Survey astronomy is a branch of astronomy that involves conducting large-scale systematic surveys of the sky to study various celestial objects and phenomena. These surveys often use advanced telescopes and imaging technologies to gather data on a wide range of astronomical objects, such as stars, galaxies, and other celestial bodies. Survey astronomy plays a crucial role in helping astronomers to map the universe, identify new astronomical objects, and study the distribution and properties of different types of objects in the cosmos. By conducting large-scale surveys, astronomers can uncover new insights into the structure and evolution of the universe, as well as improve our understanding of the physics and processes that govern celestial objects. Some of the key goals of survey astronomy include studying the distribution of galaxies in the universe, identifying and characterizing exoplanets, studying the properties of different types of stars, and searching for potential sources of gravitational waves. Survey astronomy has led to numerous discoveries and advancements in our understanding of the universe, making it a vital and active area of research in the field of astronomy.