A new era in exploring the extreme universe: The large-sized telescope sub-array is inaugurated on CTAO-north
Cherenkov Telescope Array
image:
The four Large-Sized Telescopes (LSTs) will form the core of the CTAO-North array at the Roque de los Muchachos Observatory in La Palma, Spain.
view moreCredit: LST Collaboration
La Palma, Spain, 15 October 2026 – Two hundred and fifty scientists and representatives from leading research institutions around the world celebrated the inauguration of the Large-Sized Telescope (LST) sub-array at the CTAO-North site at the Roque de los Muchachos Observatory in La Palma, Spain. The completion of the four telescopes marks a significant milestone for the global astrophysics community and represents a crucial step toward the full scientific operation of the Cherenkov Telescope Array Observatory (CTAO).
Each telescope features a 23-meter-diameter reflector and is equipped with state-of-the-art ultra-fast cameras. Designed to detect the faint Cherenkov light flashes when very high-energy gamma rays interact with the Earth's atmosphere, the LSTs are the most sensitive instruments in the world for observing gamma rays at energies between approximately 20 gigaelectronvolts (GeV) and several teraelectronvolts (TeV).
This exceptional sensitivity is crucial for detecting distant and transient gamma-ray sources. As very high-energy gamma rays are increasingly absorbed as they travel across the Universe, the LSTs’ low-energy threshold enables scientists to probe sources at cosmological distances, to look further back in cosmic history, and to see the very short variability of dynamically evolving gamma-ray sources with greater statistical accuracy.
A productive pioneer: the LST-1
Even during its commissioning phase, the Large-Sized Telescope prototype (LST-1) has produced groundbreaking results since 2020. These include observations of pulsars, studies of active galactic nuclei at cosmological distances, and rapid follow-up observations of transient phenomena such as novae and gamma-ray bursts.
With the three new LSTs (LST-2, LST-3, and LST-4) joining the existing LST-1, the four telescopes will become a true array. By observing the same gamma-ray showers simultaneously from multiple directions, the sub-array will provide substantially improved sensitivity, angular resolution, and energy reconstruction, opening up a new level of precision in the study of the gamma-ray Universe.
"The completion of the LST sub-array is the culmination of more than fifteen years of international collaboration and technological innovation," said Prof. Masahiro Teshima, the Principal Investigator of the LST Collaboration and Spokesperson of the CTAO Consortium. "These telescopes will allow us to explore some of the most extreme environments in the Universe, including supermassive black holes, neutron stars, the possible origins of cosmic rays, and the nature of dark matter."
Reaching out to the early Universe
The LSTs form the low-energy core of CTAO-North and will provide a unique opportunity to probe the Universe at an epoch roughly 12 billion years ago, when it was less than two billion years old. Their sensitivity to the lowest-energy gamma rays will enable the detection and study of bright VHE gamma-ray bursts at high redshift, potentially extending gamma-ray observations to sources at redshifts of around z∼4, and providing new insights into the early Universe.
Over the coming years, the LSTs will undergo commissioning and integration into CTAO operations. Alongside the other CTAO telescopes, planned for both of its arrays, they will address fundamental questions in astrophysics, particle physics, and cosmology, such as the nature of dark matter, the origin of cosmic rays, and the physics of extreme cosmic accelerators.
About the LST Collaboration
The Large-Sized Telescope (LST) Collaboration is an international consortium of scientists, engineers, and institutions dedicated to designing, constructing, and commissioning the LSTs for the CTAO. The collaboration has developed advanced technologies in optics, photodetectors, mechanics, and high-speed electronics to achieve the lowest energy threshold ever reached by ground-based gamma-ray observatories.
The project was made possible by a strong international partnership, involving institutions from Brazil, Bulgaria, Czech Republic, Croatia, France, Germany, Italy, Japan, Poland, Spain, and Switzerland.
About the CTAO
The CTAO (Cherenkov Telescope Array Observatory; www.ctao.org) will be the world’s largest and most powerful observatory for gamma-ray astronomy. The CTAO’s unprecedented accuracy and broad energy range (20 GeV- 300 TeV) will help to address some of the most perplexing questions in astrophysics, falling under three major themes: understanding the origin and role of relativistic cosmic particles; probing extreme environments, such as black holes or neutron stars; and exploring frontiers in physics, searching for dark matter or deviations from Einstein’s theory of relativity.
