Instrumentation, Software, and Data Analysis for Cosmology
I work on experimental cosmology with a focus on detector instrumentation, cryogenic systems, and data analysis for millimeter-wave telescopes. My research spans the full pipeline—from hardware characterization to software development and end-to-end data processing.
The Tomographic Ionized-carbon Mapping Experiment (TIME) is a spectroscopic survey instrument designed to observe large-scale structure and the epoch of reionization using [CII] line emission. I contribute to calibration, detector characterization, and data-processing pipeline development.
The CCAT-prime telescope is a large-aperture submillimeter observatory designed for cosmic microwave background and line-intensity mapping science. I work on software, instrumentation integration, and analysis tools for observations using microwave detectors (mKIDs).
Transition-Edge Sensors are cryogenic bolometric detectors that operate at superconducting transition temperatures. I work with TES arrays for TIME, focusing on characterization and noise analysis using SQUIDS.
Microwave Kinetic Inductance Detectors are resonator-based superconducting detectors used in CCAT's PrimeCam module. I work on mKID detector analysis and characterisation for large-format arrays.