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19972026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 44.2k across the 411 of their papers we have counts for

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19 papers · 1 filter

astro-ph.HE2026

Rates of tidal disruption events from constrained cosmological simulations of the local Universe: population properties and implications for transient surveys

Julian S. Sommer, Ildar Khabibullin, Klaus Dolag +4

(abridged) Motivated by upcoming surveys like LSST, we estimate tidal disruption event (TDE) rates using the constrained cosmological Simulation of the LOcal Web (SLOW) to test the…

astro-ph.HE2026

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding

Daniel Karner, Ludwig M. Böss, Klaus Dolag +1

Context. Cosmological simulation codes with subgrid models for cosmic rays (CRs) help us better understand their impact on baryonic feedback and non-thermal radiation in galaxies a…

astro-ph.HE2025

Simulating the LOcal Web (SLOW) -- VI: Gamma-ray Emission in the Local Universe

Ludwig M. Böss, Ildar Khabibullin, Daniel Karner +4

Context: Diffuse -ray emission from cosmic-ray (CR) protons scattering off the gas in the intracluster and intergalactic medium remains out of reach for current observations. De…

astro-ph.HE2025★ 1 cited

Perseus cluster in its X-ray entirety with SRG/eROSITA. Merger and Radio-Uroboroses

Eugene Churazov, Ildar Khabibullin, Natalya Lyskova +2

The Perseus cluster (Abell 426) is a nearby massive galaxy cluster that spans several degrees. We combined SRG/eROSITA, XMM-Newton, and Chandra data to get a complete coverage of t…

astro-ph.HE2024★ 371 cited

The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere

A. Merloni, G. Lamer, T. Liu +142

The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sk…

astro-ph.HE2023★ 12 cited

A formation mechanism for "Wrong Way" Radio Relics

Ludwig M. Böss, Ulrich P. Steinwandel, Klaus Dolag

Radio Relics are typically found to be arc-like regions of synchrotron emission in the outskirts of merging galaxy clusters, bowing out from the cluster center. In most cases they…

astro-ph.HE2023

Mapping the Intracluster Medium in the Era of High-resolution X-ray Spectroscopy

Congyao Zhang, Irina Zhuravleva, Maxim Markevitch +24

High-resolution spectroscopy in soft X-rays will open a new window to map multiphase gas in galaxy clusters and probe physics of the intracluster medium (ICM), including chemical e…

astro-ph.HE2023

Galaxy Cluster simulations with a spectral Cosmic Ray model -- "Wrong Way" Radio Relics

Ludwig M. Böss, Ulrich P. Steinwandel, Klaus Dolag

Non-thermal emission from relativistic electrons gives insight into the strength and morphology of intra-cluster magnetic fields, as well as providing powerful tracers of structure…

astro-ph.HE2023★ 14 cited

Prospects of detecting soft X-ray emission from typical WHIM filaments around massive clusters and the Coma cluster soft excess

E. Churazov, I. I. Khabibullin, K. Dolag +2

While hot ICM in galaxy clusters makes these objects powerful X-ray sources, the cluster's outskirts and overdense gaseous filaments might give rise to much fainter sub-keV emissio…

astro-ph.HE2022★ 21 cited

Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs

Stephan Vladutescu-Zopp, Veronica Biffi, Klaus Dolag

We provide a numerical framework with which spatially and spectrally accurate representations of X-ray binary populations can be studied from hydrodynamical cosmological simulation…

astro-ph.HE2022★ 31 cited

CRESCENDO: An on-the-fly Fokker-Planck Solver for Spectral Cosmic Rays in Cosmological Simulations

Ludwig M. Böss, Ulrich P. Steinwandel, Klaus Dolag +1

Non-thermal emission from relativistic Cosmic Ray (CR) electrons gives insight into the strength and morphology of intra-cluster magnetic fields, as well as providing powerful trac…

astro-ph.HE2020★ 18 cited

Collision of Merger and Accretion Shocks: Formation of Mpc-scale Contact Discontinuity in the Perseus Cluster

Congyao Zhang, Eugene Churazov, Klaus Dolag +2

Two Mpc-size contact discontinuities have recently been identified in the XMM-Newton and Suzaku X-ray observations of the outskirts of the Perseus cluster (Walker et al. 2020). The…

astro-ph.HE2020★ 25 cited

Characterizing the Uncertainty in Cluster Magnetic Fields derived from Rotation Measures

Andrew Johnson, Lawrence Rudnick, Thomas Jones +2

Magnetic fields play vital roles in intracluster media (ICMs), but estimating their strengths and distributions from observations is a major challenge. Faraday rotation measures (R…

astro-ph.HE2013★ 10 cited

The Hot and Energetic Universe: The missing baryons and the warm-hot intergalactic medium

Jelle Kaastra, Alexis Finoguenov, Fabrizio Nicastro +19

The backbone of the large-scale structure of the Universe is determined by processes on a cosmological scale and by the gravitational interaction of the dominant dark matter. Howev…

astro-ph.HE2013★ 20 cited

The Hot and Energetic Universe: The evolution of galaxy groups and clusters

E. Pointecouteau, T. H. Reiprich, C. Adami +45

Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and…

astro-ph.HE2013★ 395 cited

The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

Kirpal Nandra, Didier Barret, Xavier Barcons +237

This White Paper, submitted to the recent ESA call for science themes to define its future large missions, advocates the need for a transformational leap in our understanding of tw…

astro-ph.HE2011★ 37 cited

Resonant scattering in galaxy clusters for anisotropic gas motions on various spatial scales

I. Zhuravleva, E. Churazov, S. Sazonov +2

The determination of characteristic amplitudes and anisotropy of hot gas motions in galaxy clusters from observations of the brightest resonance lines is discussed. Gas motions aff…

astro-ph.HE2010★ 31 cited

Polarization of X-ray lines from galaxy clusters and elliptical galaxies - a way to measure tangential component of gas velocity

I. V. Zhuravleva, E. M. Churazov, S. Yu. Sazonov +3

We study the impact of gas motions on the polarization of bright X-ray emission lines from the hot intercluster medium (ICM). The polarization naturally arises from resonant scatte…

astro-ph.HE2009★ 45 cited

Blazar halos as probe for extragalactic magnetic fields and maximal acceleration energy

K. Dolag, M. Kachelriess, S. Ostapchenko +1

High energy photons from blazars interact within tens of kpc with the extragalactic photon background, initiating electromagnetic pair cascades. The charged component of such casca…