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About

K. Noysena is a key figure in time-domain astronomy, specializing in the rapid detection of optical counterparts to gravitational-wave sources. As a core member of the Gravitational-wave Optical Transient Observer (GOTO) collaboration, Noysena has been instrumental in designing, building, and commissioning a global network of wide-field robotic telescopes. Their major contributions span nearly a decade, from the initial conception of using arrays of cost-effective 40 cm unit telescopes on shared mounts to achieving full operational capability. This innovative design provides a massive 40-square-degree field of view per mount, enabling the team to quickly scan large areas of the sky where LIGO and Virgo detect ripples in spacetime. Noysena’s work is documented in a series of highly cited papers (2020, 2022, and 2024), which together have garnered nearly 40 citations, reflecting the project’s growing importance in multi-messenger astrophysics. By helping to build this automated alert system, Noysena is directly enabling the next generation of transient discoveries, from neutron star mergers to exotic cosmic explosions.