activity
20172023
most citedELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias

75 citations · 233 across the 15 of their papers we have counts for

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Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2023★ 3 cited

The chromatic Point Spread Function of weak lensing measurement in Chinese Space Station survey Telescope

Q. Y. Liu, X. Z. Er, Z. H. Fan +6

The weak gravitational lensing is a powerful tool in modern cosmology. To accurately measure the weak lensing signal, one has to control the systematic bias to a small level. One o…

astro-ph.CO2023★ 4 cited

CSST WL preparation I: forecast the impact from non-Gaussian covariances and requirements on systematics-control

Ji Yao, Huanyuan Shan, Ran Li +11

The precise estimation of the statistical errors and accurate removal of the systematical errors are the two major challenges for the stage IV cosmic shear surveys. We explore thei…

astro-ph.CO2022★ 14 cited

Effects of galaxy intrinsic alignment on weak lensing peak statistics

Tianyu Zhang, Xiangkun Liu, Chengliang Wei +4

The galaxy intrinsic alignment (IA) is a dominant source of systematics in weak lensing (WL) studies. In this paper, by employing large simulations with semi-analytical galaxy form…

astro-ph.CO2022

Tolerance For the Pixelation Effect in Shear Measurement

Zhi Shen, Jun Zhang, Hekun Li +6

Images taken by space telescopes typically have a superb spatial resolution, but a relatively poor sampling rate due to the finite CCD pixel size. Beyond the Nyquist limit, it beco…

astro-ph.CO2021★ 16 cited

Detection of Cosmic Magnification via Galaxy Shear -- Galaxy Number Density Correlation from HSC Survey Data

Xiangkun Liu, Dezi Liu, Zucheng Gao +5

We propose a novel method to detect cosmic magnification signals by cross-correlating foreground convergence fields constructed from galaxy shear measurements with background galax…

astro-ph.CO2020★ 17 cited

Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes

Xikai Shan, Chengliang Wei, Bin Hu

Gravitational waves (GWs) may be magnified or de-magnified due to lensing. This phenomenon will bias the distance estimation based on the matched filtering technique. Via the multi…

astro-ph.CO2018★ 15 cited

The Correspondence between Convergence Peaks from Weak Lensing and Massive Dark Matter Haloes

Chengliang Wei, Guoliang Li, Xi Kang +4

The convergence peaks, constructed from galaxy shape measurement in weak lensing, is a powerful probe of cosmology as the peaks can be connected with the underlined dark matter hal…

astro-ph.CO2018★ 1 cited

The Magnification Invariant of Circularly-symmetric Lens Models

Chengliang Wei, Zhe Chu, Yiping Shu

In the context of strong gravitational lensing, the magnification of image is of crucial importance to constrain various lens models. For several commonly used quadruple lens model…

astro-ph.CO2018★ 30 cited

Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations

Chengliang Wei, Guoliang Li, Xi Kang +15

The intrinsic alignment of galaxies is an important systematic effect in weak-lensing surveys, which can affect the derived cosmological parameters. One direct way to distinguish d…