activity
20182023
most citedHow Do Galaxies trace a large scale structure?: A case study around a massive protocluster at

43 citations · 121 across the 5 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2023

The One-hundred-deg^2 DECam Imaging in Narrowbands (ODIN): Survey Design and Science Goals

Kyoung-Soo Lee, Eric Gawiser, Changbom Park +39

We describe the survey design and science goals for ODIN (One-hundred-deg^2 DECam Imaging in Narrowbands), a NOIRLab survey using the Dark Energy Camera (DECam) to obtain deep (AB~…

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

The Role of Dust, UV Luminosity and Large-scale Environment on the Escape of Lya Photons: A Case Study of a Protocluster field at z = 3.1

Yun Huang, Kyoung-Soo Lee, Ke Shi +3

We present a detailed characterization of the Lya properties for 93 Lya emitters (LAEs) at z~3.1 selected from the D1 field of the Canada-France-Hawaii-Telescope Legacy Survey, inc…

astro-ph.GA20207 cited

A Closer Look at Two of the Most Luminous Quasars in the Universe

Jan-Torge Schindler, Xiaohui Fan, Mladen Novak +7

Ultra-luminous quasars () provide us with a rare view into the nature of the most massive and most rapidly accreting supermassive black holes (SMBHs). Following…

astro-ph.GA2020

A Complete Census of Circumgalactic MgII at Redshift z<~ 0.5

Yun-Hsin Huang, Hsiao-Wen Chen, Stephen A. Shectman +5

We present a survey of MgII absorbing gas in the vicinity of 380 random galaxies, using 156 background quasi-stellar objects(QSOs) as absorption-line probes. The sample comprises 2…

astro-ph.GA2020

Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation

Stacey Alberts, Kyoung-Soo Lee, Alexandra Pope +13

Massive galaxy clusters undergo strong evolution from z~1.6 to z~0.5, with overdense environments at high-z characterized by abundant dust-obscured star formation and stellar mass…