@inproceedings{oai:jaxa.repo.nii.ac.jp:00005013,
 author = {森井, 幹雄 and 河合, 誠之 and 寺田, 幸功 and 高橋, 弘充 and 有本, 誠 and 北本, 俊二 and 幸村, 孝由 and 柴崎, 徳明 and 山内, 茂雄 and 小林, 尚人 and 田中, 康之 and 寺田, 宏 and Morii, Mikio and Kawai, Nobuyuki and Terada, Yukikatsu and Takahashi, Hiromitsu and Arimoto, Makoto and Kitamoto, Shunji and Kohmura, Takayoshi and Shibazaki, Noriaki and Yamauchi, Shigeo and Kobayashi, Naoto and Tanaka, Yasuyuki T. and Terada, Hiroshi},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, Magnetars are strongly magnetized neutron stars ( approximately 10(exp 14) - -10(exp 15) G) (Thompson ' Duncan 1995). The energy spectra in soft/hard X-ray and IR/optical are known to be peculiar (Woods & Thompson 2006). The emissions are thought to be generated by release of magnetic energy, however the energy release mechanism is still open question. Here, we present observations for two magnetars 1E 1841-045 and 4U 0142+61 by Suzaku and Subaru, respectively., 著者人数: 12名, Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, Number of authors: 12, 資料番号: AA0064574081, レポート番号: JAXA-SP-09-008E},
 pages = {218--219},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku spectroscopy of a magnetar 1E 1841-045 and search for NIR pulsation of a magnetar 4U 0142+61},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}