activity
20122026
most citedThe ASTRO-H X-ray Observatory

106 citations · 195 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2017★ 43 cited

Temperature Structure in the Perseus Cluster Core Observed with Hitomi

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

The present paper investigates the temperature structure of the X-ray emitting plasma in the core of the Perseus cluster using the 1.8--20.0 keV data obtained with the Soft X-ray S…

astro-ph.HE2017★ 13 cited

Glimpse of the highly obscured HMXB IGR J16318-4848 with Hitomi

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We report a Hitomi observation of IGR J16318-4848, a high-mass X-ray binary system with an extremely strong absorption of N_H~10^{24} cm^{-2}. Previous X-ray studies revealed that…

astro-ph.HE2017★ 19 cited

Search for Thermal X-ray Features from the Crab nebula with Hitomi Soft X-ray Spectrometer

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

The Crab nebula originated from a core-collapse supernova (SN) explosion observed in 1054 A.D. When viewed as a supernova remnant (SNR), it has an anomalously low observed ejecta m…

astro-ph.HE2014★ 3 cited

ASTRO-H White Paper - Broad-band Spectroscopy and Polarimetry

P. Coppi, L. Stawarz, C. Done +13

The broad energy range spanned by ASTRO-H instruments, from ~0.3 to 600 keV, with its high spectral resolution calorimeter and sensitive hard X-ray imaging, offers unique opportuni…

astro-ph.HE2014★ 2 cited

ASTRO-H White Paper - Low-mass X-ray Binaries

C. Done, M. Tsujimoto, E. Cackett +20

There is still 10-20% uncertainty on the neutron star (NS) mass-radius relation. These uncertainties could be reduced by an order of magnitude through an unambiguous measure of M/R…