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Record W4411904599 · doi:10.1051/0004-6361/202553823

GOTO065054+593624: An 8.5 mag amplitude dwarf nova identified in real time via Kilonova Seekers

2025· article· en· W4411904599 on OpenAlexaff
T. Killestein, Gavin Ramsay, M. Kennedy, L Kelsey, D. Steeghs, S. P. Littlefair, B. Godson, J. Lyman, M. Pursiainen, B. Warwick, Coleman Krawczyk, L. K. Nuttall, E. G. Wickens, Svetoslav Alexandrov, Cledison Marcos da Silva, R. Leadbeater, K. Ackley, M. Dyer, F. Jiménez-Ibarra, K. Ulaczyk, D. K. Galloway, V. S. Dhillon, P. T. O’Brien, K. Noysena, R. Kotak, R. P. Breton, Ε. Πάλλη, D. Pollacco, Amit Kumar, D.H. O’Neill, T. Butterley, Richard Wilson, S. Mattila, A. Sahu, R. L. C. Starling, Chi‐Yun Wang, Qifa Liu, J. Li, Zhibin Dai, Huanbo Feng, Wei Yuan, R. Billington, Aline Bull, S. Gaudenzi, V. Gonano, H. Krawczyk, M. Mazzucato, Antonio Pasqua, José A. da Silva Campos, M. Torres-Guerrero, N. N. Antonov, S J Bean, E. T. Boeneker, Stephen M. Brincat, Graham Darlington, Franky Dubois, Franz-Josef Hambsch, David Messier, A. Oksanen, G. Poyner, F. D. Romanov, Ian D. Sharp, T. Tordai, Tonny Vanmunster, Klaus Wenzel

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsSaint Mary's University
FundersInstituto de Astrofísica de CanariasUniversitetet i OsloHáskóli ÍslandsNational Science FoundationUK Research and InnovationLiverpool John Moores UniversityChinese Academy of SciencesCentre National d’Etudes SpatialesUniversity of PortsmouthStockholms UniversitetScience and Technology Facilities CouncilNational Astronomical Research Institute of ThailandAarhus UniversitetTurun YliopistoAcademy of FinlandEuropean CommissionTurun YliopistosäätiöIsaac Newton TrustUniversity of LeicesterMonash UniversityLeverhulme TrustPeople's Government of Yunnan ProvinceSmithsonian InstitutionAlfred P. Sloan FoundationUniversity of Warwick
KeywordsPhysicsAstrophysicsDwarf novaNova (rocket)KilonovaAmplitudeAstronomyEjectaWhite dwarfStarsSupernovaOptics

Abstract

fetched live from OpenAlex

Dwarf novae are astrophysical laboratories for probing the nature of accretion, binary mass transfer, and binary evolution, but their diverse observational characteristics continue to challenge our theoretical understanding. We here present the discovery of and subsequent observing campaign on GOTO065054+593624 (hereafter GOTO0650), a dwarf nova of the WZ Sge type that was discovered in real-time by citizen scientists via the Kilonova Seekers citizen science project. The nova has an outburst amplitude of 8.5 mag. An extensive dataset charts the photometric and spectroscopic evolution of this object, and it covers the 2024 superoutburst. GOTO0650 shows an absence of visible emission lines during the high state, strong H and barely detected He II emission, and high-amplitude echo outbursts on a rapidly decreasing timescale. The comprehensive dataset we present marks GOTO0650 as a candidate period bouncer, and it highlights the important contribution made by citizen scientists to the study of Galactic transients.

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 score0.013
Threshold uncertainty score0.026

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)0.0020.001

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 head0.011
GPT teacher head0.248
Teacher spread0.237 · 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

Citations4
Published2025
Admission routes1
Has abstractyes

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