activity
20222026
most citedIntroduction to the Chinese Space Station Survey Telescope (CSST)

59 citations · 80 across the 21 of their papers we have counts for

collaborators
Showing 2024Show all

9 papers · 1 filter

astro-ph.CO2024

Exploring cosmological constraints of the weak gravitational lensing and galaxy clustering joint analysis in the CSST photometric survey

Qi Xiong, Yan Gong, Xingchen Zhou +10

We explore the joint weak lensing and galaxy clustering analysis from the photometric survey operated by the China Space Station Telescope (CSST), and study the strength of the cos…

astro-ph.CO2024

2D watershed void clustering for probing the cosmic large-scale structure

Yingxiao Song, Yan Gong, Qi Xiong +5

Cosmic void has been proven to be an effective cosmological probe of the large-scale structure (LSS). However, since voids are usually identified in spectroscopic galaxy surveys, t…

astro-ph.CO2024

Void Number Counts as a Cosmological Probe for the Large-Scale Structure

Yingxiao Song, Qi Xiong, Yan Gong +6

Void number counts (VNC) indicates the number of low-density regions in the large-scale structure (LSS) of the Universe, and we propose to use it as an effective cosmological probe…

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

Effectiveness of halo and galaxy properties in reducing the scatter in the stellar-to-halo mass relation

Wenxiang Pei, Qi Guo, Shi Shao +2

The stellar-to-halo mass relation (SHMR) is a fundamental relationship between galaxies and their host dark matter haloes. In this study, we examine the scatter in this relation fo…

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★ 15 cited

JWST's first glimpse of a z > 2 forming cluster reveals a top-heavy stellar mass function

Hanwen Sun, Tao Wang, Ke Xu +11

Clusters and their progenitors (protoclusters) at z = 2-4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves a…

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…

astro-ph.GA2024

A younger Universe implied by satellite pair correlations from SDSS observations of massive galaxy groups

Qing Gu, Qi Guo, Marius Cautun +5

Many of the satellites of galactic-mass systems such as the Miky Way, Andromeda and Centaurus A show evidence of coherent motions to a larger extent than most of the systems predic…