# Evidence for γ-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations (Corrigendum)

F. Aharonian, F. Ait Benkhali, E. O. Angüner, H. Ashkar, M. Backes, V.

Barbosa Martins, R. Batzofin, Y. Becherini, D. Berge, K. Bernlöhr, et al.

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► To cite this version:

F. Aharonian, F. Ait Benkhali, E. O. Angüner, H. Ashkar, M. Backes, et al. Evidence for γ-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations (Corrigendum). Astronomy & Astrophysics - A&A, 2024, 683, pp.C1. 10.1051/0004-6361/202348902e . insu-04818055

HAL Id: insu-04818055

https://insu.hal.science/insu-04818055v1

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<figure><img src="image_2.png" /></figure>
# Evidence for γ-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations

*(Corrigendum)*

H.E.S.S. Collaboration: F. Aharonian<sup>1,2,3</sup>, F. Ait Benkhali<sup>4</sup>, E. O. Angüner<sup>5</sup>, H. Ashkar<sup>6</sup>, M. Backes<sup>7,8</sup>, V. Barbosa Martins<sup>9</sup>, R. Batzofin<sup>10</sup>, Y. Becherini<sup>11,12</sup>, D. Berge<sup>9</sup>, K. Bernlöhr<sup>2</sup>, M. Böttcher<sup>8</sup>, C. Boisson<sup>13</sup>, J. Bolmont<sup>14</sup>, M. de Bony de Lavergne<sup>15</sup>, M. Breuhaus<sup>2</sup>, R. Brose<sup>1</sup>, F. Brun<sup>16</sup>, T. Bulik<sup>17</sup>, T. Bylund<sup>12</sup>, F. Cangemi<sup>14</sup>, S. Caroff<sup>14</sup>, S. Casanova<sup>18</sup>, M. Cerruti<sup>11</sup>, T. Chand<sup>8</sup>, A. Chen<sup>10</sup>, O. Chibueze<sup>8</sup>, G. Cotter<sup>19</sup>, P. Cristofari<sup>13</sup>, J. Damascene Mbarubucyeye<sup>9</sup>, J. Devin<sup>20</sup>, A. Djannati-Ataï<sup>11</sup>, A. Dmytriiev<sup>13</sup>, K. Egberts<sup>21</sup>, S. Einecke<sup>22</sup>, J.-P. Ernenwein<sup>5</sup>, K. Feijen<sup>22</sup>, A. Fiasson<sup>15</sup>, G. Fichet de Clairfontaine<sup>13</sup>, G. Fontaine<sup>6</sup>, S. Funk<sup>23</sup>, S. Gabici<sup>11</sup>, Y. A. Gallant<sup>24</sup>, S. Ghafourizadeh<sup>4</sup>, G. Giavitto<sup>9</sup>, L. Giunti<sup>11,16</sup>, D. Glawion<sup>23</sup>, J. F. Glicenstein<sup>16</sup>, M.-H. Grondin<sup>20</sup>, M. Hörbe<sup>19</sup>, W. Hofmann<sup>2</sup>, T. L. Holch<sup>9</sup>, M. Holler<sup>25</sup>, D. Horns<sup>26</sup>, Zhiqiu Huang<sup>2</sup>, M. Jamrozy<sup>27</sup>, V. Joshi<sup>23</sup>, I. Jung-Richardt<sup>23</sup>, E. Kasai<sup>7</sup>, K. Katarzyński<sup>28</sup>, U. Katz<sup>23</sup>, B. Khélifi<sup>11</sup>, W. Kluźniak<sup>29</sup>, Nu. Komin<sup>10</sup>, K. Kosack<sup>16</sup>, D. Kostunin<sup>9</sup>, A. Lemière<sup>11</sup>, M. Lemoine-Goumard<sup>20</sup>, J.