activity
20202022
most citedFAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252

41 citations · 82 across the 8 of their papers we have counts for

collaborators

9 papers

hep-ex202238 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.HE2021

A Time-Variability Test for Candidate Neutrino Sources Observed with IceCube

Pranav Dave

Recent studies with IceCube have shown signs of a time-integrated flux of astrophysical neutrinos from point-like sources such as TXS 0506+056 and NGC 1068. Time-variability of thi…

astro-ph.HE202141 cited

FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252

Pei Wang, Di Li, Colin J. Clark +23

High sensitivity radio searches of unassociated -ray sources have proven to be an effective way of finding new pulsars. Using the Five-hundred-meter Aperture Spherical radio Tel…

astro-ph.HE2021

Measuring the Neutrino Cross Section Using 8 years of Upgoing Muon Neutrinos Observed with IceCube

S. Robertson

The IceCube Neutrino Observatory detects neutrinos at energies orders of magnitude higher than those available to current accelerators. Above 40 TeV, neutrinos traveling through th…

astro-ph.IM20213 cited

Design and performance of the multi-PMT optical module for IceCube Upgrade

T. Anderson, L. Classen, A. T. Fienberg +5

The IceCube Upgrade is the first step towards the next-generation neutrino observatory at the South Pole, IceCube-Gen2, and will be installed in the central region of the existing…

astro-ph.IM2021

Analysis Framework for Multi-messenger Astronomy with IceCube

Kwok Lun Fan, John Evans, Michael Larson

Combining observational data from multiple instruments for multi-messenger astronomy can be challenging due to the complexity of the instrument response functions and likelihood ca…