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  • richardmitnick 12:04 pm on April 15, 2014 Permalink | Reply
    Tags: , , , Cherenkov Telescope Array, ,   

    From ESO: “ESO Site Shortlisted for Cherenkov Telescope Array” 

    European Southern Observatory

    15 April 2014

    Lars Lindberg Christensen
    Head of ESO ePOD
    ESO ePOD, Garching, Germany
    Tel: +49 89 3200 6761
    Cellular: +49 173 3872 621
    E-mail: lars@eso.org

    ESO’s Paranal–Armazones site in Chile has been shortlisted as one of two potential sites in the southern hemisphere for the international Cherenkov Telescope Array (CTA) — a large array for ground-based gamma-ray astronomy. This is an important step towards the realisation of the project and if the site is selected, this will open up a new frontier for ESO.


    On 10 April 2014 Government representatives from the 12 of the countries involved in the Cherenkov Telescope Array (CTA) project met in Munich and decided to start negotiations with the two sites — Aar in Namibia and ESO’s Paranal–Armazones site in Chile — keeping Leoncito in Argentina as a third option.

    The CTA project is an initiative to build the next generation of ground-based, very high energy gamma-ray instruments. The CTA project aims to use detection of high-energy gamma-rays to provide a deeper insight into the high-energy Universe.

    The representatives received consultation from an international Site Selection Committee as well as the CTA consortium’s extensive input on the merits of the proposed sites. The Consortium expects to close the site selection by the end of 2014.

    The spokesperson of the CTA Consortium, Professor Werner Hofmann said: “The site choice is on the critical path towards implementing CTA; this decision represents a major step forward and we appreciate very much the engagement and support of the funding agencies and the country delegates involved in the decision.”

    Gamma-rays are emitted by the hottest and most powerful objects in our Universe — such as supermassive black holes, supernovae and possibly remnants of the Big Bang. When a high-energy gamma photon hits the Earth’s atmosphere, it may produce a cascade of secondary particles and cause emission of what is known as Cherenkov radiation — a characteristic faint blue visible-light flash. This flash may last only a few billionths of a second so must be imaged with super-fast and sensitive cameras and with telescopes of enormous light gathering power.

    The Cherenkov Telescope Array is a multinational, world-wide project with which 1000 scientists and engineers from 28 countries and over 170 research institutes are involved. The CTA will provide an order-of-magnitude jump in sensitivity over current instruments, providing novel insights into some of the most extreme processes in the Universe. Most systems measuring Cherenkov radiation use only a handful of telescopes, but the CTA will consist of about 100 Cherenkov telescopes of 23-metre, 12-metre and 4-metre dish sizes located in the southern hemisphere, plus a smaller site in the northern hemisphere. An array of this size will increase the number of detected flashes, it will also cover the full energy range [3] and improve drastically upon the angular resolution [4], allowing for identification of the emitting objects at other wavelengths.

    “Although formal discussions have not yet started, the shortlisting of Paranal-Armazones as a potential site for CTA illustrates the excellence of the site and the infrastructure for the Very Large Telescope and European Extremely Large Telescope. If chosen, CTA would take advantage of ESO’s great expertise in ground-based astronomy.” said ESO’s Director General, Tim de Zeeuw. “We look forward to the discussions with CTA.”

    See the full article, with notes here.

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  • richardmitnick 11:07 am on June 27, 2012 Permalink | Reply
    Tags: , , , Cherenkov Telescope Array,   

    From ISGTW: “The grand vision of the Cherenkov Telescope Array” 

    June 27, 2012
    Adrian Giordani

    The Cherenkov Telescope Array (CTA) will consist of two arrays of telescopes in two different hemispheres, allowing full coverage of the sky. The south CTA will cover about one square kilometer (0.39 square miles) of land with around 60 telescopes that will monitor all the energy ranges in the center of the Milky Way’s galactic plane. The north CTA will cover three square kilometers (1.16 square miles) and be composed of 30 telescopes. These telescopes will be targeted at extragalactic astronomy.

    An artist’s impression of the final constructed Cherenkov Telescope Array. Image courtesy G. Perez, SMM, IAC.

    ‘CTA opens a new window of essentially unexplored photon energies,’ said Giovanni Bignami, president of the Italian National Institute for Astrophysics (INAF). ‘Its potential impact is enormous: part of it, we imagine, will consist in discovering thousands of new [very-high-energy photon] sources, and part of it will be surprises. It’s the surprises we like best, and it’s the surprises that will most appeal to the public at large.’

    The project represents a major global effort with research groups from Africa, Argentina, Brazil, India, Japan, Mexico, and the US. There are currently more than 27 countries, and over 1,000 scientists involved.

    What is the goal of the CTA?

    The project will be composed of a collection of Cherenkov telescopes that will scan the universe at very-high-energy gamma-rays from 100 giga-electronvolts to about 100 tera-electronvolts; energies which are one hundred billion to one hundred trillion times higher than of visible light.The CTA will also investigate cosmic processes that create particles travelling close to the speed of light.

    The CTA combines the fields of astronomy, astrophysics, and fundamental physics research. Studies will include the origin of cosmic rays and their impact on other bodies within the universe. Researchers will investigate galactic particle accelerators, black holes, extragalactic gamma rays, dark matter, and the effects of quantum gravity.”

    See the full article here.

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