To cover its broad energy range, the CTAO will use three types of telescopes: the Large-Sized Telescope (LST), the Medium-Sized Telescope (MST), and the Small-Sized Telescope (SST). More than 60 telescopes will be distributed between two observation stations: CTAO-North in the northern hemisphere at the Roque de los Muchachos Observatory on La Palma, Spain, and CTAO-South in the southern hemisphere at the Paranal Observatory in the Atacama Desert, Chile.
The CTAO is a Big Data project. The Observatory will generate hundreds of petabytes (PB) of data in a year (~12 PB after compression). Based on its commitment to Open Science, the CTAO will be the first gamma-ray observatory of its kind to operate as an open, proposal-driven observatory providing public access to its high-level science data and software products.
The CTAO Central Organisation (legally, the CTAO ERIC) is in charge of the construction and operation of the Observatory, as well as the management of the CTAO’s four sites. The CTAO ERIC members include Austria, Croatia, the Czech Republic, the European Southern Observatory (ESO), France, Germany, Italy, Poland, Slovenia, Spain, and Switzerland. The Netherlands is also part of the CTAO ERIC as Observer. Further contributing countries — Australia, Brazil, Japan, South Africa, and the United States — are engaged in the process of joining the CTAO ERIC as Strategic Partners or Third Parties.
This group works in close cooperation with partners from around the world, including In-Kind Contribution Collaborations that are developing essential hardware and software, as well as the CTAO Consortium, a group of researchers who works on the scientific exploitation of the Observatory.
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About the LST Collaboration
The Large-Sized Telescope (LST) Collaboration is an international consortium of scientists, engineers, and institutions dedicated to designing, constructing, and commissioning the LSTs for the CTAO. The collaboration has developed advanced technologies in optics, photodetectors, mechanics, and high-speed electronics to achieve the lowest energy threshold ever reached by ground-based gamma-ray observatories.
The project was made possible by a strong international partnership, involving institutions from Brazil, Bulgaria, Czech Republic, Croatia, France, Germany, Italy, Japan, Poland, Spain, and Switzerland.
About the CTAO
The CTAO (Cherenkov Telescope Array Observatory; www.ctao.org) will be the world’s largest and most powerful observatory for gamma-ray astronomy. The CTAO’s unprecedented accuracy and broad energy range (20 GeV- 300 TeV) will help to address some of the most perplexing questions in astrophysics, falling under three major themes: understanding the origin and role of relativistic cosmic particles; probing extreme environments, such as black holes or neutron stars; and exploring frontiers in physics, searching for dark matter or deviations from Einstein’s theory of relativity.
To cover its broad energy range, the CTAO will use three types of telescopes: the Large-Sized Telescope (LST), the Medium-Sized Telescope (MST), and the Small-Sized Telescope (SST). More than 60 telescopes will be distributed between two observation stations: CTAO-North in the northern hemisphere at the Roque de los Muchachos Observatory on La Palma, Spain, and CTAO-South in the southern hemisphere at the Paranal Observatory in the Atacama Desert, Chile.
The CTAO is a Big Data project. The Observatory will generate hundreds of petabytes (PB) of data in a year (~12 PB after compression). Based on its commitment to Open Science, the CTAO will be the first gamma-ray observatory of its kind to operate as an open, proposal-driven observatory providing public access to its high-level science data and software products.
The CTAO Central Organisation (legally, the CTAO ERIC) is in charge of the construction and operation of the Observatory, as well as the management of the CTAO’s four sites. The CTAO ERIC members include Austria, Croatia, the Czech Republic, the European Southern Observatory (ESO), France, Germany, Italy, Poland, Slovenia, Spain, and Switzerland. The Netherlands is also part of the CTAO ERIC as Observer. Further contributing countries — Australia, Brazil, Japan, South Africa, and the United States — are engaged in the process of joining the CTAO ERIC as Strategic Partners or Third Parties.
This group works in close cooperation with partners from around the world, including In-Kind Contribution Collaborations that are developing essential hardware and software, as well as the CTAO Consortium, a group of researchers who works on the scientific exploitation of the Observatory.
The four Large-Sized Telescopes (LSTs), located in bottom right of photo, form the core of the CTAO-North array at the Roque de Los Muchachos Observatory on the island of La Palma.
The four Large-Sized Telescopes (LSTs), which are the cluster of four telescopes on the right, feature 23-meter-diameter reflectors and are equipped with state-of-the-art ultra-fast cameras. Designed to detect the faint Cherenkov light flashes when very high-energy gamma rays interact with the Earth's atmosphere, the LSTs are the most sensitive instruments in the world for observing gamma rays at energies between approximately 20 gigaelectronvolts (GeV) and several teraelectronvolts (TeV).
Credit
LST Collaboration
LST Collaboration
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