معرفی
Kenny Lau is a Postdoctoral Scholar and Research Associate in Physics at the California Institute of Technology, specializing in experimental cosmology. He focuses on measuring microwave signals from the early universe, including the Epoch of Reionization (EoR) and the Cosmic Microwave Background (CMB), through collaborations like BICEP/Keck, TIME, and CMB-S4. His work involves instrument development, data analysis, and telescope deployment at remote sites such as the South Pole.
Education: Ph.D. in Physics from the University of Minnesota (2023), M.Sc. and B.Sc. from the Chinese University of Hong Kong. Research contributions include analyzing CMB B-mode polarization data to constrain inflationary models, developing the BICEP Array telescope mount, and deploying instruments at the Amundsen-Scott South Pole Station. His expertise spans cosmological parameter estimation, foreground separation, and experimental instrumentation for millimeter-wave astronomy.
Key projects include the BICEP Array telescope mount assembly and deployment, contributing to first-light observations of CMB polarization at 40 GHz. His technical work includes detector module development, vacuum window design, and calibration techniques for high-sensitivity CMB experiments.
