activity
20242026
most citedIntrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations

5 citations · 7 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2026

The Limits of Photometric Dynamics: Benchmarking Cluster Relaxation Diagnostics

Alisson P. Costa, Andre L. B. Ribeiro, Zhonglue L. Wen +1

Galaxy clusters are key probes of cosmology and structure formation, yet their dynamical classification traditionally relies on spectroscopic redshifts, which do not scale efficien…

astro-ph.CO2025★ 2 cited

Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe

Michael J. West, Roberto De Propris, Maret Einasto +2

The universe's large-scale structure forms a vast, interconnected network of filaments, sheets, and voids known as the cosmic web. For decades, astronomers have observed that the o…

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.CO2024

COSMIC: A Galaxy Cluster Finding Algorithm Using Machine Learning

Da-Chuan Tian, Yang Yang, Zhong-Lue Wen +1

Building a comprehensive catalog of galaxy clusters is a fundamental task for the studies on the structure formation and galaxy evolution. In this paper, we present COSMIC (Cluster…

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.…