The amplifier on her bench was her own fear—a low-noise, wideband instrument intended for a gravitational-wave analog front end. The specifications read like a prayer: microvolts of noise, stability across decades of temperature, a life of flawless patience. The first prototypes had been noisy, angry things that whined at low frequencies. The second prototypes were shy, timid, and lost resolution. The third had a habit of latching up under the weight of its own precision.