Search Results - "Fabjan, D"

The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics by Munari, E., Biviano, A., Borgani, S., Murante, G., Fabjan, D.

“…We present an analysis of the relation between the masses of cluster- and group-sized haloes, extracted from Λ cold dark matter (ΛCDM) cosmological N-body and…”
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The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations by Biffi, V, Planelles, S, Borgani, S, Rasia, E, Murante, G, Fabjan, D, Gaspari, M

“…Abstract The uniformity of the intracluster medium (ICM) enrichment level in the outskirts of nearby galaxy clusters suggests that chemical elements were…”
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On the role of AGN feedback on the thermal and chemodynamical properties of the hot intracluster medium by Planelles, S., Borgani, S., Fabjan, D., Killedar, M., Murante, G., Granato, G. L., Ragone-Figueroa, C., Dolag, K.

“…We present an analysis of the properties of the intracluster medium (ICM) in an extended set of cosmological hydrodynamical simulations of galaxy clusters and…”
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Simulating the effect of active galactic nuclei feedback on the metal enrichment of galaxy clusters by Fabjan, D., Borgani, S., Tornatore, L., Saro, A., Murante, G., Dolag, K.

“…We present a study of the effect of active galactic nuclei (AGN) feedback on metal enrichment and thermal properties of the intracluster medium (ICM) in…”
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Baryon census in hydrodynamical simulations of galaxy clusters by Planelles, S., Borgani, S., Dolag, K., Ettori, S., Fabjan, D., Murante, G., Tornatore, L.

“…We carry out an analysis of a set of cosmological smoothed particle hydrodynamics (SPH) hydrodynamical simulations of galaxy clusters and groups aimed at…”
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Large-scale inhomogeneities of the intracluster medium: improving mass estimates using the observed azimuthal scatter by Roncarelli, M., Ettori, S., Borgani, S., Dolag, K., Fabjan, D., Moscardini, L.

“…Achieving a robust determination of the gas density profile in the outskirts of clusters is a crucial step for measuring their baryonic content and using them…”
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Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution by Truong, N, Rasia, E, Mazzotta, P, Planelles, S, Biffi, V, Fabjan, D, Beck, A M, Borgani, S, Dolag, K, Gaspari, M, Granato, G L, Murante, G, Ragone-Figueroa, C, Steinborn, L K

“…AbstractWe analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable…”
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Pressure of the hot gas in simulations of galaxy clusters by Planelles, S., Fabjan, D., Borgani, S., Murante, G., Rasia, E., Biffi, V., Truong, N., Ragone-Figueroa, C., Granato, G. L., Dolag, K., Pierpaoli, E., Beck, A. M., Steinborn, Lisa K., Gaspari, M.

“…Abstract We analyse the radial pressure profiles, the intracluster medium (ICM) clumping factor and the Sunyaev–Zel'dovich (SZ) scaling relations of a sample…”
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The history of chemical enrichment in the intracluster medium from cosmological simulations by Biffi, V., Planelles, S., Borgani, S., Fabjan, D., Rasia, E., Murante, G., Tornatore, L., Dolag, K., Granato, G. L., Gaspari, M., Beck, A. M.

“…Abstract The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the…”
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X-ray mass proxies from hydrodynamic simulations of galaxy clusters - I by Fabjan, D., Borgani, S., Rasia, E., Bonafede, A., Dolag, K., Murante, G., Tornatore, L.

“…Using extended sets of cosmological hydrodynamical simulations of galaxy clusters, we present a detailed study of scaling relations between total cluster mass…”
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Lensing and x-ray mass estimates of clusters (simulations) by Rasia, E, Meneghetti, M, Martino, R, Borgani, S, Bonafede, A, Dolag, K, Ettori, S, Fabjan, D, Giocoli, C, Mazzotta, P, Merten, J, Radovich, M, Tornatore, L

“…We present a comparison between weak-lensing and x-ray mass estimates of a sample of numerically simulated clusters. The sample consists of the 20 most massive…”
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Mass–metallicity relation from cosmological hydrodynamical simulations and X-ray observations of galaxy groups and clusters by Truong, N, Rasia, E, Biffi, V, Mernier, F, Werner, N, Gaspari, M, Borgani, S, Planelles, S, Fabjan, D, Murante, G

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Simulation-based marginal likelihood for cluster strong lensing cosmology by Killedar, M., Borgani, S., Fabjan, D., Dolag, K., Granato, G., Meneghetti, M., Planelles, S., Ragone-Figueroa, C.

“…Abstract Comparisons between observed and predicted strong lensing properties of galaxy clusters have been routinely used to claim either tension or…”
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How baryonic processes affect strong lensing properties of simulated galaxy clusters by Killedar, M., Borgani, S., Meneghetti, M., Dolag, K., Fabjan, D., Tornatore, L.

“…ABSTRACT The observed abundance of giant arcs produced by galaxy cluster lenses and the measured Einstein radii have presented a source of tension for Λ cold…”
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The Chemical Enrichment of the ICM from Hydrodynamical Simulations by Borgani, S., Fabjan, D., Tornatore, L., Schindler, S., Dolag, K., Diaferio, A.

“…The study of the metal enrichment of the intra-cluster and inter-galactic media (ICM and IGM) represents a direct means to reconstruct the past history of star…”
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Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters by Ettori, S., Rasia, E., Fabjan, D., Borgani, S., Dolag, K.

“…We introduce a generalized scaling law, M tot= 10 K  A a  B b , to look for the minimum scatter in reconstructing the total mass of hydrodynamically simulated…”
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Evolution of the metal content of the intracluster medium with hydrodynamical simulations by Fabjan, D., Tornatore, L., Borgani, S., Saro, A., Dolag, K.

“…We present a comparison between simulation results and X-ray observational data on the evolution of the metallicity of the intracluster medium (ICM). The…”
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Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters: The generalized scaling relations by Ettori, S., Rasia, E., Fabjan, D., Borgani, S., Dolag, K.

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How baryonic processes affect strong lensing properties of simulated galaxy clusters: Baryons and cluster strong lensing by Killedar, M., Borgani, S., Meneghetti, M., Dolag, K., Fabjan, D., Tornatore, L.

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X-ray mass proxies from hydrodynamic simulations of galaxy clusters - I: Mass proxies from simulations by Fabjan, D., Borgani, S., Rasia, E., Bonafede, A., Dolag, K., Murante, G., Tornatore, L.

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