Buchumschlag

The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations

Fuente: arXiv

Gespeichert in:

Bibliographische Detailangaben
Hauptverfasser:	Contreras-Santos, Ana, Buitrago, Fernando, Knebe, Alexander, Rasia, Elena, Pearce, Frazer R., Cui, Weiguang, Power, Chris, Winstanley, Jordan
Format:	Preprint
Veröffentlicht:	2024
Schlagworte:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
Online-Zugang:	Acceder al recurso
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Ähnliche Einträge

Characterising the intra-cluster light in The Three Hundred simulations
von: Contreras-Santos, Ana, et al.
Veröffentlicht: (2024)

The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
von: Walker, Kris, et al.
Veröffentlicht: (2025)

The origin of the intra-cluster light in The Three Hundred simulations
von: Contreras-Santos, A., et al.
Veröffentlicht: (2025)

The life and times of dark matter haloes: what will I be when I grow up?
von: Onions, Julian, et al.
Veröffentlicht: (2025)

The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
von: Li, Renjie, et al.
Veröffentlicht: (2025)

The Three Hundred project: Radio luminosity evolution from merger-induced shock fronts in simulated galaxy clusters
von: Nuza, Sebastián E., et al.
Veröffentlicht: (2024)

Impact of filaments on galaxy cluster properties in The Three Hundred simulation
von: Santoni, Sara, et al.
Veröffentlicht: (2023)

The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
von: Santoni, Sara, et al.
Veröffentlicht: (2024)

The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
von: Muñoz, A. Jiménez, et al.
Veröffentlicht: (2023)

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

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

The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
von: Giocoli, Carlo, et al.
Veröffentlicht: (2025)

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

On the redshift evolution of the spin parameter in cosmological simulations
von: Riera, Tomas, et al.
Veröffentlicht: (2026)

The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
von: Rasia, Elena, et al.
Veröffentlicht: (2025)

Tidal adaptive softening and artificial fragmentation in cosmological simulations
von: Paun, Robert A. Mostoghiu, et al.
Veröffentlicht: (2025)

The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
von: Corasaniti, P. S., et al.
Veröffentlicht: (2025)

The Three Hundred: $M_{sub}-V_{circ}$ relation
von: Srivastava, Atulit, et al.
Veröffentlicht: (2023)

On bursty star formation during cosmological reionization - how does it influence the baryon mass content of dark matter halos?
von: Menon, Anand, et al.
Veröffentlicht: (2024)

Intracluster light as a dark matter tracer: how their spatial and kinematic relationship is shaped by satellite demographics
von: Martin, G, et al.
Veröffentlicht: (2026)

Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
von: Haggar, Roan, et al.
Veröffentlicht: (2024)

Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
von: Caro, Andrés, et al.
Veröffentlicht: (2024)

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

Identifying group galaxies merging with massive clusters using machine learning
von: Jordan, Rhys, et al.
Veröffentlicht: (2026)

On bursty star formation during cosmological reionization -- influence on the metal and dust content of low-mass galaxies
von: Menon, Anand, et al.
Veröffentlicht: (2025)

Galaxy catalogs from the SAGE Semi-Analytic Model calibrated on THE THREE HUNDRED hydrodynamical simulations: A method to push the limits toward lower mass galaxies in dark matter only clusters simulations
von: Gómez, Jonathan S., et al.
Veröffentlicht: (2024)

The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
von: Rohr, Eric, et al.
Veröffentlicht: (2023)

HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
von: García-Bethencourt, Guacimara, et al.
Veröffentlicht: (2026)

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

Galaxy cluster temperature maps from joint X-ray and SZ maps with The Three Hundred hydrodynamical simulations
von: Wicker, R., et al.
Veröffentlicht: (2025)

Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
von: Ilc, Samo, et al.
Veröffentlicht: (2024)

The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
von: de Andres, Daniel, et al.
Veröffentlicht: (2023)

The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
von: He, Feihong, et al.
Veröffentlicht: (2026)

Using dust to constrain dark matter models
von: Ussing, Adam, et al.
Veröffentlicht: (2024)

Constraints on the properties of $ν$MSM dark matter using the satellite galaxies of the Milky Way
von: Newton, Oliver, et al.
Veröffentlicht: (2024)

The effect of baryons on the positions and velocities of satellite galaxies in the MTNG simulation
von: Contreras, Sergio, et al.
Veröffentlicht: (2025)

Super cuspy dark matter halos of massive galaxies due to baryon-driven contraction
von: Li, Pengfei
Veröffentlicht: (2023)

Andromeda's asymmetric satellite system as a challenge to cold dark matter cosmology
von: Kanehisa, Kosuke Jamie, et al.
Veröffentlicht: (2025)

Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
von: Yesuf, Hassen M., et al.
Veröffentlicht: (2026)

Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
von: Iqbal, Asif, et al.
Veröffentlicht: (2025)