activity
20042026
most citedConstrained Simulations of the Magnetic Field in the Local Universe and the Propagation of UHECRs

335 citations · 631 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2026

Constraining Effective Viscosity in the Intracluster Medium via the Thermal Sunyaev-Zeldovich Effect -- Predictions from the SLOW Constrained Coma Cluster Simulations

Frederick Groth, Yuan Li, Joseph Golec +4

We study the effect of viscosity on the Sunyaev-Zeldovich signal in a simulated constrained Coma cluster analog. We aim to provide alternative constraints on the amount of viscosit…

astro-ph.CO2020★ 78 cited

The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data

T. H. Reiprich, A. Veronica, F. Pacaud +44

We used dedicated SRG/eROSITA X-ray, ASKAP/EMU radio, and DECam optical observations of a 15 sq.deg region around the interacting galaxy cluster system A3391/95 to study the warm-h…

astro-ph.CO2020★ 35 cited

N-body simulations of dark matter with frequent self-interactions

Moritz S. Fischer, Marcus Brüggen, Kai Schmidt-Hoberg +4

Self-interacting dark matter (SIDM) models have the potential to solve the small-scale problems that arise in the cold dark matter paradigm. Simulations are a powerful tool for stu…

astro-ph.HE2018★ 40 cited

Close-up view of an ongoing merger between the NGC 4839 group and the Coma cluster - a post-merger scenario

N. Lyskova, E. Churazov, C. Zhang +5

We study a merger of the NGC 4839 group with the Coma cluster using X-ray observations from the XMM-Newton and Chandra telescopes. X-ray data show two prominent features: (i) a lon…

astro-ph.GA2014

Simulating realistic disk galaxies with a novel sub-resolution ISM model

Giuseppe Murante, Pierluigi Monaco, Stefano Borgani +3

We present results of cosmological simulations of disk galaxies carried out with the GADGET-3 TreePM+SPH code, where star formation and stellar feedback are described using our MUl…

astro-ph.IM2011★ 143 cited

Planck Early Results. II. The thermal performance of Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +225

The performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative…