activity
20152026
most citedA cuspy dark matter halo

38 citations · 390 across the 39 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

26 papers · 1 filter

astro-ph.GA2026★ 1 cited

Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs

Xiaotong Guo, Qiusheng Gu, Guanwen Fang +7

Compton-thick active galactic nuclei (CT-AGNs), defined by column density , are so heavily absorbed that their X-ray e…

astro-ph.GA2025

Dwarf Galaxy Integral-field Survey (DGIS): survey overview and the result of global mass-metallicity relation

Xin Li, Yong Shi, Fuyan Bian +11

Low-mass galaxies are the building blocks of massive galaxies in the framework of hierarchical structure formation. To enable detailed studies of galactic ecosystems in dwarf galax…

astro-ph.GA2024

Quasars with Flare/Eclipse-like Variability Identified in ZTF

Zhiyuan Zheng, Yong Shi, Shuowen Jin +4

Active galactic nuclei (AGNs) are known to exhibit optical/UV variability and most of them can be well modeled by the damped random walks. Physical processes that are not related t…

astro-ph.GA2023

The \ion{H}{I}-rich Ultra-diffuse Galaxies follow the Extended Schmidt Law

Sai Zhai, Yong Shi, Zhi-Yu Zhang +7

The \ion{H}{I}-rich ultra-diffuse galaxies (HUDGs) offer a unique case for studies of star formation laws (SFLs) as they host low star formation efficiency (SFE) and low-metallicit…

astro-ph.GA2023★ 6 cited

An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole

Zhiyuan Zheng, Yong Shi, Fuyan Bian +5

While in massive galaxies active galactic nuclei (AGN) feedback plays an important role, the role of AGN feedback is still under debate in dwarf galaxies. With well spatially resol…

astro-ph.GA2023★ 3 cited

Multiwavelength Analysis of a Nearby Heavily Obscured AGN in NGC 449

Xiaotong Guo, Qiusheng Gu, Jun Xu +5

We presented the multiwavelength analysis of a heavily obscured active galactic nucleus (AGN) in NGC 449. We first constructed a broadband X-ray spectrum using the latest NuSTAR an…

astro-ph.GA2022★ 8 cited

The HI Gas Disk Thickness of the Ultra-diffuse Galaxy AGC 242019

Xin Li, Yong Shi, Zhi-Yu Zhang +5

Ultra-diffuse galaxies (UDGs) are as faint as dwarf galaxies but whose sizes are similar to those of spiral galaxies. A variety of formation mechanisms have been proposed, some of…

astro-ph.GA2022★ 24 cited

SDSS-IV MaNGA: Global Properties of Kinematically Misaligned Galaxies

Yuren Zhou, Yanmei Chen, Yong Shi +6

We select 456 gas-star kinematically misaligned galaxies from the internal Product Launch-10 of MaNGA survey, including 74 star-forming (SF), 136 green-valley (GV) and 206 quiescen…

astro-ph.GA2022★ 13 cited

Starbursts with suppressed velocity dispersion revealed in a forming cluster at z=2.51

Mengyuan Xiao, Tao Wang, David Elbaz +19

One of the most prominent features of galaxy clusters is the presence of a dominant population of massive ellipticals in their cores. Stellar archaeology suggests that these gigant…

astro-ph.GA2022★ 15 cited

The molecular gas resolved by ALMA in the low-metallicity dwarf merging galaxy Haro 11

Yulong Gao, Qiusheng Gu, Yong Shi +9

The physical mechanisms for starburst or quenching in less massive () galaxies are unclear. The merger is one of the inescapable processes referred to as b…

astro-ph.GA2022★ 4 cited

The Variability of the Narrow-line Seyfert 1 Galaxies from the PanSTARRS's View

Hongtao Wang, Yanping Su, Xue Ge +2

By means of the data sets from the Pan-STARRAS1 survey, we have systematically examined the relationship between the variability characteristics and the physical parameters of the…

astro-ph.GA2021

Spatially Resolved Properties of Supernova Host Galaxies in SDSS-IV MaNGA

Hongxuan Zhang, Yanmei Chen, Yong Shi +2

We crossmatch galaxies from Mapping Nearby Galaxies at Apache Point Observatory with the Open Supernova Catalog, obtaining a total of 132 SNe within MaNGA bundle. These 132 SNe can…

