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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

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6 papers · 1 filter

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.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.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.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.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…