@inproceedings{oai:jaxa.repo.nii.ac.jp:00005088,
 author = {高橋, 忠幸 and 満田, 和久 and Takahashi, Tadayuki and Mitsuda, Kazuhisa and Kelley, Richard and ASTRO-H team},
 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, The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS) The planned launch date is 2014. ASTRO-H will investigate the physics of the high-energy universe by performing high-resolution, highthroughput spectroscopy with moderate spatial resolution over the 0.3 - 600 keV energy range. ASTRO-H is a combination of wide band X-ray spectroscopy (3 - 80 keV) provided by multi-layer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3 - 10 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope and a non-focusing soft gamma-ray detector. With these instruments, ASTRO-H covers very wide energy range from 0.3 keV to 600 keV. The micro-calorimeter system is developed by international collaboration lead by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of Delta E approximately 7 eV by the micro-calorimeter will enable a wide variety of important science themes to be pursued., 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: AA0064574156, レポート番号: JAXA-SP-09-008E},
 pages = {404--407},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {The ASTRO-H Mission},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}