Evidence for γ-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations (vol 662, artn A65, 2022)

被引：1

作者：

Aharonian, F. ^{[1
,2
,3
]}

Benkhali, F. Ait ^{[4
]}

Anguner, E. O. ^{[5
]}

Ashkar, H. ^{[6
]}

Backes, M. ^{[7
,8
]}

Martins, V. Barbosa ^{[9
]}

Batzofin, R. ^{[10
]}

Becherini, Y. ^{[11
,12
]}

Berge, D. ^{[9
]}

Bernloehr, K. ^{[2
]}

Boettcher, M. ^{[8
]}

Boisson, C. ^{[13
]}

Bolmont, J. ^{[14
]}

de Lavergne, M. de Bony ^{[15
]}

Breuhaus, M. ^{[2
]}

Brose, R. ^{[1
]}

Brun, F. ^{[16
]}

Bulik, T. ^{[17
]}

Bylund, T. ^{[12
]}

Cangemi, F. ^{[14
]}

Caroff, S. ^{[14
]}

Casanova, S. ^{[18
]}

Cerruti, M. ^{[11
]}

Chand, T. ^{[8
]}

Chen, A. ^{[10
]}

Chibueze, O. ^{[8
]}

Cotter, G. ^{[19
]}

Cristofari, P. ^{[13
]}

Mbarubucyeye, J. Damascene ^{[9
]}

Devin, J. ^{[20
]}

Djannati-Atai, A. ^{[11
]}

Dmytriiev, A. ^{[13
]}

Egberts, K. ^{[21
]}

Einecke, S. ^{[22
]}

Ernenwein, J. -P. ^{[5
]}

Feijen, K. ^{[22
]}

Fiasson, A. ^{[15
]}

de Clairfontaine, G. Fichet ^{[13
]}

Fontaine, G. ^{[6
]}

Funk, S. ^{[23
]}

Gabici, S. ^{[11
]}

Gallant, Y. A. ^{[24
]}

Ghafourizadeh, S. ^{[4
]}

Giavitto, G. ^{[8
]}

Giunti, L. ^{[11
,16
]}

Glawion, D. ^{[23
]}

Glicenstein, J. F. ^{[16
]}

Grondin, M. -H. ^{[20
]}

Horbe, M. ^{[19
]}

Hofmann, W. ^{[2
]}

机构：

[1] Dublin Inst Adv Studies, 31 Fitzwilliam Pl, Dublin 2, Ireland

[2] Max Planck Inst Kernphys, POB 103980, D-69029 Heidelberg, Germany

[3] RAU, High Energy Astrophys Lab, 123 Hovsep Emin St, Yerevan 0051, Armenia

[4] Heidelberg Univ, Landessternwarte, Konigstuhl, D-69117 Heidelberg, Germany

[5] Aix Marseille Univ, CNRS, CPPM, IN2P3, Marseille, France

[6] Inst Polytech Paris, CNRS, Lab Leprince Ringuet, Ecole Polytech, F-91128 Palaiseau, France

[7] Univ Namibia, Dept Phys, Private Bag 13301, Windhoek 10005, Namibia

[8] Northwest Univ, Ctr Space Res, ZA-2520 Potchefstroom, South Africa

[9] DESY, D-15738 Zeuthen, Germany

[10] Univ Witwatersrand, Sch Phys, 1 Jan Smuts Ave, ZA-2050 Johannesburg, South Africa

[11] Univ Paris, CNRS, Astroparticule & Cosmol, F-75013 Paris, France

[12] Linnaeus Univ, Dept Phys & Elect Engn, S-35195 Vaxjo, Sweden

[13] Univ Paris, Univ PSL, Observ Paris, Lab Univers & Theories,CNRS, F-92190 Meudon, France

[14] Univ Paris Diderot, Sorbonne Univ, Sorbonne Paris Cite,CNRS, Lab Phys Nucl & Hautes Energies,IN2P3,LPNHE, 4 Pl Jussieu, F-75252 Paris, France

[15] Univ Savoie Mt Blanc, Lab Annecy Phys Particules IN2P3, CNRS, F-74000 Annecy, France

[16] Univ Paris Saclay, IRFU, CEA, F-91191 Gif Sur Yvette, France

[17] Univ Warsaw, Astron Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland

[18] Inst Fizyki Jadrowej PAN, Ul Radzikowskiego 152, PL-31342 Krakow, Poland

[19] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

[20] Univ Bordeaux, CNRS, LP2I Bordeaux, UMR 5797, F-33170 Bordeaux, France

[21] Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany

[22] Univ Adelaide, Sch Phys Sci, Adelaide, SA 5005, Australia

[23] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany

[24] Univ Montpellier, Lab Univers & Particules Montpellier, CNRS, IN2P3, CC 72,Pl Eugene Bataillon, F-34095 Montpellier 5, France

[25] Leopold Franzens Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria

[26] Univ Hamburg, Inst Expt Phys, Luruper Chaussee 149, D-22761 Hamburg, Germany

[27] Uniwersytet Jagiellonski, Obserwatorium Astron, Ul Orla 171, PL-30244 Krakow, Poland

[28] Nicolaus Copernicus Univ, Inst Astron, Fac Phys Astron & Informat, Grudziadzka 5, PL-87100 Torun, Poland

[29] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland

[30] Univ Tubingen, Inst Astron & Astrophys, Sand 1, D-72076 Tubingen, Germany

[31] Humboldt Univ, Inst Phys, Newtonstr 15, D-12489 Berlin, Germany

[32] Univ Free State, Dept Phys, POB 339, ZA-9300 Bloemfontein, South Africa

[33] Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England

[34] Univ Amsterdam, Astron Inst Anton Pannekoek, GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[35] Yerevan Phys Inst, 2 Alikhanian Bros St, Yerevan 375036, Armenia

