activity
19972022
most citedDiscovery of the X-Ray Afterglow of the Gamma-Ray Burst of February 28 1997

998 citations · 4.6k across the 103 of their papers we have counts for

collaborators

103 papers

astro-ph.GA2022★ 2 cited

The Nature of 500 Micron Risers II: Sub-mm Faint Dusty Star Forming Galaxies

J. Cairns, D. L. Clements, J. Greenslade +6

We present SCUBA-2 and SMA follow-up observations of four candidate high redshift Dusty Star-Forming Galaxies, selected as sources with rising SEDs in the 250, 350 and 500m Hers…

astro-ph.GA2016★ 500 cited

The Quiescent Intracluster Medium in the Core of the Perseus Cluster

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +213

Clusters of galaxies are the most massive gravitationally-bound objects in the Universe and are still forming. They are thus important probes of cosmological parameters and a host…

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.IM2014★ 55 cited

The ASTRO-H X-ray Astronomy Satellite

Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley +250

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions developed by the Institute of Space and Astronautical Science (ISAS), with a planne…

astro-ph.IM2013★ 7 cited

XMM-Newton Publication Statistics

J. -U. Ness, A. N. Parmar, L. A. Valencic +5

We assessed the scientific productivity and data usage statistics of XMM-Newton by examining 3272 refereed papers published until the end of 2012 that directly use XMM-Newton data.…

astro-ph.HE2012★ 59 cited

XMM-Newton observations of GX 13+1: correlation between photoionised absorption and broad line emission

M. Diaz Trigo, L. Sidoli, L. Boirin +1

We analysed data from five XMM-Newton observations of GX 13+1 to investigate the variability of the photo-ionised absorber present in this source. We fitted EPIC and RGS spectra ob…