activity
20232026
most citedLarge-scale Array for Radio Astronomy on the Farside

19 citations · 36 across the 22 of their papers we have counts for

collaborators

23 papers

astro-ph.CO2026

Cross-correlating Squared kSZ and HI Intensity Fields: A Map-level ACT--MeerKAT Forecast

Yu-Er Jiang, Yun Liu, Yan Gong +5

The kinetic Sunyaev--Zel'dovich (kSZ) effect probes the line-of-sight momentum of free electrons, but its blackbody spectrum and velocity-dependent sign make it difficult to isolat…

astro-ph.CO2026

Exploring Primordial Non-Gaussianity Measurements in the CSST Spectroscopic Survey

Jiangnan Duan, Yan Gong, Qi Xiong +5

Primordial non-Gaussianity (PNG) is a fundamental probe of the physics of the early Universe and inflation. Here we present a comprehensive study of the constraints on the local-ty…

astro-ph.CO2026

Probing Baryonic Feedback Effect with CSST Weak Lensing and Future FRB Measurements

Shuai Feng, Yan Gong, Qi Xiong +4

We explore the joint probe on the baryonic feedback effect using the weak lensing measurement from the upcoming Chinese Space-station Survey Telescope (CSST) photometric survey and…

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.CO2026

Constraining Lyman-Werner Feedback from Velocity Acoustic Oscillations in the Cosmic Dawn 21 cm Signal

Xi Du, Bin Yue, Furen Deng +4

During Cosmic Dawn, Pop III stars could be formed in minihalos through molecular hydrogen (H) cooling. The minimum halo mass required for H cooling is highly sensitive to L…

astro-ph.CO2025★ 1 cited

Forecasting the Constraint on the Hu-Sawicki Modified Gravity in the CSST pt Photometric Survey

Jun-Hui Yan, Yan Gong, Qi Xiong +5

We forecast the constraint on the Hu-Sawicki model from the photometric survey operated by the Chinese Space Station Survey Telescope (CSST). The simulated pt data…

astro-ph.CO2025

Forecasting Constraint on Primordial Black Hole Properties with the CSST pt Analysis

Dingao Hu, Yan Gong, Pengfei Su +4

This study forecasts the constraints on the properties of primordial black holes (PBHs) as a cold dark matter component using the galaxy clustering, weak lensing, and galaxy-galaxy…

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.CO2025

Supernova Classification using the Recurrent Neural Network in the CSST Ultra-Deep Field Survey

Minglin Wang, Yan Gong, Dejia Zhou +1

We study supernova (SN) classification using the Recurrent Neural Networks (RNNs) within the Chinese Space-station Survey Telescope Ultra-Deep Field (CSST-UDF) photometric survey a…

astro-ph.CO2025

Constraining and Comparing the Dynamical Dark Energy and f(R) Modified Gravity Models with Cosmological Distance Measurements

Shuai Feng, Yan Gong, Xiaohui Liu +2

We constrain and compare the CDM dynamical dark energy model and three modified gravity models using the current cosmological distance measurements, including 11…

astro-ph.CO2025

Exploring Joint Observation of the CSST Shear and clustering of astrophysical gravitational wave source measurements

Pengfei Su, Yan Gong, Qi Xiong +4

We present a comprehensive forecast for cosmological constraints using the joint observation of the cosmic shear signal from the Chinese Space Station Survey Telescope (CSST) and t…

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.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.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.CO2024

Forecasting Constraint on the Theory with the CSST SN Ia and BAO Surveys

Jun-Hui Yan, Yan Gong, Minglin Wang +2

The modified gravity theory can explain the accelerating expansion of the late Universe without introducing dark energy. In this study, we predict the constraint strength on…

astro-ph.IM2024★ 19 cited

Large-scale Array for Radio Astronomy on the Farside

Xuelei Chen, Feng Gao, Fengquan Wu +20

At the Royal Society meeting in 2023, we have mainly presented our lunar orbit array concept called DSL, and also briefly introduced a concept of a lunar surface array, LARAF. As t…

astro-ph.CO2024

Velocity acoustic oscillations on Cosmic Dawn 21 cm power spectrum as a probe of small-scale density fluctuations

Xin Zhang, Hengjie Lin, Meng Zhang +4

We investigate the feasibility of using the velocity acoustic oscillations (VAO) features on the Cosmic Dawn 21 cm power spectrum to probe small-scale density fluctuations. In the…

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.CO2024

Cosmological Prediction of the CSST Ultra Deep Field Type Ia Supernova Photometric Survey

Minglin Wang, Yan Gong, Furen Deng +3

Type Ia supernova (SN Ia) as a standard candle is an ideal tool to measure cosmic distance and expansion history of the Universe. Here we investigate the SN Ia photometric measurem…

astro-ph.CO2023

Forecasting the BAO Measurements of the CSST galaxy and AGN Spectroscopic Surveys

Haitao Miao, Yan Gong, Xuelei Chen +3

The spectroscopic survey of China's Space Survey Telescope (CSST) is expected to obtain a huge number of slitless spectra, including more than one hundred million galaxy spectra an…

astro-ph.CO2023★ 1 cited

Constraining Ultralight Axions with CSST Weak Gravitational Lensing and Galaxy Clustering Photometric Surveys

Hengjie Lin, Furen Deng, Yan Gong +1

Ultralight axion (ULA) can be one of the potential candidates for dark matter. The extremely low mass of the ULA can lead to a de Broglie wavelength the size of galaxies which resu…