activity
20152024
most citedSciences with the 2.5-meter Wide Field Survey Telescope (WFST)

117 citations · 305 across the 16 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2024

X-ray Cool Core Remnants Heated by Strong Radio AGN Feedback

Wenhao Liu, Ming Sun, G. Mark Voit +6

Strong AGN heating provides an alternative means for the disruption of cluster cool cores (CCs) to cluster mergers. In this work we present a systematic Chandra study of a sample o…

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★ 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★ 26 cited

Submillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks

Yuheng Zhang, Xian Zhong Zheng, Dong Dong Shi +18

Submillimetre galaxies represent a rapid growth phase of both star formation and massive galaxies. Mapping SMGs in galaxy protoclusters provides key insights into where and how the…

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.GA2022★ 23 cited

Systematic biases in determining dust attenuation curves through galaxy SED fitting

Jianbo Qin, Xian Zhong Zheng, Min Fang +16

While the slope of the dust attenuation curve () is found to correlate with effective dust attenuation () as obtained through spectral energy distribution (SED) fitting, it…

astro-ph.GA2021

The cosmic environment overtakes the local density in shaping galaxy star formation

Jian Ren, Zhizheng Pan, XianZhong Zheng +11

The gas supply from the cosmic web is the key to sustain star formation in galaxies. It remains to be explored how the cosmic large-scale structure (LSS) effects on galaxy evolutio…

astro-ph.GA2019★ 19 cited

A merger shock in Abell 1367

Chong Ge, Ming Sun, Ruo-Yu Liu +10

Multi-wavelength observations show that Abell 1367 (A1367) is a dynamically young cluster, with at least two subclusters merging along the SE-NW direction. With the wide-field XMM-…

astro-ph.GA2015★ 13 cited

Studying the Interstellar Medium and the inner region of NPS/Loop 1 with shadow observations toward MBM36

E. Ursino, M. Galeazzi, W. Liu

We analyzed data from a shadow observation of the high density molecular cloud MBM36 (l~4°, b~35°) with Suzaku. MBM36 is located in a region that emits relatively weakly in the 3/4…