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Record W4307722352 · doi:10.1051/0004-6361/202244393

Forbidden hugs in pandemic times

2022· article· en· W4307722352 on OpenAlexafffund
Yongzhi Cai, A. Pastorello, M. Fraser, Xiaofeng Wang, A. V. Filippenko, A. Reguitti, Kishore C. Patra, V. P. Goranskij, E. A. Barsukova, Thomas G. Brink, N. Elias–Rosa, H. F. Stevance, WeiKang Zheng, Yi Yang, К. Атапин, S. Benetti, Thomas de Boer, S. Bose, J. Burke, Ralph Byrne, E. Cappellaro, K. C. Chambers, W.-L. Chen, Najmeh Emami, Hua Gao, D. Hiramatsu, D. A. Howell, M. E. Huber, E. Kankare, Patrick L. Kelly, R. Kotak, T. Kravtsov, V. Yu. Lander, Z.-T. Li, Chien-Cheng Lin, Peter Lundqvist, E. A. Magnier, E. A. Malygin, N. A. Maslennikova, K. Matilainen, P. A. Mazzali, C. McCully, J. Mo, S. Moran, Megan Newsome, Д. В. Опарин, Estefania Padilla Gonzalez, T. Reynolds, N. I. Shatsky, S. J. Smartt, K. Smith, M. Stritzinger, А. М. Татарников, G. Terreran, Р. И. Уклеин, G. Valerin, P. Vallely, O. V. Vozyakova, R. J. Wainscoat, Shengyu Yan, J.-J. Zhang, T.-M. Zhang, S. G. Zheltoukhov, Raya Dastidar, M. Fulton, L. Galbany, Anjasha Gangopadhyay, Hongwei Ge, C. P. Gutiérrez, H. Lin, Kuntal Misra, Z. W. Ou, I. Salmaso, L. Tartaglia, Lin Xiao, Xinpeng Zhang

Bibliographic record

VenueAstronomy and Astrophysics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsScience North
FundersLos Alamos National LaboratoryEuropean Social FundPlanetary Science DivisionYouth Innovation Promotion AssociationAgencia Estatal de InvestigaciónLeibniz-GemeinschaftScience Mission DirectorateMinistry of Science and Higher Education of the Russian FederationInstituto de Astrofísica de CanariasArizona Board of RegentsMax-Planck-Institut für AstronomieJet Propulsion LaboratoryLeibniz-Institut für Astrophysik PotsdamEötvös Loránd TudományegyetemAgencia Nacional de Investigación y DesarrolloStockholms UniversitetJohns Hopkins UniversityUniversitetet i OsloMinisterio de Ciencia e InnovaciónChinese Academy of SciencesGordon and Betty Moore FoundationQueen's University BelfastNational Science FoundationUniversity of MinnesotaAarhus UniversitetLiverpool John Moores UniversitySmithsonian InstitutionOhio State UniversityNational Natural Science Foundation of ChinaTurun YliopistoSmithsonian Astrophysical ObservatoryPeople's Government of Yunnan ProvinceHáskóli ÍslandsNational Central UniversityQueen's UniversityVillum FondenUniversity of Notre DameHebei UniversityCalifornia Institute of TechnologyScience and Technology Facilities CouncilAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyNuclear Safety and Security CommissionW. M. Keck FoundationDepartment of Science and Technology, Ministry of Science and Technology, IndiaSpace Telescope Science InstituteNational Aeronautics and Space AdministrationIstituto Nazionale di AstrofisicaDurham University
KeywordsPhysicsAstrophysicsPandemicAstronomyCoronavirus disease 2019 (COVID-19)Medicine

Abstract

fetched live from OpenAlex

We present an observational study of the luminous red nova (LRN) AT 2021biy in the nearby galaxy NGC 4631. The field of the object was routinely imaged during the pre-eruptive stage by synoptic surveys, but the transient was detected only at a few epochs from ∼231 days before maximum brightness. The LRN outburst was monitored with unprecedented cadence both photometrically and spectroscopically. AT 2021biy shows a short-duration blue peak, with a bolometric luminosity of ∼1.6 × 10 41 erg s −1 , followed by the longest plateau among LRNe to date, with a duration of 210 days. A late-time hump in the light curve was also observed, possibly produced by a shell-shell collision. AT 2021biy exhibits the typical spectral evolution of LRNe. Early-time spectra are characterised by a blue continuum and prominent H emission lines. Then, the continuum becomes redder, resembling that of a K-type star with a forest of metal absorption lines during the plateau phase. Finally, late-time spectra show a very red continuum ( T BB ≈ 2050 K) with molecular features (e.g., TiO) resembling those of M-type stars. Spectropolarimetric analysis indicates that AT 2021biy has local dust properties similar to those of V838 Mon in the Milky Way Galaxy. Inspection of archival Hubble Space Telescope data taken on 2003 August 3 reveals a ∼20 M ⊙ progenitor candidate with log ( L / L ⊙ ) = 5.0 dex and T eff = 5900 K at solar metallicity. The above luminosity and colour match those of a luminous yellow supergiant. Most likely, this source is a close binary, with a 17–24 M ⊙ primary component.

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)0.000
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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.032
Threshold uncertainty score0.107

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0020.001
Scholarly communication0.0020.001
Open science0.0000.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0320.003

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 head0.009
GPT teacher head0.213
Teacher spread0.204 · 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".

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Citations23
Published2022
Admission routes2
Has abstractyes

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