117 citations · 305 across the 16 of their papers we have counts for
16 papers
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…
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…
Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)
WFST Collaboration, Tinggui Wang, Guilin Liu +60
The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility being built jointly by the University of Science and Technology of China and the Purple Mountai…
Point source contribution to the Diffuse X-ray Background below 1 keV and its effect on our understanding of the circum-galactic medium
Sicong Huang, Nico Cappelluti, Massimiliano Galeazzi +4
We studied the spectral signature of different components of the Diffuse X-ray Background (DXB), including Local Hot Bubble (LHB), Solar Wind Charge Exchange (SWCX), Galactic Halo,…
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…
A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113
D. Spence, M. Bonamente, J. Nevalainen +5
This paper presents an analysis of XMM X--ray spectra of the quasar 1ES 1553+113, in search for absorption lines from the intervening warm--hot intergalactic medium. A search for O…
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…
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…
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…
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…
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…
AGN feedback in the FR II galaxy 3C 220.1
Wenhao Liu, Ming Sun, Paul E. J. Nulsen +6
We present results from a deep (174 ks) Chandra observation of the FR-II radio galaxy 3C 220.1, the central brightest cluster galaxy (BCG) of a 4 keV cluster at .…
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-…
AGN Feedback in Galaxy Group 3C 88: Cavities, Shock and Jet Reorientation
Wenhao Liu, Ming Sun, Paul Nulsen +7
We present results from the deep Chandra observation (105 ksec), together with new Giant Metrewave Radio Telescope and Very Large Array data of the AGN outburst in the radio-loud g…
Evidence for a very low-column density hole in the Galactic halo in the direction of the high latitude molecular cloud MBM 16
Wenhao Liu, Massimiliano Galeazzi, Eugenio Ursino
Shadow observations are the only way to observe emission from the galactic halo (GH) and/or the circumgalactic medium (CGM) free of any foreground contamination from local hot bubb…
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…