# The Cherenkov Telescope Array

## TL;DR

The Cherenkov Telescope Array (CTA) is a next-generation gamma-ray observatory with over 100 telescopes, aiming to explore high-energy astrophysics with unprecedented precision and open data access.

## Contribution

This paper details the current status of CTA's construction, prototype development, and its scientific potential in gamma-ray astronomy.

## Key findings

- CTA will cover 20 GeV to 300 TeV energy range.
- It will be one of the largest astronomical infrastructures.
- The project is progressing with prototype testing and site preparations.

## Abstract

The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory for gamma-ray astronomy at very-high energies. It will be capable of detecting gamma rays in the energy range from 20 GeV to more than 300 TeV with unprecedented precision in energy and directional reconstruction. With more than 100 telescopes of three different types it will be located in the northern hemisphere at La Palma, Spain, and in the southern at Paranal, Chile. CTA will be one of the largest astronomical infrastructures in the world with open data access and it will address questions in astronomy, astrophysics and fundamental physics in the next decades. In this presentation we will focus on the status of the CTA construction, the status of the telescope prototypes and highlight some of the physics perspectives.