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About

P. Sybilski is a Polish astronomer whose research sits at the intersection of stellar astrophysics, exoplanet detection, and astronomical instrumentation. He is best known for his central role in Project Solaris, an ambitious initiative to build and operate a global network of four autonomous robotic observatories across the Southern Hemisphere. The project's primary scientific mission is the detection and characterization of circumbinary planets — worlds orbiting binary star systems — using the eclipse timing variation (ETV) method, which demands sustained, high-cadence photometric monitoring that only a dedicated network can reliably provide. Sybilski has contributed meaningfully to the physical characterization of eclipsing binary systems, including a detailed orbital and physical analysis of the double-giant system HD 187669, his most-cited work with 37 citations, which combined multi-band photometry from ASAS, SuperWASP, and robotic telescopes with high-precision spectroscopy. His 2023 Solaris photometric survey paper demonstrates the network's ongoing complementary role alongside space missions like Kepler and TESS, particularly in addressing limitations of sky and time coverage. Through instrumentation development, long-baseline photometric surveys, and binary star analysis, Sybilski has helped establish a robust southern-sky infrastructure for next-generation exoplanet and stellar science.