activity
20182021
most citedSN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova

62 citations · 95 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2021

The KBSS-KCWI Survey: The connection between extended Ly halos and galaxy azimuthal angle at

Yuguang Chen, Charles C. Steidel, Dawn K. Erb +9

We present the first statistical analysis of kinematically-resolved, spatially-extended Ly emission around galaxies in the Keck Baryonic Structure Survey (KBSS) using…

astro-ph.GA2020

Revisiting the Gas Kinematics in SSA22 Lyman- Blob 1 with Radiative Transfer Modeling in a Multiphase, Clumpy Medium

Zhihui Li, Charles C. Steidel, Max Gronke +1

We present new observations of Lyman- (Ly) Blob 1 (LAB1) in the SSA22 protocluster region ( = 3.09) using the Keck Cosmic Web Imager (KCWI) and the Keck Multi-object Spect…

astro-ph.HE202062 cited

SN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova

Yuhan Yao, Kishalay De, Mansi M. Kasliwal +28

We present observations of ZTF18abfcmjw (SN2019dge), a helium-rich supernova with a fast-evolving light curve indicating an extremely low ejecta mass () and l…

astro-ph.GA2019

On the Survival of Cool Clouds in the Circum-Galactic Medium

Zhihui Li, Philip F. Hopkins, Jonathan Squire +1

We explore the survival of cool clouds in multi-phase circum-galactic media. We revisit the "cloud crushing problem" in a large survey of simulations including radiative cooling, s…

astro-ph.GA201933 cited

The Evolution of the Interstellar Medium in Post-Starburst Galaxies

Zhihui Li, K. Decker French, Ann I. Zabludoff +1

We derive dust masses () from the spectral energy distributions of 58 post-starburst galaxies (PSBs). There is an anticorrelation between specific dust mass ($M_{\rm…

astro-ph.GA2018

Interstellar Medium and Star Formation of Starburst Galaxies on the Merger Sequence

Jinyi Shangguan, Luis C. Ho, Ruancun Li +3

The interstellar medium is a key ingredient that governs star formation in galaxies. We present a detailed study of the infrared (~ 1-500 micron) spectral energy distributions of a…