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Record W3098322373 · doi:10.1103/physrevd.104.022002

IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data

2021· article· en· W3098322373 on OpenAlexafffund
M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, Cyril Martin Alispach, A. A. Alves, N. M. Amin, K. Andeen, T. Anderson, I. Ansseau, G. Anton, C. Argüelles, Spencer Axani, X. Bai, Aswathi Balagopal, Anastasia Maria Barbano, S. W. Barwick, Benjamin Bastian, Vedant Basu, V. Baum, S. Baur, R. Bay, J. J. Beatty, K. Becker, J. Becker Tjus, Chiara Bellenghi, S. BenZvi, D. Berley, E. Bernardini, D. Besson, G. Binder, D. Bindig, E. Blaufuss, Summer Blot, S. Böser, O. Botner, J. Böttcher, Etienne Bourbeau, J. Bourbeau, Federica Bradascio, J. Braun, S. Bron, Jannes Brostean-Kaiser, A. Burgman, Raffaela Busse, Michael Campana, C. Chen, D. Chirkin, S. Choi, Brian Clark, K. Clark, Lew Classen, Alan Coleman, G. H. Collin, J. M. Conrad, Paul Coppin, Pablo Correa, D. F. Cowen, R. Cross, Pranav Dave, C. De Clercq, James DeLaunay, H.-P. Dembinski, Kunal Deoskar, S. De Ridder, Abhishek Desai, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, Sukeerthi Dharani, A. Diaz, J. C. Díaz–Vélez, Hrvoje Dujmović, M. Dunkman, M. A. DuVernois, Emily Dvorak, Thomas Ehrhardt, P. Eller, R. Engel, John Evans, P. A. Evenson, S. Fahey, A. R. Fazely, Sebastian Fiedlschuster, Aaron Fienberg, K. Filimonov, C. Finley, Leander Fischer, D. B. Fox, A. Franckowiak, Edward Friedman, Alexander Fritz, Philipp Fürst, T. K. Gaisser, J. S. Gallagher, Erik Ganster, S. Garrappa, L. Gerhardt, Theo Glauch, T. Glüsenkamp, A. Goldschmidt, J. G. González, Sreetama Goswami, D. Grant, T. Grégoire, Z. Griffith, Spencer Griswold, Mehmet Gündüz, Christian Haack, A. Hallgren, R. Halliday, L. Halve, F. Halzen, Martin Ha Minh, K. Hanson, John Hardin, A. Haungs, Simon Hauser, D. Hebecker, K. Helbing, Felix Henningsen, S. Hickford, J. Hignight, Colton Hill, G. C. Hill, K. D. Hoffman, R. Hoffmann, Tobias Hoinka, Benjamin Hokanson-Fasig, K. Hoshina, F. Huang, M. E. Huber, Thomas Huber, K. Hultqvist, Mirco Hünnefeld, Raamis Hussain, S. In, N. Iovine, A. Ishihara, Matti Jansson, G. S. Japaridze, Minjin Jeong, B. J. P. Jones, R. Joppe, Donghwa Kang, Woosik Kang, X. Kang, A. Kappes, David Kappesser, T. Karg, Martina Karl, A. Karle, T. Katori, U. Katz, M. Kauer, Moritz Kellermann, J. L. Kelley, Ali Kheirandish, J. Kim, Ken'ichi Kin, T. Kintscher, J. Kiryluk, Ramesh Koirala, H. Kolanoski, L. Köpke, Claudio Kopper, S. Kopper, D. J. Koskinen, Paras Koundal, Michael Kovacevich, M. Kowalski, K. Krings, G. Krückl, N. Kulacz, N. Kurahashi, A. Kyriacou, Cristina Lagunas Gualda, J. L. Lanfranchi, M. J. Larson, Frederik Hermann Lauber, Jeffrey Lazar, Agnieszka Leszczyńska, Y. Li, Qinrui Liu, Elisa Lohfink, L. Lu, Francesco Lucarelli, Andrew Ludwig, William Luszczak, W. Y., J. Madsen, K. B. M. Mahn, Yuya Makino, P. Mallik, Sarah Mancina, Shivesh Mandalia, Ioana Codrina Mariş, R. Maruyama, K. Mase, Frank McNally, K. Meagher, Andrés Medina, Maximilian Meier, S. Meighen-Berger, J. Merz, Jessie Micallef, D. Mockler, G. Momenté, T. Montaruli, R. W. Moore, R. Morse, Marjon Moulai, Richard Naab, R. Nagai, Uwe Naumann, Jannis Necker, G. Neer, Le Viet Nguyen, Hans Niederhausen, M. U. Nisa, Sarah Nowicki, D. R. Nygren, A. Obertacke Pollmann, M. Oehler, A. Olivas, Erin O’Sullivan, Hershal Pandya, D. V. Pankova, N. Park, Grant Parker, Ek Narayan Paudel, P. Peiffer, C. Pérez de los Heros, Saskia Philippen, D. Pieloth, Sarah Pieper, A. Pizzuto, M. Plum, Yuriy Popovych, Alessio Porcelli, Maria Prado Rodriguez, P. B. Price, G. T. Przybylski, Christoph Raab, Amirreza Raissi, M. Rameez, K. Rawlins, I. C. Rea, Abdul Rehman, R. Reimann, M. Renschler, Giovanni Renzi, E. Resconi, Simeon Reusch, W. Rhode, M. Richman, Benedikt Riedel, S. Robertson, Gerrit Roellinghoff, Martin Rongen, C. Rott, T. Ruhe, D. Ryckbosch, Devyn Rysewyk Cantu, I. Safa, S. E. Sanchez Herrera, Alexander Sandrock, J. Sandroos, M. Santander, S. Sarkar, K. Satalecka, Maximilian Karl Scharf, Merlin Schaufel, H. Schieler, P. Schlunder, T. Schmidt, A. Schneider, Judith Schneider, Frank Schröder, L. Schumacher, S. Sclafani, D. Seckel, S. Seunarine, S. Shefali, M. Silva, B. Smithers, R. Snihur, Jan Soedingrekso, Dennis Soldin, G. M. Spiczak, C. Spiering, Juliana Stachurska, M. Stamatikos, Todor Stanev, Robert Stein, J. Stettner, A. Steuer, T. Stezelberger, R. G. Stokstad, N. L. Strotjohann, Thomas Stuttard, G. W. Sullivan, I. Taboada, F. Tenholt, S. Ter–Antonyan, S. Tilav, Franziska Tischbein, Kirsten Tollefson, Lenka Tomankova, Christoph Tönnis, S. Toscano, D. Tosi, Alexander Trettin, M. Tselengidou, C. F. Tung, A. Turcati, Roxanne Turcotte, Colin Turley, Jean Pierre Twagirayezu, B. Ty, E. Unger, Martin Unland Elorrieta, J. Vandenbroucke, D. van Eijk, N. van Eijndhoven, D. Vannerom, J. V. Santen, Stef Verpoest, M. Vraeghe, C. Walck, A. Wallace, N. Wandkowsky, T. B. Watson, Ch. Weaver, A. Weindl, Matthew J. Weiss, Jan Weldert, Chris Wendt, Johannes Werthebach, Mark Weyrauch, B. J. Whelan, N. Whitehorn, K. Wiebe, C. H. Wiebusch, D. R. Williams, Martin Wolf, T. R. Wood, K. Woschnagg, Gerrit Wrede, Johan Wilfried Wulff, Xiaolin Xu, Y. Xu, S. Yoshida, Tony Yuan, Z. Zhang

