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20072026
most citedA Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics

159 citations · 2.2k across the 104 of their papers we have counts for

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Showing 2021Show all

12 papers · 1 filter

astro-ph.HE2021★ 2 cited

Supernova host galaxy association and photometric classification of over 10,000 light curves from the Zwicky Transient Facility

Braden Garretson, Dan Milisavljevic, Jack Reynolds +4

Here we present a catalog of 12,993 photometrically-classified supernova-like light curves from the Zwicky Transient Facility, along with candidate host galaxy associations. By tra…

astro-ph.HE2021★ 52 cited

Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory

Igor Andreoni, Raffaella Margutti, Om Sharan Salafia +52

The discovery of the electromagnetic counterpart to the binary neutron star merger GW170817 has opened the era of gravitational-wave multi-messenger astronomy. Rapid identification…

astro-ph.HE2021★ 66 cited

Radio and X-ray observations of the luminous Fast Blue Optical Transient AT2020xnd

Joe S. Bright, Raffaella Margutti, David Matthews +25

We present deep X-ray and radio observations of the Fast Blue Optical Transient (FBOT) AT2020xnd/ZTF20acigmel at from d to d after explosion. AT2020xnd belongs…

astro-ph.HE2021★ 141 cited

Final Moments I: Precursor Emission, Envelope Inflation, and Enhanced Mass loss Preceding the Luminous Type II Supernova 2020tlf

Wynn Jacobson-Galán, Luc Dessart, David Jones +33

We present panchromatic observations and modeling of supernova (SN) 2020tlf, the first normal type II-P/L SN with confirmed precursor emission, as detected by the Young Supernova E…

astro-ph.HE2021

Luminous Late-time Radio Emission from Supernovae Detected by the Karl G. Jansky Very Large Array Sky Survey (VLASS)

M. C. Stroh, G. Terreran, D. L. Coppejans +10

We present a population of 19 radio-luminous supernovae (SNe) with emission reaching in the first epoch of the Very Large Array…

astro-ph.HE2021

A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss

Taylor Jacovich, Daniel Patnaude, Pat Slane +4

Massive stars can shed material via steady, line-driven winds, eruptive outflows, or mass-transfer onto a binary companion. In the case of single stars, the mass is deposited by th…