MétaCan
Menu
Back to cohort
Record W1552565640 · doi:10.1088/0004-637x/811/1/52

THE DETECTION OF A SN IIn IN OPTICAL FOLLOW-UP OBSERVATIONS OF ICECUBE NEUTRINO EVENTS

2015· article· en· W1552565640 on OpenAlexafffund
M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, M. Archinger, C. Argüelles, T. C. Arlen, J. Auffenberg, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. H. Becker, E. Beiser, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Böhm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H.-P. Bretz, A. M. Brown, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, B. Christy, K. Clark, Lew Classen, S. Coenders, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, H.-P. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz–Vélez, J. P. Dumm, M. Dunkman, R. Eagan, B. Eberhardt, Thomas Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, O. Fadiran, S. Fahey, A. R. Fazely, Anatoli Fedynitch, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, T. Fischer-Wasels, S. Flis, T. Fuchs, M. Glagla, T. K. Gaisser, R. Gaïor, J. S. Gallagher, L. Gerhardt, K. Ghorbani, D. Gier, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. González, D. Góra, D. Grant, P. Gretskov, J. C. Groh, A. Groß, C. Ha, Christian Haack, A. Haj Ismail, A. Hallgren, F. Halzen, B. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, D. Hellwig, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfe, A. Homeier, K. Hoshina, F. Huang, M. E. Huber, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, K. Jero, M. Jurković, B. Kaminsky, A. Kappes, T. Karg, A. Karle, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, Ali Kheirandish, J. Kiryluk, J. Kläs, G. Kohnen, Ramesh Koirala, H. Kolanoski, R. Konietz, A. Koob, L. Köpke, Claudio Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Kroll, M. Kroll, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, E. Middlemas, J. Miller, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, Uwe Naumann, Hans Niederhausen, Sarah Nowicki, D. R. Nygren, A. Obertacke, A. Olivas, A. Omairat, A. O’Murchadha, T. Palczewski, Hershal Pandya, L. Paul, Joshua Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, J. Pütz, M. Quinnan, L. Rädel, M. Rameez, K. Rawlins, P. Redl, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, S. Richter, Benedikt Riedel, S. Robertson, Martin Rongen, C. Rott, T. Ruhe, D. Ryckbosch, S. M. Saba, L. Sabbatini, H.‐G. Sander, Alexander Sandrock, J. Sandroos, S. Sarkar, K. Schatto, F. Scheriau, M. Schimp, T. Schmidt, M. Schmitz, S. Schoenen, S. Schöneberg, A. Schönwald, A. Schukraft, L. Schulte, D. Seckel, S. Seunarine, R. Shanidze, M. W. E. Smith, Dennis Soldin, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, Todor Stanev, N. A. Stanisha, A. Stasik, T. Stezelberger, R. G. Stokstad, A. Stössl, E. A. Strahler, L. R. Strom, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, S. Ter–Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, N. van Eijndhoven, J. Vandenbroucke, J. V. Santen, S. Vanheule, J. Veenkamp, M. Vehring, M. Vöge, M. Vraeghe, C. Walck, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, N. Whitehorn, C. Wichary, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, Xiaolin Xu, Yi Xu, G. Yodh, S. Yoshida, P. Zarzhitsky, M. Zoll, E. O. Ofek, M. M. Kasliwal, P. Nugent, I. Arcavi, J. S. Bloom, S. R. Kulkarni, D. A. Perley, Tom A. Barlow, A. Horesh, A. Gal‐Yam, D. A. Howell, B. Dilday, P. A. Evans, J. A. Kennea, W. S. Burgett, K. C. Chambers, N. Kaiser, C. Waters, H. Flewelling, J. Tonry, A. Rest, S. J. Smartt

Bibliographic record

VenueThe Astrophysical Journal · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of TorontoUniversity of Alberta
FundersLawrence Berkeley National LaboratoryBrookhaven National LaboratoryPlanetary Science DivisionPlanning and Budgeting Committee of the Council for Higher Education of IsraelScience Mission DirectorateSmithsonian Astrophysical ObservatoryOffice of ScienceOffice of Polar ProgramsMax-Planck-Institut für AstronomieMarsden FundHelmholtz Alliance for Astroparticle PhysicsEötvös Loránd TudományegyetemCollege of Engineering, Michigan State UniversityKnut och Alice Wallenbergs StiftelseIsrael Science FoundationNatural Sciences and Engineering Research Council of CanadaBundesministerium für Bildung und ForschungNational Central UniversityOhio State UniversityNational Research Foundation of KoreaFonds De La Recherche Scientifique - FNRSDeutsche ForschungsgemeinschaftQueen's University BelfastNational Research FoundationVlaamse regeringWeizmann Institute of ScienceUniversity of OxfordUniversity of LeicesterDurham UniversityScience and Technology Facilities CouncilSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungYork UniversitySpace Telescope Science InstituteWestern Canada Research GridJapan Society for the Promotion of ScienceQueen's UniversityHarvard UniversityPolarforskningssekretariatetCarnegie Mellon UniversityUniversity of WashingtonPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityVetenskapsrådetIsraeli Centers for Research ExcellenceYale UniversityUniversity of Wisconsin-MadisonU.S. Department of EnergySmithsonian InstitutionCalifornia Institute of TechnologyDanmarks GrundforskningsfondNational Aeronautics and Space AdministrationW. M. Keck FoundationUniversity of PortsmouthNew Mexico State UniversityFonds Wetenschappelijk OnderzoekVanderbilt UniversityCompute CanadaBelgian Federal Science Policy OfficeNational Science Foundation
KeywordsPhysicsNeutrinoSupernovaAstrophysicsRedshiftLuminosityEjectaGalaxyObservatoryGamma-ray burstNeutrino astronomyNeutrino detectorAstronomyNeutrino oscillationParticle physics

Abstract

fetched live from OpenAlex

The IceCube neutrino observatory pursues a follow-up program selecting interesting neutrino events in real-time and issuing alerts for electromagnetic follow-up observations. In 2012 March, the most significant neutrino alert during the first three years of operation was issued by IceCube. In the follow-up observations performed by the Palomar Transient Factory (PTF), a Type IIn supernova (SN IIn) PTF12csy was found 0 2 away from the neutrino alert direction, with an error radius of 0 54. It has a redshift of z = 0.0684, corresponding to a luminosity distance of about 300 Mpc and the Pan-STARRS1 survey shows that its explosion time was at least 158 days (in host galaxy rest frame) before the neutrino alert, so that a causal connection is unlikely. The a posteriori significance of the chance detection of both the neutrinos and the SN at any epoch is 2.2 σ within IceCube's 2011/12 data acquisition season. Also, a complementary neutrino analysis reveals no long-term signal over the course of one year. Therefore, we consider the SN detection coincidental and the neutrinos uncorrelated to the SN. However, the SN is unusual and interesting by itself: it is luminous and energetic, bearing strong resemblance to the SN IIn 2010jl, and shows signs of interaction of the SN ejecta with a dense circumstellar medium. High-energy neutrino emission is expected in models of diffusive shock acceleration, but at a low, non-detectable level for this specific SN. In this paper, we describe the SN PTF12csy and present both the neutrino and electromagnetic data, as well as their analysis.

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)0.001
metaresearch head score (Gemma)0.001
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: Empirical
Teacher disagreement score0.015
Threshold uncertainty score0.030

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.024
GPT teacher head0.241
Teacher spread0.217 · 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

Citations49
Published2015
Admission routes2
Has abstractyes

Explore more

Same venueThe Astrophysical JournalSame topicAstrophysics and Cosmic PhenomenaFrench-language works237,207