@inproceedings{oai:jaxa.repo.nii.ac.jp:00004970,
 author = {萩原, 利士成 and 満田, 和久 and 山崎, 典子 and 竹井, 洋 and Hagihara, Toshishige and Yao, Yangsen and Mitsuda, Kazuhisa and Yamasaki, Noriko Y. and Takei, Yoh and McCammon, Dan and Wang, Daniel Q.},
 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 studied the hot gas in the Galactic halo in the direction of a blazer PKS 2155-304 (z = 0.117). This is the second direction for combined analysis using high resolution X-ray absorption/emission data. Absorption features of O(sub VII) and O(sub VIII) are measured with Chandra LETGS. Suzaku observations of the vicinity of PKS 2155-304 allows us to study emission lines (O(sub VII) , O(sub VIII) , N(sub VII) and N(sub EIX) ). We performed a joint analysis of emission and absorption data assuming a vertically exponential galactic disk. The gas temperature and density at the Galactic plane are determined to be 3.2(+0.7,-0.6) x 10(exp 6) K and 1.3(+0.4,-0.6) x 10(exp -3) cm(exp -3) and the scale heights of the gas temperature and density 2.2(+4.4,-2.1) kpc and 5.1(+3.9,-4.7) kpc, respectively., 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: AA0064574038, レポート番号: JAXA-SP-09-008E},
 pages = {104--105},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Line-of-sight spatial extent of warm-hot medium in the direction of PKS 2155-304},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}