[36] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Univ Tokyo Inst Adv Study UTIAS, 5-1-5 Kashiwa No Ha, Kashiwa, Chiba 2778583, Japan

[37] Konan Univ, Dept Phys, 8-9-1 Okamoto, Kobe, Hyogo 6588501, Japan

[38] Rikkyo Univ, Dept Phys, 3-34-1 Nishi Ikebukuro,Toshima Ku, Tokyo 1718501, Japan

来源：

ASTRONOMY & ASTROPHYSICS | 2024年 / 683卷

关键词：

gamma rays: general; supernovae: individual: Kepler; ISM: supernova remnants; radiation mechanisms: non-thermal; errata; addenda;

D O I：

10.1051/0004-6361/202348902e

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页数：2

共 34 条

[1] Erratum: Evidence for γ-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations (Astronomy and Astrophysics (2022) 662 (A65) DOI: 10.1051/0004-6361/202243096)
Astronomy and Astrophysics, 1600, 683
[2] Evidence for γ-ray emission from the remnant of Kepleras supernova based on deep H.E.S.S. observations
Aharonian, F.
Benkhali, F.Ait
Angüner, E.O.
Ashkar, H.
Backes, M.
Martins, V. Barbosa
Batzofin, R.
Becherini, Y.
Berge, D.
Bernlöhr, K.
Böttcher, M.
Boisson, C.
Bolmont, J.
Lavergne, M. De Bony De
Breuhaus, M.
Brose, R.
Brun, F.
Bulik, T.
Bylund, T.
Cangemi, F.
Caroff, S.
Casanova, S.
Cerruti, M.
Chand, T.
Chen, A.
Chibueze, O.
Cotter, G.
Cristofari, P.
Mbarubucyeye, J. Damascene
Devin, J.
Djannati-Ataï, A.
Dmytriiev, A.
Egberts, K.
Einecke, S.
Ernenwein, J.-P.
Feijen, K.
Fiasson, A.
Clairfontaine, G. Fichet De
Fontaine, G.
Funk, S.
Gabici, S.
Gallant, Y.A.
Ghafourizadeh, S.
Giavitto, G.
Giunti, L.
Glawion, D.
Glicenstein, J.F.
Grondin, M.-H.
Hörbe, M.
Hofmann, W.
Astronomy and Astrophysics, 2022, 662
[3] Evidence for γ-ray emission from the remnant of Kepler's supernova based on deep HESS observations
Aharonian, F.
Benkhali, F. Ait
Anguner, E. O.
Ashkar, H.
Backes, M.
Martins, V. Barbosa
Batzofin, R.
Becherini, Y.
Berge, D.
Bernloehr, K.
Bottcher, M.
Boisson, C.
Bolmont, J.
de Lavergne, M. de Bony
Breuhaus, M.
Brose, R.
Brun, F.
Bulik, T.
Bylund, T.
Cangemi, F.
Caroff, S.
Casanova, S.
Cerruti, M.
Chand, T.
Chen, A.
Chibueze, O.
Cotter, G.
Cristofari, P.
Mbarubucyeye, J. Damascene
Devin, J.
Djannati-Atai, A.
Dmytriiev, A.
Egberts, K.
Einecke, S.
Ernenwein, J-P
Feijen, K.
Fiasson, A.
de Clairfontaine, G. Fichet
Fontaine, G.
Funk, S.
Gabici, S.
Gallant, Y. A.
Ghafourizadeh, S.
Giavitto, G.
Giunti, L.
Glawion, D.
Glicenstein, J. F.
Grondin, M-H
Horbe, M.
Hofmann, W.
ASTRONOMY & ASTROPHYSICS, 2022, 662
[4] Gamma-ray emission expected from Kepler's supernova remnant
Berezhko, E. G.
Ksenofontov, L. T.
Voelk, H. J.
ASTRONOMY & ASTROPHYSICS, 2006, 452 (01): : 217 - 221
[5] Gamma-ray emission expected from Kepler's supernova remnant
Berezhko, E.G.
Ksenofontov, L.T.
Völk, H.J.
Astronomy and Astrophysics, 1600, 452 (01): : 217 - 221
[6] A search for new supernova remnant shells in the Galactic plane with H.E.S.S.
1600, EDP Sciences (612):
[7] NONTHERMAL EMISSION OF SUPERNOVA REMNANT SN 1006 REVISITED: THEORETICAL MODEL AND THE H.E.S.S. RESULTS
Berezhko, E. G.
Ksenofontov, L. T.
Voelk, H. J.
ASTROPHYSICAL JOURNAL, 2012, 759 (01):
[8] The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT
1600, EDP Sciences (612):
[9] Simulated X-ray emission for a runaway model of Kepler's supernova remnant
Velazquez, Pablo F.
Vigh, Carlos D.
Reynoso, Estela M.
Gomez, Daniel O.
Schneiter, E. Matias
ASTROPHYSICAL JOURNAL, 2006, 649 (02): : 779 - 787
[10] X-RAY EMISSION FROM STRONGLY ASYMMETRIC CIRCUMSTELLAR MATERIAL IN THE REMNANT OF KEPLER'S SUPERNOVA
Burkey, Mary T.
Reynolds, Stephen P.
Borkowski, Kazimierz J.
Blondin, John M.
ASTROPHYSICAL JOURNAL, 2013, 764 (01):

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