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- EC| SHARPCollaboration, H. E. S. S.; Aharonian, F.; Benkhali, F. Ait; Anguner, E. O.; Ashkar, H.;
Backes, M.; Backes, M.
Harvested from ORCID Public Data FileBackes, M. in OpenAIRE Martins, V. Barbosa; Batzofin, R.; Becherini, Y.; Berge, D.; Bernloehr, K.; Boettcher, M.; Boisson, C.;Martins, V. Barbosa
Harvested from ORCID Public Data FileMartins, V. Barbosa in OpenAIRE Bolmont, J.; de Lavergne, M. de Bony; Breuhaus, M.; Brose, R.; Brun, F.;Bolmont, J.
Harvested from ORCID Public Data FileBolmont, J. in OpenAIRE Bulik, T.; Bylund, T.; Cangemi, F.; Caroff, S.; Caroff, S.
Harvested from ORCID Public Data FileCaroff, S. in OpenAIRE Casanova, S.; Cerruti, M.; Chand, T.;Casanova, S.
Harvested from ORCID Public Data FileCasanova, S. in OpenAIRE 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.;Egberts, K.
Harvested from ORCID Public Data FileEgberts, K. in OpenAIRE Feijen, K.; Fiasson, A.; de Clairfontaine, G. Fichet; Fontaine, G.;Feijen, K.
Harvested from ORCID Public Data FileFeijen, K. in OpenAIRE Funk, S.; Gabici, S.; Gallant, Y. A.; Ghafourizadeh, S.; Giavitto, G.; Giunti, L.; Giunti, L.
Harvested from ORCID Public Data FileGiunti, L. in OpenAIRE Glawion, D.; Glicenstein, J. F.; Grondin, M. -H.; Hoerbe, M.; Hofmann, W.;Glawion, D.
Harvested from ORCID Public Data FileGlawion, D. in OpenAIRE Holch, T. L.; Holch, T. L.
Harvested from ORCID Public Data FileHolch, T. L. in OpenAIRE Holler, M.; Holler, M.
Harvested from ORCID Public Data FileHoller, M. in OpenAIRE Horns, D.; Huang, Zhiqiu; Jamrozy, M.; Joshi, V.; Jung-Richardt, I.; Kasai, E.; Katarzynski, K.; Katz, U.; Khelifi, B.; Kluzniak, W.; Komin, Nu.;Kluzniak, W.
Harvested from ORCID Public Data FileKluzniak, W. in OpenAIRE Kosack, K.; Kostunin, D.; Lemiere, A.; Lemoine-Goumard, M.;Kosack, K.
Harvested from ORCID Public Data FileKosack, K. in OpenAIRE Lenain, J. -P.; Lenain, J. -P.
Harvested from ORCID Public Data FileLenain, J. -P. in OpenAIRE Leuschner, F.; Lohse, T.; Luashvili, A.; Lypova, I.;Leuschner, F.
Harvested from ORCID Public Data FileLeuschner, F. in OpenAIRE Mackey, J.; Malyshev, D.; Malyshev, D.;Mackey, J.
Harvested from ORCID Public Data FileMackey, J. in OpenAIRE Marandon, V.; Marandon, V.
Harvested from ORCID Public Data FileMarandon, V. in OpenAIRE Marchegiani, P.; Marcowith, A.; Marti-Devesa, G.; Marx, R.;Marchegiani, P.
Harvested from ORCID Public Data FileMarchegiani, P. in OpenAIRE Maurin, G.; Maurin, G.
Harvested from ORCID Public Data FileMaurin, G. in OpenAIRE Meintjes, P. J.; Meintjes, P. J.
Harvested from ORCID Public Data FileMeintjes, P. J. in OpenAIRE Meyer, M.; Mitchell, A.; Moderski, R.; Moderski, R.
Harvested from ORCID Public Data FileModerski, R. in OpenAIRE Mohrmann, L.; Montanari, A.; Moulin, E.; Muller, J.; Nakashima, K.; de Naurois, M.;Mohrmann, L.
Harvested from ORCID Public Data FileMohrmann, L. in OpenAIRE Nayerhoda, A.; Nayerhoda, A.
Harvested from ORCID Public Data FileNayerhoda, A. in OpenAIRE Niemiec, J.; Noel, A. Priyana;Niemiec, J.
