activity
19972026
most citedAre Great Disks Defined by Satellite Galaxies in Milky-Way Type Halos Rare in CDM model?

88 citations · 367 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

The influence of plasma lensing magnification to the luminosity function of fast radio bursts

Xinzhong Er, Weishan Zhu, Shude Mao +1

Small scale clumps of ionized gas have been suggested by observations in interstellar medium and circumgalactic medium. The propagation of radio signals can be deflected by these p…

astro-ph.CO2011★ 7 cited

Effects of supermassive binary black holes on gravitational lenses

Nan Li, Shude Mao, Liang Gao +2

Recent observations indicate that many if not all galaxies host massive central black holes (BHs). In this paper we explore the influence of supermassive binary black holes (SMBBHs…

astro-ph.CO2009★ 9 cited

Impacts of Source Properties on Strong Lensing by Rich Galaxy Clusters

G. J. Gao, Y. P. Jing, S. Mao +2

We use a high-resolution -body simulation to investigate the influence of background galaxy properties, including redshift, size, shape and clustering, on the efficiency of form…

astro-ph.CO2009★ 24 cited

Properties of Long Gamma-Ray Burst Host Galaxies in Cosmological Simulation

M. A. Campisi, G. De Lucia, L. -X. Li +2

We use galaxy catalogues constructed by combining high-resolution N-body simulations with semi-analytic models of galaxy formation to study the properties of Long Gamma-Ray Burst (…

astro-ph2007★ 25 cited

Properties of Wide-separation Lensed Quasars by Clusters of Galaxies in the SDSS

G. L. Li, S. Mao, Y. P. Jing +2

We use high-resolution N-body numerical simulations to study the number of predicted large-separation multiply-imaged systems produced by clusters of galaxies in the SDSS photometr…

astro-ph2005★ 63 cited

Is the Number of Giant Arcs in LCDM Consistent With Observations?

G. L. Li, S. Mao, Y. P. Jing +3

We use high-resolution N-body simulations to study the galaxy-cluster cross-sections and the abundance of giant arcs in the CDM model. Clusters are selected from the simulations…