MétaCan
Menu
Back to cohort
Record W4415345549 · doi:10.18154/rwth-2026-03659

A Search for Millimeter-Bright Blazars as Astrophysical Neutrino Sources

2025· article· en· W4415345549 on OpenAlexfundno aff
R. Abbasi, J. Adams, Sanjib Kumar Agarwalla, J. A. Aguilar, M. Ahlers, Jean-Marco Alameddine, N. M. Amin, K. Andeen, C. Argüelles, Y. Ashida, S. Athanasiadou, S. N. Axani, Rishi Babu, X. Bai, J. Baines-Holmes, Aswathi Balagopal, S. W. Barwick, Simeon Bash, Vedant Basu, R. Bay, J. J. Beatty, J. Becker Tjus, Peter Behrens, Jakob Beise, C. Bellenghi, B. Benkel, S. BenZvi, David Berley, E. Bernardini, D. Z. Besson, E. Blaufuss, Lucas Bloom, Summer Blot, Imre Bodó, F. Bontempo, Julia Book, Caterina Boscolo Meneguolo, S. Böser, O. Botner, J. Böttcher, J. Braun, Bennett Brinson, Zoe Brisson-Tsavoussis, Ryan T. Burley, Delaney Butterfield, M. A. Campana, Kiara Carloni, Sharmistha Chattopadhyay, Thien Nhan Chau, Z. Chen, D. Chirkin, S. Choi, B. A. Clark, A. Coleman, Peter John Cusack Coleman, G. H. Collin, A. Connolly, Rebecca Corley, D. F. Cowen, C. De Clercq, James DeLaunay, D. Delgado, T. Delmeulle, S. Deng, P. Desiati, K. D. de Vries, G. de Wasseige, T. DeYoung, J. C. Díaz–Vélez, Stephen DiKerby, M. Dittmer, Alba Domi, Lincoln Draper, L. Dueser, Daniel Durnford, Kaustav Dutta, M. A. DuVernois, T. Ehrhardt, Leonhard Eidenschink, A. Eimer, P. Eller, E. Ellinger, Dominik Elsässer, R. Engel, H. Erpenbeck, Waleed Esmail, S. Eulig, John Evans, P. A. Evenson, Kwok Lung Fan, Kareem Ramadan Farrag, A. R. Fazely, A. Fedynitch, Nora Feigl, C. Finley, D. B. Fox, A. Franckowiak, Satoshi Fukami, Philipp Fürst, J. Gallagher, Erik Ganster, A. Garcia, M. García, Gaurav Garg, Eliot Genton, L. Gerhardt, A. Ghadimi, C. Glaser, T. Glüsenkamp, J. G. González, Sreetama Goswami, Alejandra Granados, D. Grant, S. J. Gray, S. Griswold, Kathrine Mørch Groth, David Joseph Guevel, Christoph Günther, Pascal Gutjahr, C. Ha, Christian Haack, A. Hallgren, L. Halve, F. Halzen, Leon Hamacher, M. Ha Minh, Michael Handt, K. Hanson, John Hardin, A. A. Harnisch, P. Hatch, A. Haungs, Jonas Häußler, K. Helbing, Jonas Hellrung, Lukas Hennig, L. Heuermann, R. Hewett, Nils Heyer, S. Hickford, A. Hidvegi, Colton Hill, G. C. Hill, Ramy Hmaid, K. D. Hoffman, Dan Hooper, Sam Hori, K. Hoshina, Matheus Hostert, Wenjie Hou, Thomas Huber, K. Hultqvist, Karolin Hymon, A. Ishihara, W. Iwakiri, M. Jacquart, Samyak Jain, Oliver Janik, Minjin Jeong, Miaochen Jin, N. Kamp, Donghwa Kang, Xinyue Kang, A. Kappes, L. Kardum, T. Karg, Martina Karl, A. Karle, Akanksha Katil, M. Kauer, J. L. Kelley, Manish Khanal, A. Khatee Zathul, Ali Kheirandish, H. Kimku, J. Kiryluk, Carolin Klein, S. R. Klein, Yukiho Kobayashi, A. Kochocki, Ramesh Koirala, H. Kolanoski, T. Kontrimas, L. Köpke, C. Kopper, D. J. Koskinen, Paras Koundal, T. Kozynets, Gerhard Krieger, J. Krishnamoorthi, T. Krishnan, K. Kruiswijk, E. Krupczak, Anil Kumar, Emma Kun, N. Kurahashi, Cristina Lagunas Gualda, Laurent Arnaud, M. Lamoureux, M. J. Larson, Frederik Hermann Lauber, J. P. Lazar, Kayla Leonard DeHolton, A. Leszczyńska, Yantao Liu, M. Liubarska, Christy Love, F. Lucarelli, W. Luszczak, J. Madsen, Else Magnus, K. B. M. Mahn, Y. Makino, Elena Manao, S. Mancina, Alicia Mand, I. C. Mariş, Szabolcs Márka, Z. Márka, L. Marten, I. Martinez-Soler, R. Maruyama, F. Mayhew, F. McNally, J. V. Mead, K. Meagher, S. Mechbal, Andrés Muñoz Medina, L. Lu, Y. Merckx, Lukas Merten, Justin Mitchell, L. Molchany, T. Montaruli, R. W. Moore, Yasutsugu Morii, Anke Mosbrugger, M. Moulai, D. Mousadi, Tista Mukherjee, Richard Naab, M. Nakos, Uwe Naumann, J. Necker, Ludwig Neste, M.A. Neumann, H. Niederhausen, M. U. Nisa, K. Noda, A. Noell, Alexander Novikov, A. Obertacke Pollmann, Vivian O'Dell, A. Olivas, R. Orsoe, J. Osborn, Erin O’Sullivan, Veronika Palušová, H. Pandya, A. Parenti, N. Park, V. A. Parrish, Ek Narayan Paudel, Larissa Paul, C. Pérez de los Heros, Teresa Pernice, Josh Peterson, M. Plum, Axel Ponten, V. Poojyam, Y. Popovych, M. Prado Rodriguez, B. Pries, R. Procter-Murphy, G. T. Przybylski, Lilly Pyras, Christoph Raab, J. Rack-Helleis, N. Rad, Martin Langgård Ravn, K. Rawlins, Z. Rechav, I. Reistroffer, E. Resconi, S. Reusch, Chang Dong Rho, W. Rhode, B. Riedel, Adam Rifaie, E. J. Roberts, S. Robertson, Martin Rongen, Aske Rosted, C. Rott, T. Ruhe, L. Ruohan, Julian Saffer, Daniel Salazar-Gallegos, P. Sampathkumar, A. Sandrock, Grace Sanger-Johnson, Marcos Santander, S. Sarkar, J. Savelberg, Patrick Schaile, M. Schaufel, H. Schieler, S. Schindler, Lea Schlickmann, B. Schlüter, Felix Schlüter, Nick Schmeisser, T. Schmidt, F. G. Schröder, L. Schumacher, Sonke Schwirn, S. Sclafani, D. Seckel, Leo Seen, Mohammad Ful Hossain Seikh, S. Seunarine, Per Arne Sevle Myhr, Riya Shah, S. Shefali, N. Shimizu, B. Skrzypek, R. Snihur, J. Soedingrekso, A. Søgaard, D. Soldin, Philipp Soldin, Giacomo Sommani, C. Spannfellner, G. M. Spiczak, C. Spiering, Juliana Stachurska, M. Stamatikos, T. Stanev, T. Stezelberger, T. Stürwald, T. Stuttard, G. W. Sullivan, I. Taboada, S. Ter–Antonyan, A. Terliuk, A. Thakuri, Matthias Thiesmeyer, W. G. Thompson, J. Thwaites, S. Tilav, K. Tollefson, S. Toscano, D. Tosi, Alexandra Trettin, K. Upshaw, A. Vaidyanathan, N. Valtonen-Mattila, Janeth Valverde, J. Vandenbroucke, Thijs van Eeden, N. van Eijndhoven, L. Van Rootselaar, J. van Santen, J. Vara, Fahim Varsi, M. Venugopal, M. Vereecken, Sebastian Vergara Carrasco, S. Verpoest, Doğa Veske, A. Vijai, Joshua Villarreal, C. Walck, Andrew Wang, E. H. S. Warrick, C. Weaver, P. Weigel, A. Weindl, Gerrit Wrede, X. W. Xu, Robert A. Young, Shuo Zhang, Adam D. Hincks

