Modeling the Unseen: Inference and Reconstruction in Accretion Disk Physics
The 87th Fujihara Seminar: The 50th Anniversary Workshop of the Disk Instability Model in Compact Binary Stars, 22-26 Sep. 2025, Talk
Hiroshima Astrophysical Science Center, Hiroshima University
The 87th Fujihara Seminar: The 50th Anniversary Workshop of the Disk Instability Model in Compact Binary Stars, 22-26 Sep. 2025, Talk
日本天文学会2025年春季年会, 17-20 Mar., Poster
Uemura, M., Koga, Y., Sazaki, R., Yukino, T., Nakaoka, T., et al., “Smart Kanata: A framework for autonomous decision-making in rapid follow-up observations of cataclysmic variables”, PASJ, 77, 219, 2025
Studying the early stages of transient events provides crucial information about the fundamental physical processes in cataclysmic variables (CVs). However, determining an appropriate observation mode immediately after the discovery of a new transient presents challenges due to significant uncertainties regarding its nature. We developed a framework designed for autonomous decision-making in prompt follow-up observations of CVs using the Kanata 1.5-m telescope. The system, named Smart Kanata, first estimates the class probabilities of variable star types using a generative model. It then selects the optimal observation mode from three possible options based on the mutual information calculated from the class probabilities.