activity
20022023
most citedThe Importance of Satellite Quenching for the Build-Up of the Red Sequence of Present Day Galaxies

458 citations · 5.6k across the 114 of their papers we have counts for

collaborators

113 papers

astro-ph.GA2023★ 19 cited

Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission

Joel Bregman, Renyue Cen, Yang Chen +51

The Hot Universe Baryon Surveyor (HUBS) is a proposed space-based X-ray telescope for detecting X-ray emissions from the hot gas content in our universe. With its unprecedented spa…

astro-ph.CO2023

Relieving the Tension: Exploring the Surface-type DBI Model as a Dark Matter Paradigm

Xingpao Suo, Xi Kang, Huanyuan Shan

Recent observations from weak gravitational lensing (WL) surveys indicate a smoother Universe compared to the predictions of the Cosmic Microwave Background (CMB). This inconsisten…

astro-ph.GA2023★ 2 cited

A rotating satellite plane around Milky Way-like galaxy from the TNG50 simulation

Yingzhong Xu, Xi Kang, Noam I. Libeskind

We study the Satellite Plane Problem of the Milky Way\ (MW) by using the recently published simulation data of TNG50-1. Here, we only consider the satellite plane consisting of the…

astro-ph.CO2023

AI-assisted reconstruction of cosmic velocity field from redshift-space spatial distribution of halos

Ziyong Wu, Liang Xiao, Xu Xiao +6

The peculiar velocities of dark matter halos are crucial to study many issues in cosmology and galaxy evolution. In this study, by using the state-of-the-art deep learning techniqu…

astro-ph.GA2022★ 1 cited

Can we constrain galaxy geometry parameters using spatially integrated SED fitting?

Yisheng Qiu, Xi Kang, Yu Luo

Sophisticated spectral energy distribution (SED) models describe dust attenuation and emission using geometry parameters. This treatment is natural since dust effects are driven by…

astro-ph.GA2022★ 2 cited

Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations

Yaoxin Chen, Yingzhong Xu, Xi Kang

Galaxies display several well-behaved scaling relations between their properties, such as the star formation rate-stellar mass relation (the main sequence) and the stellar mass-hal…