activity
20242026
most citedCSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys

17 citations · 21 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.CO2026

Shape-Preserving Evolution of the Global Ultraviolet Quasar Luminosity Function to

Wenjie Wang, Zunli Yuan, Yu Luo +1

We present a global unbinned-likelihood analysis of the rest-frame ultraviolet (UV) quasar luminosity function (QLF) over , using a final analysis sample of 70,960…

astro-ph.GA2026

Comparative analysis of missing data imputation methods for CSST survey: Impact on photometric redshift estimation performance

Ling Wang, Zhu Chen, Zhijian Luo +42

Improving the accuracy of photometric redshifts (photo-) is essential for reliable statistical studies of cosmology and galaxy evolution. However, missing photometric bands are…

astro-ph.GA2026

The Steep-spectrum Radio-loud AGN Luminosity Function and Its Implications for Black Hole Growth and Star Formation

Wenjie Wang, Zunli Yuan, B. Šlaus +2

We study the cosmic evolution of radio-loud active galactic nuclei (AGNs) using a beaming-minimized sample of 4{,}555 steep-spectrum sources over , compiled from the…

astro-ph.IM2025

Mock Observations for the CSST Mission: Main Surveys -- the Mock Catalogue

Cheng-Liang Wei, Yu Luo, Hao Tian +17

The Chinese Space Station Survey Telescope (CSST) is a flagship space mission, designed to carry out a large-area sky survey to explore the nature of dark matter and dark energy in…

astro-ph.GA2025

Revisiting the 150 MHz Radio Luminosity Function of Star-Forming Galaxies with LOFAR Deep Fields through a Refined Statistical Framework

Wenjie Wang, Zunli Yuan, Hongwei Yu +3

We present a comprehensive analysis of the 150~MHz radio luminosity function (LF) of star-forming galaxies (SFGs) using deep observations from the LOFAR Two-metre Sky Survey in the…

astro-ph.CO2025

Modeling the impacts of galaxy intrinsic alignments on weak lensing peak statistics

Tianyu Zhang, Xiangkun Liu, Ziwei Li +5

Weak gravitational lensing (WL) peak statistics capture cosmic non-linear structures and can provide additional cosmological information complementary to cosmic shear two-point cor…

astro-ph.GA2025

ViT-based Local Volume dwarf galaxy Identificationin (VIDA) in the CSST survey

Han Qu, Zhen Yuan, Chengliang Wei +11

Identifying dwarf galaxies within the Local Volume is crucial for constraining the luminosity function of satellite galaxies in the nearby universe. We report the detection capabil…

astro-ph.CO2025★ 1 cited

The Jiutian simulations for the CSST extra-galactic surveys

Jiaxin Han, Ming Li, Wenkang Jiang +23

We provide an overview of the Jiutian simulations, a hybrid simulation suite for the China Space Survey Telescope (CSST) extragalactic surveys. It consists of four complementary mo…

astro-ph.CO2025

Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. VIII. Revisiting the Lensing is Low Effect

Xiaolin Luo, Kun Xu, Yipeng Jing +6

The issue of over-predicting the galaxy-galaxy lensing (GGL) signal using conventional galaxy-halo connection models has become well-known as the ``Lensing is Low'' problem, which…

astro-ph.GA2024★ 3 cited

Intermediate Mass Ratio Inspirals in Milky Way Galaxies

Jillian Bellovary, Yuantong Luo, Thomas Quinn +3

A consequence of a non-zero occupation fraction of massive black holes (MBHs) in dwarf galaxies is that these MBHs can become residents of larger galaxy halos via hierarchical merg…

astro-ph.CO2024

Cosmological Prediction of the Void and Galaxy Clustering Measurements in the CSST Spectroscopic Survey

Yingxiao Song, Qi Xiong, Yan Gong +10

The void power spectrum is related to the clustering of low-density regions in the large-scale structure (LSS) of the Universe, and can be used as an effective cosmological probe t…

astro-ph.GA2024

Simulating emission line galaxies for the next generation of large-scale structure surveys

Wenxiang Pei, Qi Guo, Ming Li +8

We investigate emission line galaxies across cosmic time by combining the modified L-Galaxies semi-analytical galaxy formation model with the JiuTian cosmological simulation. We im…

astro-ph.GA2024★ 17 cited

CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys

Yizhou Gu, Xiaohu Yang, Jiaxin Han +29

In this paper, we set out to construct a set of reference mock galaxy redshift surveys (MGRSs) for the future Chinese Space-station Survey Telescope (CSST) observation, where subse…

astro-ph.CO2024

Cosmological Forecast of the Void Size Function Measurement from the CSST Spectroscopic Survey

Yingxiao Song, Qi Xiong, Yan Gong +11

Void size function (VSF) contains information of the cosmic large-scale structure (LSS), and can be used to derive the properties of dark energy and dark matter. We predict the VSF…