邹虎，中国科学院国家天文台博士生导师，大视场巡天与星系物理团组首席科学家，入选国家级青年人才计划。2006年本科毕业于中南大学数学系，2011 年博士毕业于中国科学院研究生院，毕业后留台工作至今。发表论文130余篇，专注于大视场巡天和星系形成演化研究，在近邻星系、星系团致密环境、星系标度关系及星系活动性等领域取得了重要研究成果。领导国内两项测光巡天项目：南银冠u波段巡天（SCUSS）和北京-亚利桑那巡天，并深度参与SDSS-IV和DESI国际合作，担任DESI中方合作组负责人。The Dark Energy Spectroscopic Instrument (DESI) is a large-scale international collaborative spectroscopic survey project supported by the U.S. Department of Energy, recognized as a Stage IV dark energy experiment. The project involves upgrading the 4-meter Mayall Telescope at Kitt Peak National Observatory, equipping it with 5,000 robotic fiber positioners to achieve highly efficient observations within a 3.2-degree field of view. Over its five-year mission, DESI aims to collect spectroscopic data from over 40 million celestial objects. Its primary scientific goals are to construct the most detailed three-dimensional map of the universe, precisely chart the history of cosmic accelerated expansion, and study the growth patterns of large-scale structures, thereby unveiling the nature of dark energy. By gathering an order of magnitude more spectroscopic data than previous galaxy redshift surveys, DESI will significantly advance our understanding of dark energy, galaxy formation and evolution, and the structure of the Milky Way. This talk provides an overview of the DESI project, highlights its latest scientific achievements, showcases research progress by the survey team at NAOC based on DESI data, and explores future spectroscopic survey initiatives in China.