Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 1 h ago
Peer-reviewedCC BY 4.0The Astrophysical Journal

Investigating IceCube Neutrino Alerts with the HAWC Gamma-Ray Observatory

87 more authors

60 listed; 99 in total.

26 affiliations
  1. 1Universidad Nacional Autónoma de México
  2. 2Universidad Autónoma de Chiapas
  3. 3Universidad de Costa Rica
  4. 4Universidad Michoacana de San Nicolás de Hidalgo
  5. 5Temple University
  6. 6Michigan State University
  7. 7Instituto Nacional de Astrofísica
  8. 8Institute of Nuclear Physics Polish Academy of Sciences
  9. 9Benemérita Universidad Autónoma de Puebla
  10. 10Universitat de València
  11. 11Centro Universitario de Ciencias Exactase Ingenierias
  12. 12University of Wisconsin–Madison
  13. 13Stanford University
  14. 14University of Maryland
  15. 15Tecnologico de Monterrey
  16. 16Michigan Technological University
  17. 17Department of Physics
  18. 18Los Alamos National Laboratory
  19. 19Shanghai Jiao Tong University
  20. 20Max-Planck Institute for Nuclear Physics
  21. 21University of Delaware
  22. 22Universidad Politecnica de Pachuca
  23. 23University of Utah
  24. 24University of Seoul
  25. 25Instituto Politécnico Nacional
  26. 26University of New Mexico

Abstract

Neutrino emission from astrophysical sources has long been considered a signature of cosmic-ray acceleration. The IceCube Neutrino Observatory has observed a diffuse flux of TeV–PeV neutrinos, but very few confirmed sources have emerged. With the recent publication of the IceCube Event Catalog (IceCat-1), IceCube has released a list of probable astrophysical neutrinos from 2011 May to 2020 December, with follow-up alerts released via the Astrophysical Multi-messenger Observatory Network (AMON). Using the archival data from the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory, we search for gamma-ray outbursts spatially coincident with these neutrino alerts using a Bayesian block algorithm. In this work, we consider 380 alerts, up to 2026 May 19, that are within HAWC’s field of view. We observe approximately a 5% coincident detection rate, which is consistent with expectations from background. Two of these detections contain the active galactic nuclei (AGNs) Mrk 421 and Mrk 501. We discuss the possibility of these AGNs producing the observed neutrino events when considering the HAWC results.

