activity
20202026
most citedA Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics

159 citations · 213 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics

Emma McGinness, Rebecca Diesing, Damiano Caprioli +1

SN 1006 is a historical Type Ia supernova remnant that exhibits non-thermal emission ranging from radio to multi-TeV -rays. Most of this emission (particularly X-rays and -ra…

astro-ph.HE2022★ 15 cited

Photometric and spectroscopic analysis of the Type II SN 2020jfo with a short plateau

B. Ailawadhi, R. Dastidar, K. Misra +34

We present high-cadence photometric and spectroscopic observations of SN~2020jfo in ultraviolet and optical/near-infrared bands starting from to days after the…

astro-ph.HE2022★ 15 cited

The Lick Observatory Supernova Search follow-up program: photometry data release of 70 stripped-envelope supernovae

WeiKang Zheng, Benjamin E. Stahl, Thomas de Jaeger +85

We present BVRI and unfiltered Clear light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search (LOSS) foll…

physics.ins-det2022★ 159 cited

A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics

J. Aalbers, K. Abe, V. Aerne +591

The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leadi…

hep-ph2021★ 15 cited

Solar Neutrinos at DARWIN

André de Gouvêa, Emma McGinness, Ivan Martinez-Soler +1

The DARWIN collaboration recently argued that DARWIN (DARk matter WImp search with liquid xenoN) can collect, via neutrino--electron scattering, a large, useful sample of solar $pp…

astro-ph.CO2020★ 9 cited

On the relationship between Type Ia supernova luminosity and host-galaxy properties

Yukei S. Murakami, Benjamin E. Stahl, Keto D. Zhang +4

A string of recent studies has debated the exact form and physical origin of an evolutionary trend between the peak luminosity of Type Ia supernovae (SNe Ia) and the properties of…