Impact of the Galactic Compact-Binary Foreground on Stochastic Gravitational-Wave Background Amplitude Inference in the Millihertz Band

Oral presentation (morning session, July 31) at the 2026 Mid-Year Exchange Meeting of the project “Signal Simulation, Processing, and Verification Technologies for Space Gravitational-Wave Detection” (空间引力波探测信号仿真、处理与验证技术研究), under the Gravitational-Wave Detection Special Project of the National Key R&D Program of China (国家重点研发计划引力波探测专项), held July 30 – August 2, 2026 in Yangzhou, Jiangsu.

The talk presents the work in arXiv:2607.25349 on how residual power from the Galactic compact-binary foreground in the millihertz band affects the inference of the stochastic gravitational-wave background amplitude.