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@ARTICLE{Abdalla:403344,
      author       = {Abdalla, H. and Abramowski, A. and Aharonian, F. and
                      Benkhali, F. Ait and Angüner, E. O. and Arakawa, M. and
                      Arrieta, M. and Aubert, P. and Backes, M. and Balzer, A. and
                      Barnard, M. and Becherini, Y. and Tjus, J. Becker and Berge,
                      D. and Bernhard, S. and Bernlöhr, K. and Blackwell, R. and
                      Böttcher, M. and Boisson, C. and Bolmont, J. and Bonnefoy,
                      S. and Bordas, P. and Bregeon, J. and Brun, F. and Brun, P.
                      and Bryan, M. and Büchele, M. and Bulik, T. and Capasso, M.
                      and Carrigan, S. and Caroff, S. and Carosi, A. and Casanova,
                      S. and Cerruti, M. and Chakraborty, N. and Chaves, R. C. G.
                      and Chen, A. and Chevalier, J. and Colafrancesco, S. and
                      Condon, B. and Conrad, J. and Davids, I. D. and Decock, J.
                      and Deil, C. and Devin, J. and deWilt, P. and Dirson, L. and
                      Djannati-Ataï, A. and Domainko, W. and Donath, A. and
                      Drury, L. O’C. and Dutson, K. and Dyks, J. and Edwards, T.
                      and Egberts, K. and Eger, P. and Emery, G. 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 Funk, S. and Füßling, M. and Gabici, S.
                      and Gallant, Y. A. and Garrigoux, T. and Gast, H. and Gaté,
                      F. and Giavitto, G. and Giebels, B. and Glawion, D. and
                      Glicenstein, J. F. and Gottschall, D. and Grondin, M.-H. and
                      Hahn, J. and Haupt, M. and Hawkes, J. and Heinzelmann, G.
                      and Henri, G. and Hermann, G. and Hinton, J. A. and Hofmann,
                      W. and Hoischen, C. and Holch, T. L. and Holler, M. and
                      Horns, D. and Ivascenko, A. and Iwasaki, H. and
                      Jacholkowska, A. and Jamrozy, M. and Jankowsky, D. and
                      Jankowsky, F. and Jingo, M. and Jouvin, L. and
                      Jung-Richardt, I. and Kastendieck, M. A. and Katarzyński,
                      K. and Katsuragawa, M. and Katz, U. and Kerszberg, D. and
                      Khangulyan, D. and Khélifi, B. and King, J. and Klepser, S.
                      and Klochkov, D. and Kluźniak, W. and Komin, Nu. and
                      Kosack, K. and Krakau, S. and Kraus, M. and Krüger, P. P.
                      and Laffon, H. and Lamanna, G. and Lau, J. and Lees, J.-P.
                      and Lefaucheur, J. 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 Malyshev, D. 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 Nakashima, S. and de
                      Naurois, M. and Ndiyavala, H. and Niederwanger, F. and
                      Niemiec, J. and Oakes, L. and O’Brien, P. and Odaka, H.
                      and Ohm, S. and Ostrowski, M. and Oya, I. and Padovani, M.
                      and Panter, M. and Parsons, R. D. and Paz Arribas, M. and
                      Pekeur, N. W. and Pelletier, G. and Perennes, C. and
                      Petrucci, P.-O. and Peyaud, B. and Piel, Q. and Pita, S. and
                      Poireau, V. and Poon, H. and Prokhorov, D. and Prokoph, H.
                      and Pühlhofer, G. and Punch, M. and Quirrenbach, A. and
                      Raab, S. and Rauth, R. and Reimer, A. and Reimer, O. and
                      Renaud, M. and de los Reyes, R. and Rieger, F. and
                      Rinchiuso, L. and Romoli, C. and Rowell, G. and Rudak, B.
                      and Rulten, C. B. and Safi-Harb, S. and Sahakian, V. and
                      Saito, S. and Sanchez, D. A. and Santangelo, A. and Sasaki,
                      M. and Schandri, M. and Schlickeiser, R. and Schüssler, F.
                      and Schulz, Anneli and Schwanke, U. and Schwemmer, S. and
                      Seglar-Arroyo, M. and Settimo, M. and Seyffert, A. S. and
                      Shafi, N. and Shilon, I. and Shiningayamwe, K. and Simoni,
                      R. and Sol, H. and Spanier, F. and Spir-Jacob, M. and
                      Stawarz, Ł. and Steenkamp, R. and Stegmann, C. and Steppa,
                      C. 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
                      Tsirou, M. and Tsuji, N. 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 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 Zaborov,
                      D. and Zacharias, M. and Zanin, R. and Zdziarski, A. A. and
                      Zech, A. and Zefi, F. and Ziegler, A. and Zorn, J. and
                      Żywucka, N.},
      collaboration = {H. E. S. S.{ Collaboration}},
      title        = {{T}he {H}.{E}.{S}.{S}. {G}alactic plane survey},
      journal      = {Astronomy and astrophysics},
      volume       = {612},
      issn         = {1432-0746},
      address      = {Les Ulis},
      publisher    = {EDP Sciences},
      reportid     = {PUBDB-2018-02035, arXiv:1804.02432},
      pages        = {A1},
      year         = {2018},
      note         = {© ESO},
      abstract     = {We present the results of the most comprehensive survey of
                      the Galactic plane in very high-energy (VHE) γ-rays,
                      including a public release of Galactic sky maps, a catalog
                      of VHE sources, and the discovery of 16 new sources of VHE
                      γ-rays. The High Energy Spectroscopic System (H.E.S.S.)
                      Galactic plane survey (HGPS) was a decade-long observation
                      program carried out by the H.E.S.S. I array of Cherenkov
                      telescopes in Namibia from 2004 to 2013. The observations
                      amount to nearly 2700 h of quality-selected data, covering
                      the Galactic plane at longitudes from ℓ = 250° to 65°
                      and latitudes |b|≤ 3°. In addition to the unprecedented
                      spatial coverage, the HGPS also features a relatively high
                      angular resolution (0.08° ≈ 5 arcmin mean point spread
                      function $68\%$ containment radius), sensitivity $(≲1.5\%$
                      Crab flux for point-like sources), and energy range
                      (0.2–100 TeV). We constructed a catalog of VHE γ-ray
                      sources from the HGPS data set with a systematic procedure
                      for both source detection and characterization of morphology
                      and spectrum. We present this likelihood-based method in
                      detail, including the introduction of a model component to
                      account for unresolved, large-scale emission along the
                      Galactic plane. In total, the resulting HGPS catalog
                      contains 78 VHE sources, of which 14 are not reanalyzed
                      here, for example, due to their complex morphology, namely
                      shell-like sources and the Galactic center region. Where
                      possible, we provide a firm identification of the VHE source
                      or plausible associations with sources in other astronomical
                      catalogs. We also studied the characteristics of the VHE
                      sources with source parameter distributions. 16 new sources
                      were previously unknown or unpublished, and we individually
                      discuss their identifications or possible associations. We
                      firmly identified 31 sources as pulsar wind nebulae (PWNe),
                      supernova remnants (SNRs), composite SNRs, or gamma-ray
                      binaries. Among the 47 sources not yet identified, most of
                      them (36) have possible associations with cataloged objects,
                      notably PWNe and energetic pulsars that could power VHE
                      PWNe.},
      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       = {1804.02432},
      howpublished = {arXiv:1804.02432},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1804.02432;\%\%$},
      UT           = {WOS:000429404700001},
      doi          = {10.1051/0004-6361/201732098},
      url          = {https://bib-pubdb1.desy.de/record/403344},
}