The splashback radius and the radial velocity profile of galaxy clusters in IllustrisTNG

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Pizzardo, Michele, Geller, Margaret J., Kenyon, Scott J., Damjanov, Ivana
Formato:	Preprint
Publicado:	2023
Materias:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Kinematic morphology of low-mass galaxies in IllustrisTNG
por: Zeng, Guangquan, et al.
Publicado: (2024)

Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
por: Yu, Guangyao, et al.
Publicado: (2025)

Polarization-shape alignment of IllustrisTNG star-forming galaxies
por: Zhou, Rui, et al.
Publicado: (2025)

Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation
por: Pasté, Jade, et al.
Publicado: (2026)

Dynamics of the response of dark matter halo to galaxy evolution in IllustrisTNG
por: Velmani, Premvijay, et al.
Publicado: (2024)

Peculiar velocities of galaxy clusters in a IllustrisTNG simulation based on mock observations of Sunyaev-Zel'dovich effects
por: Du, Kaiyi, et al.
Publicado: (2025)

The formation and evolution of Supermassive disks in IllustrisTNG
por: Pallero, Diego, et al.
Publicado: (2025)

Galaxy Populations in the IllustrisTNG Caustic Skeleton
por: Hertzsch, Benjamin, et al.
Publicado: (2026)

Dynamical friction and measurements of the splashback radius in galaxy clusters
por: O'Shea, Talia M., et al.
Publicado: (2024)

The Magellanic Clouds are very rare in the IllustrisTNG simulations
por: Haslbauer, Moritz, et al.
Publicado: (2024)

A deep learning model for the density profiles of subhaloes in IllustrisTNG
por: Lucie-Smith, Luisa, et al.
Publicado: (2024)

Constraining cosmological parameters using the splashback radius of galaxy clusters
por: Haggar, Roan, et al.
Publicado: (2024)

Entropy Evolution Towards DARKexp of IllustrisTNG Dark Matter Halos
por: Francis, Ashley, et al.
Publicado: (2025)

Environmental effects on Low Surface Brightness Galaxies in the IllustrisTNG simulation
por: Pérez-Montaño, Luis Enrique, et al.
Publicado: (2024)

Cluster Lensing Mass Inversion (CLUMI+): Combining Dynamics and Weak Lensing around Galaxy Clusters
por: Umetsu, Keiichi, et al.
Publicado: (2025)

Clustering of emission line galaxies with IllustrisTNG -- II. cosmology challenge with anisotropic correlation functions and ELG-halo connections
por: Osato, Ken, et al.
Publicado: (2026)

Exploring the link between galaxy assembly and dark matter halo assembly in IllustrisTNG: Insights from the Mutual Information
por: Camargo, Y. D., et al.
Publicado: (2025)

The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
por: Xu, Shuo, et al.
Publicado: (2024)

Spatial and velocity anisotropies of stellar halos across cosmic web environments: Insights from IllustrisTNG simulation
por: Mondal, Amit, et al.
Publicado: (2025)

Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
por: Yang, Hong-Gang, et al.
Publicado: (2025)

Living on the edge. A quantitative warning on boundary artifacts in the IllustrisTNG
por: Mitrašinović, Ana
Publicado: (2025)

Quenching pathways in the green valley at low redshift: confronting SDSS AGN hosts with IllustrisTNG and EAGLE
por: Gawade, Gaurav
Publicado: (2025)

IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L$^\star$ Galaxies
por: Ramesh, Rahul, et al.
Publicado: (2024)

Mass Proxy Quality of Massive Halo Properties in the IllustrisTNG and FLAMINGO Simulations: I. Hot Gas
por: Aljamal, Eddie, et al.
Publicado: (2025)

Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
por: Xu, Kun, et al.
Publicado: (2025)

Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
por: Polzin, Ava, et al.
Publicado: (2024)

Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
por: Pizzardo, Michele, et al.
Publicado: (2025)

Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
por: Kimmig, Lucas C., et al.
Publicado: (2025)

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

Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z > 3$: A Comparative Study With IllustrisTNG and ASTRID
por: Weller, Emma Jane, et al.
Publicado: (2024)

Can the splashback radius be an observable boundary of galaxy clusters?
por: Lebeau, Théo, et al.
Publicado: (2024)

The effects of projection on measuring the splashback feature
por: Sun, Xiaoqing, et al.
Publicado: (2025)

The AIDA-TNG project. Abundance, radial distribution, and clustering properties of halos in alternative dark matter models
por: Romanello, Massimiliano, et al.
Publicado: (2025)

X-ray shocks in the cool cores of galaxy clusters: insights from TNG-Cluster
por: Prunier, Marine, et al.
Publicado: (2025)

Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
por: Miller, Daniel, et al.
Publicado: (2025)

AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
por: Lesci, G. F., et al.
Publicado: (2026)

Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
por: Joshi, Jitendra, et al.
Publicado: (2025)

Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
por: Monjo, Robert, et al.
Publicado: (2024)

Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
por: Nandi, Anindita, et al.
Publicado: (2025)

Measuring the splashback feature: Dependence on halo properties and history
por: Yu, Qiaorong S., et al.
Publicado: (2025)