Search for correlations of high-energy neutrinos detected in IceCube with radio-bright AGN and gamma-ray emission from blazars

IceCube Collaboration

doi:10.3847/1538-4357/acdfcb

Search for correlations of high-energy neutrinos detected in IceCube with radio-bright AGN and gamma-ray emission from blazars

IceCube Collaboration

Research output: Contribution to journal › Article › peer-review

15 Citations (Scopus)

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Abstract

The IceCube Neutrino Observatory sends realtime neutrino alerts with high probability of being astrophysical in origin. We present a new method to correlate these events and possible candidate sources using $2,089$ blazars from the Fermi-LAT 4LAC-DR2 catalog and with $3,413$ AGNs from the Radio Fundamental Catalog. No statistically significant neutrino emission was found in any of the catalog searches. The result is compatible with a small fraction, $

Original language	English
Article number	75
Number of pages	11
Journal	The Astrophysical Journal
Volume	954
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/acdfcb
Publication status	Published - 23 Aug 2023

Bibliographical note

Funding Information:
The IceCube collaboration acknowledges the significant contribution to this manuscript from Cristina Lagunas Gualda. The authors gratefully acknowledge the support from the following agencies and institutions: USA –U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, U.S. National Science Foundation-EPSCoR, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin–Madison, Open Science Grid (OSG), Advanced Cyberinfrastructure Coordination Ecosystem: Services & Support (ACCESS), Frontera computing project at the Texas Advanced Computing Center, U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium –Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany –Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden –Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; European Union –EGI Advanced Computing for research; Australia –Australian Research Council; Canada –Natural Sciences and Engineering Research Council of Canada, Calcul Québec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark –Villum Fonden, Carlsberg Foundation, and European Commission; New Zealand –Marsden Fund; Japan –Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea –National Research Foundation of Korea (NRF); Switzerland –Swiss National Science Foundation (SNSF); and United Kingdom –Department of Physics, University of Oxford.

Publisher Copyright:
© 2023. The Author(s). Published by the American Astronomical Society.

Keywords

astro-ph.HE

Access to Document

10.3847/1538-4357/acdfcbLicence: CC BY

Abbasi_2023_ApJ_954_75Final published version, 1.42 MBLicence: CC BY

Cite this

@article{844096891e3f455e9474066dd242f1a8,

title = "Search for correlations of high-energy neutrinos detected in IceCube with radio-bright AGN and gamma-ray emission from blazars",

abstract = " The IceCube Neutrino Observatory sends realtime neutrino alerts with high probability of being astrophysical in origin. We present a new method to correlate these events and possible candidate sources using $2,089$ blazars from the Fermi-LAT 4LAC-DR2 catalog and with $3,413$ AGNs from the Radio Fundamental Catalog. No statistically significant neutrino emission was found in any of the catalog searches. The result is compatible with a small fraction, $",

keywords = "astro-ph.HE",

author = "{IceCube Collaboration} and Paul Coppin and {Correa Camiroaga}, Pablo and {De Clercq}, Catherine and {De Vries}, Krijn and Yarno Merckx and {Van Eijndhoven}, Nicolaas",

note = "Funding Information: The IceCube collaboration acknowledges the significant contribution to this manuscript from Cristina Lagunas Gualda. The authors gratefully acknowledge the support from the following agencies and institutions: USA –U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, U.S. National Science Foundation-EPSCoR, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin–Madison, Open Science Grid (OSG), Advanced Cyberinfrastructure Coordination Ecosystem: Services & Support (ACCESS), Frontera computing project at the Texas Advanced Computing Center, U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium –Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany –Bundesministerium f{\"u}r Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden –Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; European Union –EGI Advanced Computing for research; Australia –Australian Research Council; Canada –Natural Sciences and Engineering Research Council of Canada, Calcul Qu{\'e}bec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark –Villum Fonden, Carlsberg Foundation, and European Commission; New Zealand –Marsden Fund; Japan –Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea –National Research Foundation of Korea (NRF); Switzerland –Swiss National Science Foundation (SNSF); and United Kingdom –Department of Physics, University of Oxford. Publisher Copyright: {\textcopyright} 2023. The Author(s). Published by the American Astronomical Society.",

