Probing the Connection between IceCube Neutrinos and MOJAVE AGN

R Abbasi; M Ackermann; J Adams; S K Agarwalla; J A Aguilar; M Ahlers; J M Alameddine; N M Amin; K Andeen; C Argüelles; Y Ashida; S Athanasiadou; L Ausborm; S N Axani; X Bai; A Balagopal V; M Baricevic; S W Barwick; S Bash; R Bay; J J Beatty; V Basu; J Becker Tjus; J Beise; C Bellenghi; C Benning; S BenZvi; D Berley; E Bernardini; D Z Besson; E Blaufuss; L Bloom; S Blot; F Bontempo; JY Book Motzkin; C Boscolo Meneguolo; S Böser; O Botner; J Böttcher; J Braun; B Brinson; J Brostean-Kaiser; L Brusa; R T Burley; D Butterfield; M A Campana; I Caracas; K Carloni; J Carpio; S Chattopadhyay; N Chau; Z Chen; D Chirkin; S Choi; B A Clark; A Coleman; G H Collin; A Connolly; J M Conrad; R Corley; D F Cowen; P Dave; C De Clercq; J J DeLaunay; D Delgado; S Deng; A Desai; P Desiati; K D de Vries; G de Wasseige; T DeYoung; A Diaz; J C Díaz-Vélez; P Dierichs; M Dittmer; A Domi; L Draper; H Dujmovic; D Durnford; K Dutta; M A DuVernois; T Ehrhardt; L Eidenschink; A Eimer; P Eller; E Ellinger; S El Mentawi; D Elsässer; R Engel; H Erpenbeck; J Evans; P A Evenson; K L Fan; K Fang; K Farrag; A R Fazely; A Fedynitch; N Feigl; S Fiedlschuster; C Finley; M Hostert

doi:10.3847/1538-4357/ad643d

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Probing the Connection between IceCube Neutrinos and MOJAVE AGN

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Probing the Connection between IceCube Neutrinos and MOJAVE AGN

R Abbasi, M Ackermann, J Adams, S K Agarwalla, J A Aguilar, M Ahlers, J M Alameddine, N M Amin, K Andeen, C Argüelles, …

The Astrophysical journal, Vol.973(2), 97

10/01/2024

DOI: 10.3847/1538-4357/ad643d

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Abstract

Active galactic nuclei (AGN) are prime candidate sources of the high-energy, astrophysical neutrinos detected by IceCube. This is demonstrated by the real-time multimessenger detection of the blazar TXS 0506+056 and the recent evidence of neutrino emission from NGC 1068 from a separate time-averaged study. However, the production mechanism of the astrophysical neutrinos in AGN is not well established, which can be resolved via correlation studies with photon observations. For neutrinos produced due to photohadronic interactions in AGN, in addition to a correlation of neutrinos with high-energy photons, there would also be a correlation of neutrinos with photons emitted at radio wavelengths. In this work, we perform an in-depth stacking study of the correlation between 15 GHz radio observations of AGN reported in the MOJAVE XV catalog, and 10 yr of neutrino data from IceCube. We also use a time-dependent approach, which improves the statistical power of the stacking analysis. No significant correlation was found for both analyses, and upper limits are reported. When compared to the IceCube diffuse flux, at 100 TeV and for a spectral index of 2.5, the upper limits derived are ∼3% and ∼9% for the time-averaged and time-dependent cases, respectively.

