activity
19972025
most citedX-ray Imaging Spectroscopy of Abell 1835

536 citations · 2.1k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2025★ 12 cited

Delving into the depths of NGC 3783 with XRISM II. Cross-calibration of X-ray instruments used in the large, multi-mission observational campaign

XRISM collaboration

Accurate X-ray spectroscopic measurements are fundamental for deriving basic physical parameters of the most abundant baryon components in the Universe. The plethora of X-ray obser…

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.CO2010★ 76 cited

HST Observations of the Double-Peaked Emission Lines in the Seyfert Galaxy Markarian 78: Mass Outflows from a Single AGN

T. C. Fischer, D. M. Crenshaw, S. B. Kraemer +3

Previous ground based observations of the Seyfert 2 galaxy Mrk 78 revealed a double set of emission lines, similar to those seen in several AGN from recent surveys. Are the double…

astro-ph2008★ 51 cited

On Active Galactic Nuclei as Sources of Ultra-High Energy Cosmic Rays

Matthew R. George, Andrew C. Fabian, Wayne H. Baumgartner +2

We measure the correlation between sky coordinates of the Swift BAT catalogue of active galactic nuclei with the arrival directions of the highest energy cosmic rays detected by th…

astro-ph2003★ 4 cited

Cluster of Galaxies: An X-ray Perspective

Richard F. Mushotzky

There has been extensive recent progress in X-ray observations of clusters of galaxies with the analysis of the entire ASCA database and recent new results from Beppo-SAX, Chandra,…

astro-ph2003★ 24 cited

The XMM-Newton view of the X-ray halo and jet of NGC 6251

R. M. Sambruna, M. Gliozzi, D. Donato +3

We present an XMM observation of the radio jet and diffuse halo of the nearby radio galaxy NGC6251. The EPIC spectrum of the galaxy's halo is best-fitted by a thermal model with te…