Tuesday, 2 July 8:50 Registration 9:25 Welcome Session 1: Nuclear Structure and Reaction for Astrophysics I 9:45 1-1 S. Cherubini (INFN) Trojan Horse Method: basics and recent applications 10:10 1-2 R. G. Pizzone (INFN) Fluorine burning in stars studied with Trojan Horse Method 10:30 1-3 T. Ahn (University of Notre Dame) Precision measurements of the 24Mg(α,pγ)27Al cross section and 27Al(p,αγ)24Mg cross sections 10:50 1-4 J. Glorius (GSI) Cooled ions and explosive nucleosynthesis: The proton-capture campaign at the GSI storage rings 11:10 Coffee Break Session 2: Astronomical Observations with Light X-Ray Gamma-Ray and Cosmic-Ray 11:40 2-1 H. Yamaguchi (Institute of Space and Astronautical Science) Probing the stellar nucleosynthesis and explosion with X-ray observations of supernova remnants 12:05 2-2 W. Wang (Wuhan University) Detections of 44Ti signals in young supernova remnants 12:25 2-3 R. Diehl (Max Planck Institut für extraterrestrische Physik) Cosmicradioactivity: Gamma-ray line observations with the INTEGRAL Satellite 12:50 2-4 T. Takemura (Kyoto University) SMILE-2+: Balloon observation of electron-positron annihilation line gamma-ray in the galactic center region 13:10 Lunch Session 3: Nucleosynthesis in Neutron Star Mergers 14:40 3-1 S. Wanajo (Max Planck Institute for Gravitational Physics) r-process and kilonovae 15:05 3-2 C. Ishizuka (Tokyo Institute of Technology) Influence of fission-fragment yields on r-process nucleosynthesis 15:30 3-3 S. Fujimoto (National Institute of Technology, Kumamoto College) Impacts of isomers on a light curve of a kilonova associated with newtron star mergers 15:50 3-4 N. Nishimura (YITP, Kyoto University) Observational signatures of magneto-rotational supernovae associated with r-process jets 16:10 Coffee Break Session 4: First Generation Stars and Galactic Chemical Evolution 16:35 4-1 I. U. Roederer (University of Michigan) The environment of the r-process: New advances enabled by the study of the orbits of r-process-enhanced stars 17:00 4-2 Q. Xing (National Astronomical Observatories, Chinese Academy of Sciences) Evidence for the accretion origin of halo stars with an extreme r-process enhancement 17:20 4-3 Y. Hirai (RIKEN) Enrichment of heavy elements in chemodynamical evolution models 17:40 4-4 A. Choplin (Konan University) The early generations of rotating massive stars and the abundances of extremely metal-poor stars 18:00 4-5 M. Kusakabe (Beihang University) Modern results for the cosmic ray nucleosynthesis of p-nuclei 18:20 Move to poster session 18:40 Poster session 20:10 End of poster session