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Record W4407245004 · doi:10.3204/pubdb-2025-05397

VERITAS and Multiwavelength Observations of the Blazar B3 2247+381 in Response to an IceCube Neutrino Alert

2025· preprint· en· W4407245004 on OpenAlexfundno aff
A. Acharyya, C. B. Adams, P. Bangale, J. T. Bartkoske, W. Benbow, J. H. Buckley, Yu Chen, Jodi Christiansen, A. J. Chromey, A. Duerr, M. Errando, Miguel Escobar Godoy, Abe Falcone, Q. Feng, L. Fortson, A. Furniss, W. Hanlon, D.C. Hanna, Jamie Holder, T. B. Humensky, Philip Kaaret, M. P. Kertzman, D. Kieda, T. K. Kleiner, Mx. Nikolas Korzoun, F. Krennrich, M. J. Lang, M. Lundy, Conor McGrath, M. J. Millard, J. Millis, P. Moriarty, Ken Ragan, P. T. Reynolds, D. Ribeiro, Emmet Thomas Roache, Jamie L. Ryan, I. Sadeh, M. Santander, Ruo-Yu Shang, M. Splettstoesser, D. Tak, A. K. Talluri, J. V. Tucci, Janeth Valverde, Jooyun Woo, R. Abbasi, M. Ackermann, Jean-Marco Alameddine, K. Andeen, Y. Ashida, R. Babu, M. Baricevic, S. W. Barwick, V. Basu, R. Bay, J. Becker Tjus, Chiara Bellenghi, D. Berley, E. Blaufuss, F. Bontempo, Caterina Boscolo Meneguolo, J. Braun, Zoe Brisson-Tsavoussis, J. Brostean-Kaiser, L. Brusa, R. T. Burley, Delaney Butterfield, Ioana Caracas, K. Carloni, J. Graciá‐Carpio, Sharmistha Chattopadhyay, Thien Nhan Chau, Z. Chen, D. Chirkin, S. Choi, Alan Coleman, Peter John Cusack Coleman, G. H. Collin, J. M. Conrad, Rebecca Corley, D. F. Cowen, C. De Clercq, James DeLaunay, Diyaselis Delgado, Sen Deng, A. Desai, T. DeYoung, Adriel Herrero Díaz, J. C. Díaz–Vélez, P. Dierichs, M. Dittmer, A. Domi, H. Dujmovic, K. Dutta, M. A. DuVernois, T. Ehrhardt, Leonhard Eidenschink, E. Ellinger, Dominik Elsässer, R. Engel, Waleed Esmail, J. Evans, P. A. Evenson, Kwok Lung Fan, A. R. Fazely, A. Fedynitch, Nora Feigl, Sebastian Fiedlschuster, C. Finley, A. Franckowiak, S. Fukami, Erik Ganster, M. García, L. Gerhardt, A. Ghadimi, C. Girard-Carillo, C. Glaser, T. Glüsenkamp, J. G. González, Alejandra Granados, D. Grant, S. Griffin, S. Griswold, Kathrine Mørch Groth, David Joseph Guevel, C. Günther, Pascal Gutjahr, C. Haack, A. Hallgren, L. Halve, Leon Hamacher, H. Hamdaoui, M. Ha Minh, Michael Handt, K. Hanson, J. Hardin, Alexander Harnisch, P. Hatch, A. Haungs, Jonas Häußler, K. Helbing, Jonas Hellrung, J. Hermannsgabner, L. Heuermann, Nils Heyer, S. Hickford, Attila Hidvégi, Colton Hill, G. C. Hill, Ramy Hmaid, K. D. Hoffman, Sam Hori, K. Hoshina, Matheus Hostert, Wenjie Hou, Thomas S. Huber, M. Hünnefeld, R. Hussain, K. Hymon, A. Ishihara, M. Jacquart, Samyak Jain, Oliver Janik, Matti Jansson, M. Jeong, Miaochen Jin, B. J. P. Jones, N. Kamp, Woosik Kang, X. S. Kang, A. Kappes, David Kappesser, M. Karl, A. Karle, Akanksha Katil, U. Katz, J. L. Kelley, Manish Khanal, A. Khatee Zathul, Yukiho Kobayashi, T. Kontrimas, C. Kopper, T. Kozynets, K. Kruiswijk, E. Krupczak, Anil Kumar, E. Kun, N. Kurahashi, N. Lad, Cristina Lagunas Gualda, M. Lamoureux, M. J. Larson, Jeffrey Lazar, Kayla Leonard DeHolton, A. Leszczyńska, Massimiliano Lincetto, M. Liubarska, Christina Love, Francesco Lucarelli, William Luszczak, J. Madsen, K. B. M. Mahn, Y. Makino, Alicia Mand, W. Marie Sainte, M. Marsee, F. McNally, J. V. Mead, A. Medina, M. Meier, Lukas Merten, J. Mitchell, T. Montaruli, R. W. Moore, Y. Morii, R. Morse, Tista Mukherjee, R. Naab, M. Nakos, U. Naumann, J. Necker, Ludwig Neste, M. Neumann, M. U. Nisa, A. Noell, A. Novikov, A. Olivas, R. Orsoe, J. Osborn, Veronika Palušová, H. Pandya, N. Park, G. K. Parker, V. A. Parrish, Ek Narayan Paudel, L. Paul, C. Pérez de los Heros, Teresa Pernice, A. Pizzuto, Axel Pontén, Y. Popovych, R. Procter-Murphy, G. T. Przybylski, Lilly Pyras, C. Raab, J. Rack-Helleis, N. Rad, Martin Langgård Ravn, K. Rawlins, Z. Rechav, E. Resconi, S. Reusch, W. Rhode, B. Riedel, Adam Rifaie, E. J. Roberts, S. Robertson, Martin Rongen, Aske Rosted, C. Rott, T. Ruhe, L. Ruohan, I. Safa, A. Sandrock, S. Sarkar, J. Savelberg, P. Savina, Patrick Schaile, Merlin Schaufel, H. Schieler, S. Schindler, Lea Schlickmann, B. Schlüter, Felix Schlüter, Nick Schmeisser, Torsten C. Schmidt, J. Schneider, Frank Schröder, L. Schumacher, Sonke Schwirn, S. Sclafani, D. Seckel, Leo Seen, Mohammad Ful Hossain Seikh, Minhye Seo, Per Arne Sevle Myhr, R. Shah, S. Shefali, N. Shimizu, B. Skrzypek, B. Smithers, R. Snihur, J. Soedingrekso, A. Søgaard, D. Soldin, Giacomo Sommani, Christian Spannfellner, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, T. Stürwald, Thomas Stuttard, G. W. Sullivan, I. Taboada, A. Terliuk, S. Tilav, K. Tollefson, C. Tönnis, A. Trettin, Anuj Kumar Upadhyay, K. Upshaw, A. Vaidyanathan, Nora Valtonen-Mattila, J. Vandenbroucke, N. van Eijndhoven, D. Vannerom, J. van Santen, J. Vara, F. Varsi, M. Venugopal, M. Vereecken, Sebastian Vergara Carrasco, S. Verpoest, D. Veske, A. Vijai, C. Walck, Andrew Wang, C. Weaver, P. Weigel, A. Weindl, J. Weldert, C. Wendt, J. Werthebach, M. Weyrauch, N. Whitehorn, D. R. Williams, Lucas Witthaus, Martin Wolf, G. Wrede, Xiaolin Xu, J. P. Yanez, Emre Burak Yildizci, R. Young, F. Yu, Shiqi Yu, Tianlu Yuan, A. Zegarelli, S. Zhang, Z. Zhang, P. Zhelnin, Perri Zilberman, Melany Zimmerman, Pablo Drake, Elizabeth Spira-Savett, P. Lusen

