{"paper":{"title":"Particle Transport within the Pulsar Wind Nebula HESS J1825-137","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Zdziarski, A. Carosi, A. Chen, A. Djannati-Ata\\\"i, A. Dmytriiev, A. Donath, A. Fiasson, A. Jacholkowska, A. Lemi\\`ere, A. Marcowith, A.M. Taylor, A.M.W. Mitchell, A. Priyana Noel, A. Quirrenbach, A. Reimer, A. Santangelo, A. Schulz, A. Sinha, A. Specovius, A.S. Seyffert, A. Wierzcholska, A. Zech, A. Ziegler, B. Condon, B. Kh\\'elifi, B. Peyaud, B. Rudak, B. van Soelen, C. Arcaro, C. Armand, C. Boisson, C. Deil, C. Hoischen, C. Mariaud, C. Moore, C. Perennes, C. Romoli, C. Stegmann, C. Steppa, C. Trichard, C. van Eldik, C. van Rensburg, C. Venter, D.A. Prokhorov, D.A. Sanchez, D. Berge, D. Glawion, D. Gottschall, D. Horns, D. Huber, D. Jankowsky, D.J. van der Walt, D. Kerszberg, D. Khangulyan, D. Malyshev, D. Tiziani, D. Zaborov, E. Leser, E. Moulin, E.O. Ang\\\"uner, E. Ruiz-Velasco, F. Aharonian, F. Ait Benkhali, F. Brun, F. Gat\\'e, F. Jankowsky, F. Niederwanger, F. Rieger, F. Sch\\\"ussler, F. Voisin, F. Zefi, G. Emery, G. Fontaine, G. Giavitto, G. Heinzelmann, G. Henri, G. Hermann, G. Lamanna, G. Mart\\'i-Devesa, G. Maurin, G. P\\\"uhlhofer, G. Rowell, G. Vasileiadis, H. Abdalla, H.E.S.S. collaboration, H. Iwasaki, H.J. V\\\"olk, H. Ndiyavala, H. Odaka, H. Prokoph, H. Schutte, H. Sol, H. Yoneda, I.D. Davids, I. Jung-Richardt, I. Lypova, I. Oya, I. Shilon, J.A. Hinton, J. Becker Tjus, J. Bolmont, J. Bregeon, J. Devin, J. Dyks, J.F. Glicenstein, J. Hahn, J. King, J. Lau, J. Lefaucheur, J. Niemiec, J.-P. Ernenwein, J.-P. Lenain, J.-P. Tavernet, J. Veh, J. Vink, J. Zorn, K. Bernl\\\"ohr, K. Egberts, K. Katarzy\\'nski, K. Kosack, K. Shiningayamwe, L. Dirson, L. Jouvin, L. Mohrmann, L. Oakes, L.O'C. Drury, L. Rinchiuso, \\L. Stawarz, L. Tibaldo, M.A. Kastendieck, M. Arakawa, M. Arrieta, M. Backes, M. Barnard, M. B\\\"ottcher, M. Bryan, M. B\\\"uchele, M. Capasso, M. Cerruti, M. de Naurois, M. F\\\"u{\\ss}ling, M. Haupt, M.-H. Grondin, M. Holler, M. Jamrozy, M. Katsuragawa, M. Kraus, M. Lemoine-Goumard, M. Mohamed, M. Ostrowski, M. Panter, M. Punch, M. Renaud, M. Sasaki, M. Seglar-Arroyo, M. Senniappan, M. Spir-Jacob, M. Tluczykont, M. Tsirou, M. Zacharias, N. Chakraborty, N. Shafi, N. Tsuji, Nu. Komin, N. Zywucka, O. Reimer, P. Bordas, P. Brun, P. deWilt, P.J. Meintjes, P. O'Brien, P.-O. Petrucci, P. Vincent, Q. Piel, R. Blackwell, R.C.G. Chaves, R.D. Parsons, R. L\\'opez-Coto, R. Marx, R. Moderski, R.M. Wagner, R. Rauth, R. Schlickeiser, R. Simoni, R. Steenkamp, R. Terrier, R. Tuffs, R. White, R. Yang, R. Zanin, S. Bonnefoy, S. Caroff, S. Casanova, S. Chandra, S. Colafrancesco, S. Eschbach, S. Fegan, S. Funk, S. Gabici, S.J. Wagner, S. Klepser, S. Nakashima, S. Ohm, S. Pita, S. Raab, S. Saito, S. Schwemmer, T. Bulik, T. Bylund, T. Chand, T. L. Holch, T. Lohse, T. Murach, T. Takahashi, T. Tavernier, T. Vuillaume, U. Katz, U. Schwanke, V. Doroshenko, V. Marandon, V. Poireau, V. Sahakian, W. Hofmann, W. Klu\\'zniak, Y.A. Gallant, Y. Becherini, Y. Uchiyama, Z.Wadiasingh","submitted_at":"2018-10-30T11:39:00Z","abstract_excerpt":"Aims: We present a detailed view of the pulsar wind nebula (PWN) HESS J1825-137. We aim to constrain the mechanisms dominating the particle transport within the nebula, accounting for its anomalously large size and spectral characteristics. Methods: The nebula is studied using a deep exposure from over 12 years of H.E.S.S. I operation, together with data from H.E.S.S. II improving the low energy sensitivity. Enhanced energy-dependent morphological and spatially-resolved spectral analyses probe the Very High Energy (VHE, E > 0.1 TeV) gamma-ray properties of the nebula. Results: The nebula emiss"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.12676","kind":"arxiv","version":2},"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"}