Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research interests include Physics, Astrophysics, Astronomy, Spectroscopy, Intracluster medium, and Spectrometer.
X-Ray Imaging and Spectroscopy Mission
The bulk motion of gas in the core of the Centaurus galaxy cluster
Structured ionized winds shooting out from a quasar at relativistic speeds
Delving into the depths of NGC 3783 with XRISM
Stratified wind from a super-Eddington X-ray binary is slower than expected
Chlorine and potassium enrichment in the Cassiopeia A supernova remnant
The XRISM first-light observation: Velocity structure and thermal properties of the supernova remnant N 132D
Lynx x-ray microcalorimeter
A High Spectral Resolution Study of the Soft X-Ray Background with the X-Ray Quantum Calorimeter
Unlocking the Capabilities of Future High-Resolution X-ray Spectroscopy Missions Through Laboratory Astrophysics
Unlocking the Capabilities of Future High-Resolution X-ray Spectroscopy Missions Through Laboratory Astrophysics
The ATHENA x-ray integral field unit (X-IFU)
Concept of the X-ray Astronomy Recovery Mission
Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi
Constraints on the chemical enrichment history of the Perseus Cluster of galaxies from high-resolution X-ray spectroscopy
Design, implementation, and performance of the Astro-H SXS calorimeter array and anticoincidence detector
Atmospheric gas dynamics in the Perseus cluster observed with Hitomi
Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster
Solar abundance ratios of the iron-peak elements in the Perseus cluster
Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer
Hitomi X-ray studies of giant radio pulses from the Crab pulsar
Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta
The quiescent intracluster medium in the core of the Perseus cluster
The ASTRO-H (Hitomi) x-ray astronomy satellite
The design, implementation, and performance of the Atro-H SXS calorimeter array and anti-coincidence detector
The ASTRO-H X-ray Observatory
OBSERVED LIMITS ON CHARGE EXCHANGE CONTRIBUTIONS TO THE DIFFUSE X-RAY BACKGROUND