activity
20222026
most citedSubmillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks

26 citations · 58 across the 8 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Tracing cosmic star formation history through radio continuum spectral energy distribution and non-thermal emission

Fangxia An, Fatemeh S. Tabatabaei, Nick Seymour +11

As a tracer of massive star formation unaffected by dust, the radio continuum emission provides a unique window into the formation of the first stars and galaxies in the Universe.…

astro-ph.GA2025

A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco

Chao Yang, Zhizheng Pan, Min Fang +34

We carry out deep imaging of the Milky Way satellite galaxies, Bootes III and Draco, with WFST as one pilot observing program to demonstrate the capability of WFST. Combining catal…

astro-ph.GA2024

A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon

Shuang Liu, Xian Zhong Zheng, Valentino Gonzalez +10

The process of galaxy cluster formation likely leaves an imprint on the properties of its individual member galaxies. Understanding this process is essential for uncovering the evo…

astro-ph.GA202226 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.GA202223 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…