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The H.E.S.S. Extragalactic sky survey with the first decade of observations

  • F. Aharonian
  • , F. Ait Benkhali
  • , J. Aschersleben
  • , H. Ashkar
  • , M. Backes
  • , V. Barbosa Martins
  • , R. Batzofin
  • , Y. Becherini
  • , D. Berge
  • , K. Bernlöhr
  • , M. Böttcher
  • , C. Boisson
  • , J. Bolmont
  • , M. De Bony De Lavergne
  • , J. Borowska
  • , M. Bouyahiaoui
  • , F. Bradascio
  • , R. Brose
  • , A. Brown
  • , F. Brun
  • B. Bruno, T. Bulik, C. Burger-Scheidlin, T. Bylund, S. Casanova, J. Celic, M. Cerruti, T. Chand, S. Chandra, A. Chen, J. Chibueze, O. Chibueze, G. Cotter, P. Cristofari, J. D. Mbarubucyeye, I. D. Davids, J. Devin, J. Djuvsland, A. Dmytriiev, K. Egberts, S. Einecke, S. Fegan, G. Fontaine, S. Funk, S. Gabici, J. F. Glicenstein, J. Glombitza, P. Goswami, G. Grolleron, L. Haerer, B. Hea, J. A. Hinton, W. Hofmann, T. L. Holch, M. Holler, D. Horns, Zhiqiu Huang, M. Jamrozy, F. Jankowsky, A. Jardin-Blicq, E. Kasai, K. Katarzyaski, R. Khatoon, B. Khélifi, Nu Komin, K. Kosack, D. Kostunin, A. Kundu, R. G. Lang, S. Le Stum, A. Lemière, M. Lemoine-Goumard, J. P. Lenain, F. Leuschner, A. Luashvili, J. Mackey, D. Malyshev, V. Marandon, G. Martí-Devesa, R. Marx, A. Mehta, A. Mitchell, R. Moderski, L. Mohrmann, A. Montanari, M. De Naurois, J. Niemiec, P. O-Brien, L. Olivera-Nieto, E. De Ona Wilhelmi, M. Ostrowski, S. Panny, M. Panter, U. Pensec, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Ravikularaman, M. Regeard, A. Reimer, O. Reimer, I. Reis, H. Ren, B. Reville, F. Rieger, G. Rowell, B. Rudak, E. Ruiz-Velasco, V. Sahakian, H. Salzmann, D. A. Sanchez, A. Santangelo, M. Sasaki, J. Schäfer, F. Schüssler, J. N.S. Shapopi, A. Sharma, H. Sol, S. Spencer, Stawarz, R. Steenkamp, S. Steinmassl, C. Steppa, H. Suzuki, T. Takahashi, T. Tanaka, A. M. Taylor, R. Terrier, A. Thakur, M. Tsirou, C. Van Eldik, M. Vecchi, C. Venter, J. Vink, H. J. Völk, T. Wach, S. J. Wagner, A. Wierzcholska, M. Zacharias, A. A. Zdziarski, A. Zech, N. Åywucka
  • Dublin Institute for Advanced Studies
  • Max-Planck-Institut für Kernphysik
  • Yerevan State University
  • Landessternwarte Heidelberg
  • University of Groningen
  • University of Namibia
  • North-West University
  • c/o DESY
  • University of Potsdam
  • Astroparticule and Cosmol APC
  • Linnaeus University, Växjö
  • Humboldt-Universität zu Berlin
  • LUTH - Laboratoire de l'Univers et de ses Theories
  • Sorbonne Université
  • Université Paris-Saclay
  • University of Oxford
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • University of Warsaw
  • Institute for Nuclear Physics
  • University of the Witwatersrand, Johannesburg
  • Laboratoire Univers et Particules de Montpellier
  • University of Adelaide
  • Ip Paris
  • University of Tübingen
  • University of Innsbruck
  • Universität Hamburg
  • Jagiellonian University
  • UMR 5797
  • Nicolaus Copernicus University
  • Aix-Marseille Université
  • Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
  • University of Leicester
  • Université Savoie Mont Blanc
  • Yerevan Physics Institute
  • Konan University
  • University of Tokyo
  • University of Amsterdam

Research output: Contribution to journalArticlepeer-review

Abstract

The results of the first extragalactic gamma-ray survey by the High Energy Stereoscopic System (H.E.S.S.) are presented. The survey comprises 2720 hours of very high-energy gamma-ray observations of the extragalactic sky, recorded with H.E.S.S. from 2004 up to the end of 2012. These data have been re-analysed using a common consistent set of up-to-date data calibration and analysis tools. From this analysis, a list of 23 detected objects, predominantly blazars, was obtained. This catalogue was assessed in terms of the source class populations that it contains. The level of source parameter bias for the blazar sources, probed by this observational dataset, was evaluated using Monte-Carlo simulations. Spectral results obtained with the H.E.S.S. data were compared with the Fermi-LAT catalogues to present the full gamma-ray picture of the detected objects. Lastly, this unique dataset was used to assess the contribution of BL Lacertae objects and flat-spectrum radio quasars to the extragalactic gamma-ray background light at several hundreds of gigaelectronvolts. These results are accompanied by the release of the high-level data to the astrophysical community.

Original languageEnglish
Article numberA261
JournalAstronomy and Astrophysics
Volume695
DOIs
Publication statusPublished - 1 Mar 2025

Keywords

  • BL Lacertae objects: general
  • Galaxies: Active
  • Galaxies: jets
  • Gamma rays: galaxies
  • Gamma rays: general

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