Bibliographic record

VenueDesy publication database (The Deutsches Elektronen-Synchrotron) · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersOffice of Experimental Program to Stimulate Competitive ResearchJapan Society for the Promotion of ScienceNatural Sciences and Engineering Research Council of CanadaNational Institute of Standards and TechnologyHelmholtz Alliance for Astroparticle PhysicsInstitute for Global Prominent Research, Chiba UniversityRWTH Aachen UniversityKnut och Alice Wallenbergs StiftelseMarsden FundBundesministerium für Bildung und ForschungUniversity of TorontoSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNational Science FoundationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftDeutsches Elektronen-SynchrotronNational Energy Research Scientific Computing CenterAlliance de recherche numérique du CanadaChiba UniversityGovernment of OntarioWestern Canada Research GridFonds De La Recherche Scientifique - FNRSPolarforskningssekretariatetNational Research Foundation of KoreaVillum FondenOffice of Polar ProgramsCollege of Engineering, Michigan State UniversityPrinceton UniversityMarquette UniversityVetenskapsrådetU.S. Department of EnergyUniversity of Wisconsin-MadisonNational Research FoundationMichigan State UniversityFonds Wetenschappelijk OnderzoekNational Aeronautics and Space AdministrationAgencia Nacional de Investigación y DesarrolloNvidiaUniversity of PennsylvaniaOffice of Advanced CyberinfrastructureEuropean CommissionCompute Canada
KeywordsBlazarNeutrinoNeutrino astronomyMuonNeutrino detectorJet (fluid)CosmologyMassless particle

Abstract

fetched live from OpenAlex

The powerful jets of blazars have been historically considered as likely sites of high-energy cosmic-ray acceleration. However, particulars of the launched jet and the locations of leptonic and hadronic jet loading remain unclear. In the case when leptonic and hadronic particle injection occur jointly, a temporal correlation between synchrotron radiation and neutrino production is expected. We use a first catalog of millimeter (mm) wavelength blazar light curves from the Atacama Cosmology Telescope for a time-dependent correlation with twelve years of muon neutrino events from the IceCube South Pole Neutrino Observatory. Such mm emission is known to trace activity of the bright jet base, which is often self-absorbed at lower frequencies and potentially gamma-ray opaque. We perform an analysis of the population, as well as analyses of individual, selected sources. We do not observe a significant signal from the stacked population. TXS 0506+056 is found as the most significant, individual source, though this detection is not globally significant in our analysis of selected AGN. Our results suggest that the majority of mm-bright blazars are neutrino dim. In general, it is possible that many blazars have lighter, leptonic jets, or that only selected blazars provide exceptional conditions for neutrino production.

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)0.000
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: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.821
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.001
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.000
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 head0.014
GPT teacher head0.261
Teacher spread0.247 · 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 designTheoretical or conceptual
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

Explore more

Same venueDesy publication database (The Deutsches Elektronen-Synchrotron)Same topicAstrophysics and Cosmic PhenomenaFrench-language works237,207