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Record W4290055950 · doi:10.48550/arxiv.2208.02782

Panchromatic evolution of three luminous red novae: Forbidden hugs in pandemic times -- IV

2022· preprint· en· W4290055950 on OpenAlexfundno aff
A. Pastorello, G. Valerin, M. Fraser, A. Reguitti, N. Elias-Rosa, A. V. Filippenko, C. Rojas-Bravo, L. Tartaglia, T. M. Reynolds, S. Valenti, J. E. Andrews, C. Ashall, K. A. Bostroem, T. G. Brink, J. Burke, Yongzhi Cai, E. Cappellaro, D. A. Coulter, R. Dastidar, K. W. Davis, G. Dimitriadis, A. Fiore, R. J. Foley, D. Fugazza, L. Galbany, A. Gangopadhyay, S. Geier, C. P. Gutiérrez, J. Haislip, D. Hiramatsu, S. Holmbo, D. A. Howell, E. Y. Hsiao, T. Hung, S. W. Jha, E. Kankare, E. Karamehmetoglu, C. D. Kilpatrick, R. Kotak, V. Kouprianov, T. Kravtsov, S. Kumar, Z. -T. Li, M. Lundquist, Peter Lundqvist, K. Matilainen, P. A. Mazzali, C. McCully, K. Misra, A. Morales-Garoffolo, S. Moran, N. Morrell, Megan Newsome, Estefania Padilla Gonzalez, Y. -C. Pan, C. Pellegrino, M. M. Phillips, G. Pignata, A. L. Piro, D. E. Reichart, A. Rest, I. Salmaso, D. J. Sand, Matt Siebert, S. J. Smartt, K. W. Smith, Shubham Srivastav, M. Stritzinger, K. Taggart, Samaporn Tinyanont, S. -Y. Yan, L. Wang, X. -F. Wang, S. C. Williams, S. Wyatt, Tianzi Zhang, Thomas de Boer, K. C. Chambers, He Gao, E. A. Magnier

Bibliographic record

VenuearXiv (Cornell University) · 2022
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersEuropean Social FundPlanetary Science DivisionAgencia Estatal de InvestigaciónEuropean Regional Development FundSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryMax-Planck-Institut für AstronomieEötvös Loránd TudományegyetemStockholms UniversitetMinisterio de Ciencia e InnovaciónNuclear Safety and Security CommissionLos Alamos National LaboratoryUniversity of WashingtonJohns Hopkins UniversityMinistero dell’Istruzione, dell’Università e della RicercaChina Postdoctoral Science FoundationChinese Academy of SciencesSmithsonian InstitutionNational Natural Science Foundation of ChinaNational Science FoundationScience Foundation IrelandGordon and Betty Moore FoundationQueen's University BelfastChinese Academy of Sciences South America Center for AstronomyNational Central UniversityVillum FondenSpace Telescope Science InstituteDurham UniversityWashington Research FoundationQueen's UniversityNASA Exoplanet Science InstituteAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyAgencia Nacional de Investigación y DesarrolloDepartment of Science and Technology, Ministry of Science and Technology, IndiaDeutsches Elektronen-SynchrotronTencentCalifornia Institute of TechnologyNational Aeronautics and Space Administration
KeywordsAstrophysicsLight curvePhysicsBalmer seriesLuminosityAstronomySpectral lineEmission spectrumGalaxy

Abstract

fetched live from OpenAlex

We present photometric and spectroscopic data on three extragalactic luminous red novae (LRNe): AT2018bwo, AT2021afy, and AT2021blu. AT2018bwo was discovered in NGC45 (at 6.8 Mpc) a few weeks after the outburst onset. During the monitoring period, the transient reached a peak luminosity of 10^40 erg/s. AT2021afy, hosted by UGC10043 (49.2 Mpc), showed a double-peaked light curve, with the two peaks reaching a similar luminosity of 2.1(+-0.6)x10^41 erg/s. For AT2021blu in UGC5829, (8.6 Mpc), the pre-outburst phase was well-monitored by several photometric surveys, and the object showed a slow luminosity rise before the outburst. The light curve of AT2021blu was sampled with an unprecedented cadence until the object disappeared behind the Sun, and it was then recovered at late phases. The light curve of AT2021blu shows a double peak, with a prominent early maximum reaching a luminosity of 6.5x10^40 erg/s, which is half of that of AT2021afy. The spectra of AT2021afy and AT2021blu display the expected evolution for LRNe: a blue continuum dominated by prominent Balmer lines in emission during the first peak, and a redder continuum consistent with that of a K-type star with narrow absorption metal lines during the second, broad maximum. The spectra of AT2018bwo are markedly different, with a very red continuum dominated by broad molecular features in absorption. As these spectra closely resemble those of LRNe after the second peak, AT2018bwo was probably discovered at the very late evolutionary stages. This would explain its fast evolution and the spectral properties compatible with that of an M-type star. From the analysis of deep frames of the LRN sites years before the outburst, and considerations of the light curves, the quiescent progenitor systems of the three LRNe were likely massive, with primaries ranging from 13Mo for AT2018bwo, to 13-18Mo for AT2021blu, and over 40Mo for AT2021afy.

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)0.000
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 score0.003
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
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 head0.051
GPT teacher head0.189
Teacher spread0.138 · 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

Citations2
Published2022
Admission routes1
Has abstractyes

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