Masanori Ohno (ISAS/JAXA). HXD: 10-600 keV WAM: 50keV-5MeV XIS: 0.2-12keV X-ray Afterglow (XIS + HXD withToO) Wide energy band (0.2-600 keV) Ultra-low.
Suzaku Results of SN 1006: Chemical abundances of the youngest Galactic Type Ia Supernova Remnant Katsuji Koyama Department of physics, Kyoto University,
