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Record W3216465877 · doi:10.1093/mnras/stab3402

The return of the spin period in DW Cnc and evidence of new high state outbursts

2021· preprint· en· W3216465877 on OpenAlexfundno aff
C Duffy, Gavin Ramsay, D. Steeghs, Mark Kennedy, R. G. West, P. J. Wheatley, V. S. Dhillon, K. Ackley, M. Dyer, D. K. Galloway, Samuel Gill, Jack S Acton, M. R. Burleigh, S. L. Casewell, M. R. Goad, Beth A Henderson, Rosanna H Tilbrook, P. A. Wilson, D. R. Anderson

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersDivision of Loan RepaymentDeutsches Elektronen-SynchrotronScience and Technology Facilities CouncilStockholms UniversitetTurun YliopistoIrish Research CouncilNational Astronomical Research Institute of ThailandUniversity of WarwickQueen's UniversityUniversity of LeicesterNational Science FoundationUniversity of WashingtonUniversité de GenèveUniversity of PortsmouthUniversity of CambridgeQueen's University BelfastUniversity of MarylandCalifornia Institute of Technology
KeywordsAmplitudePhysicsAccretion (finance)AstrophysicsPeriod (music)White dwarfPolarState (computer science)Spin (aerodynamics)Magnetorotational instabilityIntermediate polarAccretion discAstronomyMagnetic fieldStarsOpticsComputer scienceAcoustics

Abstract

fetched live from OpenAlex

ABSTRACT DW Cnc is an intermediate polar which has previously been observed in both high and low states. Observations of the high state of DW Cnc have previously revealed a spin period at ∼38.6 min, however, observations from the 2018 to 2019 low state showed no evidence of the spin period. We present results from our analysis of 12 s cadence photometric data collected by Next Generation Transit Survey of DW Cnc during the high state which began in 2019. Following the previously reported suppression of the spin period signal, we identify the return of this signal during the high state, consistent with previous observations of it. We identify this as the restarting of accretion during the high state. We further identified three short outbursts lasting ∼1 d in DW Cnc with a mean recurrence time of ∼60 d and an amplitude of ∼1 mag. These are the first outbursts identified in DW Cnc since 2008. Due to the short nature of these events, we identify them not as a result of accretion instabilities but instead either from instabilities originating from the interaction of the magnetorotational instability in the accretion disc and the magnetic field generated by the white dwarf or the result of magnetic gating.

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)0.001
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 score0.013
Threshold uncertainty score0.027

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
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 head0.015
GPT teacher head0.235
Teacher spread0.220 · 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

Citations1
Published2021
Admission routes1
Has abstractyes

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