astro-ph.GA2021★ 11 cited

A universal relationship between stellar masses and binding energies of galaxies

Yong Shi, Xiaoling Yu, Shude Mao +3

In this study we demonstrate that stellar masses of galaxies (Mstar) are universally correlated through a double power law function with the product of the dynamical velocities (Ve…

astro-ph.GA2021★ 16 cited

The major mechanism to drive turbulence in star-forming galaxies

Xiaoling Yu, Fuyan Bian, Mark R. Krumholz +3

Two competing models, gravitational instability-driven transport and stellar feedback, have been proposed to interpret the high velocity dispersions observed in high-redshift galax…

astro-ph.GA2021★ 5 cited

PGC 38025: A Star-forming Lenticular Galaxy With an Off-nuclear Star-forming Core

Zhengyi Chen, Qiu-Sheng Gu, Rubén García-Benito +4

Lenticular galaxies (S0s) were considered mainly as passive evolved spirals due to environmental effects for a long time; however, most S0s in the field cannot fit into this common…

astro-ph.GA2021★ 7 cited

SDSS-IV MaNGA: Enhanced Star Formation in Galactic-scale Outflows

Min Bao, Yanmei Chen, Qirong Yuan +8

Using the integral field unit (IFU) data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, we collect a sample of 36 star forming galaxies that host galactic…

astro-ph.GA2021

Probing possible effects of circumgalactic media on the metal content of galaxies through the mass-metallicity relationship

Sai Zhai, Yong Shi, Jianhang Chen +4

The circumgalactic medium (CGM) connects the gas between the interstellar medium (ISM) and the intergalactic medium, which plays an important role in galaxy evolution. We use the s…

astro-ph.GA2021★ 38 cited

A cuspy dark matter halo

Yong Shi, Zhi-Yu Zhang, Junzhi Wang +4

The cusp-core problem is one of the main challenges of the cold dark matter paradigm on small scales: the density of a dark matter halo is predicted to rise rapidly toward the cent…

astro-ph.GA2020★ 8 cited

Multi-wavelength Selected Compton-thick AGNs in Chandra Deep Field-South Survey

Xiaotong Guo, Qiusheng Gu, Nan Ding +2

Even in deep X-ray surveys, Compton-thick active galactic nuclei (CT AGNs, ) are difficult to be identified due to X-ray flux…

astro-ph.GA2020★ 17 cited

Host Galaxy Properties of Changing-look AGN Revealed in the MaNGA Survey

Xiaoling Yu, Yong Shi, Yanmei Chen +6

Changing-look Active Galactic Nuclei (CL-AGNs) are a subset of AGNs in which the broad Balmer emission lines appear or disappear within a few years. We use the Mapping Nearby Galax…

astro-ph.GA2019★ 31 cited

The Impact of Merging on The Origin of Kinematically Misaligned and Counter-rotating Galaxies in MaNGA

Song-lin Li, Yong Shi, Dmitry Bizyaev +7

Galaxy mergers and interactions are expected to play a significant role leading to offsets between gas and stellar motions in galaxies. Herein we crossmatch galaxies in MaNGA MPL-8…

astro-ph.GA2019★ 7 cited

Discovery of an Edge-on Galaxy with X-shaped Bi-cone --- SDSS J171359.00+333625.5

Min Bao, Yanmei Chen, Qirong Yuan +5

Using the integral field unit (IFU) data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, we study the kinematics of gas and stellar components in an edge-o…

astro-ph.GA2019★ 34 cited

The spatial extension of extended narrow line regions in MaNGA AGN

Jianhang Chen, Yong Shi, Ross Dempsey +10

In this work, we revisit the size-luminosity relation of the extended narrow line regions (ENLRs) using a large sample of nearby active galactic nuclei (AGN) from the Mapping Nearb…

astro-ph.GA2019★ 32 cited

Spatially Resolved Studies of Local Massive Red Spiral Galaxies

Cai-Na Hao, Yong Shi, Yanmei Chen +5

We report two-dimensional spectroscopic analysis of massive red spiral galaxies ( 10 ) and compare them to blue spiral and red elliptical galaxies ab…