Gallant, YA, Gérard, L, Giebels, B, Glicenstein, JF, Glück, B, Goret, P, Hadjichristidis, C, Hauser, D, Hauser, M, Heinz, S, Heinzelmann, G, Henri, G, Hermann, G, Hinton, JA, Hoffmann, A, Hofmann, W, Holleran, M, Hoppe, S, Horns, D, Jacholkowska, A, De Jager, OC, Jung, I, Katarzyński, K, Kaufmann, S, Kendziorra, E, Kerschhaggl, M, Khangulyan, D, Khélifi, B, Keogh, D, Komin, N, Kosack, K, Lamanna, G, Lenain, JP, Lohse, T, Marandon, V, Martin, JM, Martineau-Huynh, O, Marcowith, A, Maurin, D, McComb, TJL, Medina, MC, Moderski, R, Moulin, E, Naumann-Godo, M, De Naurois, M, Nedbal, D, Nekrassov, D, Niemiec, J, Nolan, SJ, Ohm, S, Olive, JF & De Oña Wilhelmi, E 2009, 'HESS observations of γ-ray bursts in 2003-2007', Astronomy and Astrophysics, VOL. 495, Numéro 2, p. 505-512. https://doi.org/10.1051/0004-6361:200811072

TY - JOUR

T1 - HESS observations of γ-ray bursts in 2003-2007

AU - Aharonian, F.

AU - Akhperjanian, A. G.

AU - De Almeida, U. Barres

AU - Bazer-Bachi, A. R.

AU - Beheral, B.

AU - Benbow, W.

AU - Bernlöhr, K.

AU - Boisson, C.

AU - Bochow, A.

AU - Borrel, V.

AU - Braun, I.

AU - Brion, E.

AU - Brucker, J.

AU - Brun, P.

AU - Bühler, R.

AU - Bulik, T.

AU - Büsching, I.

AU - Boutelier, T.

AU - Carrigan, S.

AU - Chadwick, P. M.

AU - Charbonnier, A.

AU - Chaves, R. C.G.

AU - Cheesebrough, A.

AU - Chounet, L. M.

AU - Clapson, A. C.

AU - Coignet, G.

AU - Dalton, M.

AU - Degrange, B.

AU - Deil, C.

AU - Dickinson, H. J.

AU - Djannati-Ataï, A.

AU - Domainko, W.

AU - Drury, L. O.C.

AU - Dubois, F.

AU - Dubus, G.

AU - Dyks, J.

AU - Dyrda, M.

AU - Egberts, K.

AU - Emmanoulopoulos, D.

AU - Espigat, P.

AU - Farnier, C.

AU - Feinstein, F.

AU - Fiasson, A.

AU - Förster, A.

AU - Fontaine, G.

AU - Füßling, M.

AU - Gabici, S.

AU - Gallant, Y. A.

AU - Gérard, L.

AU - Giebels, B.

AU - Glicenstein, J. F.

AU - Glück, B.

AU - Goret, P.

AU - Hadjichristidis, C.

AU - Hauser, D.

AU - Hauser, M.

AU - Heinz, S.

AU - Heinzelmann, G.

AU - Henri, G.

AU - Hermann, G.

AU - Hinton, J. A.

AU - Hoffmann, A.

AU - Hofmann, W.

AU - Holleran, M.

AU - Hoppe, S.

AU - Horns, D.

AU - Jacholkowska, A.

AU - De Jager, O. C.

AU - Jung, I.

AU - Katarzyński, K.

AU - Kaufmann, S.

AU - Kendziorra, E.

AU - Kerschhaggl, M.

AU - Khangulyan, D.

AU - Khélifi, B.

AU - Keogh, D.

AU - Komin, Nu

AU - Kosack, K.

AU - Lamanna, G.

AU - Lenain, J. P.

AU - Lohse, T.

AU - Marandon, V.

AU - Martin, J. M.

AU - Martineau-Huynh, O.

AU - Marcowith, A.

AU - Maurin, D.

AU - McComb, T. J.L.

AU - Medina, M. C.

AU - Moderski, R.

AU - Moulin, E.

AU - Naumann-Godo, M.

AU - De Naurois, M.

AU - Nedbal, D.

AU - Nekrassov, D.

AU - Niemiec, J.

AU - Nolan, S. J.

AU - Ohm, S.

AU - Olive, J. F.

AU - De Oña Wilhelmi, E.

PY - 2009/2/1

Y1 - 2009/2/1

N2 - Aims. Very-high-energy (VHE; ≳100 GeV) γ-rays are expected from γ-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the energetics and properties of GRBs. Methods. GRBs have been one of the prime targets for the HESS experiment, which makes use of four Imaging Atmospheric Cherenkov Telescopes (IACTs) to detect VHE γ-rays. Dedicated observations of 32 GRB positions were made in the years 2003-2007 and a search for VHE γ-ray counterparts of these GRBs was made. Depending on the visibility and observing conditions, the observations mostly start minutes to hours after the burst and typically last two hours.Results. Results from observations of 22 GRB positions are presented. Evidence of a VHE signal was found neither in observations of any individual GRBs nor from stacking data from subsets of GRBs with higher expected VHE flux according to a model-independent ranking scheme. Upper limits for the VHE γ-ray flux from the GRB positions were derived. For those GRBs with measured redshifts, differential upper limits at the energy threshold after correcting for absorption due to extra-galactic background light are also presented.

AB - Aims. Very-high-energy (VHE; ≳100 GeV) γ-rays are expected from γ-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the energetics and properties of GRBs. Methods. GRBs have been one of the prime targets for the HESS experiment, which makes use of four Imaging Atmospheric Cherenkov Telescopes (IACTs) to detect VHE γ-rays. Dedicated observations of 32 GRB positions were made in the years 2003-2007 and a search for VHE γ-ray counterparts of these GRBs was made. Depending on the visibility and observing conditions, the observations mostly start minutes to hours after the burst and typically last two hours.Results. Results from observations of 22 GRB positions are presented. Evidence of a VHE signal was found neither in observations of any individual GRBs nor from stacking data from subsets of GRBs with higher expected VHE flux according to a model-independent ranking scheme. Upper limits for the VHE γ-ray flux from the GRB positions were derived. For those GRBs with measured redshifts, differential upper limits at the energy threshold after correcting for absorption due to extra-galactic background light are also presented.

KW - Gamma rays: bursts

KW - Gamma rays: observations

U2 - 10.1051/0004-6361:200811072

DO - 10.1051/0004-6361:200811072

M3 - Article

AN - SCOPUS:61349122604

SN - 0004-6361

VL - 495

SP - 505

EP - 512

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 2

ER -

HESS observations of γ-ray bursts in 2003-2007

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