Harvested from ORCID Public Data FileNiemiec, J. in OpenAIRE O'Brien, P.; Ohm, S.;O'Brien, P.
Harvested from ORCID Public Data FileO'Brien, P. in OpenAIRE Olivera-Nieto, L.; Wilhelmi, E. de Ona; Ostrowski, M.;Olivera-Nieto, L.
Harvested from ORCID Public Data FileOlivera-Nieto, L. in OpenAIRE Panny, S.; Panter, M.; Parsons, R. D.; Peron, G.; Poireau, V.; Prokhorov, D. A.; Puehlhofer, G.; Punch, M.; Quirrenbach, A.; Quirrenbach, A.
Harvested from ORCID Public Data FileQuirrenbach, A. in OpenAIRE Reichherzer, P.; Reimer, A.;Reichherzer, P.
Harvested from ORCID Public Data FileReichherzer, P. in OpenAIRE Reimer, O.; Reimer, O.
Harvested from ORCID Public Data FileReimer, O. in OpenAIRE Renaud, M.; Renaud, M.
Harvested from ORCID Public Data FileRenaud, M. in OpenAIRE Reville, B.; Rieger, F.; Rowell, G.;Reville, B.
Harvested from ORCID Public Data FileReville, B. in OpenAIRE Rudak, B.; Ricarte, H. Rueda; Sahakian, V.; Sailer, S.; Salzmann, H.; Sanchez, D. A.; Santangelo, A.; Sasaki, M.; Schafer, J.; Schussler, F.; Schutte, H. M.; Schwanke, U.; Shapopi, J. N. S.; Simoni, R.; Sol, H.; Specovius, A.;Santangelo, A.
Harvested from ORCID Public Data FileSantangelo, A. in OpenAIRE Spencer, S.; Stawarz, L.;Spencer, S.
Harvested from ORCID Public Data FileSpencer, S. in OpenAIRE Steinmassl, S.; Steppa, C.; Sushch, I.; Takahashi, T.; Tanaka, T.; Taylor, A. M.;Steinmassl, S.
Harvested from ORCID Public Data FileSteinmassl, S. in OpenAIRE Terrier, R.; Terrier, R.
Harvested from ORCID Public Data FileTerrier, R. in OpenAIRE Tsirou, M.; Uchiyama, Y.; Unbehaun, T.; van Eldik, C.;Tsirou, M.
Harvested from ORCID Public Data FileTsirou, M. in OpenAIRE Veh, J.; Vink, J.; Voelk, H. J.; Wagner, S. J.; Werner, F.; White, R.; Wierzcholska, A.; Wong, Yu Wun; Yusafzai, A.; Zacharias, M.;Wierzcholska, A.
Harvested from ORCID Public Data FileWierzcholska, A. in OpenAIRE Zargaryan, D.; Zargaryan, D.
Harvested from ORCID Public Data FileZargaryan, D. in OpenAIRE Zdziarski, A. A.; Zech, A.; Zhu, S. J.; Zouari, S.; Zywucka, N.;Zdziarski, A. A.
Harvested from ORCID Public Data FileZdziarski, A. A. in OpenAIREObservations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of nearby supernova (SN) remnants with ages younger than 500 yr by establishing Cassiopeia A and the remnant of Tycho’s SN as very-high-energy (VHE) γ-ray sources. The remnant of Kepler’s SN, which is the product of the most recent naked-eye SN in our Galaxy, is comparable in age to the other two, but is significantly more distant. If the γ-ray luminosities of the remnants of Tycho’s and Kepler’s SNe are similar, then the latter is expected to be one of the faintest γ-ray sources within reach of the current generation IACT arrays. Here we report evidence at a statistical level of 4.6σ for a VHE signal from the remnant of Kepler’s SN based on deep observations by the High Energy Stereoscopic System (H.E.S.S.) with an exposure of 152 h. The measured integral flux above an energy of 226 GeV is ∼0.3% of the flux of the Crab Nebula. The spectral energy distribution (SED) reveals a γ-ray emitting component connecting the VHE emission observed with H.E.S.S. to the emission observed at GeV energies with Fermi-LAT. The overall SED is similar to that of the remnant of Tycho’s SN, possibly indicating the same nonthermal emission processes acting in both these young remnants of thermonuclear SNe.
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