A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions.

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Atmospheric gas dynamics in the Perseus cluster observed with Hitomi*

Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi*

Detections of hard X-ray emissions from bright early-type galaxies with ASCA ⬇️

Discovery of a luminous, variable, off-center source in the nucleus of M82 with the Chandra high-resolution camera ⬇️

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Discovery of an abundance gradient in the central region of the Virgo cluster

scientific article published in January 1996

EDGE: Explorer of diffuse emission and gamma-ray burst explosions

EDGE: explorer of diffuse emission and gamma-ray burst explosions

Glimpse of the highly obscured HMXB IGR J16318−4848 with Hitomi*

Hitomi X-ray observation of the pulsar wind nebula G21.5−0.9

scientific article published in January 2018

Hitomi X-ray studies of giant radio pulses from the Crab pulsar*

scientific article published on 01 April 2018

Hitomi observation of radio galaxy NGC 1275: The first X-ray microcalorimeter spectroscopy of Fe-Kα line emission from an active galactic nucleus*

Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta*

Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS*

Multiwavelength observation of an active M-dwarf star EV Lacertae and its stellar flare accompanied by a delayed prominence eruption

scholarly article

Peculiar chemical abundances in the starburst galaxy M82 and hypernova nucleosynthesis ⬇️

scientific article published in January 2002

Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer*

Temperature structure in the Perseus cluster core observed with Hitomi*

The ASTRO-H (Hitomi) x-ray astronomy satellite

The ASTRO-H Mission

The ASTRO-H X-ray Observatory

The ASTRO-H X-ray astronomy satellite ⬇️

Time variability of the neutral iron lines from the Sagittarius B2 region and its implication of a past outburst of Sagittarius A*

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X-ray echo from the Sagittarius C complex and 500-year activity history of Sagittarius A*

scientific article published in January 2013

X-ray filament with a strong 6.7-keV line in the Galactic center region ⬇️

X-ray imaging spectrometer (XIS) on board Suzaku

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