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4siWe employ a set of Magneticum cosmological hydrodynamic simulations that span over 15 different c...
Context. Upcoming X-ray surveys like eROSITA require precise calibration between X-ray observables a...
We study the scaling relations between the baryonic content and total mass of groups of galaxies, as...
We investigate the X-ray vs. optical scaling relations of poor groupsto small clusters ( 100−700 km...
Context. Clusters are potentially powerful tools for cosmology provided their observed properties, ...
We examine the scalings of X-ray luminosity, temperature, and dark matter or galaxy velocity dispers...
We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling rel...
Rights Copyright © is held by the author. Digital access to this material is made possible by the Un...
Cluster scaling relations from cosmological hydrodynamic simulations in a dark-energy dominated univ...
`Galaxy groups' have hardly been realized as a separate class of objects with specific characteristi...
We analyze hierarchical structure formation based on scale-free initial conditions in an Einstein-de...
We study the scaling relations between the baryonic content and total mass of groups of galaxies, as...
Galaxy groups are more than an intermediate scale between clusters and halos hosting individual gala...
`Galaxy groups' have hardly been realized as a separate class of objects with specific characteristi...
We study the redshift evolution of the X-ray and Sunyaev-Zel'dovich (SZ) scaling relations for galax...
4siWe employ a set of Magneticum cosmological hydrodynamic simulations that span over 15 different c...
Context. Upcoming X-ray surveys like eROSITA require precise calibration between X-ray observables a...
We study the scaling relations between the baryonic content and total mass of groups of galaxies, as...
We investigate the X-ray vs. optical scaling relations of poor groupsto small clusters ( 100−700 km...
Context. Clusters are potentially powerful tools for cosmology provided their observed properties, ...
We examine the scalings of X-ray luminosity, temperature, and dark matter or galaxy velocity dispers...
We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling rel...
Rights Copyright © is held by the author. Digital access to this material is made possible by the Un...
Cluster scaling relations from cosmological hydrodynamic simulations in a dark-energy dominated univ...
`Galaxy groups' have hardly been realized as a separate class of objects with specific characteristi...
We analyze hierarchical structure formation based on scale-free initial conditions in an Einstein-de...
We study the scaling relations between the baryonic content and total mass of groups of galaxies, as...
Galaxy groups are more than an intermediate scale between clusters and halos hosting individual gala...
`Galaxy groups' have hardly been realized as a separate class of objects with specific characteristi...
We study the redshift evolution of the X-ray and Sunyaev-Zel'dovich (SZ) scaling relations for galax...
4siWe employ a set of Magneticum cosmological hydrodynamic simulations that span over 15 different c...
Context. Upcoming X-ray surveys like eROSITA require precise calibration between X-ray observables a...
We study the scaling relations between the baryonic content and total mass of groups of galaxies, as...