Skip to main navigation Skip to search Skip to main content

All-flavor Time-dependent Search for Transient Neutrino Sources

  • Icecube Collaboration
  • University of Delaware
  • RWTH Aachen University
  • Karlsruhe Institute of Technology
  • Adelaide University
  • Loyola University Chicago
  • German Electron Synchrotron
  • University of Canterbury
  • University of Wisconsin-Madison
  • Université libre de Bruxelles
  • University of Copenhagen
  • TU Dortmund University
  • University of Kansas
  • Marquette University
  • Harvard University
  • University of Utah
  • Michigan State University
  • South Dakota School of Mines & Technology
  • University of California at Irvine
  • Technical University of Munich
  • University of California at Berkeley
  • Ohio State University
  • Ruhr University Bochum
  • Uppsala University
  • University of Rochester
  • University of Maryland, College Park
  • University of Padua
  • University of Alabama
  • Johannes Gutenberg University Mainz
  • Georgia Institute of Technology
  • Queen's University Kingston

Research output: Contribution to journalConference articlepeer-review

Abstract

Transient sources are among the preferred candidates for the sources of high-energy neutrino emission. Intriguing examples so far include blazar flares and tidal disruption events coincident with IceCube neutrinos. Here, we report the first all-flavor, all-sky time-dependent search for neutrino sources by combining IceCube throughgoing tracks, starting tracks and cascades. Throughgoing tracks provide the best sensitivity in the Northern Sky, while cascades have worse angular resolution but yield better sensitivity in the Southern Sky than tracks. The relatively new starting tracks sample has reduced contamination from atmospheric muons. This analysis takes advantage of the strengths of each of the datasets, combining them for increased statistics and obtaining the best accessible all-sky sensitivity for transient searches. In this search, we look for unbound E-γ power-law sources, as well as E−2 sources with low and high-energy exponential cutoffs, optimizing the sensitivity for the duration of the flares.

Original languageEnglish
Article number1007
JournalProceedings of Science
Volume501
DOIs
StatePublished - Dec 30 2025
Event39th International Cosmic Ray Conference, ICRC 2025 - Geneva, Switzerland
Duration: Jul 15 2025Jul 24 2025

Fingerprint

Dive into the research topics of 'All-flavor Time-dependent Search for Transient Neutrino Sources'. Together they form a unique fingerprint.

Cite this