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Corrado Bartolini is a leading figure in the study of gamma-ray bursts (GRBs) and fast optical transients, with a career dedicated to understanding the most violent explosions in the universe. His seminal 1999 work, cited over 112 times, provided critical early evidence for the fireball model of GRBs. By orchestrating broad-band ultraviolet to near-infrared observations of the exceptionally bright GRB 990123, Bartolini and his team helped decode the physics of relativistic jets and their afterglows, laying foundational groundwork for modern high-energy astrophysics. Building on this legacy, Bartolini pioneered the development of wide-field, high-time-resolution optical monitoring systems. His work on the TORTORA and MegaTORTORA projects, detailed in a 2010 paper, introduced a novel approach to capturing elusive, short-duration optical flares from GRBs, supernovae, and near-Earth objects. By designing cameras capable of surveying hundreds of square degrees with TV-like cadence, he enabled the detection of transient events that would otherwise be missed by traditional telescopes. This innovative instrumentation has opened a new window on the dynamic universe, allowing researchers to study stochastic cosmic flares and their origins. Bartolini’s contributions bridge observational astrophysics and advanced instrumentation, making him a key figure in the ongoing quest to map the transient sky.