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@ARTICLE{Abramowski:293359,
      author       = {Abramowski, A. and Acero, F. and Aharonian, F. and Ait
                      Benkhali, F. and Akhperjanian, A. G. and Anguner, E. and
                      Anton, G. and Balenderan, S. and Balzer, A. and Barnacka, A.
                      and Becherini, Y. and Becker Tjus, J. and Bernlohr, K. and
                      Birsin, E. and Bissaldi, E. and Biteau, J. and Bottcher, M.
                      and Boisson, C. and Bolmont, J. and Bordas, P. and Brucker,
                      J. and Brun, F. and Brun, P. and Bulik, T. and Carrigan, S.
                      and Casanova, S. and Cerruti, M. and Chadwick, P. M. and
                      Chalme-Calvet, R. and Chaves, R. C. G. and Cheesebrough, A.
                      and Chretien, M. and Clapson, A.- C. and Colafrancesco, S.
                      and Cologna, G. and Conrad, J. and Couturier, C. and Cui, Y.
                      and Dalton, M. and Daniel, M. K. and Davids, I. D. and
                      Degrange, B. and Deil, C. and deWilt, P. and Dickinson, H.
                      J. and Djannati-Atai, A. and Domainko, W. and Drury, L. O.
                      and Dubus, G. and Dutson, K. and Dyks, J. and Dyrda, M. and
                      Edwards, T. and Egberts, K. and Eger, P. and Espigat, P. and
                      Farnier, C. and Fegan, S. and Feinstein, F. and Fernandes,
                      M. V. and Fernandez, D. and Fiasson, A. and Fontaine, G. and
                      Forster, A. and Fussling, M. and Gajdus, M. and Gallant, Y.
                      A. and Garrigoux, T. and Giavitto, G. and Giebels, B. and
                      Glicenstein, J. F. and Grondin, M.- H. and Grudzi ska, M.
                      and Haffner, S. and Hahn, J. and Harris, J. and Heinzelmann,
                      G. and Henri, G. and Hermann, G. and Hervet, O. and Hillert,
                      A. and Hinton, J. A. and Hofmann, W. and Hofverberg, P. and
                      Holler, M. and Horns, D. and Jacholkowska, A. and Jahn, C.
                      and Jamrozy, M. and Janiak, M. and Jankowsky, F. and Jung,
                      I. and Kastendieck, M. A. and Katarzy ski, K. and Katz, U.
                      and Kaufmann, S. and Khelifi, B. and Kieffer, M. and
                      Klepser, S. and Klochkov, D. and Klu niak, W. and Kneiske,
                      T. and Kolitzus, D. and Komin, N. and Kosack, K. and Krakau,
                      S. and Krayzel, F. and Kruger, P. P. and Laffon, H. and
                      Lamanna, G. and Lefaucheur, J. and Lemiere, A. and
                      Lemoine-Goumard, M. and Lenain, J.- P. and Lennarz, D. and
                      Lohse, T. and Lopatin, A. and Lu, C.- C. and Marandon, V.
                      and Marcowith, A. and Marx, R. and Maurin, G. and Maxted, N.
                      and Mayer, M. and McComb, T. J. L. and Mehault, J. and
                      Meintjes, P. J. and Menzler, U. and Meyer, M. and Moderski,
                      R. and Mohamed, M. and Moulin, E. and Murach, T. and
                      Naumann, C. L. and de Naurois, M. and Niemiec, J. and Nolan,
                      S. J. and Oakes, L. and Ohm, S. and de Ona Wilhelmi, E. and
                      Opitz, B. and Ostrowski, M. and Oya, I. and Panter, M. and
                      Parsons, R. D. and Paz Arribas, M. and Pekeur, N. W. and
                      Pelletier, G. and Perez, J. and Petrucci, P.- O. and Peyaud,
                      B. and Pita, S. and Poon, H. and Puhlhofer, G. and Punch, M.
                      and Quirrenbach, A. and Raab, S. and Raue, M. and Reimer, A.
                      and Reimer, O. and Renaud, M. and de los Reyes, R. and
                      Rieger, F. and Rob, L. and Romoli, C. and Rosier-Lees, S.
