Roque de los Muchachos Observatory

Large Size Telescope

LST
Large Size Telescope (LST)
Diameter
Ø 2300.00 cm
Purpose
Owner institution
State
Operation year
2018

    The Large Size Telescopes (LSTs) are the largest CTA telescopes, and are
    optimized to detect the lowest energy gamma-rays. That energy regime is
    extremely relevant because it allows the detection of the most distant gamma
    ray sources (extragalactic objects such as active galatic nuclei at cosmological
    distances) and of those sources with a limited acceleration power (galactic
    sources such as pulsars). It should also allow the discovery of VHE gamma ray
    emission in Gamma Ray Bursts (GRB).
    The fact that GRBs are very fast is behind the very low weight of the LSTs:
    they should be able to reposition to any direction in the sky in less than 20
    seconds after receiving an alert from a GRB monitor. In order to achieve a
    large size and light weight, the telescope structure is made of a carbon-fibre
    tube network (mirroring the design of the MAGIC telescope). Since strong
    winds may lift such a large and light-weight structure, the rail and bogies
    are designed to prevent uplift. And in order to discriminate the light flashes
    produced by the lowest energy gamma rays from the light of the night sky the
    LST camera is the fastest and most sensitive one in CTA.
    Four such telescopes will operate in each hemisphere to observe the gamma
    rays “in stereo”, a technique that allows a cleaner reconstruction of the
    properties of the gamma ray.
    The cost of each LST is about eight million euros and the first one will be a
    prototype to be tested during 2017.

    • Prototype for the most sensitive array of Cherenkov telescopes in the world
      below 100 GeV
      • Dish diameter: 23 metres
      • Energy Range: very-high-energy gamma rays between 20 GeV and several TeV
      • Objective: the study of the origin of cosmic rays and their impact on the constituents
      of the Universe and the study of the ultimate nature of matter and physics
      beyond the Standard Model, searching for dark matter and effects of quantum
      gravity.

    Existing Cherenkov telescopes, MAGIC (in La Palma), HESS (in Namibia) and
    VERITAS (in USA) have revealed a Universe rich in objects producing the
    highest energy gamma ray radiation. Over 150 sources have been discovered.
    They reveal the existence of powerful particle accelerators in the sky.
    To understand how these cosmic machines work, over one thousand
    scientists and engineers from around the world are working together to build
    a new observatory: the Cherenkov Telescope Array (CTA). Two observatories
    composed by arrays of tens of telescopes will be built, one in each of the
    hemispheres, so as to cover the whole sky. Each array will consist of different
    telescope types.
    A few large (23 m diameter) telescopes will be at the centre, surrounded by a
    handful of medium sized (12 m diameter) telescopes. In addition, the Southern
    array will host tens of small telescopes (around 6 m diameter).
    It should be completed in 2021 and its operation should span over 30 years.

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