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@ARTICLE{Abdalla:418010,
      author       = {Abdalla, H. and Abramowski, A. and Aharonian, F. and Ait
                      Benkhali, F. and Akhperjanian, A. G. and Andersson, T. and
                      Angüner, E. O. and Arrieta, M. and Aubert, P. and Backes,
                      M. and Balzer, A. and Barnard, M. and Becherini, Y. and
                      Becker Tjus, J. and Berge, D. and Bernhard, S. and
                      Bernlöhr, K. and Blackwell, R. and Böttcher, M. and
                      Boisson, C. and Bolmont, J. and Bordas, P. and Bregeon, J.
                      and Brun, F. and Brun, P. and Bryan, M. and Bulik, T. and
                      Capasso, M. and Carr, J. and Casanova, S. and Cerruti, M.
                      and Chakraborty, N. and Chalme-Calvet, R. and Chaves, R. C.
                      G. and Chen, A. and Chevalier, J. and Chrétien, M. and
                      Colafrancesco, S. and Cologna, G. and Condon, B. and Conrad,
                      J. and Cui, Y. and Davids, I. D. and Decock, J. and
                      Degrange, B. and Deil, C. and Devin, J. and deWilt, P. and
                      Dirson, L. and $Djannati-Ata\'i,$ A. and Domainko, W. and
                      Donath, A. and Drury, L. O'C. and Dubus, G. and Dutson, K.
                      and Dyks, J. and Edwards, T. and Egberts, K. and Eger, P.
                      and Ernenwein, J.-P. and Eschbach, S. and Farnier, C. and
                      Fegan, S. and Fernandes, M. V. and Fiasson, A. and Fontaine,
                      G. and Förster, A. and Fukuyama, T. and Funk, S. and
                      Füßling, M. and Gabici, S. and Gajdus, M. and Gallant, Y.
                      A. and Garrigoux, T. and Giavitto, G. and Giebels, B. and
                      Glicenstein, J. F. and Gottschall, D. and Goyal, A. and
                      Grondin, M.-H. and Hadasch, D. and Hahn, J. and Haupt, M.
                      and Hawkes, J. and Heinzelmann, G. and Henri, G. and
                      Hermann, G. and Hervet, O. and Hinton, J. A. and Hofmann, W.
                      and Hoischen, C. and Holler, M. and Horns, D. and Ivascenko,
                      A. and Jacholkowska, A. and Jamrozy, M. and Janiak, M. and
                      Jankowsky, D. and Jankowsky, F. and Jingo, M. and Jogler, T.
                      and Jouvin, L. and Jung-Richardt, I. and Kastendieck, M. A.
                      and Katarzyński, K. and Katz, U. and Kerszberg, D. and
                      Khélifi, B. and Kieffer, M. and King, J. and Klepser, S.
                      and Klochkov, D. and Kluźniak, W. and Kolitzus, D. and
                      Komin, Nu. and Kosack, K. and Krakau, S. and Kraus, M. and
                      Krayzel, F. and Krüger, P. P. and Laffon, H. and Lamanna,
                      G. and Lau, J. and Lees, J.-P. and Lefaucheur, J. and
                      Lefranc, V. and Lemière, A. and Lemoine-Goumard, M. and
                      Lenain, J.-P. and Leser, E. and Lohse, T. and Lorentz, M.
                      and Liu, R. and López-Coto, R. and Lypova, I. and Marandon,
                      V. and Marcowith, A. and Mariaud, C. and Marx, R. and
                      Maurin, G. and Maxted, N. and Mayer, M. and Meintjes, P. J.
                      and Meyer, M. and Mitchell, A. M. W. and Moderski, R. and
                      Mohamed, M. and Mohrmann, L. and Morå, K. and Moulin, E.
                      and Murach, T. and de Naurois, M. and Niederwanger, F. and
                      Niemiec, J. and Oakes, L. and O'Brien, P. and Odaka, H. and
                      Öttl, S. and Ohm, S. and Ostrowski, M. and Oya, I. and
                      Padovani, M. and Panter, M. and Parsons, R. D. and Pekeur,
                      N. W. and Pelletier, G. and Perennes, C. and Petrucci, P.-O.
                      and Peyaud, B. and Piel, Q. and Pita, S. and Poon, H. and
                      Prokhorov, D. and Prokoph, H. and Pühlhofer, G. and Punch,
                      M. and Quirrenbach, A. and Raab, S. and Reimer, A. and
                      Reimer, O. and Renaud, M. and de los Reyes, R. and Rieger,
                      F. and Romoli, C. and Rosier-Lees, S. and Rowell, G. and
                      Rudak, B. and Rulten, C. B. and Sahakian, V. and Salek, D.
