activity
20242026
most citedCharacterising the intra-cluster light in The Three Hundred simulations

29 citations · 56 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2026

Identifying backsplash galaxies using machine learning

Roan Haggar, Elizaveta Sazonova, Cameron R. Morgan +5

The galaxy population in the outskirts of a cluster contains members that have been pre-processed in groups and filaments, as well as backsplash galaxies -- those that have recentl…

astro-ph.CO2026

Probing the baryonic--dark matter connection in galaxy clusters using X-rays with gated recurrent unit neural networks

Asif Iqbal, Subhabrata Majumdar, Weiguang Cui +3

Accurate cluster mass measurements are crucial for cosmology, yet conventional hydrostatic equilibrium (HSE) methods can suffer from systematic biases, particularly in dynamically…

astro-ph.CO2025★ 1 cited

Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks

Asif Iqbal, Subhabrata Majumdar, Elena Rasia +4

Precise determination of galaxy cluster masses is crucial for establishing reliable mass-observable scaling relations in cluster cosmology. We employ graph neural networks (GNNs) t…

astro-ph.GA2025

The life and times of dark matter haloes: what will I be when I grow up?

Julian Onions, Frazer Pearce, Alexander Knebe +6

Are the most massive objects in the Universe today the direct descendants of the most massive objects at higher redshift? We address this question by tracing the evolutionary histo…

astro-ph.GA2025★ 3 cited

The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles

Kris Walker, Aaron Ludlow, Chris Power +2

We examine the splashback structure of galaxy clusters using hydrodynamical simulations from the GIZMO run of The Three Hundred Project, focusing on the relationship between the st…

astro-ph.GA2025

PyMGal: A Python Package for Generating Optical Mock Observations from Hydrodynamical Simulations

Patrick Janulewicz, Weiguang Cui

We introduce PyMGal, a Python package for generating optical mock observations of galaxies from hydrodynamical simulations. PyMGal reads the properties of stellar particles from th…

astro-ph.CO2024

Constraining neutrino mass with the CSST galaxy clusters

Mingjing Chen, Yufei Zhang, Wenjuan Fang +2

With the advent of next-generation surveys, constraints on cosmological parameters are anticipated to become more stringent, particularly for the total neutrino mass. This study fo…

astro-ph.GA2024

Stellar stripping efficiencies of satellites in numerical simulations: the effect of resolution, satellite properties and numerical disruption

G. Martin, F. R. Pearce, N. A. Hatch +3

The stellar stripping of satellites in cluster haloes is understood to play an important role in the production of intracluster light. Increasingly, cosmological simulations have b…

astro-ph.GA2024★ 3 cited

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

Ana Contreras-Santos, Fernando Buitrago, Alexander Knebe +5

The observation of a massive galaxy with an extremely low dark matter content (i.e. NGC 1277) has posed questions about how such objects form and evolve in a hierarchical universe.…

astro-ph.GA2024★ 15 cited

Reconsidering the dynamical states of galaxy clusters using PCA and UMAP

Roan Haggar, Federico De Luca, Marco De Petris +10

Numerous metrics exist to quantify the dynamical state of galaxy clusters, both observationally and within simulations. Many of these correlate strongly with one another, but it is…

astro-ph.CO2024

How much do we know the halo mass function? Predictions beyond resolution

Weiguang Cui

As a common gravitation virialized object in the standard CDM cosmology, dark matter halo connects from the large-scale structure all the way down to galaxy and star formation.…

astro-ph.CO2024★ 5 cited

Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations

Mingjing Chen, Weiguang Cui, Wenjuan Fang +1

The main systematics in cluster cosmology is the uncertainty in the mass-observable relation. In this paper, we focus on the most direct cluster observable in optical surveys, i.e.…

astro-ph.CO2024★ 29 cited

Characterising the intra-cluster light in The Three Hundred simulations

Ana Contreras-Santos, Alexander Knebe, Weiguang Cui +7

We characterise the intra-cluster light (ICL) in ensembles of full-physics cluster simulations from The Three Hundred project, a suite of 324 hydrodynamical resimulations of cluste…