Bibliographic record

VenueDesy publication database (The Deutsches Elektronen-Synchrotron) · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersOffice of Experimental Program to Stimulate Competitive ResearchJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of Polar ProgramsCollege of Engineering, Michigan State UniversityOffice of ScienceHelmholtz Alliance for Astroparticle PhysicsAlliance de recherche numérique du CanadaChiba UniversityInstitute for Global Prominent Research, Chiba UniversityRWTH Aachen UniversityKnut och Alice Wallenbergs StiftelseNuclear Safety and Security CommissionMarsden FundBundesministerium für Bildung und ForschungSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNational Science FoundationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftQueen's University BelfastDeutsches Elektronen-SynchrotronNational Energy Research Scientific Computing CenterSpace Telescope Science InstituteWestern Canada Research GridFonds De La Recherche Scientifique - FNRSQueen's UniversityPolarforskningssekretariatetNational Research Foundation of KoreaVillum FondenMarquette UniversityVetenskapsrådetSmithsonian InstitutionU.S. Department of EnergyUniversity of Wisconsin-MadisonFonds Wetenschappelijk OnderzoekNvidiaNational Aeronautics and Space AdministrationOffice of Advanced CyberinfrastructureEuropean CommissionNational Research FoundationMichigan State UniversityBarnard College
KeywordsBlazarNeutrinoPhysicsAstronomyAstrophysicsParticle physicsGamma ray

Abstract

fetched live from OpenAlex

While the sources of the diffuse astrophysical neutrino flux detected by the IceCube Neutrino Observatory are still largely unknown, one of the promising methods used towards understanding this is investigating the potential temporal and spatial correlations between neutrino alerts and the electromagnetic radiation from blazars. We report on the multiwavelength target-of-opportunity observations of the blazar B3 2247+381, taken in response to an IceCube multiplet alert for a cluster of muon neutrino events compatible with the source location between May 20, 2022 and November 10, 2022. B3 2247+381 was not detected with VERITAS during this time period. The source was found to be in a low-flux state in the optical, ultraviolet and gamma-ray bands for the time interval corresponding to the neutrino event, but was detected in the hard X-ray band with NuSTAR during this period. We find the multiwavelength spectral energy distribution is well described using a simple one-zone leptonic synchrotron self-Compton radiation model. Moreover, assuming the neutrinos originate from hadronic processes within the jet, the neutrino flux would be accompanied by a photon flux from the cascade emission, and the integrated photon flux required in such a case would significantly exceed the total multiwavelength fluxes and the VERITAS upper limits presented here. The lack of flaring activity observed with VERITAS, combined with the low multiwavelength flux levels, and given the significance of the neutrino excess is at 3$σ$ level (uncorrected for trials), makes B3 2247+381 an unlikely source of the IceCube multiplet. We conclude that the neutrino excess is likely a background fluctuation.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.675
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.001
Open science0.0020.002
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.027
GPT teacher head0.265
Teacher spread0.238 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2025
Admission routes1
Has abstractyes

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