                      and Sanchez, D. A. and Santangelo, A. and Sasaki, M. and
                      Schlickeiser, R. and Schüssler, F. and Schulz, Anneli and
                      Schwanke, U. and Schwemmer, S. and Settimo, M. and Seyffert,
                      A. S. and Shafi, N. and Shilon, I. and Simoni, R. and Sol,
                      H. and Spanier, F. and Spengler, G. and Spies, F. and
                      Steenkamp, R. and Stegmann, C. and Stinzing, F. and Stycz,
                      K. and Sushch, I. and Takahashi, T. and Tavernet, J.-P. and
                      Tavernier, T. and Taylor, A. M. and Terrier, R. and Tibaldo,
                      L. and Tiziani, D. and Tluczykont, M. and Trichard, C. and
                      Tuffs, R. and Uchiyama, Y. and van der Walt, D. J. and van
                      Eldik, C. and van Rensburg, C. and van Soelen, B. and
                      Vasileiadis, G. and Veh, J. and Venter, C. and Viana, A. and
                      Vincent, P. and Vink, J. and Voisin, F. and Völk, H. J. and
                      Volpe, F. and Vuillaume, T. and Wadiasingh, Z. and Wagner,
                      S. J. and Wagner, P. and Wagner, R. M. and White, R. and
                      Wierzcholska, A. and Willmann, P. and Wörnlein, A. and
                      Wouters, D. and Yang, R. and Zabalza, V. and Zaborov, D. and
                      Zacharias, M. and Zdziarski, A. A. and Zech, A. and Zefi, F.
                      and Ziegler, A. and Żywucka, N.},
      collaboration = {H. E. S. S.{ Collaboration}},
      title        = {{H}.{E}.{S}.{S}. observations of {RX} {J}1713.7−3946 with
                      improved angular and spectral resolution: {E}vidence for
                      gamma-ray emission extending beyond the {X}-ray emitting
                      shell},
      journal      = {Astronomy and astrophysics},
      volume       = {612},
      issn         = {1432-0746},
      address      = {Les Ulis},
      publisher    = {EDP Sciences},
      reportid     = {PUBDB-2019-00138, arXiv:1609.08671},
      pages        = {A6},
      year         = {2018},
      note         = {(c) ESO},
      abstract     = {Supernova remnants exhibit shock fronts (shells) that can
                      accelerate charged particles up to very high energies. In
                      the past decade, measurements of a handful of shell-type
                      supernova remnants in very high-energy gamma rays have
                      provided unique insights into the acceleration process.
                      Among those objects, RX J1713.7−3946 (also known as
                      G347.3−0.5) has the largest surface brightness, allowing
                      us in the past to perform the most comprehensive study of
                      morphology and spatially resolved spectra of any such very
                      high-energy gamma-ray source. Here we present extensive new
                      H.E.S.S. measurements of RX J1713.7−3946, almost doubling
                      the observation time compared to our previous publication.
                      Combined with new improved analysis tools, the previous
                      sensitivity is more than doubled. The H.E.S.S. angular
                      resolution of 0.048° (0.036° above 2 TeV) is unprecedented
                      in gamma-ray astronomy and probes physical scales of 0.8
                      (0.6) parsec at the remnant’s location. The new H.E.S.S.
                      image of RX J1713.7−3946 allows us to reveal clear
                      morphological differences between X-rays and gamma rays. In
                      particular, for the outer edge of the brightest shell
                      region, we find the first ever indication for particles in
                      the process of leaving the acceleration shock region. By
                      studying the broadband energy spectrum, we furthermore
                      extract properties of the parent particle populations,
                      providing new input to the discussion of the leptonic or
                      hadronic nature of the gamma-ray emission mechanism.Key
                      words: acceleration of particles / cosmic rays / ISM:
                      supernova remnants / gamma rays: general / astroparticle
                      physic★ All images (FITS files)are available at the CDS
                      via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or
                      via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/612/A6†
                      Deceased.},
      keywords     = {gamma ray: emission (INSPIRE) / gamma ray: VHE (INSPIRE) /
                      X-ray: emission (INSPIRE) / HESS (INSPIRE) / acceleration
                      (INSPIRE) / supernova (INSPIRE) / angular resolution
                      (INSPIRE) / charged particle (INSPIRE) / energy spectrum
                      (INSPIRE) / sensitivity (INSPIRE) / brightness (INSPIRE) /
                      resolution (INSPIRE) / spectral (INSPIRE) / doubling
                      (INSPIRE) / surface (INSPIRE)},
      cin          = {ZEU-HESS},
      ddc          = {520},
      cid          = {I:(DE-H253)ZEU-HESS-20140213},
      pnm          = {613 - Matter and Radiation from the Universe (POF3-613)},
      pid          = {G:(DE-HGF)POF3-613},
      experiment   = {EXP:(DE-H253)HESS-20170101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)16},
      eprint       = {1609.08671},
      howpublished = {arXiv:1609.08671},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1609.08671;\%\%$},
      UT           = {WOS:000429404700006},
      doi          = {10.1051/0004-6361/201629790},
      url          = {https://bib-pubdb1.desy.de/record/418010},
}