activity
20152023
most citedEmission-line diagnostics of nearby HII regions including interacting binary populations

135 citations · 366 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2023

A Superluminous Supernova Lightened by Collisions with Pulsational Pair-instability Shells

Weili Lin, Xiaofeng Wang, Lin Yan +23

Superluminous supernovae are among the most energetic stellar explosions in the Universe, but their energy sources remain an open question. Here we present long-term observations o…

astro-ph.HE2023

JWST Discovery of Dust Reservoirs in Nearby Type IIP Supernovae 2004et and 2017eaw

Melissa Shahbandeh, Arkaprabha Sarangi, Tea Temim +36

Supernova (SN) explosions have been sought for decades as a possible source of dust in the Universe, providing the seeds of galaxies, stars, and planetary systems. SN 1987A offers…

astro-ph.SR2022★ 17 cited

Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope

Maokai Hu, Lei Hu, Ji-an Jiang +4

Type Ia Supernovae (SNe Ia) are the thermonuclear explosion of a carbon-oxygen white dwarf (WD) and are well-known as a distance indicator. However, it is still unclear how WDs inc…

astro-ph.HE2022★ 27 cited

A Mid-infrared Study of Superluminous Supernovae

Luming Sun, Lin Xiao, Ge Li

We present the mid-infrared (MIR) light curves (LC) of 10 superluminous supernovae (SLSNe) at based on WISE data at 3.4 and 4.6 m. Three of them, including PS15br, SN 2…

astro-ph.GA2021★ 87 cited

Infrared Echoes of Optical Tidal Disruption Events: ~1% Dust Covering Factor or Less at sub-parsec Scale

Ning Jiang, Tinggui Wang, Xueyang Hu +3

The past decade has experienced an explosive increase of optically-discovered tidal disruption events (TDEs) with the advent of modern time-domain surveys. However, we still lack a…

astro-ph.GA2019★ 30 cited

The distance, supernova rate and supernova progenitors of NGC 6946

J. J. Eldridge, Lin Xiao

The distance to the fireworks galaxy NGC 6946 is highly uncertain. Recent distance estimates using the tip of the red giant branch of 7.7 to 7.8 Mpc are larger than the distance co…

astro-ph.GA2018★ 135 cited

Emission-line diagnostics of nearby HII regions including interacting binary populations

Lin Xiao, Elizabeth Stanway, J. J. Eldridge

We present numerical models of the nebular emission from H II regions around young stellar populations over a range of compositions and ages. The synthetic stellar pop- ulations in…

astro-ph.GA2017★ 45 cited

Spatially resolved MaNGA observations of the host galaxy of superluminous supernova 2017egm

Ting-Wan Chen, Patricia Schady, Lin Xiao +6

Superluminous supernovae (SLSNe) are found predominantly in dwarf galaxies, indicating that their progenitors have a low metallicity. However, the most nearby SLSN to date, SN 2017…

astro-ph.GA2017

Emission-line Diagnostics of Nearby HII Regions Including Supernova Hosts

Lin Xiao, J. J. Eldridge, Elizabeth Stanway +1

We present a new model of the optical nebular emission from HII regions by combin- ing the results of the Binary Population and Spectral Synthesis (bpass) code with the photoion- i…

astro-ph.GA2015★ 25 cited

Core-Collapse Supernova Rate Synthesis Within 11 Mpc

Lin Xiao, J. J. Eldridge

The 11 Mpc H-alpha and Ultraviolet Galaxy (11HUGS) Survey traces the star formation activity of nearby galaxies. In addition within this volume the detection completeness of core-c…