The MagAO (Magellan Adaptive Optics) project is a research area focused on developing and implementing adaptive optics technology for the Magellan telescopes located at the Las Campanas Observatory in Chile. Adaptive optics is a technique used to reduce the blurring effects of Earth's atmosphere on astronomical images, allowing for clearer and more detailed observations of celestial objects. The MagAO project aims to improve the resolution and quality of images obtained by the Magellan telescopes through the use of advanced adaptive optics systems. This research area has led to significant advancements in high-resolution imaging and spectroscopy of stars, galaxies, and other astronomical objects.