                      and Rowell, G. and Rudak, B. and Rulten, C. B. and Sahakian,
                      V. and Sanchez, D. A. and Santangelo, A. and Schlickeiser,
                      R. and Schussler, F. and Schulz, A. and Schwanke, U. and
                      Schwarzburg, S. and Schwemmer, S. and Sol, H. and Spengler,
                      G. and Spies, F. and Stawarz,  . and Steenkamp, R. and
                      Stegmann, C. and Stinzing, F. and Stycz, K. and Sushch, I.
                      and Szostek, A. and Tavernet, J.- P. and Tavernier, T. and
                      Taylor, A. M. and Terrier, R. and Tluczykont, M. and
                      Trichard, C. and Valerius, K. and van Eldik, C. and van
                      Soelen, B. and Vasileiadis, G. and Venter, C. and Viana, A.
                      and Vincent, P. and Volk, H. J. and Volpe, F. and Vorster,
                      M. and Vuillaume, T. and Wagner, S. J. and Wagner, P. and
                      Ward, M. and Weidinger, M. and Weitzel, Q. and White, R. and
                      Wierzcholska, A. and Willmann, P. and Wornlein, A. and
                      Wouters, D. and Zabalza, V. and Zacharias, M. and Zajczyk,
                      A. and Zdziarski, A. A. and Zech, A. and Zechlin, H.- S.},
      collaboration = {H.E.S.S.{ Collaboration}},
      title        = {{D}iscovery of the {VHE} gamma-ray source {HESS}
                      {J}1832-093 in the vicinity of {SNR} {G}22.7-0.2},
      journal      = {Monthly notices of the Royal Astronomical Society},
      volume       = {446},
      number       = {2},
      issn         = {1365-2966},
      address      = {Oxford},
      publisher    = {Oxford Univ. Press},
      reportid     = {PUBDB-2016-00464, arXiv:1411.0572},
      pages        = {1163 - 1169},
      year         = {2015},
      note         = {(c) The Authors},
      abstract     = {The region around the supernova remnant (SNR) W41 contains
                      several TeV sources and has prompted the HESS Collaboration
                      to perform deep observations of this field of view. This
                      resulted in the discovery of the new very high energy (VHE)
                      source HESS J1832−093, at the position
                      $RA=18^{h}32^{m}50^{s} \pm
                      3^{s}_{stat}\pm2^{s}_{syst},Dec=−9^\circ22^{\prime}
                      36^{\prime\prime} \pm 32^{\prime\prime}_{stat} \pm
                      20^{\prime\prime}_{syst}(J2000)$, spatially coincident with
                      a part of the radio shell of the neighbouring remnant
                      G22.7−0.2. The photon spectrum is well described by a
                      power law of index Γ = 2.6 $\pm$ 0.3$_{stat}$ $\pm$
                      0.1$_{syst}$ and a normalization at 1 TeV of Φ$_{0}=(4.8
                      \pm 0.8_{stat} \pm 1.0_{syst})
                      ×10^{−13}cm^{−2}s^{−1}TeV^{−1}$. The location of
                      the gamma-ray emission on the edge of the SNR rim first
                      suggested a signature of escaping cosmic rays illuminating a
                      nearby molecular cloud. Then a dedicated XMM–Newton
                      observation led to the discovery of a new X-ray point source
                      spatially coincident with the TeV excess. Two other
                      scenarios were hence proposed to identify the nature of HESS
                      J1832−093. Gamma-rays from inverse Compton radiation in
                      the framework of a pulsar wind nebula scenario or the
                      possibility of gamma-ray production within a binary system
                      are therefore also considered. Deeper multiwavelength
                      observations will help to shed new light on this intriguing
                      VHE source.},
      cin          = {ZEU-HESS},
      ddc          = {520},
      cid          = {I:(DE-H253)ZEU-HESS-20140213},
      pnm          = {523 - High-energy gamma ray astronomy (POF2-523)},
      pid          = {G:(DE-HGF)POF2-523},
      experiment   = {EXP:(DE-MLZ)External-20140101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000350272200004},
      eprint       = {1411.0572},
      howpublished = {arXiv:1411.0572},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1411.0572;\%\%$},
      doi          = {10.1093/mnras/stu2148},
      url          = {https://bib-pubdb1.desy.de/record/293359},
}