4.6 Article

Search for Multi-flare Neutrino Emissions in 10 yr of IceCube Data from a Catalog of Sources

Journal

ASTROPHYSICAL JOURNAL LETTERS
Volume 920, Issue 2, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/2041-8213/ac2c7b

Keywords

-

Funding

  1. USA-U.S. National Science Foundation-Office of Polar Programs
  2. U.S. National Science Foundation-Physics Division
  3. U.S. National Science Foundation-EPSCoR
  4. Wisconsin Alumni Research Foundation
  5. Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison
  6. Open Science Grid (OSG)
  7. Extreme Science and Engineering Discovery Environment (XSEDE)
  8. Frontera computing project at the Texas Advanced Computing Center
  9. U.S. Department of Energy-National Energy Research Scientific Computing Center
  10. Particle astrophysics research computing center at the University of Maryland
  11. Institute for Cyber-Enabled Research at Michigan State University
  12. Astroparticle physics computational facility at Marquette University
  13. Belgium-Funds for Scientific Research (FRS-FNRS)
  14. Belgium-Funds for Scientific Research (FWO)
  15. FWO Odysseus programme
  16. FWO Big Science programme
  17. Belgian Federal Science Policy Office (Belspo)
  18. Germany-Bundesministerium fur Bildung und Forschung (BMBF)
  19. Germany-Deutsche Forschungsgemeinschaft (DFG)
  20. Germany-Helmholtz Alliance for Astroparticle Physics (HAP)
  21. Germany-Initiative and Networking Fund of the Helmholtz Association
  22. Germany-Deutsches Elektronen Synchrotron (DESY)
  23. Germany-High Performance Computing cluster of the RWTH Aachen
  24. Sweden-Swedish Research Council
  25. Swedish Polar Research Secretariat
  26. Swedish National Infrastructure for Computing (SNIC)
  27. Knut and Alice Wallenberg Foundation
  28. Australia-Australian Research Council
  29. Canada-Natural Sciences and Engineering Research Council of Canada
  30. Calcul Quebec
  31. Compute Ontario
  32. Canada Foundation for Innovation
  33. WestGrid
  34. Compute Canada
  35. Denmark-Villum Fonden
  36. Carlsberg Foundation
  37. New Zealand-Marsden Fund
  38. Japan-Japan Society for Promotion of Science (JSPS)
  39. Institute for Global Prominent Research (IGPR) of Chiba University
  40. Korea-National Research Foundation of Korea (NRF)
  41. Switzerland-Swiss National Science Foundation (SNSF)
  42. United Kingdom-Department of Physics, University of Oxford

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A recent study analyzed data collected by IceCube from 2008 to 2018 and found a cumulative neutrino excess associated with several sources. Among them, M87 was identified as the most significant time-dependent source, and TXS 0506+056 was the only source with two flares. Furthermore, a binomial test reported a cumulative neutrino excess in the Northern Hemisphere associated with four sources.
A recent time-integrated analysis of a catalog of 110 candidate neutrino sources revealed a cumulative neutrino excess in the data collected by IceCube between 2008 April 6 and 2018 July 10. This excess, inconsistent with the background hypothesis in the Northern Hemisphere at the 3.3 sigma level, is associated with four sources: NGC 1068, TXS 0506+056, PKS 1424+240, and GB6 J1542+6129. This Letter presents two time-dependent neutrino emission searches on the same data sample and catalog: a point-source search that looks for the most significant time-dependent source of the catalog by combining space, energy, and time information of the events, and a population test based on binomial statistics that looks for a cumulative time-dependent neutrino excess from a subset of sources. Compared to previous time-dependent searches, these analyses enable a feature to possibly find multiple flares from a single direction with an unbinned maximum-likelihood method. M87 is found to be the most significant time-dependent source of this catalog at the level of 1.7 sigma post-trial, and TXS 0506+056 is the only source for which two flares are reconstructed. The binomial test reports a cumulative time-dependent neutrino excess in the Northern Hemisphere at the level of 3.0 sigma associated with four sources: M87, TXS 0506+056, GB6 J1542+6129, and NGC 1068.

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