{"paper":{"title":"HESS J1741-302: a hidden accelerator in the Galactic plane","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. Carosi, A. Chen, A. Djannati-Ata\\\"i, A. Donath, A. Fiasson, 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. Kh\\'elifi, B. Peyaud, B. Rudak, B. van Soelen, C. Armand, C. Boisson, C.B. Rulten, C. Deil, C. Farnier, C. Hoischen, C. Mariaud, 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. Jankowsky, D.J. van der Walt, D. Kerszberg, D. Khangulyan, D. Klochkov, D. Malyshev, D. Tiziani, D. Wouters, D. Zaborov, E. Leser, E. Moulin, E.O. Ang\\\"uner, F. Aharonian, F. Ait Benkhali, F. Brun, F. Gat\\'e, F. Jankowsky, F. Niederwanger, F. Rieger, F. Sch\\\"ussler, F. Spanier, F. Voisin, F. Zefi, G. Emery, G. Fontaine, G. Giavitto, G. Heinzelmann, G. Henri, G. Hermann, G. Lamanna, G. Maurin, G. Pelletier, G. P\\\"uhlhofer, G. Rowell, G. Vasileiadis, H.E.S.S. Collaboration: H. Abdalla, H. Iwasaki, H.J. V\\\"olk, H. Laffon, H. Ndiyavala, H. Odaka, H. Prokoph, H. Sol, H. Yamamoto, 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. Chevalier, J. Conrad, J. Decock, J. Devin, J. Dyks, J.F. Glicenstein, J. Hahn, J. Hawkes, 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. Mor{\\aa}, K. Shiningayamwe, K. Torii, 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. Jingo, M. Katsuragawa, 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. Seglar-Arroyo, M. Spir-Jacob, M. Tluczykont, M. Tsirou, M.V. Fernandes, M. Zacharias, NANTEN Collaboration: R. Enokiya, N. Chakraborty, N. Maxted, N. Shafi, N. Tsuji, Nu. Komin, N.W. Pekeur, N. \\.Zywucka, O. Reimer, P. Bordas, P. Brun, P. deWilt, 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. de los Reyes, R.D. Parsons, R. Liu, 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. Bernhard, S. Bonnefoy, S. Caroff, S. Casanova, S. Colafrancesco, S. Eschbach, S. Fegan, S. Funk, S. Gabici, S.J. Wagner, S. Klepser, S. Krakau, S. Nakashima, S. Ohm, S. Pita, S. Raab, S. Saito, S. Schwemmer, T. Bulik, T. Edwards, T. Garrigoux, T. Hayakawa, T.L. Holch, T. Lohse, T. Murach, T. Okuda, T. Takahashi, T. Tavernier, T. Vuillaume, U. Katz, U. Schwanke, V. Marandon, V. Poireau, V. Sahakian, W. Hofmann, W. Klu\\'zniak, Y.A. Gallant, Y. Becherini, Y. Fukui, Y. Uchiyama, Z. Wadiasingh","submitted_at":"2017-11-03T22:32:43Z","abstract_excerpt":"The H.E.S.S. collaboration has discovered a new very high energy (VHE, E $>$ 0.1 TeV) $\\gamma$-ray source, HESS J1741-302, located in the Galactic plane. Despite several attempts to constrain its nature, no plausible counterpart has been found so far at X-ray and MeV/GeV $\\gamma$-ray energies, and the source remains unidentified. An analysis of 145-hour of observations of HESS J1741-302 at VHEs has revealed a steady and relatively weak TeV source ($\\sim$1$\\%$ of the Crab Nebula flux), with a spectral index of $\\Gamma$ = 2.3 $\\pm$ 0.2$_{\\text{stat}}$ $\\pm$ 0.2$_{\\text{sys}}$, extending to energ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01350","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"}