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About

V. Krushinski is a leading figure in time-domain astrophysics, specializing in the optical follow-up and characterization of explosive transients. Their work centers on the rapid identification and multi-wavelength study of gamma-ray bursts (GRBs) and luminous red novae, leveraging the global network of MASTER robotic telescopes. A key contribution is the discovery and detailed analysis of MASTER OT J004207.99+405501.1, a rare luminous red nova in the Andromeda Galaxy (M31N 2015-01a), for which they provided a unique, homogeneous light curve and hydrodynamic interpretation (43 citations). Krushinski has also made significant advances in GRB science, including early polarization measurements of GRB 150301B, which detected a minimum polarization of 8% at the initial stage (41 citations), and the successful optical identification of the poorly-localized Fermi GBM GRB 140801A, demonstrating the MASTER network’s unique capability to autonomously scan large error boxes (38 citations). Their work is instrumental in bridging robotic survey capabilities with transient physics, enabling rapid, multi-observatory responses to high-energy alerts.