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20112022
most citedThe MUSIC of CLASH: predictions on the concentration-mass relation

150 citations · 814 across the 16 of their papers we have counts for

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13 papers · 1 filter

astro-ph.CO2022★ 25 cited

Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations

Daniel de Andres, Gustavo Yepes, Federico Sembolini +5

In this paper we study the applicability of a set of supervised machine learning (ML) models specifically trained to infer observed related properties of the baryonic component (st…

astro-ph.CO2020★ 77 cited

Exploring the hydrostatic mass bias in MUSIC clusters: application to the NIKA2 mock sample

Giulia Gianfagna, Marco De Petris, Gustavo Yepes +10

Clusters of galaxies are useful tools to constrain cosmological parameters, only if their masses can be correctly inferred from observations. In particular, X-ray and Sunyaev-Zeldo…

astro-ph.CO2019★ 18 cited

Impact of ICM disturbances on the mean pressure profile of galaxy clusters: a prospective study of the NIKA2 SZ large program with MUSIC synthetic clusters

F. Ruppin, F. Sembolini, M. De Petris +6

. The mean pressure profile of the galaxy cluster population plays an essential role in cosmological analyses. An accurate characterization of the shape, intrinsic scatter…

astro-ph.CO2018★ 35 cited

Kinetic Sunyaev--Zel'dovich effect in rotating galaxy clusters from MUSIC simulations

Anna Silvia Baldi, Marco De Petris, Federico Sembolini +3

The masses of galaxy clusters are a key tool to constrain cosmology through the physics of large-scale structure formation and accretion. Mass estimates based on X-ray and Sunyaev-…

astro-ph.CO2017★ 39 cited

Morphological estimators on Sunyaev--Zel'dovich maps of MUSIC clusters of galaxies

Giammarco Cialone, Marco De Petris, Federico Sembolini +3

The determination of the morphology of galaxy clusters has important repercussion on their cosmological and astrophysical studies. In this paper we address the morphological charac…

astro-ph.CO2016★ 18 cited

On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters

Anna Silvia Baldi, Marco De Petris, Federico Sembolini +3

We present a study on the coherent rotation of the intracluster medium and dark matter components of simulated galaxy clusters extracted from a volume-limited sample of the MUSIC p…

astro-ph.CO2015★ 60 cited

nIFTy galaxy cluster simulations II: radiative models

Federico Sembolini, Pascal Jahan Elahi, Frazer R. Pearce +19

We have simulated the formation of a massive galaxy cluster (M = 1.110) in a CDM universe using 10 different codes (RAMSES, 2 in…

astro-ph.CO2015★ 87 cited

nIFTy galaxy cluster simulations I: dark matter & non-radiative models

Federico Sembolini, Gustavo Yepes, Frazer R. Pearce +24

We have simulated the formation of a galaxy cluster in a CDM universe using twelve different codes modeling only gravity and non-radiative hydrodynamics (\art, \arepo, \hydra\ a…

astro-ph.CO2014★ 150 cited

The MUSIC of CLASH: predictions on the concentration-mass relation

M. Meneghetti, E. Rasia, J. Vega +42

We present the results of a numerical study based on the analysis of the MUSIC-2 simulations, aimed at estimating the expected concentration-mass relation for the CLASH cluster sam…

astro-ph.CO2014★ 47 cited

The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations

Veronica Biffi, Federico Sembolini, Marco De Petris +3

We present the X-ray properties and scaling relations of a large sample of clusters extracted from the Marenostrum MUltidark SImulations of galaxy Clusters (MUSIC) dataset. We focu…

astro-ph.CO2013★ 31 cited

The MUSIC of Galaxy Clusters III: Properties, evolution and Y-M scaling relation of protoclusters of galaxies

Federico Sembolini, Marco De Petris, Gustavo Yepes +3

In this work we study the properties of protoclusters of galaxies by employing the MUSIC set of hydrodynamical simulations, featuring a mass-limited sample of 282 resimulated clust…

astro-ph.CO2012★ 117 cited

The MUSIC of Galaxy Clusters I: Baryon properties and Scaling Relations of the thermal Sunyaev-Zel'dovich Effect

Federico Sembolini, Gustavo Yepes, Marco De Petris +3

We introduce the Marenostrum-MultiDark SImulations of galaxy Clusters (MUSIC) Dataset, one of the largest sample of hydrodynamically simulated galaxy clusters with more than 500 cl…

astro-ph.CO2011

Baryon and Sunyaev-Zel'dovich effect properties of MareNostrum and MultiDark simulated clusters (MUSIC)

Federico Sembolini, Gustavo Yepes, Marco De Petris

We report the first results of the MUSIC project. It consists of two data sets of resimulates clusters extracted from two large dark matter only simulations: Marenostrum Universe a…