activity
20152022
most citedEvolution of the Cool Gas in the Circumgalactic Medium (CGM) of Massive Halos -- A Keck Cosmic Web Imager (KCWI) Survey of Ly Emission around QSOs at

115 citations · 633 across the 27 of their papers we have counts for

collaborators

49 papers

astro-ph.GA202214 cited

Spatially resolved molecular interstellar medium in a quasar host galaxy

Jianan Li, Bram P. Venemans, Fabian Walter +3

We present high spatial resolution (0.4", 2.2kpc) observations of the CO(6-5), CO(7-6) and [CI] lines and dust continuum emission from the interstellar medium in the host galaxy of…

astro-ph.GA202111 cited

A [C II] 158m Emitter Associated with an OI Absorber at the End of the Reionization Epoch

Yunjing Wu, Zheng Cai, Marcel Neeleman +12

The physical and chemical properties of the circumgalactic medium (CGM) at have been studied successfully through the absorption in the spectra of background Quasi-Stel…

astro-ph.GA2021

Spectroscopic Confirmation of two Extremely Massive Protoclusters BOSS1244 and BOSS1542 at

Dongdong Shi, Zheng Cai, Xiaohui Fan +3

We present spectroscopic confirmation of two new massive galaxy protoclusters at , BOSS1244 and BOSS1542, traced by groups of Coherently Strong Ly Absorption (CoS…

astro-ph.GA2021

More variable quasars have stronger emission lines

Wen-Yong Kang, Jun-Xian Wang, Zhen-Yi Cai +1

The UV/optical variation, likely driven by accretion disc turbulence, is a defining characteristic of type 1 active galactic nuclei (AGNs) and quasars. In this work we investigate…

astro-ph.GA202134 cited

Accelerated galaxy growth and environmental quenching in a protocluster at z=3.24

Ke Shi, Jun Toshikawa, Kyoung-Soo Lee +3

We present a multiwavelength study of galaxies around D4UD01, a spectroscopically confirmed protocluster at z = 3.24 to investigate environmental trends. 450 galaxies are selected…

astro-ph.HE2021

"A more probable explanation" is still impossible to explain GN-z11-flash: in response to Steinhardt et al. (arXiv:2101.12738)

Linhua Jiang, Shu Wang, Bing Zhang +8

In Jiang et al. (2020), we reported a possible bright flash (hereafter GN-z11-flash) from a galaxy GN-z11 at z ~ 11. Recently, Steinhardt et al. (2021; arXiv:2101.12738) found 27 i…