activity
20192026
most citedThe IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data

380 citations · 2k across the 76 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.IM2022★ 12 cited

D-Egg: a Dual PMT Optical Module for IceCube

R. Abbasi, M. Ackermann, J. Adams +389

The D-Egg, an acronym for ``Dual optical sensors in an Ellipsoid Glass for Gen2,'' is one of the optical modules designed for future extensions of the IceCube experiment at the Sou…

astro-ph.HE2022★ 11 cited

A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade Events

R. Abbasi, M. Ackermann, J. Adams +382

This paper presents the results of a search for neutrinos that are spatially and temporally coincident with 22 unique, non-repeating Fast Radio Bursts (FRBs) and one repeating FRB…

astro-ph.HE2022★ 12 cited

Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore

R. Abbasi, M. Ackermann, J. Adams +383

The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric lumin…

hep-ex2022★ 38 cited

Graph Neural Networks for Low-Energy Event Classification & Reconstruction in IceCube

R. Abbasi, M. Ackermann, J. Adams +380

IceCube, a cubic-kilometer array of optical sensors built to detect atmospheric and astrophysical neutrinos between 1 GeV and 1 PeV, is deployed 1.45 km to 2.45 km below the surfac…

astro-ph.HE2022★ 65 cited

Searches for Neutrinos from Gamma-Ray Bursts using the IceCube Neutrino Observatory

R. Abbasi, M. Ackermann, J. Adams +378

Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs) due to their large power output. Observing a neutrino flux from GRBs would off…

astro-ph.HE2022★ 19 cited

Searching for High-Energy Neutrino Emission from Galaxy Clusters with IceCube

R. Abbasi, M. Ackermann, J. Adams +378

Galaxy clusters have the potential to accelerate cosmic rays (CRs) to ultra-high energies via accretion shocks or embedded CR acceleration sites. CRs with energies below the Hillas…