activity
20182022
most citedCan Non-standard Recombination Resolve the Hubble Tension?

56 citations · 175 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2022

On the Kinematic Morphology around Halos

Xiaolin Luo, Xiangling Xu, Xin Wang

In this paper, we report an interesting kinematic phenomenon around the halos' edge related to the splashback radius. After the shell-crossing, cosmic flow exhibits various rotatio…

astro-ph.CO2022

Cosmological constraints from the density gradient weighted correlation function

Xiaoyuan Xiao, Yizhao Yang, Xiaolin Luo +8

The mark weighted correlation function (MCF) is a computationally efficient statistical measure which can probe clustering information beyond that of the conventional 2-po…

astro-ph.CO2021★ 22 cited

Cosmic Velocity Field Reconstruction Using AI

Ziyong Wu, Zhenyu Zhang, Shuyang Pan +6

We develop a deep learning technique to infer the non-linear velocity field from the dark matter density field. The deep learning architecture we use is an "U-net" style convolutio…

astro-ph.CO2020★ 18 cited

Reconciling low and high redshift GRB luminosity correlations

Lu Huang, Zhiqi Huang, Xiaolin Luo +2

The correlation between the peak spectra energy () and the equivalent isotropic energy () of long gamma-ray bursts (GRBs), the so-called Amati relation, is often…

astro-ph.CO2020★ 27 cited

Reaffirming the Cosmic Acceleration without Supernova and CMB

Xiaolin Luo, Zhiqi Huang, Qiyue Qian +1

Recent discussions about supernova magnitude evolution have raised doubts about the robustness of the late-universe acceleration. In a previous letter, Huang did a null test of the…

astro-ph.CO2019★ 1 cited

Exploring the Latest Pantheon SNIa Dataset by Using Three Kinds of Statistics Techniques

Shuang Wang, Xiaolin Luo

In this work, we explore the cosmological consequences of the latest Type Ia supernova (SN Ia) data-set, Pantheon, by adopting the model. The Pantheon data-set is the larges…