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doi = "10.3847/1538-4357/acdfcb",

language = "English",

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T1 - Search for correlations of high-energy neutrinos detected in IceCube with radio-bright AGN and gamma-ray emission from blazars

AU - IceCube Collaboration

AU - Coppin, Paul

AU - Correa Camiroaga, Pablo

AU - De Clercq, Catherine

AU - De Vries, Krijn

AU - Merckx, Yarno

AU - Van Eijndhoven, Nicolaas

N1 - Funding Information: The IceCube collaboration acknowledges the significant contribution to this manuscript from Cristina Lagunas Gualda. The authors gratefully acknowledge the support from the following agencies and institutions: USA –U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, U.S. National Science Foundation-EPSCoR, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin–Madison, Open Science Grid (OSG), Advanced Cyberinfrastructure Coordination Ecosystem: Services & Support (ACCESS), Frontera computing project at the Texas Advanced Computing Center, U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium –Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany –Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden –Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; European Union –EGI Advanced Computing for research; Australia –Australian Research Council; Canada –Natural Sciences and Engineering Research Council of Canada, Calcul Québec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark –Villum Fonden, Carlsberg Foundation, and European Commission; New Zealand –Marsden Fund; Japan –Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea –National Research Foundation of Korea (NRF); Switzerland –Swiss National Science Foundation (SNSF); and United Kingdom –Department of Physics, University of Oxford. Publisher Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

PY - 2023/8/23

Y1 - 2023/8/23

N2 - The IceCube Neutrino Observatory sends realtime neutrino alerts with high probability of being astrophysical in origin. We present a new method to correlate these events and possible candidate sources using $2,089$ blazars from the Fermi-LAT 4LAC-DR2 catalog and with $3,413$ AGNs from the Radio Fundamental Catalog. No statistically significant neutrino emission was found in any of the catalog searches. The result is compatible with a small fraction, $

AB - The IceCube Neutrino Observatory sends realtime neutrino alerts with high probability of being astrophysical in origin. We present a new method to correlate these events and possible candidate sources using $2,089$ blazars from the Fermi-LAT 4LAC-DR2 catalog and with $3,413$ AGNs from the Radio Fundamental Catalog. No statistically significant neutrino emission was found in any of the catalog searches. The result is compatible with a small fraction, $

KW - astro-ph.HE

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U2 - 10.3847/1538-4357/acdfcb

DO - 10.3847/1538-4357/acdfcb

M3 - Article

VL - 954

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 75

ER -

Search for correlations of high-energy neutrinos detected in IceCube with radio-bright AGN and gamma-ray emission from blazars

Abstract

Bibliographical note

Keywords

Access to Document

Other files and links

Fingerprint

FWOIRI11: Exploring the Extreme Universe with the (Extended) IceCube Neutrino and Cosmic Ray Observatory at the South Pole

SRP72: SRP-Onderzoekszwaartepunt: High-energy physics (HEP@VUB).

FWOTM1076: IceCube Search for High-Energy Neutrinos from Obscured Sources in the Great Observatories All-Sky LIRG Survey (GOALS)

Cite this

Search for correlations of high-energy neutrinos detected in IceCube with radio-bright AGN and gamma-ray emission from blazars

Abstract

Bibliographical note

Keywords

Access to Document

Other files and links

Fingerprint

Projects

FWOIRI11: Exploring the Extreme Universe with the (Extended) IceCube Neutrino and Cosmic Ray Observatory at the South Pole

SRP72: SRP-Onderzoekszwaartepunt: High-energy physics (HEP@VUB).

FWOTM1076: IceCube Search for High-Energy Neutrinos from Obscured Sources in the Great Observatories All-Sky LIRG Survey (GOALS)

Cite this