activity
20142017
most citedHitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

124 citations · 389 across the 7 of their papers we have counts for

collaborators

7 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★ 88 cited

The Structure of the Local Hot Bubble

W. Liu, M. Chiao, M. R. Collier +14

DXL (Diffuse X-rays from the Local Galaxy) is a sounding rocket mission designed to quantify and characterize the contribution of Solar Wind Charge eXchange (SWCX) to the Diffuse X…

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-ph.HE2016★ 16 cited

Solar Wind Charge Exchange contribution to the ROSAT All Sky Survey Maps

Y. Uprety, M. Chiao, M. R. Collier +15

DXL (Diffuse X-ray emission from the Local Galaxy) is a sounding rocket mission designed to estimate the contribution of Solar Wind Charge eXchange (SWCX) to the Diffuse X-ray Back…

astro-ph.HE2015★ 2 cited

Evidence for a very low-column density hole in the Galactic halo in the direction of the high latitude molecular cloud MBM 16

Wenhao Liu, Massimiliano Galeazzi, Eugenio Ursino

Shadow observations are the only way to observe emission from the galactic halo (GH) and/or the circumgalactic medium (CGM) free of any foreground contamination from local hot bubb…