Related

  1. Resolving the Galactic Center Region's Gamma-Ray Emission and Searching for its Neutrino Counterpart with HAWC and IceCube
    S. Yun-Carcamo, R. Babu, for the HAWC +1
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsarXiv
  2. Radio measurements of air showers with the IceCube-Gen2 surface prototype station at the Pierre Auger Observatory
    Stef Verpoest, for the IceCube-Gen2 Collaboration, for the Pierre Auger Collaboration
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsInstrumentation & methodsarXiv
  3. IceCube Real-time Searches for High-energy Neutrinos Coincident with LIGO/Virgo/KAGRA Gravitational-Wave Alerts in O4a
    The IceCube Collaboration, R. Abbasi, M. Ackermann +418
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsarXiv
  4. Neutrino Fingerprints: Image-Based Encodings of IceCube Events for CNN Direction Reconstruction
    Floriano Tori, Brecht F. Verbeken, Vincent Ginis
    arXivPreprintCC BY 4.0Full textInstrumentation & methodsarXiv
  5. Hidden Neutrino Active Galaxy Candidates: Prospects for Catalog and Stacking Searches with IceCube, IceCube-Gen2, and KM3NeT
    Mainak Mukhopadhyay, Jose Alonso Carpio, Heer Patel +2
    arXivPreprintCC BY 4.0Full textGalaxiesHigh-energy astrophysicsarXiv
BibTeX
@article{alfaro2026investigating,
  title = {{Investigating IceCube Neutrino Alerts with the HAWC Gamma-Ray Observatory}},
  author = {R. Alfaro and C. Alvarez and A. Andrés and E. Anita-Rangel and M. Araya and J. C. Arteaga-Velázquez and D. Avila Rojas and H. A. Ayala Solares and R. Babu and E. Belmont-Moreno and A. Bernal and K. S. Caballero-Mora and T. Capistrán and A. Carramiñana and F. Carreón and S. Casanova and J. Cotzomi and S. Coutiño de León and C. de León and E. De la Fuente and P. Desiati and N. Di Lalla and R. Diaz Hernandez and M. A. DuVernois and J. C. Díaz-Vélez and K. Engel and C. Espinoza and N. Fraija and S. Fraija and A. Galván-Gámez and J. A. García-González and F. Garfias and N. Ghosh and A. Gonzalez Muñoz and M. M. González and J. A. González and J. A. Goodman and D. Guevel and J. Gyeong and J. P. Harding and S. Hernández-Cadena and I. Herzog and J. Hinton and D. Huang and F. Hueyotl-Zahuantitla and P. Hüntemeyer and A. Iriarte and S. Kaufmann and D. Kieda and K. Leavitt and J. Lee and W. H. Lee and H. León Vargas and J. T. Linnemann and A. L. Longinotti and G. Luis-Raya and K. Malone and O. Martinez and J. Martínez- Castro and J.A. Matthews},
  journal = {The Astrophysical Journal},
  year = {2026},
  month = oct,
  doi = {10.3847/1538-4357/aea154},
  url = {https://iopscience.iop.org/article/10.3847/1538-4357/aea154},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - Investigating IceCube Neutrino Alerts with the HAWC Gamma-Ray Observatory
AU  - R. Alfaro
AU  - C. Alvarez
AU  - A. Andrés
AU  - E. Anita-Rangel
AU  - M. Araya
AU  - J. C. Arteaga-Velázquez
AU  - D. Avila Rojas
AU  - H. A. Ayala Solares
AU  - R. Babu
AU  - E. Belmont-Moreno
AU  - A. Bernal
AU  - K. S. Caballero-Mora
AU  - T. Capistrán
AU  - A. Carramiñana
AU  - F. Carreón
AU  - S. Casanova
AU  - J. Cotzomi
AU  - S. Coutiño de León
AU  - C. de León
AU  - E. De la Fuente
AU  - P. Desiati
AU  - N. Di Lalla
AU  - R. Diaz Hernandez
AU  - M. A. DuVernois
AU  - J. C. Díaz-Vélez
AU  - K. Engel
AU  - C. Espinoza
AU  - N. Fraija
AU  - S. Fraija
AU  - A. Galván-Gámez
AU  - J. A. García-González
AU  - F. Garfias
AU  - N. Ghosh
AU  - A. Gonzalez Muñoz
AU  - M. M. González
AU  - J. A. González
AU  - J. A. Goodman
AU  - D. Guevel
AU  - J. Gyeong
AU  - J. P. Harding
AU  - S. Hernández-Cadena
AU  - I. Herzog
AU  - J. Hinton
AU  - D. Huang
AU  - F. Hueyotl-Zahuantitla
AU  - P. Hüntemeyer
AU  - A. Iriarte
AU  - S. Kaufmann
AU  - D. Kieda
AU  - K. Leavitt
AU  - J. Lee
AU  - W. H. Lee
AU  - H. León Vargas
AU  - J. T. Linnemann
AU  - A. L. Longinotti
AU  - G. Luis-Raya
AU  - K. Malone
AU  - O. Martinez
AU  - J. Martínez- Castro
AU  - J.A. Matthews
PY  - 2026
DA  - 2026/10/29
JO  - The Astrophysical Journal
DO  - 10.3847/1538-4357/aea154
UR  - https://iopscience.iop.org/article/10.3847/1538-4357/aea154
AB  - Neutrino emission from astrophysical sources has long been considered a signature of cosmic-ray acceleration. The IceCube Neutrino Observatory has observed a diffuse flux of TeV–PeV neutrinos, but very few confirmed sources have emerged. With the recent publication of the IceCube Event Catalog (IceCat-1), IceCube has released a list of probable astrophysical neutrinos from 2011 May to 2020 December, with follow-up alerts released via the Astrophysical Multi-messenger Observatory Network (AMON). Using the archival data from the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory, we search for gamma-ray outbursts spatially coincident with these neutrino alerts using a Bayesian block algorithm. In this work, we consider 380 alerts, up to 2026 May 19, that are within HAWC’s field of view. We observe approximately a 5% coincident detection rate, which is consistent with expectations from background. Two of these detections contain the active galactic nuclei (AGNs) Mrk 421 and Mrk 501. We discuss the possibility of these AGNs producing the observed neutrino events when considering the HAWC results.
SN  - 1538-4357
SN  - 0004-637X
ER  -