Gamma-ray blazar spectra with H.E.S.S. II mono analysis: The case of PKS 2155−304 and PG 1553+113
2017
The support of the Namibian authorities and of the University
of Namibia in facilitating the construction and operation of H.E.S.S. is
gratefully acknowledged, as is the support by the German Ministry for Education
and Research (BMBF), the Max Planck Society, the German Research
Foundation (DFG), the French Ministry for Research, the CNRS-IN2P3 and the
Astroparticle Interdisciplinary Programme of the CNRS, the UK Science and
Technology Facilities Council (STFC), the IPNP of the Charles University, the
Czech Science Foundation, the Polish Ministry of Science and Higher Education,
the South African Department of Science and Technology and National
Research Foundation, the University of Namibia, the Innsbruck University, the
Austrian Science Fund (FWF), and the Austrian Federal Ministry for Science,
Research and Economy, and by the University of Adelaide and the Australian
Research Council. We appreciate the excellent work of the technical support
staff in Berlin, Durham, Hamburg, Heidelberg, Palaiseau, Paris, Saclay, and in
Namibia in the construction and operation of the equipment. This work bene-
fited from services provided by the H.E.S.S. Virtual Organisation, supported by
the national resource providers of the EGI Federation. The Fermi-LAT Collaboration
acknowledges generous ongoing support from a number of agencies and
institutes that have supported both the development and the operation of the LAT
as well as scientific data analysis. These include the National Aeronautics and
Space Administration and the Department of Energy in the United States, the
Commissariat a l’Energie Atomique and the Centre National de la Recherche
Scientifique/Institut National de Physique Nucleaire et de Physique des Particules
in France, the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica
Nucleare in Italy, the Ministry of Education, Culture, Sports, Science and Technology
(MEXT), High Energy Accelerator Research Organization (KEK) and
Japan Aerospace Exploration Agency (JAXA) in Japan, and the K. A. Wallenberg
Foundation, the Swedish Research Council and the Swedish National Space
Board in Sweden. Additional support for science analysis during the operations
phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in
Italy and the Centre National d’Etudes Spatiales in France. This research has
made use of NASA’s Astrophysics Data System. This research has made use of
the SIMBAD database, operated at CDS, Strasbourg, France. This research made
use of Enrico, a community-developed Python package to simplify Fermi-LAT
analysis (Sanchez & Deil 2013). M. Razzano is funded by contract FIRB-2012-
RBFR12PM1F from the Italian Ministry of Education, University and Research
(MIUR).
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