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Fernando Gago is a leading instrumentalist in ground-based astronomy, recognized for his pivotal role in the development of EMIR, the near-infrared multi-object imager-spectrograph for the Gran Telescopio Canarias (GTC). His key research area centers on the design, construction, and scientific exploitation of cutting-edge astronomical instrumentation for the 10-meter class telescope. Gago’s major contribution lies in shepherding EMIR from its initial conceptual and design phases through to its fabrication, assembly, integration, and verification (AIV). This instrument, one of the first common-user tools for the GTC, enables simultaneous multi-object spectroscopy and imaging in the near-infrared, providing a critical capability for studying star formation, galaxy evolution, and the distant universe. His most cited work (2006, 27 citations) details the final global design and performance of EMIR, outlining the plan for its early scientific exploitation. While his citation counts reflect a specialized engineering-focused field, Gago’s impact is profound: EMIR represents a foundational piece of infrastructure for Spanish and European astronomy, directly enabling a generation of observational discoveries. His work exemplifies the crucial, often unsung, role of the instrument builder in advancing astrophysical knowledge.