activity
20242026
most citedStatistical properties of filaments in the cosmic web

6 citations · 13 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

Growth from KiDS: Stellar mass assembly of galaxies since z=2 in the light of Kilo-Degree Survey

Qingshan Wang, Antonios Katsianis, Nicola R. Napolitano +10

We measure the galaxy stellar mass function at using 28M galaxies from the KiDS DR4 which spans an effective survey area of 676.9 deg. Combining nine-band photometry…

astro-ph.GA2026

Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster

Hangxin Pu, Antonios Katsianis, Weiguang Cui +8

We investigate the co-evolution of supermassive black holes (SMBHs) and central galaxies in massive clusters using the GIZMO-SIMBA and TNG-Cluster zoom-in simulations at . W…

astro-ph.CO2026

Multi-tracer mass bias in matched cosmic voids from SDSS DR7 and the ELUCID constrained simulation

Youcai Zhang, Xiaohu Yang, Hong Guo +1

Cosmic voids provide a unique environment for studying the relationship between galaxies, subhaloes, and dark matter in the underdense Universe. Using the SDSS galaxy catalogue and…

astro-ph.CO2026★ 1 cited

Robustness of cosmic void statistics: insights from SDSS DR7 and the ELUCID simulation

Youcai Zhang, Xiaohu Yang, Hong Guo +2

We present a systematic analysis of the statistical properties of cosmic voids using galaxies from the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) and subhaloes from the ELU…

astro-ph.GA2026

BayeSED-GALAXIES II. Bayesian full spectrum analysis of galaxies and application in the CSST wide-field slitless spectroscopy survey

Yunkun Han, Xian Zhong Zheng, Xiaohu Yang +21

The China Space Station Telescope (CSST) will conduct wide-field multiband photometric imaging and slitless spectroscopic surveys, advancing cosmology and galaxy evolution studies.…

astro-ph.CO2026

First Observational Evidence for Split Infall Flow of Cosmic Filaments into Clusters

Ji Yao, Huanyuan Shan, Pengjie Zhang +5

Velocity fields in the cosmic web are fundamental to structure formation but remain difficult to observe directly beyond the linear regime. Here we present observational evidence t…

astro-ph.GA2025★ 1 cited

Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8

Antonios Katsianis, Qingshan Wang, Xiaohu Yang +13

The growth model is an effective parameterization employed across various scientific disciplines and scales to depict growth. It has been demonstrated that the cosmic star form…

astro-ph.CO2025★ 5 cited

Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation

Youcai Zhang, Xiaohu Yang, Hong Guo +2

Using galaxies from the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) along with haloes from the dark matter only constrained ELUCID (Exploring the Local Universe with the reC…

astro-ph.GA2024

A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon

Shuang Liu, Xian Zhong Zheng, Valentino Gonzalez +10

The process of galaxy cluster formation likely leaves an imprint on the properties of its individual member galaxies. Understanding this process is essential for uncovering the evo…

astro-ph.CO2024★ 6 cited

Statistical properties of filaments in the cosmic web

Youcai Zhang, Hong Guo, Xiaohu Yang +1

In the context of the cosmological and constrained ELUCID simulation, this study explores the statistical characteristics of filaments within the cosmic web, focussing on aspects s…