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Martyn Brake is a key figure in the development of next-generation astronomical instrumentation, with a primary focus on high-precision radial velocity spectrographs for exoplanet detection. His most notable contribution is his leadership in the design and integration of the HARPS3 instrument, a high-resolution (R≈115,000) echelle spectrograph covering 380–690 nm, planned for installation on a roboticized Isaac Newton Telescope. Brake’s work on the HARPS3 software system is particularly significant: he designed a distributed, event-driven control architecture enabling fully robotic operation, a critical advancement for long-term, automated exoplanet surveys. This system allows for the precise, stable measurements needed to detect Earth-mass planets around Sun-like stars. While his most-cited paper (2016, 34 citations) outlines the instrument’s capabilities, his later work on the software integration (2018, 2 citations) details the practical engineering challenges of coordinating complex subsystems. Brake’s contributions bridge the gap between cutting-edge optical design and robust, autonomous observatory control, making him a vital contributor to the next generation of exoplanet discovery tools.