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A. Kutyrev is a leading figure in astronomical instrumentation, specializing in the development of robotic observatories and wide-field optical transient imagers. His work has been instrumental in advancing the automation of ground-based telescopes for rapid-response astrophysics. Notably, Kutyrev led the automation of the 1.5-meter Harold Johnson telescope at the Observatorio Astronómico Nacional in Mexico, enabling robotic operations for the Reionization And Transients Infra-Red (RATIR) camera. This work, published in 2012 and cited over 50 times, has been foundational for time-domain astronomy, allowing for autonomous follow-up of gamma-ray bursts and other transient phenomena. Kutyrev further expanded the field’s capabilities with the Deca-Degree Optical Transient Imager (DDOTI), a wide-field robotic system comprising six 28-cm telescopes. Described in a 2016 paper (17 citations), DDOTI achieves a 10-sigma limiting magnitude of r ~ 19 in just 60 seconds, covering a 72 square-degree field of view. These contributions have significantly enhanced the ability to detect and study fast-evolving cosmic events, cementing Kutyrev’s reputation as a key innovator in robotic transient surveys and multi-messenger astronomy.