dr Grzegorz Dudziński

Research interests

physical properties of asteroids

asteroid shape modelling

Education

2019

PhD in astronomy

thesis title: Determining non-convex asteroid models from photometric data.

advisors: prof. dr hab. Tadeusz Michałowski, dr Przemysław Bartczak

2015

Master of Science (astronomy)

thesis title: The use of graphic cards and OpenGL in simulated photometric and radar observations of asteroids.

advisor: dr Przemysław Bartczak

Publications

ADS list

• Hanuš, J., et al., "(704) Interamnia: a transitional object between a dwarf planet and a typical irregular-shaped minor body", (2020), Astronomy & Astrophysics, Volume 633
• Vernazza, P., et al., "A basin-free spherical shape as an outcome of a giant impact on asteroid Hygiea", (2019), Nature Astronomy, Advanced Online Publication
• Bartczak, P. & Dudziński, G., "Volume uncertainty assessment method of asteroid models from disc-integrated visual photometry", (2019), Monthly Notices of the Royal Astronomical Society, 485, 2431.
• Hanuš, J., et al., "The shape of (7) Iris as evidence of an ancient large impact?", (2019), Astronomy and Astrophysics, 624, A121.
• Fétick, R. JL., et al., "Closing the gap between Earth-based and interplanetary mission observations: Vesta seen by VLT/SPHERE", (2019), Astronomy and Astrophysics, 623, A6.
• Kim, M. -J., et al., "Optical observations of NEA 3200 Phaethon (1983 TB) during the 2017 apparition", (2018), Astronomy and Astrophysics, 619, A123.
• Müller, T. G., et al., "Small Bodies Near and Far (SBNAF): A benchmark study on physical and thermal properties of small bodies in the Solar System", (2018), Advances in Space Research, 62, 2326.
• Vernazza, P., et al., "The impact crater at the origin of the Julia family detected with VLT/SPHERE?", (2018), Astronomy and Astrophysics, 618, A154.
• Bartczak, P. & Dudziński, G., "Shaping asteroid models using genetic evolution (SAGE)", (2018), Monthly Notices of the Royal Astronomical Society, 473, 5050.
• Marciniak, A., et al., "Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids", (2018), Astronomy and Astrophysics, 610, A7.
• Ortiz, J. L., et al., "The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation", (2017), Nature, 550, 219.
• Bartczak, P., et al., "A new non-convex model of the binary asteroid (809) Lundia obtained with the SAGE modelling technique", (2017), Monthly Notices of the Royal Astronomical Society, 471, 941.
• Butkiewicz-Bąk, M., et al., "Statistical analysis of the ambiguities in the asteroid period determinations", (2017), Monthly Notices of the Royal Astronomical Society, 470, 1314.
• Santana-Ros, T., et al., "Shape Models and Physical Properties of Asteroids", (2017), Assessment and Mitigation of Asteroid Impact Hazards: Proceedings of the 2015 Barcelona Asteroid Day, 46, 55.
• Bartczak, P., et al., "A new non-convex model of the binary asteroid 90 Antiope obtained with the SAGE modelling technique", (2014), Monthly Notices of the Royal Astronomical Society, 443, 1802.