Cherenkov Telescope Array

The Cherenkov Telescope Array Observatory (CTAO) is a multinational project to build a new generation of ground-based gamma-ray instruments in the energy range extending from some tens of GeV to about 300 TeV. It is proposed as an open observatory and will consist of two arrays of imaging atmospheric Cherenkov telescopes, a first array at the Northern Hemisphere, on the Spanish island of La Palma, with emphasis on the study of extragalactic objects at the lowest possible energies, and a second array at the Southern Hemisphere, in the Atacama Desert in Chile, which is to cover the full energy range and concentrate on galactic sources. The physics program of the CTAO goes beyond high-energy astrophysics into cosmology and fundamental physics.

Building on the technology of current-generation ground-based gamma-ray detectors ( MAGIC, HESS, and VERITAS), the CTAO will be ten times more sensitive and have unprecedented accuracy in its detection of high-energy gamma rays. Current gamma-ray telescope arrays host up to five individual telescopes, but the CTAO is designed to detect gamma rays over a larger area and a wider range of views, with more than 60 telescopes located in the northern and southern hemispheres.

In January 2025, the CTAO was established as a European Research Infrastructure Consortium (ERIC) by the European Commission.

The project is part of the Aspera European Astroparticle network and of Astronet.

Locations

The CTAO headquarters is hosted by the National Institute for Astrophysics in Italy, and the Science Data Management Centre is hosted by the Deutsches Elektronen-Synchrotron in Zeuthen, Germany.

The CTAO's northern-hemisphere site, CTAO-North, is located on the existing site of the  Instituto de Astrofísica de Canarias' Roque de los Muchachos Observatory, on the island of La Palma, the fifth largest of the Canary Islands. At 2,200 metres of altitude and nestled on a plateau below the rim of an extinct volcanic crater, the site hosts a prototype of the LST, the LST-1, and LST-2, LST-3, and LST-4 are under construction. The site will also host MSTs.

The CTAO's southern-hemisphere site, CTAO-South, is located less than 10 km southeast of the ESO's Paranal Observatory, in the Atacama Desert of Chile. The site will host MSTs and SSTs.

Science

The CTAO will look at higher-energy photons than ever measured before. Its cosmic particle accelerators can reach energies inaccessible to such accelerators as the Large Hadron Collider. The CTAO will seek to understand the impact of high-energy particles in the evolution of cosmic systems and to gain insight into the most extreme and unusual phenomena in the Universe. It will also search for annihilating dark matter particles and deviations from Einstein's theory of special relativity, even conducting a census of particle acceleration in the universe.

Research at the CTAO will seek to address questions in and beyond astrophysics. The CTAO's observations will include the following key targets: Galactic Center, Large Magellanic Cloud, Galactic Plane, galaxy clusters, cosmic ray PeVatrons, star-forming systems, active galactic nuclei, and transient phenomena.

Possible increase of light pollution

The planned INNA megaproject by  AES Andes, with 1,000 light sources installed just five km from the southern part of the CTAO, threatens to increase light pollution at the location by 55%.

See also

* Cherenkov radiation
* List of telescope types
* Major Atmospheric Cerenkov Experiment Telescope
* Pavel Cherenkov
* Segmented mirror

References

External links

*

European Commission's Decision to Establish the CTAO as an ERIC

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