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Title: Subtitle: Probing the Connection between IceCube Neutrinos and MOJAVE AGN
Creators: R Abbasi - Loyola University Chicago
M Ackermann - Deutsches Elektronen-Synchrotron DESY
J Adams - University of Canterbury
S K Agarwalla - University of Wisconsin–Madison
J A Aguilar
M Ahlers - University of Copenhagen
J M Alameddine - TU Dortmund University
N M Amin - University of Delaware
K Andeen - Marquette University
C Argüelles - Harvard University
Y Ashida - University of Utah
S Athanasiadou - Deutsches Elektronen-Synchrotron DESY
L Ausborm - RWTH Aachen University
S N Axani - University of Delaware
X Bai - South Dakota School of Mines and Technology
A Balagopal V
M Baricevic - University of Wisconsin–Madison
S W Barwick - University of California, Irvine
S Bash - Technical University of Munich
R Bay - University of California, Berkeley
J J Beatty - The Ohio State University
V Basu - University of Wisconsin–Madison
J Becker Tjus
J Beise - Uppsala University
C Bellenghi - Ludwig-Maximilians-Universität München
C Benning - RWTH Aachen University
S BenZvi - University of Rochester
D Berley - University of Maryland, College Park
E Bernardini
D Z Besson - University of Kansas
E Blaufuss - University of Maryland, College Park
L Bloom - University of Alabama
S Blot - Deutsches Elektronen-Synchrotron DESY
F Bontempo - Karlsruhe Institute of Technology
JY Book Motzkin
C Boscolo Meneguolo
S Böser
O Botner - Uppsala University
J Böttcher - RWTH Aachen University
J Braun
B Brinson - Georgia Institute of Technology
J Brostean-Kaiser - Deutsches Elektronen-Synchrotron DESY
L Brusa - RWTH Aachen University
R T Burley - The University of Adelaide
D Butterfield
M A Campana - Drexel University
I Caracas
K Carloni - Harvard University
J Carpio - University of Nevada, Reno
S Chattopadhyay
N Chau - Université Libre de Bruxelles
Z Chen
D Chirkin
S Choi - Sungkyunkwan University
B A Clark - University of Maryland, College Park
A Coleman
G H Collin - Massachusetts Institute of Technology
A Connolly - The Ohio State University
J M Conrad
R Corley - University of Utah
D F Cowen - Pennsylvania State University
P Dave
C De Clercq - Vrije Universiteit Brussel
J J DeLaunay - University of Alabama
D Delgado - Harvard University
S Deng - RWTH Aachen University
A Desai
P Desiati
K D de Vries
G de Wasseige
T DeYoung - Michigan State University
A Diaz
J C Díaz-Vélez
P Dierichs - RWTH Aachen University
M Dittmer - University of Münster
A Domi - Friedrich-Alexander-Universität Erlangen-Nürnberg
L Draper - University of Utah
H Dujmovic
D Durnford - University of Alberta
K Dutta
M A DuVernois
T Ehrhardt
L Eidenschink - Ludwig-Maximilians-Universität München
A Eimer - Friedrich-Alexander-Universität Erlangen-Nürnberg
P Eller - Ludwig-Maximilians-Universität München
E Ellinger - University of Wuppertal
S El Mentawi
D Elsässer - TU Dortmund University
R Engel - Karlsruhe Institute of Technology
H Erpenbeck
J Evans - University of Maryland, College Park
P A Evenson - University of Delaware
K L Fan
K Fang
K Farrag - Chiba University
A R Fazely
A Fedynitch - Institute of Physics, Academia Sinica
N Feigl - Humboldt-Universität zu Berlin
S Fiedlschuster - Friedrich-Alexander-Universität Erlangen-Nürnberg
C Finley
M Hostert (Contributor) - University of Iowa, Physics and Astronomy
Resource Type: Journal article
Publication Details: The Astrophysical journal, Vol.973(2), 97
DOI: 10.3847/1538-4357/ad643d
ISSN: 0004-637X
eISSN: 1538-4357
Publisher: IOP
Grant note: USA-US National Science Foundation-Office of Polar Programs, US National Science Foundation-Physics Division, US National Science FoundationEPSCoR, US National Science Foundation-Office of Advanced Cyberinfrastructure, Wisconsin Alumni Research FoundationCenter for High Throughput Computing (CHTC) at the University of Wisconsin-MadisonAdvanced Cyberinfrastructure Coordination Ecosystem: Services & Support (ACCESS)NVIDIA CorporationFWO Odysseus and Big Science programsBelgian Federal Science Policy Office (Belspo)Germany-Bundesministerium fur Bildung und Forschung (BMBF)Deutsche Forschungsgemeinschaft (DFG)Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz AssociationSweden-Swedish Research CouncilSwedish Polar Research SecretariatKnut and Alice Wallenberg FoundationEuropean Union-EGI Advanced Computing for researchAustralia-Australian Research CouncilDigital Research Alliance of CanadaDenmark-Villum FondenCarlsberg FoundationEuropean CommissionNew Zealand-Marsden FundKorea-National Research Foundation of Korea (NRF)Switzerland-Swiss National Science Foundation (SNSF)
u The IceCube Collaboration acknowledges the significant contributions to this manuscript from Abhishek Desai and Justin Vandenbroucke. The authors would like to thank M. Lister, Y. Kovalev, and A. Plavin for useful discussions regarding the MOJAVE and RFC catalogs and the required completeness calculation. The authors would also like to thank M. J. Romfoe for the useful comments on the paper draft. The authors gratefully acknowledge the support from the following agencies and institutions: USA-US National Science Foundation-Office of Polar Programs, US National Science Foundation-Physics Division, US National Science FoundationEPSCoR, US National Science Foundation-Office of Advanced Cyberinfrastructure, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Partnership to Advance Throughput Computing (PATh), Advanced Cyberinfrastructure Coordination Ecosystem: Services & Support (ACCESS), Frontera computing project at the Texas Advanced Computing Center, US Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for CyberEnabled Research at Michigan State University, Astroparticle physics computational facility at Marquette University, NVIDIA Corporation, and Google Cloud Platform; Belgium -Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programs, and Belgian Federal Science Policy Office (Belspo); Germany-Bundesministerium fur 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; CanadaNatural Sciences and Engineering Research Council of Canada, Calcul Quebec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Digital Research Alliance of 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).
Language: English
Date published: 10/01/2024
Academic Unit: Physics and Astronomy
Record Identifier: 9984945914902771

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