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Record W4393405288 · doi:10.1051/0004-6361/202449600

The orbital parameters of the<i>δ</i>Cep inner binary system determined using 2019 HARPS-N spectroscopic data

2024· article· en· W4393405288 on OpenAlexfundno aff
N. Nardetto, V. Hocdé, P. Kervella, A. Gallenne, W. Gieren, D. Graczyk, A. Mérand, M. Rainer, J. Storm, G. Pietrzyński, B. Pilecki, E. Poretti, M. Bailleul, Garance Bras, Anton V. Afanasiev

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersEuropean Research CouncilInstituto MilleniumCentre National de la Recherche ScientifiqueAgencia Nacional de Investigación y DesarrolloNational Aeronautics and Space AdministrationEuropean Space AgencyAgence Nationale de la RechercheEuropean CommissionWorkplace Safety and Insurance Board
KeywordsPhysicsRadial velocityAstrophysicsOrbital periodCepheid variableOrbital elementsOrbital inclinationBinary starContext (archaeology)Binary numberStars

Abstract

fetched live from OpenAlex

Context.An inner companion has recently been discovered orbiting the prototype of classical Cepheids,δCep, whose orbital parameters are still not fully constrained. Aims.We collected new precise radial velocity measurements ofδCep in 2019 using the HARPS-N spectrograph mounted at the Telescopio NazionaleGalileo. Using these radial velocity measurements, we aimed to improve the orbital parameters of the system. Methods.We considered a template available in the literature as a reference for the radial velocity curve of the pulsation of the star. We then calculated the residuals between our global dataset (composed of the new 2019 observations plus data from the literature) and the template as a function of the pulsation phase and the barycentric Julian date. This provides the orbital velocity of the Cepheid component. Using a Bayesian tool, we derived the orbital parameters of the system. Results.Considering priors based on already publishedGaiaconstraints, we find for the orbital period a maximum a posteriori probability ofPorb = 9.32−0.04+0.03years (uncertainties correspond to the 95% highest density probability interval), and we obtain an eccentricitye = 0.71−0.02+0.02, a semimajor axisa = 0.029−0.003+0.002arcsec, and a center-of-mass velocityV0 = −17.28−0.08+0.08km s−1, among other parameters. Conclusions.In this short analysis we derive the orbital parameters of theδCep inner binary system and provide a cleaned radial velocity curve of the pulsation of the star, which will be used to study its Baade–Wesselink projection factor in a future publication.

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 score0.004
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.016
GPT teacher head0.229
Teacher spread0.213 · 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
Published2024
Admission routes1
Has abstractyes

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