MAGAO-X (Magellan Adaptive Optics-Xtreme) is a cutting-edge adaptive optics system installed on the Magellan Clay telescope in Chile. It is designed to provide astronomers with high-resolution images of distant astronomical objects by compensating for the distortion caused by Earth's atmosphere. MAGAO-X utilizes advanced technology such as deformable mirrors and wavefront sensors to correct for atmospheric turbulence in real-time, allowing for clearer and more detailed observations of celestial bodies. This research area aims to improve our understanding of the universe by enabling astronomers to study phenomena such as exoplanets, star formation, and black holes with unprecedented clarity and detail.