activity
19972019
most citedMonte-Carlo Simulator and Ancillary Response Generator of Suzaku XRT/XIS System for Spatially Extended Source Analysis

463 citations · 1.3k across the 21 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

7 papers · 1 filter

astro-ph.HE2019★ 54 cited

Hard X-ray Cataclysmic Variables

D. de Martino, F. Bernardini, K. Mukai +2

Among hard X-ray Galactic sources detected in the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have suprisingly boosted in number in the recent ye…

astro-ph.HE2018★ 39 cited

Detection of polarized gamma-ray emission from the Crab nebula with Hitomi Soft Gamma-ray Detector

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrom…

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.HE2017★ 68 cited

Measurements of resonant scattering in the Perseus cluster core with Hitomi SXS

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

Thanks to its high spectral resolution (~5 eV at 6 keV), the Soft X-ray Spectrometer (SXS) on board Hitomi enables us to measure the detailed structure of spatially resolved emissi…

astro-ph.HE2017★ 20 cited

The Peculiar Multi-Wavelength Evolution Of V1535 Sco

J. D. Linford, L. Chomiuk, T. Nelson +8

We present multi-wavelength observations of the unusual nova V1535 Sco throughout its outburst in 2015. Early radio observations were consistent with synchrotron emission, and earl…

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…