Search Results - "Gheller, C"

A survey of the thermal and non-thermal properties of cosmic filaments by Gheller, C, Vazza, F

“…ABSTRACT In this paper, we exploit a large suite of enzo cosmological magneto-hydrodynamical simulations adopting uniform mesh resolution, to investigate the…”
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Convolutional deep denoising autoencoders for radio astronomical images by Gheller, C, Vazza, F

“…ABSTRACT We apply a Machine Learning technique known as Convolutional Denoising Autoencoder to denoise synthetic images of state-of-the-art radio telescopes,…”
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On the amplification of magnetic fields in cosmic filaments and galaxy clusters by Vazza, F., Brüggen, M., Gheller, C., Wang, P.

“…The amplification of primordial magnetic fields via a small-scale turbulent dynamo during structure formation might be able to explain the observed magnetic…”
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Multiwavelength cross-correlation analysis of the simulated cosmic web by Gheller, C, Vazza, F

“…ABSTRACT We used magnetohydrodynamical cosmological simulations to investigate the cross-correlation between different observables (i.e. X-ray emission,…”
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Constraining the efficiency of cosmic ray acceleration by cluster shocks by Vazza, F., Brüggen, M., Wittor, D., Gheller, C., Eckert, D., Stubbe, M.

“…We study the acceleration of cosmic rays by collisionless structure formation shocks with enzo grid simulations. Data from the Fermi satellite enable the use…”
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Turbulence and vorticity in Galaxy clusters generated by structure formation by Vazza, F, Jones, T W, Brueggen, M, Brunetti, G, Gheller, C, Porter, D, Ryu, D

“…Turbulence is a key ingredient for the evolution of the intracluster medium, whose properties can be predicted with high-resolution numerical simulations. We…”
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Shock waves in Eulerian cosmological simulations: main properties and acceleration of cosmic rays by Vazza, F., Brunetti, G., Gheller, C.

“…Large-scale shocks are responsible for the heating of the intracluster medium and can be important sources of cosmic rays (CRs) in the Universe. However, the…”
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The turbulent pressure support in galaxy clusters revisited by Vazza, F, Angelinelli, M, Jones, T W, Eckert, D, Brüggen, M, Brunetti, G, Gheller, C

“…ABSTRACT Due to their late formation in cosmic history, clusters of galaxies are not fully in hydrostatic equilibrium and the gravitational pull of their mass…”
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Radio U-Net: a convolutional neural network to detect diffuse radio sources in galaxy clusters and beyond by Stuardi, C, Gheller, C, Vazza, F, Botteon, A

“…ABSTRACT The forthcoming generation of radio telescope arrays promises significant advancements in sensitivity and resolution, enabling the identification and…”
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Deep learning based detection of cosmological diffuse radio sources by Gheller, C, Vazza, F, Bonafede, A

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On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web by Banfi, S, Vazza, F, Gheller, C

“…ABSTRACT The continuous flow of gas and dark matter across scales in the cosmic web can generate correlated dynamical properties of haloes and filaments (and…”
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Probing the origin of extragalactic magnetic fields with Fast Radio Bursts by Vazza, F, Brüggen, M, Hinz, P M, Wittor, D, Locatelli, N, Gheller, C

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Properties of cosmological filaments extracted from Eulerian simulations by Gheller, C., Vazza, F., Favre, J., Brüggen, M.

“…Using a new parallel algorithm implemented within the VisIt framework, we analysed large cosmological grid simulations to study the properties of baryons in…”
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Magnetic field evolution in cosmic filaments with LOFAR data by Carretti, E, O’Sullivan, S P, Vacca, V, Vazza, F, Gheller, C, Vernstrom, T, Bonafede, A

“…ABSTRACT Measuring the magnetic field in cosmic filaments reveals how the Universe is magnetized and the process that magnetized it. Using the Rotation…”
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A radio ridge connecting two galaxy clusters in a filament of the cosmic web by Govoni, F, Orrù, E, Bonafede, A, Iacobelli, M, Paladino, R, Vazza, F, Murgia, M, Vacca, V, Giovannini, G, Feretti, L, Loi, F, Bernardi, G, Ferrari, C, Pizzo, R F, Gheller, C, Manti, S, Brüggen, M, Brunetti, G, Cassano, R, de Gasperin, F, Enßlin, T A, Hoeft, M, Horellou, C, Junklewitz, H, Röttgering, H J A, Scaife, A M M, Shimwell, T W, van Weeren, R J, Wise, M

“…Galaxy clusters are the most massive gravitationally bound structures in the Universe. They grow by accreting smaller structures in a merging process that…”
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Evolution of cosmic filaments and of their galaxy population from MHD cosmological simulations by Gheller, C., Vazza, F., Brüggen, M., Alpaslan, M., Holwerda, B. W., Hopkins, A. M., Liske, J.

“…Despite containing about a half of the total matter in the Universe, at most wavelengths the filamentary structure of the cosmic web is difficult to observe…”
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Orb5: A global electromagnetic gyrokinetic code using the PIC approach in toroidal geometry by Lanti, E., Ohana, N., Tronko, N., Hayward-Schneider, T., Bottino, A., McMillan, B.F., Mishchenko, A., Scheinberg, A., Biancalani, A., Angelino, P., Brunner, S., Dominski, J., Donnel, P., Gheller, C., Hatzky, R., Jocksch, A., Jolliet, S., Lu, Z.X., Martin Collar, J.P., Novikau, I., Sonnendrücker, E., Vernay, T., Villard, L.

“…This paper presents the current state of the global gyrokinetic code Orb5 as an update of the previous reference (Jolliet et al., 2007). The Orb5 code solves…”
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Thermal and non-thermal traces of AGN feedback: results from cosmological AMR simulations by Vazza, F., Brüggen, M., Gheller, C.

“…We investigate the observable effects of feedback from active galactic nuclei (AGN) on non-thermal components of the intracluster medium (ICM). We have…”
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A comparison of cosmological codes: properties of thermal gas and shock waves in large-scale structures by Vazza, F., Dolag, K., Ryu, D., Brunetti, G., Gheller, C., Kang, H., Pfrommer, C.

“…Cosmological hydrodynamical simulations are a valuable tool for understanding the growth of large-scale structure and the observables connected with this. Yet,…”
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Interactive 3D visualization for theoretical virtual observatories by Dykes, T, Hassan, A, Gheller, C, Croton, D, Krokos, M

“…Abstract Virtual observatories (VOs) are online hubs of scientific knowledge. They encompass a collection of platforms dedicated to the storage and…”
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