activity
20012025
most citedHard X-ray Detector (HXD) on Board Suzaku

647 citations · 4.6k across the 67 of their papers we have counts for

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Showing 2017Show all

13 papers · 1 filter

astro-ph.HE2017★ 1 cited

Search For Gravitational Redshifted Absorption Lines In LMXB Serpens X-1

Hiroki Yoneda, Chris Done, Frits Paerels +2

The equation of state for ultra-dense matter can be tested from observations of the ratio of mass to radius of neutron stars. This could be measured precisely from the redshift of…

astro-ph.HE2017★ 126 cited

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

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

The Hitomi SXS spectrum of the Perseus cluster, with 5 eV resolution in the 2-9 keV band, offers an unprecedented benchmark of the atomic modeling and database for hot collis…

astro-ph.HE2017★ 18 cited

Hitomi Observations of the LMC SNR N132D: Highly Redshifted X-ray Emission from Iron Ejecta

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We present Hitomi observations of N132D, a young, X-ray bright, O-rich core-collapse supernova remnant in the Large Magellanic Cloud (LMC). Despite a very short observation of only…

astro-ph.IM2017★ 23 cited

Development of Si-CMOS hybrid detectors towards electron tracking based Compton imaging in semiconductor detectors

Hiroki Yoneda, Shinya Saito, Shin Watanabe +2

Electron tracking based Compton imaging is a key technique to improve the sensitivity of Compton cameras by measuring the initial direction of recoiled electrons. To realize this t…

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★ 58 cited

Hitomi Observation of Radio Galaxy NGC 1275: The First X-ray Microcalorimeter Spectroscopy of Fe-Kα Line Emission from an Active Galactic Nucleus

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

The origin of the narrow Fe-Kα fluorescence line at 6.4 keV from active galactic nuclei has long been under debate; some of the possible sites are the outer accretion disk, the bro…