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Davide Lasi
Project Manager of cross-functional teams • MIT System Design and Management • Stanford Certified PM • SCPO
Davide Lasi is currently the Science Instrument Project Manager at TMT International Observatory, LLC, where he plays a significant role in managing the development of advanced astronomical instruments. He has been particularly involved with the Wide-Field Optical Spectrometer (WFOS), a major project aimed at enhancing observational capabilities for astronomy. Under his leadership, WFOS successfully passed its Conceptual Design Review, marking a critical milestone in its development.24
Professional Background
Lasi's expertise lies in project management and system engineering within the field of astronomy. His work on WFOS involves overseeing cross-functional teams and ensuring that the instrument meets its scientific and engineering requirements. The WFOS is designed to be the largest UV/visible monolithic optical imaging spectrograph, intended for use with the Thirty Meter Telescope (TMT), which aims to significantly advance our understanding of various astronomical phenomena.23
Education and Research
Davide Lasi has an academic background that includes research contributions published in various scientific journals. He has been cited in numerous publications, indicating his active involvement in research and development within the astronomical community.3 His educational credentials include a degree from MIT's System Design and Management program, which equips him with a robust foundation in both technical and managerial aspects of complex projects.1
Current Role
In his role at TMT International Observatory, Lasi is responsible for ensuring that the WFOS instrument is designed for high sensitivity across a wide spectral range, facilitating studies of galaxy formation, stellar populations, and transient astrophysical events.24 His leadership is crucial to the success of this international collaboration involving teams from multiple countries.
Overall, Davide Lasi's contributions to the TMT project are pivotal in pushing the boundaries of astronomical research and technology.

