@inproceedings{oai:jaxa.repo.nii.ac.jp:00005065,
 author = {Tombesi, Francesco and Cappi, M. and Yaqoob, T. and Reeves, J. and Palumbo, G.G.C.},
 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 have performed several simulations in order to test the scientific capabilities of the IXO calorimeter, with particular emphasis on the detection of absorption lines in the 3 - 11 keV band. We derived the flux limits for their detection on several time-scales, compared different response matrices available and simulated realistic spectra from photo-ionized warm absorbers in AGNs. This study illustrates the considerable improvements that this instrument will bring to high resolution spectroscopy, especially related to the study of accretion and outflows in the central regions of AGNs., 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: AA0064574133, レポート番号: JAXA-SP-09-008E},
 pages = {340--341},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Highly Ionized Warm Absorbers in AGNs: Simulations with the IXO Calorimeter},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}