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20082026
most citedCosmology from the Chinese Space Station Optical Survey (CSS-OS)

306 citations · 2.6k across the 63 of their papers we have counts for

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Showing astro-ph.COShow all

25 papers · 1 filter

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.CO2023★ 6 cited

Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model

Wei Du, Liping Fu, Yiping Shu +3

With mock strong gravitational lensing images, we investigate the performance of the broken power-law (BPL) model proposed by \citet{2020ApJ...892...62D} on the mass reconstruction…

astro-ph.CO2023★ 8 cited

Strong gravitational lensing's 'external shear' is not shear

Amy Etherington, James W. Nightingale, Richard Massey +19

The distribution of mass in galaxy-scale strong gravitational lenses is often modelled as an elliptical power law plus 'external shear', which notionally accounts for neighbouring…

astro-ph.CO2022★ 9 cited

Scanning For Dark Matter Subhalos in Hubble Space Telescope Imaging of 54 Strong Lenses

James W. Nightingale, Qiuhan He, Xiaoyue Cao +9

The cold dark matter (DM) model predicts that every galaxy contains thousands of DM subhalos; almost all other DM models include a physical process that smooths away the subhalos.…

astro-ph.CO2022★ 32 cited

Testing strong lensing subhalo detection with a cosmological simulation

Qiuhan He, James Nightingale, Andrew Robertson +9

Strong gravitational lensing offers a compelling test of the cold dark matter paradigm, as it allows for subhaloes with masses of M and below to be detected. W…

astro-ph.CO2022★ 50 cited

Automated galaxy-galaxy strong lens modelling: no lens left behind

Amy Etherington, James W. Nightingale, Richard Massey +9

The distribution of dark and luminous matter can be mapped around galaxies that gravitationally lens background objects into arcs or Einstein rings. New surveys will soon observe h…