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C. G. Tinney is a leading figure in exoplanetary science, with a career defined by the discovery and characterization of planets beyond our solar system. His key research areas include the detection of exoplanets via radial velocity and transit methods, the development of precision instrumentation, and the study of planetary system architectures. Tinney’s major contributions are exemplified by his leadership in the MINERVA-Australis project, a dedicated telescope array in the Southern Hemisphere designed for the follow-up and mass measurement of planets discovered by NASA’s TESS mission. This facility is almost unique in its ability to confirm and characterize TESS candidates, providing critical mass measurements for these worlds. With over 21 citations, the foundational paper on MINERVA-Australis highlights its impact on the field. Tinney is also renowned for his work on the Anglo-Australian Planet Search, which discovered numerous long-period giant planets, and for his role in the development of the HARPS spectrograph, a gold standard for radial velocity precision. His research has profoundly shaped our understanding of planetary demographics and the techniques used to explore them.