The Simons Observatory (SO) is a next-generation cosmic microwave background experiment designed to make definitive measurements of CMB polarization, including a sensitive search for primordial B-modes from cosmic inflation.

I hold a central leadership role in SO detector readout and data processing, overseeing readout performance and serving as time-ordered data preprocessing lead. This work includes coordinating on-site readout operations, developing and maintaining the preprocessing pipeline, and ensuring that instrument performance translates directly into analysis-ready data.

I am also part of a small core team delivering the inflationary B-mode analysis, where tight control of instrumental systematics and data quality is essential. This role places me at the interface between instrumentation and cosmological inference, enabling direct contributions to one of the most sensitive probes of early-universe physics.