@inproceedings{oai:jaxa.repo.nii.ac.jp:00005064,
 author = {Ballo, Lucia and Sambruna, Rita and Braito, Valentina and Reeves, James N. and Tavecchio, Fabrizio},
 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, Here we report on a Suzaku observation of the nearby BLRG 3C 111, a bright FR II with a single sided jet exhibiting superluminal motion. Preliminary results indicate that the 0.5 - 200 keV spectrum is dominated by a disklike component, with a power law with photon index approximately 1.6 cutting off around 100 keV, and a reflection R approximately 0.04. The Suzaku data do not indicate the presence of a hard X-ray component associated with the jet emission, that should become dominant at GeV energies (i.e. in the range covered by FERMI )., 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: AA0064574132, レポート番号: JAXA-SP-09-008E},
 pages = {338--339},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {The Suzaku view of the BLRG 3C 111},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}