{"paper":{"title":"The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Abramowski, A.A. Zdziarski, A. Balzer, A. Chen, A. Djannati-Ata\\\"i, A. Donath, A. Fiasson, A. F\\\"orster, A.G. Akhperjanian, A. Goyal, A. Ivascenko, A. Jacholkowska, A. Lemi\\`ere, A. Marcowith, A.M. Taylor, A.M.W. Mitchell, A. Quirrenbach, A. Reimer, A. Santangelo, A. Schulz, A.S. Seyffert, A. Viana, A. Wierzcholska, A. W\\\"ornlein, A. Zech, A. Ziegler, B. Condon, B. Degrange, B. Giebels, B. Kh\\'elifi, B. Peyaud, B. Rudak, B. van Soelen, C. Boisson, C.B. Rulten, C. Deil, C. Farnier, C. Hoischen, C. Mariaud, C. Perennes, C. Romoli, C. Stegmann, C. Trichard, C. van Eldik, C. van Rensburg, C. Venter, D.A. Sanchez, D. Berge, D. Gottschall, D. Hadasch, D. Horns, D. Jankowsky, D.J. van der Walt, D. Kerszberg, D. Klochkov, D. Kolitzus, D. Prokhorov, D. Salek, D. Tiziani, D. Wouters, D. Zaborov, E. Leser, E. Moulin, E.O. Ang\\\"uner, F. Aharonian, F. Ait Benkhali, F. Brun, Fermi-LAT Collaboration, F. Jankowsky, F. Krayzel, F. Niederwanger, F. Rieger, F. Sch\\\"ussler, F. Spanier, F. Spies, F. Stinzing, F. Voisin, F. Zefi, G. Cologna, G. Dubus, G. Fontaine, G. Giavitto, G. Heinzelmann, G. Henri, G. Hermann, G. Lamanna, G. Maurin, G. Pelletier, G. P\\\"uhlhofer, G. Rowell, G. Spengler, G. Vasileiadis, H. Abdalla, H.E.S.S. collaboration, H.J. V\\\"olk, H. Laffon, H. Odaka, H. Poon, H. Prokoph, H. Sol, I.D. Davids, I. Jung-Richardt, I. Lypova, I. Oya, I. Shilon, I. Sushch, J.A. Hinton, J. Becker Tjus, J. Bolmont, J. Bregeon, J. Carr, J. Chevalier, J. Conrad, J. Decock, J. Devin, J. Dyks, J.F. Glicenstein, J. Hahn, J. Hawkes, J. Katsuta, J. King, J. Lau, J. Lefaucheur, J. Niemiec, J.-P. Ernenwein, J.-P. Lees, J.-P. Lenain, J.-P. Tavernet, J. Veh, J. Vink, K. Bernl\\\"ohr, K. Dutson, K. Egberts, K. Katarzy\\'nski, K. Kosack, K. Mor{\\aa}, K. Stycz, L. Dirson, L. Jouvin, L. Mohrmann, L. Oakes, L.O'C. Drury, \\L. Stawarz, L. Tibaldo, M.A. Kastendieck, M. Arrieta, M. Backes, M. Barnard, M. B\\\"ottcher, M. Bryan, M. Capasso, M. Cerruti, M. Chr\\'etien, M. de Naurois, M. F\\\"u{\\ss}ling, M. Gajdus, M. Haupt, M.-H. Grondin, M. Holler, M. Jamrozy, M. Janiak, M. Jingo, M. Kieffer, M. Kraus, M. Lemoine-Goumard, M. Lorentz, M. Mayer, M. Meyer, M. Mohamed, M. Ostrowski, M. Padovani, M. Panter, M. Punch, M. Renaud, M. Sasaki, M. Settimo, M. Tluczykont, M.V. Fernandes, M. Zacharias, N. Chakraborty, N. Maxted, N. Shafi, Nu. Komin, N.W. Pekeur, N. \\.Zywucka, O. Hervet, O. Reimer, P. Aubert, P. Bordas, P. Brun, P. deWilt, P. Eger, P.J. Meintjes, P. O'Brien, P.-O. Petrucci, P.P. Kr\\\"uger, P. Vincent, P. Wagner, P. Willmann, Q. Piel, R. Blackwell, R.C.G. Chaves, R. Chalme-Calvet, R. de los Reyes, R.D. Parsons, R. Liu, R. L\\'opez-Coto, R. Marx, R. Moderski, R.M. Wagner, R. Schlickeiser, R. Simoni, R. Steenkamp, R. Terrier, R. Tuffs, R. White, R. Yang, S. Bernhard, S. Casanova, S. Colafrancesco, S. Eschbach, S. Fegan, S. Funk, S. Gabici, S.J. Wagner, S. Klepser, S. Krakau, S. Ohm, S. \\\"Ottl, S. Pita, S. Raab, S. Rosier-Lees, S. Schwemmer, T. Andersson, T. Bulik, T. Edwards, T. Garrigoux, T. Jogler, T. Lohse, T. Murach, T. Tavernier, T. Vuillaume, U. Katz, U. Schwanke, V. Lefranc, V. Marandon, V. Sahakian, V. Zabalza, W. Domainko, W. Hofmann, W. Klu\\'zniak, Y.A. Gallant, Y. Becherini, Y. Cui, Y. Uchiyama, Z. Wadiasingh","submitted_at":"2016-09-02T13:49:45Z","abstract_excerpt":"The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one and four thousand years ago, and subsequently evolved into a mixed-morphology remnant, which is interacting with molecular clouds (MC). $\\gamma$-ray observations of SNR/MC associations are a powerful tool to constrain the origin of Galactic cosmic-rays, as they can probe the acceleration of hadrons through their interaction with the surrounding medium and subsequent emission of non-thermal photons. The detection of a $\\gamma$-ray source coincident with W49B at very high energies (VHE; E > 100 G"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.00600","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}