| 2025年9月11日 （木） 午前 （09:30-11:40） [G会場］ | ||
| 09:30 | Z101r | Astronomical Applications of Differentiable Programming 河原 創(JAXA宇宙科学研究所) |
| 09:49 | Z102a | A differentiable N-body code for dynamical modeling of multi-planet systems 増田 賢人(大阪大学) |
| 09:58 | Z103a | \texttt {microjax}: A GPU-Accelerated, Auto-Differentiable Framework for Microlensing Modeling in the Roman Era Shota Miyazaki(ISAS/JAXA) |
| 10:07 | Z104a | Probing Two-dimensional Asymmetries of an Exoplanet Atmosphere from Chromatic Transit Variation Shotaro Tada(ISAS/JAXA) |
| 10:16 | Z105r | Applications of Differential Programming in Observational Astronomy 大澤亮(国立天文台) |
| 10:36 | Z106a | The JASMINE iterative solver: using JAX to achieve a fast yet flexible framework for astrometric missions RAMOS Pau(NAOJ) |
| 10:45 | Z107a | Differentiable cosmological parameter estimation in the era of Stage-IV cosmological surveys 大里健(千葉大学) |
| 10:54 | Z108a | Fast differentiable code of one-loop power spectrum of large-scale structure Yosuke Kobayashi(Kyoto Sangyo University) |
| 11:03 | Z109a | A Differentiable Cosmological Emulator for Halo Assembly Bias Studies Keitaro Ishikawa(Nagoya University) |
| 11:12 | Z110a | Interpretable deep neural networks reveal environmental influences on galaxy properties 内田舜也(名古屋大学) |
| 11:21 | Z111a | JFlow: Model-Independent Spherical Jeans Analysis using Equivariant Continuous Normalizing Flows Sung Hak Lim(CTPU-PTC, Institute for Basic Science) |
| 2025年9月11日 （木） 午後 （13:00-15:10） [G会場］ | ||
| 13:00 | Z112r | Differentiable Physical Models for Astronomy Benjamin Pope(Macquarie University) |
| 13:24 | Z113a | Exploration of Feasible Optical Designs and Sensitivity Analysis Using Differentiable Programming 柴井すばる(東京大学) |
| 13:33 | Z114a | Experimental Determination of CH$_4$ Pressure-Broadening in Hot H$_2$/He Atmosphere Using Bayesian Inference Ko Hosokawa(National Astronomical Observatory of Japan) |
| 13:42 | Z115r | Differentiable modeling of the Universe in the age of machine learning Yin Li(Peng Cheng Laboratory) |
| 14:06 | Z116a | Field Level Inference in Hydrodynamical Simulations with JAX Horowitz, Benjamin(Kavli IPMU) |
| 14:15 | Z117a | Forward Modeling and Cosmological Inference of Galaxy Clustering the Field Level Nguyen, Nhat-Minh(Kavli IPMU) |
| 14:24 | Z118a | Reconstructing the Primordial Density Field with Differentiable N-body Simulations Sirawich Saranakomkoop(Department of Physics, Nagoya University) |
| 14:33 | Z119a | Differentiable mapping of stellar surface for solar-type stars 幾田 佳(一橋大学) |
| 14:42 | Z120a | Bayesian inference for the inclination of stars, brown dwarfs, and exoplanets using time-series spectroscopy 嬉野大和(JAXA宇宙科学研究所) |
| 14:51 | Z121a | High-resolution spectral analysis of Luhman 16AB with Gaussian Process T-P profile and auto-differentiable spectrum model ExoJAX Hibiki Yama(The University of Osaka) |
| Z122c | Parameter Estimation for SEP Event Modeling: A Bayesian Approach Using Multi-Spacecraft Observations of the October 2021 Event 加藤裕太(富士通株式会社、名古屋大学) | |