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19972023
most citedASCA Measurements of Silicon and Iron Abundances in the Intracluster Medium

204 citations · 1.7k across the 72 of their papers we have counts for

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20 papers · 1 filter

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.GA2023★ 23 cited

What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24

Shuang Liu, Xianzhong Zheng, Dongdong Shi +10

Characterizing the structural properties of galaxies in high-redshift protoclusters is key to our understanding of the environmental effects on galaxy evolution in the early stages…

astro-ph.GA2022★ 13 cited

MaNGA 8313-1901: gas accretion observed in a blue compact dwarf galaxy?

Mengting Ju, Jun Yin, Rongrong Liu +13

Gas accretion is an important process in the evolution of galaxies, but it has limited direct observational evidences. In this paper, we report the detection of a possible ongoing…

astro-ph.GA2022★ 1 cited

The Physical Properties of Star-Forming Galaxies with Strong [O III] Lines at z=3.25

Run Wen, FangXia An, Xian Zhong Zheng +13

We present an analysis of physical properties of 34 [O III] emission-line galaxies (ELGs) at z=3.2540.029 in the Extended Chandra Deep Field South (ECDFS). These ELGs are sele…

astro-ph.GA2022★ 5 cited

Chandra view of Abell 407: the central compact group of galaxies and the interaction between the radio AGN and the ICM

Chao Geng, Chong Ge, Dharam V. Lal +8

Abell 407 (A407) is a unique galaxy cluster hosting a central compact group of nine galaxies (named as 'Zwicky's Nonet'; G1 - G9 in this work) within a 30 kpc radius region. The cl…

astro-ph.GA2021★ 25 cited

An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs

Gaoxiang Jin, Y. Sophia Dai, Hsi-An Pan +10

The role of active galactic nuclei (AGNs) during galaxy interactions and how they influence the star formation in the system are still under debate. We use a sample of 1156 galaxie…