@inproceedings{oai:jaxa.repo.nii.ac.jp:00005057,
 author = {河原, 大 and 寺島, 雄一 and 粟木, 久光 and Kawahara, Hiroshi and Terashima, Yuichi and Yaqoob, Tahir and Awaki, Hisamitsu},
 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, We present results from a Suzaku observation of the Seyfert 1.9 galaxy NGC 7314. The light curve in the 2-10 keV band shows rapid variability on timescales of approximately 1000 sec. The time-averaged spectrum in 0.5 - 25 keV is explained a model consisting of absorbed and unabsorbed power laws, a reflection continuum and a gaussian at 6.4 keV. The line at 6.4 keV is relatively narrow (sigma approximately 50 eV) and does not vary on a timescale of approximately 10 years. This narrow line is likely to be primarily from distant matter. We analyze spectra in the time intervals with fluxes higher/lower than the mean. The normalization of the absorbed power law varies by a factor 1.6, while the photon index, the amount of the reflection, and the intensity of the Fe line remains constant., Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, 資料番号: AA0064574125, レポート番号: JAXA-SP-09-008E},
 pages = {324--325},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Fe -K line Profile and X-ray Spectral Variability of the Seyfert 1.9 Galaxy NGC 7314 Observed with Suzaku},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}