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20052023
most citedEffects of Dark Matter Substructures on Gravitational Lensing: Results from the Aquarius Simulations

115 citations · 800 across the 38 of their papers we have counts for

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Showing 2022Show all

8 papers · 1 filter

astro-ph.GA2022★ 15 cited

Local Group Dwarf Galaxy Detection Limit in the CSST survey

Han Qu, Zhen Yuan, Amandine Doliva-Dolinsky +9

We predict the dwarf galaxy detection limits for the upcoming Chinese Space Station Telescope (CSST) survey that will cover 17,500 deg of the sky with a wide field of view of…

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.IM2022★ 2 cited

The spherical Fast Multipole Method (sFMM) for Gravitational Lensing Simulation

Xingpao Suo, Xi Kang, Chengliang Wei +1

In this paper, we present a spherical Fast Multipole Method (sFMM) for ray tracing simulation of gravitational lensing (GL) on a curved sky. The sFMM is a non-trivial extension of…

astro-ph.IM2022★ 9 cited

Towards Super-resolution via Iterative multi-exposure Coaddition

Lei Wang, Guoliang Li, Xi Kang

In this article, we provide an alternative up-sampling and PSF deconvolution method for the iterative multi-exposure coaddition. Different from the previous works, the new method h…

astro-ph.CO2022★ 20 cited

Wave effect of gravitational waves intersected with a microlens field: a new algorithm and supplementary study

Xikai Shan, Guoliang Li, Xuechun Chen +2

The increase in gravitational wave (GW) events has allowed receiving strong lensing image pairs of GWs. However, the wave effect (diffraction and interference) due to the microlens…

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…