スポンサーリンク
Department of Physics and Astronomy, Johns Hopkins University | 論文
- The X-Ray Observatory Suzaku
- Soft X-Ray Coronal Structure Surrounding High-Latitude Dark Filaments Observed by Yohkoh
- Suzaku Wide-Band X-Ray Spectroscopy of the Seyfert 2 AGN in NGC 4945
- Revealing the High Energy Emission from the Obscured Seyfert Galaxy MCG -5-23-16 with Suzaku
- A Suzaku Observation of the Low-Ionization Fe-Line Emission from RCW 86
- Monte Carlo Simulator and Ancillary Response Generator of Suzaku XRT/XIS System for Spatially Extended Source Analysis
- The Long Suzaku Observation of MCG-6-30-15(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
- Suzaku Observations of the Hard X-Ray Variability of MCG -6-30-15 : the Effects of Strong Gravity around a Kerr Black Hole
- Low/Hard State Spectra of GRO J1655-40 Observed with Suzaku
- Suzaku Observation of 1H0707-495 : Puzzling Spectral Drop around 7keV(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
- X-Ray Spectral Study of the Extended Emission, 'the Cap', Located 11.6kpc above the Disk of M82
- The Suzaku Observation of NGC 3516 : Complex Absorption and the Broad and Narrow Fe K Lines
- Precision Fe Kα and Fe Kβ Line Spectroscopy of the Seyfert 1.9 Galaxy NGC 2992 with Suzaku
- A Suzaku Observation of the Low-Ionization Fe-Line Emission from RCW 86(Chapter 4. Warm and Hot IntraGalactic Medium, The Extreme Universe in the Suzaku Era)
- SDSS J1335+0118 : A New Two-Image Gravitational Lens
- Wide-Band Spectroscopy of the Compton Thick Seyfert 2 Galaxy Markarian 3 with Suzaku
- TRACE Observation of an Arcade Flare Showing Evidence Supporting Quadruple Magnetic Source Model for Arcade Flares
- Dynamic Current Injection into Magnetic Loops in Active Regions II. A 3D Magnetodynamic Model for Loop Flares
- Dynamic Current Injection into Magnetic Loops in Active Regions I. Supplies of Energy and Mass to Active-Region Corona in the Form of Dynamic Loop Brightenings
- A Quadruple Magnetic Source Model for Arcade Flares and X-Ray Arcade Formations outside Active Regions I. Dark Filament Suspension and the Magnetic Structure in the Pre-Event Regions