MétaCan
Menu
Back to cohort
Record W4415337528 · doi:10.5303/jkas.2025.58.2.209

The Outbursting YSOs Catalogue (OYCAT)

2025· article· en· W4415337528 on OpenAlexfundaboutno aff
Carlos Contreras Peña, Jeong‐Eun Lee, G. J. Herczeg, Doug Johnstone, P. Ábrahám, S. Antoniucci, M. Audard, Muhammad Ashraf, Giseon Baek, A. Caratti o Garatti, Airton Torres Carvalho, Lucas A. Cieza, Fernando Cruz-Sáenz de Miera, J. Eislöffel, D. Froebrich, T. Giannini, J. Green, Arindam Ghosh, Zhe Guo, L. Hillenbrand, K. W. Hodapp, H. Jheonn, J. José, Yongman Kim, Á. Kóspál, Hyung-Ik Lee, P. W. Lucas, T. Yu. Magakian, Z. Nagy, T. Naylor, Joe P. Ninan, S. Peneva, Bo Reipurth, A. Scholz, E. Semkov, A. Sicilia-Aguilar, Krishna Kant Singh, M. Siwak, B. Stecklum, Zsófia Marianna Szabó, V. Wolf, Sehyoun Yoon

Bibliographic record

VenueKent Academic Repository (University of Kent) · 2025
Typearticle
Languageen
FieldEarth and Planetary Sciences
TopicGeophysics and Gravity Measurements
Canadian institutionsnot available
FundersUniversity of California, Los AngelesNatural Sciences and Engineering Research Council of CanadaMinistry of Science and ICT, South KoreaNational Research, Development and Innovation OfficeInternational Max Planck Research School for Advanced Methods in Process and Systems EngineeringNemzeti Kutatási Fejlesztési és Innovációs HivatalMagyar Tudományos AkadémiaAgencia Nacional de Investigación y DesarrolloNational Research Foundation of KoreaCalifornia Institute of TechnologyEuropean CommissionSeoul National UniversityNational Natural Science Foundation of ChinaNational Research FoundationInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyJet Propulsion LaboratoryChinese Academy of Sciences South America Center for AstronomyNational Aeronautics and Space AdministrationNemzeti Kutatási, Fejlesztési és Innovaciós AlapHungarian Scientific Research FundUniversity of St Andrews
KeywordsGovernment (linguistics)ExcellenceScholarshipChinaCenter of excellenceResearch centerAccretion (finance)

Abstract

fetched live from OpenAlex

Funding: C.C.P. was supported by the National Research Foundation of Korea (NRF) grant funded by the Korean government (MEST) (No. 2019R1A6A1A10073437). J.E.L. was supported by the New Faculty Startup Fund from Seoul National University and the NRF grant funded by the Korean government (MSIT) (grant number 2021R1A2C1011718 and RS-2024-00416859). GJH is supported by the National Key R&D program of China 2022YFA1603102 and by general grant 12173003 from the National Natural Science Foundation of China. D.J. is supported by NRC Canada and by an NSERC Discovery Grant. A.K. was supported by the NKFIH excellence grant TKP2021-NKTA-64. Zs.N. acknowledges the Hungarian National Research, Development and Innovation Office grant OTKA FK 146023. Zs.N. was supported by the János Bolyai Research Scholarship of the Hungarian Academy of Sciences. Zs.N. acknowledges support from the ESA PRODEX contract No. 4000132054. Zs.M.Sz. acknowledges funding from a St. Leonards scholarship from the University of St. Andrews. Zs.M.Sz. is a member of the International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne. A.C.G. acknowledges support from PRIN-MUR 2022 20228JPA3A “The path to star and planet formation in the JWST era (PATH)” funded by NextGeneration EU and by INAF-GoG 2022 “NIR-dark Accretion Outbursts in Massive Young stellar objects (NAOMY)” and Large Grant INAF 2022 “YSOs Outflows, Disks and Accretion: towards a global framework for the evolution of planet forming systems (YODA)”. F.C.S.M. received financial support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (ERC Starting Grant “Chemtrip”, grant agreement No 949278). G.B was supported by Basic Science Research Program through the National Research Foundation ofKorea(NRF) funded by the Ministry of Education(grant number RS-2023-00247790). Z.G. is funded by ANID, Millennium Science Initiative, AIM23-001. Z.G. is supported by the China-Chile Joint Research Fund (CCJRF No.2301) and Chinese Academy of Science South America Center for Astronomy (CASSACA) Key Research Project E52H540301. This work was also supported by the NKFIHNKKPgrantADVANCED149943. Project no.149943 has been implemented with the support provided by the Ministry of Culture and Innovation of Hungary from the National Research, Development and Innovation Fund, financed under the NKKP ADVANCED funding scheme.

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)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Dataset · Consensus signal: Dataset
Teacher disagreement score0.052
Threshold uncertainty score0.173

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0020.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0070.007
Science and technology studies0.0010.000
Scholarly communication0.0030.002
Open science0.0020.003
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0520.081

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 head0.012
GPT teacher head0.191
Teacher spread0.180 · 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 designNot applicable
Domainnot available
GenreDataset

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

Citations7
Published2025
Admission routes2
Has abstractyes

Explore more

Same venueKent Academic Repository (University of Kent)Same topicGeophysics and Gravity MeasurementsFrench-language works237,207