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Satoshi Honda∗1, Wako Aoki1, Yuhri Ishimaru2, Shinya Wanajo3, Sean G. Ryan4, Toshitaka Kajino1, Hiroyasu Ando1, and Timothy C. Beers5 1National Astronomical Observatory of Japan 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan 2Department of General Education, Kogakuin University 2665-1 Nakano-Cho, Hachioji, Tokyo 192-0015, Japan 3Graduate School of Science, University of Tokyo Bunkyo-ku, Tokyo 113-0033, Japan 4Centre for Astrophysics Research, STRI, University of Hertfordshire College Lane, Hatfield AL10 9AB, UK 5Department of Physics and Astronomy and JINA: Joint Institute for Nuclear Astrophysics Michigan State University, East Lansing, MI 48824, USA. E-mail: honda@optik.mtk.nao.ac.jp E-mail: aoki.wako@nao.ac.jp E-mail: kt13121@ms.kogakuin.ac.jp E-mail: wanajo@resceu.s.u-tokyo.ac.jp E-mail: s.g.ryan@herts.ac.jp E-mail: kajino@nao.ac.jp E-mail: ando@optik.mtk.nao.ac.jp E-mail: beers@pa.msu.edu

The Detailed Abundance Patterns of Light Neutron-Capture Elements in Very Metal-Poor Stars