Kovac leads the BICEP/Keck CMB-polarization program at the South Pole, designing and deploying multiple generations of radio telescopes and cryogenic detector arrays (TES bolometers with SQUID-multiplexed readout) to search for the inflationary gravitational-wave signature in the cosmic microwave background. This is an astronomy pivot squarely enabled by quantum-limited cryogenic detector technology, matching the CMB-instrumentation branch of the quantum-sensing tree.