Image de couverture de livre

The Three Hundred project: Radio luminosity evolution from merger-induced shock fronts in simulated galaxy clusters

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Nuza, Sebastián E., Hoeft, Matthias, Contreras-Santos, Ana, Knebe, Alexander, Yepes, Gustavo
Format:	Preprint
Publié:	2024
Sujets:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

The origin of the intra-cluster light in The Three Hundred simulations
par: Contreras-Santos, A., et autres
Publié: (2025)

Characterising the intra-cluster light in The Three Hundred simulations
par: Contreras-Santos, Ana, et autres
Publié: (2024)

The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations
par: Contreras-Santos, Ana, et autres
Publié: (2024)

The Three Hundred Project: The relationship between the shock and splashback radii of simulated galaxy clusters
par: Zhang, M., et autres
Publié: (2024)

Diffuse radio emission from merger shocks in simulated galaxy clusters
par: Nuza, Sebastián E.
Publié: (2024)

The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
par: Gómez, Jonathan S., et autres
Publié: (2025)

The Three Hundred project: cosmic web identification from 2D gas and Compton-$y$ maps of galaxy clusters outskirts
par: Santoni, Sara, et autres
Publié: (2026)

The rise and fall of radio-luminous merger shocks from a large sample of galaxy cluster simulations
par: Nuza, Sebastián E.
Publié: (2025)

The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
par: Giocoli, Carlo, et autres
Publié: (2025)

II- A hydrodynamical CLONE of the Virgo cluster to confront observed and synthetic galaxy population twins in a dense environment
par: Sorce, Jenny G., et autres
Publié: (2026)

Impact of filaments on galaxy cluster properties in The Three Hundred simulation
par: Santoni, Sara, et autres
Publié: (2023)

The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution
par: Schaye, Joop, et autres
Publié: (2025)

Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
par: Euclid Collaboration, et autres
Publié: (2023)

The luminosity function and clustering of bright quasars in the FLAMINGO cosmological simulations
par: Ding, Boyi, et autres
Publié: (2025)

The origin of scatter in the X-ray luminosity - halo mass relation of galaxy clusters
par: Braspenning, Joey, et autres
Publié: (2025)

Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
par: Jose, Charles, et autres
Publié: (2024)

The signature of major mergers on the hydrostatic mass bias of galaxy clusters
par: Barranco-Llorca, Isac, et autres
Publié: (2025)

Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
par: Caro, Andrés, et autres
Publié: (2024)

Stellar stripping efficiencies of satellites in numerical simulations: the effect of resolution, satellite properties and numerical disruption
par: Martin, G., et autres
Publié: (2024)

The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
par: Santoni, Sara, et autres
Publié: (2024)

The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations
par: Contreras, Sergio, et autres
Publié: (2026)

PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
par: Adame, Adrian G., et autres
Publié: (2023)

The FLAMINGO Project: A comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richness
par: Kugel, Roi, et autres
Publié: (2024)

The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
par: de Andres, Daniel, et autres
Publié: (2023)

Identification of low redshift groups and clusters of galaxies in the X-CLASS survey and the X-ray luminosity-temperature relation
par: Moysan, Q., et autres
Publié: (2026)

X-ray shocks in the cool cores of galaxy clusters: insights from TNG-Cluster
par: Prunier, Marine, et autres
Publié: (2025)

The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
par: Walker, Kris, et autres
Publié: (2025)

The longest known tails of ram-pressure-stripped star-forming galaxies are caused by an intracluster medium shock in Abell 1367
par: Edler, H. W., et autres
Publié: (2025)

The functional form of galaxy and halo luminosity and mass functions
par: Ford, Amelia, et autres
Publié: (2026)

An improved Halo Occupation Distribution prescription from UNITsim H_alpha Emission Line Galaxies: conformity and modified radial profile
par: Reyes-Peraza, Guillermo, et autres
Publié: (2023)

Digging into the ultraviolet luminosity functions of galaxies at high redshifts: galaxies evolution, reionization, and cosmological parameters
par: Wang, Yi-Ying, et autres
Publié: (2024)

Probing inflationary features with galaxy ultraviolet luminosity function observables
par: Acharya, Sandeep Kumar
Publié: (2026)

The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
par: Muñoz, A. Jiménez, et autres
Publié: (2023)

Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
par: Fontanot, Fabio, et autres
Publié: (2024)

Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations
par: Braspenning, Joey, et autres
Publié: (2024)

The THESAN-ZOOM project: Long-term imprints of external reionization on galaxy evolution
par: Zier, Oliver, et autres
Publié: (2025)

The impact of feedback on the evolution of gas density profiles from galaxies to clusters: a universal fitting formula from the Simba suite of simulations
par: Sorini, Daniele, et autres
Publié: (2024)

Bridging observations and simulations: a machine learning approach to galaxy clusters
par: Gatuzz, Efrain
Publié: (2025)

The conditional colour-magnitude distribution: II. A comparison of galaxy colour and luminosity distribution in galaxy groups
par: Xu, Haojie, et autres
Publié: (2023)

The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
par: Das, Apashanka, et autres
Publié: (2024)