activity
19962019
most citedeROSITA Science Book: Mapping the Structure of the Energetic Universe

421 citations · 2.6k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2019★ 4 cited

Magnetic fields and extraordinarily bright radio emission in the X-ray faint galaxy group MRC 0116+111

F. Mernier, N. Werner, J. Bagchi +4

MRC 0116+111 is a nearby () poor galaxy group, which was previously known for exhibiting a bright diffuse radio emission with no central point-like source, presumably rela…

astro-ph.CO2017★ 18 cited

Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters

G. Foëx, H. Böhringer, G. Chon

The main goal of this work is to compare the results of three dynamical mass estimators to the X-ray hydrostatic values, focussing on massive galaxy clusters at intermediate redshi…

astro-ph.HE2012★ 421 cited

eROSITA Science Book: Mapping the Structure of the Energetic Universe

A. Merloni, P. Predehl, W. Becker +22

eROSITA is the primary instrument on the Russian SRG mission. In the first four years of scientific operation after its launch, foreseen for 2014, it will perform a deep survey of…

astro-ph2008★ 19 cited

XMM-Newton studies of a massive cluster of galaxies: RXCJ2228.6+2036

S. M. Jia, H. Boehringer, E. Pointecouteau +2

We present the X-ray properties of a massive cluster of galaxies (RXCJ2228.6+2036 at ) using {\it XMM-Newton} data. The X-ray mass modeling is based on the temperature and…

astro-ph2008★ 172 cited

Detection of hot gas in the filament connecting the clusters of galaxies Abell 222 and Abell 223

N. Werner, A. Finoguenov, J. S. Kaastra +4

About half of the baryons in the local Universe are invisible and - according to simulations - their dominant fraction resides in filaments connecting clusters of galaxies in the f…

astro-ph2007★ 109 cited

Metal-rich multi-phase gas in M87: AGN-driven metal transport, magnetic-field supported multi-temperature gas, and constraints on non-thermal emission observed with XMM-Newton

A. Simionescu, N. Werner, A. Finoguenov +2

We use deep (~120 ks) XMM-Newton data of the M87 halo to analyze its spatially resolved temperature structure and chemical composition. We focus particularly on the regions of enha…