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of AlbertaSnolab
FundersJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of Polar ProgramsCollege of Engineering, Michigan State UniversityHelmholtz Alliance for Astroparticle PhysicsInstitute for Global Prominent Research, Chiba UniversityRWTH Aachen UniversityKnut och Alice Wallenbergs StiftelseFonds Wetenschappelijk OnderzoekCarlsbergfondetMarsden FundBundesministerium für Bildung und ForschungDanmarks GrundforskningsfondSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNational Science FoundationUK Research and InnovationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftUniversity of OxfordMarquette UniversityCanada Foundation for InnovationDeutsches Elektronen-SynchrotronNational Energy Research Scientific Computing CenterAustralian Research CouncilWestern Canada Research GridFonds De La Recherche Scientifique - FNRSPolarforskningssekretariatetUniversity of MarylandWisconsin Alumni Research FoundationNational Research Foundation of KoreaVillum FondenChiba UniversityRoyal SocietyCompute CanadaVetenskapsrådetU.S. Department of EnergyUniversity of Wisconsin-MadisonNational Research FoundationMichigan State University
KeywordsCharacterization (materials science)Event (particle physics)Sample (material)Flux (metallurgy)Environmental scienceComputer scienceAstrophysicsPhysicsMaterials scienceOpticsThermodynamics

Abstract

fetched live from OpenAlex

The IceCube Neutrino Observatory has established the existence of a high-energy all-sky neutrino flux of astrophysical origin. This discovery was made using events interacting within a fiducial region of the detector surrounded by an active veto and with reconstructed energy above 60 TeV, commonly known as the high-energy starting event sample (HESE). We revisit the analysis of the HESE sample with an additional 4.5 years of data, newer glacial ice models, and improved systematics treatment. This paper describes the sample in detail, reports on the latest astrophysical neutrino flux measurements, and presents a source search for astrophysical neutrinos. We give the compatibility of these observations with specific isotropic flux models proposed in the literature as well as generic power-law-like scenarios. Assuming ${\ensuremath{\nu}}_{e}:{\ensuremath{\nu}}_{\ensuremath{\mu}}:{\ensuremath{\nu}}_{\ensuremath{\tau}}=1:1:1$, and an equal flux of neutrinos and antineutrinos, we find that the astrophysical neutrino spectrum is compatible with an unbroken power law, with a preferred spectral index of ${2.87}_{\ensuremath{-}0.19}^{+0.20}$ for the 68% confidence interval.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.004
metaresearch head score (Gemma)0.008
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.008
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.008
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.004
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0060.003

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 head0.021
GPT teacher head0.350
Teacher spread0.329 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
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

Citations373
Published2021
Admission routes2
Has abstractyes

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