activity
20232026
most citedPrincipal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties

12 citations · 27 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

AKRA 3.0: A matrix-free Inversion Framework for Weak Lensing Mass Mapping and Its Application to DES Y3 Data

Yuan Shi, Pengjie Zhang, Li Cui +2

Weak gravitational lensing mass mapping offers a direct probe of the matter distribution. Accurate reconstruction of mass maps from masked shear catalogs remains challenging due to…

astro-ph.CO2025

The first AKRA mass map reconstruction from HSC Y1 data

Yuan Shi, Pengjie Zhang, Zhao Chen +4

Weak lensing mass-mapping from shear catalogs faces systematic challenges from survey masks and spatially varying noise. To overcome these issues and reconstruct unbiased convergen…

astro-ph.CO2025

Proposal to construct the dark-matter-only counterpart of the observed universe combining weak lensing and baryon censuses

Shuren Zhou, Pengjie Zhang

Baryonic effects such as AGN feedback can significantly impact the matter clustering, are harder to model from first principles, and emerge as a severe limiting factor in weak lens…

astro-ph.CO2025

Cavendish experiment with fast radio bursts on cosmological scales

Shuren Zhou, Pengjie Zhang

A key measure of gravity is the relation between the Weyl potential and the matter overdensity , encapsulated as an effective gravitational constant for…

astro-ph.CO2025

Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies

Jian Qin, Pengjie Zhang, Zhu Chen +6

Weak lensing alters galaxy sizes and fluxes, influencing the clustering patterns of galaxies through cosmic magnification. This effect enables the reconstruction of weak lensing co…

astro-ph.CO2024

The direct measurement of gravitational potential decay rate at cosmological scales II -- Improved dark energy constraint from

Fuyu Dong, Pengjie Zhang, Haojie Xu +1

The gravitational potential decay rate (DR) is caused by the cosmic acceleration of the universe, providing a direct probe into the existence of dark energy (DE). We present measur…

astro-ph.IM2024★ 4 cited

AKRA 2.0: Accurate Kappa Reconstruction Algorithm for masked shear catalog

Yuan Shi, Pengjie Zhang, Furen Deng +4

Cosmic shear surveys serve as a powerful tool for mapping the underlying matter density field, including non-visible dark matter. A key challenge in cosmic shear surveys is the acc…

astro-ph.CO2024★ 3 cited

Challenges in Cosmic Magnification Reconstruction by Magnification Response

Shuren Zhou, Pengjie Zhang

Cosmic magnification on the observed galaxy overdensity is a promising weak gravitational lensing tracer. Current cosmic magnification reconstruction algorithms, ABS (Analytical me…

astro-ph.CO2024★ 3 cited

Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering

Shuren Zhou, Pengjie Zhang

The stochasticity in galaxy clustering, the mismatch between galaxy and underlying matter distribution, suppresses the matter clustering amplitude reconstructed by the combination…

astro-ph.CO2024

Enhancing Morphological Measurements of Cosmic Web with Delaunay Tessellation Field Estimation

Yu Liu, Yu Yu, Pengjie Zhang +1

The density fields constructed by traditional mass assignment methods are susceptible to irritating discreteness, which hinders morphological measurements of cosmic large-scale str…

astro-ph.CO2023★ 5 cited

Accurate Kappa Reconstruction Algorithm for masked shear catalog (AKRA)

Yuan Shi, Pengjie Zhang, Zeyang Sun +1

Weak gravitational lensing is an invaluable tool for understanding fundamental cosmological physics. An unresolved issue in weak lensing cosmology is to accurately reconstruct the…

astro-ph.CO2023★ 12 cited

Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties

Shuren Zhou, Pengjie Zhang, Ziyang Chen

Ongoing and upcoming galaxy surveys are providing precision measurements of galaxy clustering. However a major obstacle in its cosmological application is the stochasticity in the…