activity
20082026
most citedReconstructing the cosmic density field with the distribution of dark matter halos

89 citations · 185 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2026

ELUCID-DESI II. Revealing dark matter mass, tidal, and velocity (MTV) fields using galaxy group phase information

Qingyang Li, Xiaohu Yang, Wensheng Hong +24

We introduce a novel method for reconstructing the cosmic mass, tidal, and velocity (MTV) fields over the redshift range using the phase information of galaxy groups.…

astro-ph.CO2026

A possible detection of gas rotation in galaxy groups via the kinetic Sunyaev-Zeldovich effect

Tianyi Yang, Yan-Chuan Cai, Weiguang Cui +5

We utilise the kinetic Sunyaev-Zeldovich effect (kSZ) to measure the rotation of ionised gas within galaxy groups defined in the SDSS-DR7 galaxy sample, via their dipolar imprint o…

astro-ph.GA2026

ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations

Wensheng Hong, Xiaohu Yang, Junde Li +10

We present a highly scalable, MPI-parallelized framework for reconstructing the initial cosmic density field, designed to meet the computational demands of next-generation cosmolog…

astro-ph.CO2025★ 1 cited

The Jiutian simulations for the CSST extra-galactic surveys

Jiaxin Han, Ming Li, Wenkang Jiang +23

We provide an overview of the Jiutian simulations, a hybrid simulation suite for the China Space Survey Telescope (CSST) extragalactic surveys. It consists of four complementary mo…

astro-ph.CO2025★ 6 cited

DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample

Feng Shi, Zitong Wang, Xiaohu Yang +10

Reconstructing the mass density, velocity, and tidal (MTV) fields of dark matter from galaxy surveys is essential for advancing our understanding of the LSS of the Universe. In thi…

astro-ph2008★ 89 cited

Reconstructing the cosmic density field with the distribution of dark matter halos

H. Y. Wang, H. J. Mo, Y. P. Jing +3

We develop a new method to reconstruct the cosmic density field from the distribution of dark matter haloes above a certain mass threshold. Our motivation is that well-defined samp…