activity
19962017
most citedHitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

124 citations · 441 across the 6 of their papers we have counts for

collaborators

6 papers

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★ 116 cited

Solar abundance ratios of the iron-peak elements in the Perseus Cluster

Hitomi Collaboration

The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy…

astro-ph.HE2016★ 124 cited

Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

Hitomi Collaboration, Felix A. Aharonian, Hiroki Akamatsu +215

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E=3.5 keV emission line reported in several low-resolution studies of va…

astro-ph2005★ 75 cited

The XMM-Newton view of PG quasars: II. Properties of the Fe K-alpha line

E. Jimenez-Bailon, E. Piconcelli, M. Guainazzi +3

The properties of the fluorescence Fe K-alpha emission lines of a sample of 38 quasars (QSOs) observed with XMM-Newton are studied. These objects are included in the optically sele…

astro-ph2003★ 53 cited

The X-ray afterglow of GRB030329

A. Tiengo, S. Mereghetti, G. Ghisellini +3

We report on XMM-Newton and Rossi-XTE observations of the bright (fluence 10 erg cm) and nearby (z=0.1685) Gamma-Ray Burst GRB030329 associated to SN2003dh. Th…

astro-ph1996★ 30 cited

ROSAT Soft X-Ray Properties of the Large Bright Quasar Survey: Modeling of Stacked X-Ray Spectra

Norbert Schartel, Paul J. Green, Scott F. Anderson +6

We develop and apply a novel method of analysis to study the X-ray spectral properties of 908 QSOs in the Large Bright Quasar Survey (LBQS) that were observed during the soft X-ray…