activity
20152023
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 1.1k across the 17 of their papers we have counts for

collaborators

58 papers

astro-ph.EP2023

UV to near-IR observations of the DART-Dimorphos collision

E. O. Ofek, D. Kushnir, D. Polishook +15

The impact of the Double Asteroid Redirection Test (DART) spacecraft with Dimorphos allows us to study asteroid collision physics, including momentum transfer, the ejecta propertie…

astro-ph.HE202155 cited

IceCube Data for Neutrino Point-Source Searches Years 2008-2018

IceCube Collaboration, R. Abbasi, M. Ackermann +370

IceCube has performed several all-sky searches for point-like neutrino sources using track-like events, including a recent time-integrated analysis using 10 years of IceCube data.…

hep-ex2020

Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube

R. Abbasi, M. Ackermann, J. Adams +361

The flux of high-energy neutrinos passing through the Earth is attenuated due to their interactions with matter. The interaction rate is modulated by the neutrino interaction cross…

astro-ph.HE2020

The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data

R. Abbasi, M. Ackermann, J. Adams +362

The IceCube Neutrino Observatory has established the existence of a high-energy all-sky neutrino flux of astrophysical origin. This discovery was made using events interacting with…

astro-ph.HE2020

The Zwicky Transient Facility Bright Transient Survey. II. A Public Statistical Sample for Exploring Supernova Demographics

Daniel A. Perley, Christoffer Fremling, Jesper Sollerman +34

We present a public catalog of transients from the Zwicky Transient Facility (ZTF) Bright Transient Survey (BTS), a magnitude-limited (m<19 mag in either the g or r filter) survey…

astro-ph.HE2020

Bright, months-long stellar outbursts announce the explosion of interaction-powered supernovae

Nora L. Strotjohann, Eran O. Ofek, Avishay Gal-Yam +53

Interaction-powered supernovae (SNe) explode within an optically-thick circumstellar medium (CSM) that could be ejected during eruptive events. To identify and characterize such pr…