activity
20212026
most citedSpectroscopic and Photometric Redshift Estimation by Neural Networks For the China Space Station Optical Survey (CSS-OS)

29 citations · 125 across the 26 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2026

CSST large-scale structure analysis pipeline: IV. Cosmic Voids Identified from Galaxy Group Samples as Probes of the Large-scale Structure

Yingxiao Song, Xiaohu Yang, Yan Gong +16

Because groups are directly associated with halos, they allow for considerably simpler theoretical modeling than approaches based on individual galaxies. We therefore propose to us…

astro-ph.GA2026

Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7

Yingxiao Song, Xiaohu Yang, Yan Gong +4

Cosmic voids provide a distinct low-density region for studying the environmental effects of galaxy properties. Using the SDSS DR7 catalog, we identify non-spherical voids via Voro…

astro-ph.CO2026

Lyman- forest constraints on pure and mixed fuzzy dark matter

Jianxiang Liu, Yan Gong, Xingchen Zhou

Fuzzy dark matter (FDM), often realized as an ultralight scalar field, can suppress the growth of small-scale structures and could be strictly tested with Lyman- forest measurem…

astro-ph.IM2026

Extracting redshifts from 2D slitless spectroscopic images using deep learning for the CSST galaxy survey

Xingchen Zhou, Yan Gong, Xin Zhang +4

Wide-field slitless spectroscopic galaxy surveys, such as the one performed by the upcoming Chinese Space Station Survey Telescope (CSST), are crucial for precision cosmology but p…

astro-ph.GA2026

Cross-Comparison of Galaxies Detected in the CSST Spectroscopic Survey and the SKA HI Survey

Yingfeng Liu, Furen Deng, Wenxiang Pei +8

We present a forward-modeling framework to forecast the galaxies detected in the Chinese Space Station Survey Telescope (CSST) spectroscopic survey and the Square Kilometre Array (…

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.…

cs.LG2025

AI Agent for Source Finding by SoFiA-2 for SKA-SDC2

Xingchen Zhou, Nan Li, Peng Jia +7

Source extraction is crucial in analyzing data from next-generation, large-scale sky surveys in radio bands, such as the Square Kilometre Array (SKA). Several source extraction pro…

astro-ph.CO2025

Exploring Cosmological Constraints of the Void-Lensing Cross-Correlation in the CSST Photometric Survey

Qi Xiong, Yan Gong, Junhui Yan +8

We investigate the cosmological constraints from the void-lensing cross-correlation assuming the CDM model for the Chinese Space Station Survey Telescope (CSST) photometric surv…

astro-ph.IM2025

Photo- Estimation with Normalizing Flow

Yiming Ren, Kwan Chuen Chan, Le Zhang +6

Accurate photometric redshift (photo-) estimation is a key challenge in cosmology, as uncertainties in photo- directly limit the scientific return of large-scale structure an…

astro-ph.CO2025

Cosmological Prediction from the joint observation of MeerKAT and CSST at = 0.4 1.2

Yu-Er Jiang, Yan Gong, Qi Xiong +10

Cross-correlating neutral hydrogen (HI) 21cm intensity mapping with galaxy surveys provides an effective probe of astrophysical and cosmological information. This work presents a c…

astro-ph.IM2025★ 3 cited

GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations

Xingchen Zhou, Hang Yang, Nan Li +11

We introduce GalaxyGenius, a Python package designed to produce synthetic galaxy images tailored to different telescopes based on hydrodynamical simulations. Its implementation wil…

astro-ph.CO2025

Improving Photometric Redshift Estimation for CSST Mock Catalog Using SED Templates Calibrated with Perturbation Algorithm

Yicheng Li, Liping Fu, Zhu Chen +11

Photometric redshifts of galaxies obtained by multi-wavelength data are widely used in photometric surveys because of its high efficiency. Although various methods have been develo…

astro-ph.CO2025

Cosmological distance forecasts for the CSST Galaxy Survey using BAO peaks

Feng Shi, Jieyi Tian, Zhejie Ding +21

The measurement of cosmological distances using baryon acoustic oscillations (BAO) is crucial for studying the universe's expansion. The Chinese Space Station Telescope (CSST) gala…

astro-ph.CO2025★ 15 cited

Future Cosmology: New Physics and Opportunity from the China Space Station Telescope (CSST)

Yan Gong, Haitao Miao, Xingchen Zhou +12

The China Space Station Telescope (CSST) is the next-generation Stage~IV survey telescope. It can simultaneously perform multi-band imaging and slitless spectroscopic wide- and dee…

astro-ph.CO2025★ 1 cited

Cosmological Constraints using the Void Size Function Data from BOSS DR16

Yingxiao Song, Yan Gong, Xingchen Zhou +3

We measure the void size function (VSF) from the Baryon Oscillation Spectroscopic Survey (BOSS DR16) and perform the cosmological constraints. The BOSS DR16 galaxy sample is select…

astro-ph.GA2024★ 7 cited

Estimating Photometric Redshifts for Galaxies from the DESI Legacy Imaging Surveys with Bayesian Neural Networks Trained by DESI EDR

Xingchen Zhou, Nan Li, Hu Zou +6

We present a catalogue of photometric redshifts for galaxies from DESI Legacy Imaging Surveys, which includes billion sources covering 14,000 . The photomet…

astro-ph.CO2024★ 5 cited

MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys

Cheng Zhao, Song Huang, Mengfan He +41

The MUltiplexed Survey Telescope (MUST) is a 6.5-meter telescope under development. Dedicated to highly-multiplexed, wide-field spectroscopic surveys, MUST observes over 20,000 tar…

astro-ph.GA2024

Photometric Redshift Estimation for CSST Survey with LSTM Neural Networks

Zhijian Luo, Yicheng Li, Junhao Lu +11

Accurate estimation of photometric redshifts (photo-s) is crucial for cosmological surveys. Various methods have been developed for this purpose, such as template fitting method…

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★ 6 cited

Accurately Estimating Redshifts from CSST Slitless Spectroscopic Survey using Deep Learning

Xingchen Zhou, Yan Gong, Xin Zhang +10

Chinese Space Station Telescope (CSST) has the capability to conduct slitless spectroscopic survey simultaneously with photometric survey. The spectroscopic survey will measure sli…

astro-ph.IM2024

Imputation of Missing Photometric Data and Photometric Redshift Estimation for CSST

Zhijian Luo, Zhirui Tang, Zhu Chen +10

Accurate photometric redshift (photo-) estimation requires support from multi-band observational data. However, in the actual process of astronomical observations and data proce…

astro-ph.CO2023★ 1 cited

Estimating Photometric Redshift from Mock Flux for CSST Survey by using Weighted Random Forest

Junhao Lu, Zhijian Luo, Zhu Chen +10

Accurate estimation of photometric redshifts (photo-) is crucial in studies of both galaxy evolution and cosmology using current and future large sky surveys. In this study, we…

astro-ph.CO2023★ 8 cited

Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys

Yuer Jiang, Yan Gong, Meng Zhang +6

Cross-correlating the data of neutral hydrogen (HI) 21cm intensity mapping with galaxy surveys is an effective method to extract astrophysical and cosmological information. In this…

astro-ph.CO2022★ 8 cited

Foreground Removal of CO Intensity Mapping Using Deep Learning

Xingchen Zhou, Yan Gong, Furen Deng +3

Line intensity mapping (LIM) is a promising probe to study star formation, the large-scale structure of the Universe, and the epoch of reionization (EoR). Since carbon monoxide (CO…