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The upgrade of the H.E.S.S. cameras

Authors :
Marko Kossatz
Francois Toussnel
M. Füßling
Marek Penno
Markus Schade
Thomas Chaminade
Albert Jahnke
J. Thornhill
C. Stegmann
P. Manigot
Rachel Simoni
P. Nayman
Stefan Ohm
Constantin Steppa
Francois Brun
Jim Hinton
H. Leich
Stefan Klepser
Terry Ashton
Emmanuel Moulin
Vincent Marandon
Mathieu de Naurois
Gianluca Giavitto
Jean-Francois Glicenstein
V. Lefranc
H. Lüdecke
Iryna Lypova
Eric Delagnes
D. Ross
Thomas Schwab
D. Salek
David Berge
A. Kretzschmann
Tobias Gräber
G. Fontaine
A. Balzer
B. Giebels
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Laboratoire Leprince-Ringuet (LLR)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Deutsches Elektronen-Synchrotron [Zeuthen] (DESY)
Helmholtz-Gemeinschaft = Helmholtz Association
University of Leicester
Gravitation AstroParticle Physics Amsterdam (GRAPPA)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Department of Computer and Information Sciences [Univ Strathclyde]
University of Strathclyde [Glasgow]
Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Source :
AIP Conf.Proc., 6th International Symposium on High-Energy Gamma-Ray Astronomy, 6th International Symposium on High-Energy Gamma-Ray Astronomy, Jul 2016, Heidelberg, Germany. pp.070008, ⟨10.1063/1.4969005⟩, Nuclear instruments & methods in physics research / A 876, 35-38 (2017). doi:10.1016/j.nima.2016.12.057, Nucl.Instrum.Meth.A, 9th International Workshop on Ring Imaging Cherenkov Detectors, 9th International Workshop on Ring Imaging Cherenkov Detectors, Sep 2016, Bled, Slovenia. pp.35-38, ⟨10.1016/j.nima.2016.12.057⟩
Publication Year :
2016
Publisher :
HAL CCSD, 2016.

Abstract

International audience; The High Energy Stereoscopic System (HESS) is an array of imaging atmospheric Cherenkov telescopes (IACTs) located in the Khomas highland in Namibia. It was built to detect Very High Energy (VHE >100GeV ) cosmic gamma rays. Since 2003, HESS has discovered the majority of the known astrophysical VHE gamma-ray sources, opening a new observational window on the extreme non-thermal processes at work in our universe. HESS consists of four 12-m diameter Cherenkov telescopes (CT1–4), which started data taking in 2002, and a larger 28-m telescope (CT5), built in 2012, which lowers the energy threshold of the array to 30GeV . The cameras of CT1–4 are currently undergoing an extensive upgrade, with the goals of reducing their failure rate, reducing their readout dead time and improving the overall performance of the array. The entire camera electronics has been renewed from ground-up, as well as the power, ventilation and pneumatics systems, and the control and data acquisition software. Only the PMTs and their HV supplies have been kept from the original cameras. Novel technical solutions have been introduced, which will find their way into some of the Cherenkov cameras foreseen for the next-generation Cherenkov Telescope Array (CTA) observatory. In particular, the camera readout system is the first large-scale system based on the analog memory chip NECTAr, which was designed for CTA cameras. The camera control subsystems and the control software framework also pursue an innovative design, exploiting cutting-edge hardware and software solutions which excel in performance, robustness and flexibility. The CT1 camera has been upgraded in July 2015 and is currently taking data; CT2-4 have been upgraded in fall 2016. Together they will assure continuous operation of HESS at its full sensitivity until and possibly beyond the advent of CTA. This contribution describes the design, the testing and the in-lab and on-site performance of all components of the newly upgraded HESS camera.

Details

Language :
English
Database :
OpenAIRE
Journal :
AIP Conf.Proc., 6th International Symposium on High-Energy Gamma-Ray Astronomy, 6th International Symposium on High-Energy Gamma-Ray Astronomy, Jul 2016, Heidelberg, Germany. pp.070008, ⟨10.1063/1.4969005⟩, Nuclear instruments & methods in physics research / A 876, 35-38 (2017). doi:10.1016/j.nima.2016.12.057, Nucl.Instrum.Meth.A, 9th International Workshop on Ring Imaging Cherenkov Detectors, 9th International Workshop on Ring Imaging Cherenkov Detectors, Sep 2016, Bled, Slovenia. pp.35-38, ⟨10.1016/j.nima.2016.12.057⟩
Accession number :
edsair.doi.dedup.....9851e9efc5a3f6627859d5b52a3ef0b4
Full Text :
https://doi.org/10.1063/1.4969005⟩