H.E.S.S. High Energy Stereoscopic System

Largest ever Cherenkov telescope sees first light

With a mass of almost 600 tons and its 28-meter mirror - the area of two tennis courts – the new arrival is just huge. This very large telescope named H.E.S.S. II saw its first light at 0:43 a.m. on 26 July 2012, detecting its very first images of atmospheric particle cascades generated by cosmic gamma rays and by cosmic rays, marking the next big step in exploring the Southern sky at gamma-ray energies. “The new telescope not only provides the largest mirror area among instruments of this type worldwide, but also resolves the cascade images at unprecedented detail, with four times more pixels per sky area compared to the smaller telescopes” states Pascal Vincent from the French team responsible for the photo sensor package at the focus of the mirror.

Gamma rays are believed to be produced by natural cosmic particle accelerators such as supermassive black holes, supernovae, pulsars, binary stars, and maybe even relics of the Big Bang. The universe is filled with these natural cosmic accelerators, impelling charged particles such as electrons and ions to energies far beyond what the particle accelerators built by mankind can reach. As high-energy gamma rays are secondary products of these cosmic acceleration processes, gamma ray telescopes allow us to study these high-energy sources. Today, well over one hundred cosmic sources of very high-energy gamma rays are known. With H.E.S.S. II, processes in these objects can be investigated in superior detail, also anticipating many new sources, as well as new classes of sources. In particular, H.E.S.S. II will explore the gamma ray sky at energies in the range of tens of Giga-electronvolts – the poorly-explored transition regime between space-based instruments and current ground-based telescopes, with a huge discovery potential.

The most extreme gamma ray emitters – Active Galactic Nuclei – shine in gamma rays with an apparent energy output which is one hundred times the luminosity of the entire Milky Way, yet the radiation seems to emerge from a volume much smaller than that of our Solar System, and turns on and off in a matter of minutes, a strong signature of supermassive black holes. For some of the objects seen with the four H.E.S.S. telescopes in the last years, no counterpart at other wavelengths is known; they may represent a new type of celestial object that H.E.S.S. II will help to characterize.

When gamma rays interact high up in the atmosphere, they generate a cascade of secondary particles that can be imaged by the telescopes on the ground and recorded in their ultra-fast photo sensor 'cameras', thanks to the emission known as Cherenkov radiation – a faint flash of blue light. The high-tech camera of H.E.S.S. II is able to record this very faint flash with an “exposure time” of a few billionths of a second, almost a million times faster than a normal camera. The H.E.S.S. II camera – with an area of the size of a garage door and a weight of almost 3 tons – is “flying” 36 meters above the primary mirror in the focal plane – at the height of a 20-story building when pointing up. Despite its size, the new telescope will be able to slew twice as fast as the smaller telescopes to immediately respond to fast and transient phenomena such as gamma ray bursts anywhere in the sky.

The telescope structure and its drive system were designed by engineers in Germany and South Africa, and produced in Namibia and Germany. The 875 hexagonal mirror facets which make up the huge reflector were manufactured in Armenia, and individually characterized in Germany. The mirror alignment system results from a cooperation of German and Polish institutes. The camera, with its integrated electronics, was designed and built in France. The construction of the new H.E.S.S. II telescope was driven and financed largely by German and French institutions, with significant contributions from Austria, Poland, South Africa and Sweden.

“The successful commissioning of the new H.E.S.S. II telescope represents a big step forward for the scientists of H.E.S.S., for the astronomical community as a whole, and for Southern Africa as a prime location for this field of astronomy” - so Werner Hofmann, spokesperson of the project – “H.E.S.S. II also paves the way to the realization of CTA – the Cherenkov Telescope Array— the next generation instrument ranked top priority by astroparticle physicists and funding agencies in Europe”.

The H.E.S.S. observatory has been operated for almost a decade by the collaboration of more than 170 scientists, from 32 scientific institutions and 12 different countries: Namibia and South Africa, Germany, France, the UK, Ireland, Austria, Poland, the Czech Republic, Sweden, Armenia, and Australia. To date, the H.E.S.S. Collaboration has published over 100 articles in high-impact scientific journals, including the top-ranked ‘Nature’ and ‘Science’ journals.

H.E.S.S. was awarded in 2006 the Descartes Prize of the European Commission - the highest recognition for collaborative research - and in 2010 the prestigious Rossi Prize of the American Astronomical Society. In a survey in 2006, H.E.S.S. was ranked the 10th most influential observatory worldwide, joining the ranks with the Hubble Space Telescope or the telescopes of the European Southern Observatory ESO in Chile.

For more information, see: H.E.S.S. home page and more information about the Cherenkov technique and the H.E.S.S. telescopes and about the physics of gamma sources studies with H.E.S.S.

Contacts

Prof. Dr. Werner Hofmann (H.E.S.S. Spokesperson), Max-Planck-Institut für Kernphysik, Heidelberg, +49 6221 516 330, werner.hofmann (at) mpi-hd.mpg.de

Dr. Michael Panter (H.E.S.S. Technical Coordinator), Max-Planck-Institut für Kernphysik, Heidelberg, +49 6221 516 273, michael.panter (at) mpi-hd.mpg.de

Prof. Dr. Stefan Wagner, Landessternwarte Heidelberg, +49 6221 541 712, S.Wagner (at) lsw.uni-heidelberg.de

Dr. Michael Punch (Deputy Spokesperson), APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, Paris, +33 1 57 27 60 81, punch (at) apc.univ-paris7.fr

Dr. Gerard Fontaine (Chair H.E.S.S. Board), Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, Palaiseau, +33 1 69 33 55 51, fontaine (at) admin.in2p3.fr

Dr. Pascal Vincent, LPNHE, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, Paris, +33 1 44 27 48 43, vincentp (at) in2p3.fr

Characteristics of the H.E.S.S. II telescope

Mount Mount type Alt-Az mount Azimuth drive system 12 wheels in 6 bogies on 36 m diameter rail

4 wheels driven by servo motors, plus backup motors

peak positioning speed 200 degr./minute

range +– 280 degr. from park position Height of elevation axis 24 m Elevation drive system Toothed ring on either side of the dish

2 drive units with 2 servo motors each, plus backup motors

peak positioning speed 100 degr./minute

range –125 degr. +90 degr. from vertical Dish Dimensions 32.6 m by 24.3 m; equivalent to 28 m circular dish Shape of reflector Parabolic Focal length 36 m Total mirror area 614 m2 Mirror facets 875 hexagonal facets of 90 cm (flat-to-flat) size

quartz-coated aluminized glass

weight per facet approx. 25 kg Facet alignment Each facet equipped with 2 actuators with 2 μm positioning step size Focal plane instrumentation (Camera) Photo sensors 2048 1-1/4’ photo multipliers Packaging 128 drawers of 16 PMTs each, drawer includes digitization, trigger, slow control, high voltage generation Pixel size 42 mm (hexagonal, flat-to-flat), equivalent to 0.067 degr. Sensitive area / field of view approx. 200 cm Ø, equivalent to 3.2 degr. on the sky Signal recording 1 GHz signal sampling using the SAM ASIC

2 gain channels for each pixel for large dynamic range

records signal amplitude, timing, and shape Effective exposure time 16 nano-seconds Image recording rate 3600 images/second Power consumption 8 kW Dimensions of camera body 227 cm wide x 240 cm high x 184 cm deep Camera weight 2.8 tons Camera support Quadrupod Weight of complete telescope 580 tons (incl. mirrors, camera)

Images

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