activity
20172023
most citedThe discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck

465 citations · 985 across the 23 of their papers we have counts for

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Showing astro-ph.HEShow all

8 papers · 1 filter

astro-ph.HE2023★ 27 cited

Collapsars as Sites of r-process Nucleosynthesis: Systematic Near-Infrared Follow-up of Type Ic-BL Supernovae

Shreya Anand, Jennifer Barnes, Sheng Yang +41

One of the open questions following the discovery of GW170817 is whether neutron star mergers are the only astrophysical sites capable of producing -process elements. Simulation…

astro-ph.HE2023★ 13 cited

HAFFET: Hybrid Analytic Flux FittEr for Transients

Sheng Yang, Jesper Sollerman

The progenitors for many types of supernovae (SNe) are still unknown, and an approach to diagnose their physical origins is to investigate the light curve brightness and shape of a…

astro-ph.HE2021★ 10 cited

SN 2018bsz: significant dust formation in a nearby superluminous supernova

T. -W. Chen, S. J. Brennan, R. Wesson +41

We investigate the thermal emission and the extinction from dust associated with the nearby (z = 0.0267) superluminous supernova (SLSN) 2018bsz. Our dataset combines daily-cadence,…

astro-ph.HE2021★ 16 cited

Magnetar-Driven Shock Breakout Revisited and Implications for Double-Peaked Type I Superluminous Supernovae

Liang-Duan Liu, He Gao, Xiao-Feng Wang +1

The discovery of early bumps in some type-I superluminous supernovae (SLSNe-I) before the main peaks offers an important clue to their energy source mechanisms. In this paper, we u…

astro-ph.HE2019★ 33 cited

Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey

Sheng Yang, David J. Sand, Stefano Valenti +7

We describe the GW follow-up strategy and subsequent results of the DLT40 during the second science run (O2) of the LVC. Depending on the information provided in the GW alert toget…

astro-ph.HE2018

Gravitational wave optical counterpart searching based on GRAWITA and DLT40 project during LIGO O2 run

Sheng Yang

The identification of the electromagnetic(EM) counterpart of gravitational wave(GW) trigger in the sky localization is a very difficult task because of the large uncertainty. Two c…

astro-ph.HE2017★ 465 cited

The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck

Stefano Valenti, David J. Sand, Sheng Yang +7

During the second observing run of the Laser Interferometer gravitational- wave Observatory (LIGO) and Virgo Interferometer, a gravitational-wave signal consistent with a binary ne…

astro-ph.HE2017★ 41 cited

An empirical limit on the kilonova rate from the DLT40 one day cadence Supernova Survey

Sheng Yang, Stefano Valenti, Enrico Cappellaro +6

Binary neutron star mergers are important to understand stellar evolution, the chemical enrichment of the universe via the r-process, the physics of short gamma-ray bursts, gravita…