27 citations · 140 across the 11 of their papers we have counts for
11 papers
Understanding the Universal Dust Attenuation Scaling Relation of Star-Forming Galaxies
J. Qin, X. Z. Zheng, S. Wuyts +17
Star-forming galaxies (SFGs) adhere to a surprisingly tight scaling relation of dust attenuation parameterized by the infrared excess (IRX=), being jointly d…
The Dust Attenuation Scaling Relation of Star-Forming Galaxies in the EAGLE Simulations
Man Qiao, Xian Zhong Zheng, Antonios Katsianis +11
Dust attenuation in star-forming galaxies (SFGs), as parameterized by the infrared excess (IRX ), is found to be tightly correlated with star formatio…
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…
The Spatially Resolved Properties of the GW170817 Host Galaxy
Yubin Li, Jirong Mao, Jianbo Qin +4
GW170817 is the unique gravitational-wave (GW) event that is associated to the electromagnetic (EM) counterpart GRB 170817A. NGC 4993 is identified as the host galaxy of GW170817/G…
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…
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…
Long Tidal Tails in Merging Galaxies and Their Implications
Jian Ren, Xian Zhong Zheng, David Valls-Gabaud +8
We investigate the properties of long tidal tails using the largest to date sample of 461 merging galaxies with within from th…
Understanding the Discrepancy between IRX and Balmer Decrement in Tracing Galaxy Dust Attenuation
Jianbo Qin, Xian Zhong Zheng, Stijn Wuyts +2
We compare the infrared excess (IRX) and Balmer decrement () as dust attenuation indicators in relation to other galaxy parameters using a sample of 32 000 local…
A Universal Relation of Dust Obscuration Across Cosmic Time
Jianbo Qin, X. Z. Zheng, Stijn Wuyts +2
We investigate dust obscuration as parameterised by the infrared excess IRX in relation to global galaxy properties, using a sample of 3200…