E. V. Emelyanov

Papers

Total Citations

H-Index

About

Dr. E. V. Emelyanov is a leading figure in exoplanetary science, whose work bridges observational astronomy and planetary dynamics. Their primary research focuses on the detection and characterization of exoplanets, particularly through transit photometry and long-term monitoring programs. Dr. Emelyanov’s major contributions include the discovery of eight new exoplanet candidates as part of the Special Astrophysical Observatory (SAO) survey, using a 50-cm robotic telescope to identify shallow transits with depths as low as 0.01 magnitudes. This work has garnered over 5 citations, underscoring its significance in expanding the census of exoplanets in the northern sky. Beyond detection, Dr. Emelyanov has advanced our understanding of planetary system architectures, notably through studies of orbital stability and the dynamics of multiple-planet systems. Their research has been instrumental in refining techniques for distinguishing true planetary signals from stellar variability. With a career marked by meticulous observational campaigns and theoretical insights, Dr. Emelyanov continues to shape the field, inspiring students and researchers to explore the frontiers of exoplanet discovery.