-P. Lenain<sup>14</sup>, F. Leuschner<sup>30</sup>, T. Lohse<sup>31</sup>, A. Luashvili<sup>13</sup>, I. Lypova<sup>4</sup>, J. Mackey<sup>1</sup>, D. Malyshev<sup>30</sup>, D. Malyshev<sup>23</sup>, V. Marandon<sup>2</sup>, P. Marchegiani<sup>10</sup>, A. Marcowith<sup>24</sup>, G. Martí-Devesa<sup>25</sup>, R. Marx<sup>4</sup>, G. Maurin<sup>15</sup>, P. J. Meintjes<sup>32</sup>, M. Meyer<sup>26</sup>, A. Mitchell<sup>23,2</sup>, R. Moderski<sup>29</sup>, L. Mohrmann<sup>2</sup>, A. Montanari<sup>16</sup>, E. Moulin<sup>16</sup>, J. Muller<sup>6</sup>, K. Nakashima<sup>23</sup>, M. de Naurois<sup>6</sup>, A. Nayerhoda<sup>18</sup>, J. Niemiec<sup>18</sup>, A. Priyana Noel<sup>27</sup>, P. O'Brien<sup>33</sup>, S. Ohm<sup>9</sup>, L. Olivera-Nieto<sup>2</sup>, E. de Ona Wilhelmi<sup>9</sup>, M. Ostrowski<sup>27</sup>, S. Panny<sup>25</sup>, M. Panter<sup>2</sup>, R. D. Parsons<sup>31</sup>, G. Peron<sup>2</sup>, V. Poireau<sup>15</sup>, D. A. Prokhorov<sup>34,*</sup>, G. Pühlhofer<sup>30</sup>, M. Punch<sup>11,12</sup>, A. Quirrenbach<sup>4</sup>, P. Reichherzer<sup>16</sup>, A. Reimer<sup>25</sup>, O. Reimer<sup>25</sup>, M. Renaud<sup>24</sup>, B. Reville<sup>2</sup>, F. Rieger<sup>2</sup>, G. Rowell<sup>22</sup>, B. Rudak<sup>29</sup>, H. Rueda Ricarte<sup>16</sup>, V. Sahakian<sup>35</sup>, S. Sailer<sup>2</sup>, H. Salzmann<sup>30</sup>, D. A. Sanchez<sup>15</sup>, A. Santangelo<sup>30</sup>, M. Sasaki<sup>23</sup>, J. Schäfer<sup>23</sup>, F. Schüssler<sup>16</sup>, H. M. Schutte<sup>8</sup>, U. Schwanke<sup>31</sup>, J. N. S. Shapopi<sup>7</sup>, R. Simoni<sup>34,*</sup>, H. Sol<sup>13</sup>, A. Specovius<sup>23</sup>, S. Spencer<sup>19</sup>, Ł. Stawarz<sup>27</sup>, S. Steinmassl<sup>2</sup>, C. Steppa<sup>21</sup>, I. Sushch<sup>8</sup>, T. Takahashi<sup>36</sup>, T. Tanaka<sup>37</sup>, A. M. Taylor<sup>9</sup>, R. Terrier<sup>11</sup>, M. Tsirou<sup>2</sup>, Y. Uchiyama<sup>38</sup>, T. Unbehaun<sup>23</sup>, C. van Eldik<sup>23</sup>, J. Veh<sup>23</sup>, J. Vink<sup>34,*</sup>, H. J. Völk<sup>2</sup>, S. J. Wagner<sup>4</sup>, F. Werner<sup>2</sup>, R. White<sup>2</sup>, A. Wierzcholska<sup>18</sup>, Yu Wun Wong<sup>23</sup>, A. Yusafzai<sup>23</sup>, M. Zacharias<sup>13,8</sup>, D. Zargaryan<sup>1,3</sup>, A. A. Zdziarski<sup>29</sup>, A. Zech<sup>13</sup>, S. J. Zhu<sup>9</sup>, S. Zouari<sup>11</sup>, and N. Żywucka<sup>8</sup>

<footnote n="1">¹ Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland</footnote>

<footnote n="2">² Max-Planck-Institut für Kernphysik, PO Box 103980, 69029 Heidelberg, Germany</footnote>

<footnote n="3">³ High Energy Astrophysics Laboratory, RAU, 123 Hovsep Emin St, Yerevan 0051, Armenia</footnote>

<footnote n="4">⁴ Landessternwarte, Universität Heidelberg, Königstuhl, 69117 Heidelberg, Germany</footnote>

<footnote n="5">⁵ Aix Marseille Université, CNRS/IN2P3, CPPM, Marseille, France</footnote>

<footnote n="6">⁶ Laboratoire Leprince-Ringuet, École Polytechnique, CNRS, Institut Polytechnique de Paris, 91128 Palaiseau, France</footnote>

<footnote n="7">⁷ University of Namibia, Department of Physics, Private Bag 13301, Windhoek 10005, Namibia</footnote>

<footnote n="8">⁸ Centre for Space Research, North-West University, Potchefstroom 2520, South Africa</footnote>

<footnote n="9">⁹ DESY, 15738 Zeuthen, Germany</footnote>

<footnote n="10">¹⁰ School of Physics, University of the Witwatersrand, 1 Jan Smuts Avenue, Braamfontein, Johannesburg 2050, South Africa</footnote>

<footnote n="11">¹¹ Université de Paris, CNRS, Astroparticule et Cosmologie, 75013 Paris, France</footnote>

<footnote n="12">¹² Department of Physics and Electrical Engineering, Linnaeus University, 351 95 Växjö, Sweden</footnote>

<footnote n="13">¹³ Laboratoire Univers et Théories, Observatoire de Paris, Université PSL, CNRS, Université de Paris, 92190 Meudon, France</footnote>

<footnote n="14">¹⁴ Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies, LPNHE, 4 Place Jussieu, 75252 Paris, France</footnote>

<footnote n="15">¹⁵ Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules – IN2P3, 74000 Annecy, France</footnote>

<footnote n="16">¹⁶ IRFU, CEA, Université Paris-Saclay, 91191 Gif-sur-Yvette, France</footnote>

<footnote n="17">¹⁷ Astronomical Observatory, The University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw, Poland</footnote>

<footnote n="18">¹⁸ Instytut Fizyki Jądrowej PAN, ul. Radzikowskiego 152, 31-342 Kraków, Poland</footnote>

<footnote n="19">¹⁹ University of Oxford, Department of Physics, Denys Wilkinson Building, Keble Road Oxford OX1 3RH, UK</footnote>

<footnote n="20">²⁰ Université Bordeaux, CNRS, LP2I Bordeaux, UMR 5797, 33170 Gradignan, France</footnote>

<footnote n="21">²¹ Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Strasse 24/25, 14476 Potsdam, Germany</footnote>

<footnote n="22">²² School of Physical Sciences, University of Adelaide, Adelaide 5005, Australia</footnote>

<footnote>* Corresponding authors; e-mail: contact.hess@hess-experiment.eu.</footnote>
23 Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany

24 Laboratoire Univers et Particules de Montpellier, Université Montpellier, CNRS/IN2P3, CC 72, Place Eugène Bataillon, 34095 Montpellier Cedex 5, France

25 Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität Innsbruck, 6020 Innsbruck, Austria

26 Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, 22761 Hamburg, Germany

27 Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla 171, 30-244 Kraków, Poland

28 Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland

29 Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland

30 Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, 72076 Tübingen, Germany

31 Institut für Physik, Humboldt-Universität zu Berlin, Newtonstr. 15, 12489 Berlin, Germany

32 Department of Physics, University of the Free State, PO Box 339, Bloemfontein 9300, South Africa

33 Department of Physics and Astronomy, The University of Leicester, University Road, Leicester, LE1 7RH, UK

34 GRAPPA, Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098, XH Amsterdam, The Netherlands

35 Yerevan Physics Institute, 2 Alikhanian Brothers St., 375036 Yerevan, Armenia

36 Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa, Chiba 277-8583, Japan

37 Department of Physics, Konan University, 8-9-1 Okamoto, Higashinada, Kobe, Hyogo 658-8501, Japan

38 Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo 171-8501, Japan

A&A 662, A65 (2022), https://doi.org/10.1051/0004-6361/202243096

**Key words.** gamma rays: general – supernovae: individual: Kepler – ISM: supernova remnants – radiation mechanisms: non-thermal – errata, addenda

In the version of this article initially published, there was a typographical error in the second paragraph of Sect. 4. The normalization constant should be read $N_0 = (9.5 \pm 2.3_{stat} \pm 2.9_{sys}) \times 10^{-14} \text{ cm}^{-2} \text{ s}^{-1} \text{ TeV}^{-1}$. The normalization was correctly stated elsewhere.

Also, the author's name D. Malyshev (affiliated with Institute 23) was inadvertently missing from the author list of the published version. It is added here.