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Record W4416133912 · doi:10.3847/1538-3881/ae0e0d

NGTS-EB-8: A Double-lined Eclipsing M+M Binary Discovered by Citizen Scientists

2025· article· en· W4416133912 on OpenAlexfundno aff
Sean O'Brien, Megan E. Schwamb, C. A. Watson, Louise D. Nielsen, Edward M. Bryant, S. L. Casewell, M. R. Burleigh, L. Fortson, Samuel Gill, Chris Lintott, K. Hobbs, Ioannis Apergis, Daniel Bayliss, Jorge Fernández Fernández, Maximilian N. Günther, Faith Hawthorn, J. S. Jenkins, Alicia Kendall, J. McCormac, Ernst de Mooij, Toby Rodel, Suman Saha, Laura Trouille, R. G. West, P. J. Wheatley, Marius Constantin Agafitei, Deniz Rüzgar Apaydın, Elisabeth Baeten, B. Baller, Jeff Carabott, Sallyann Chesson, Sebastián A. Freigeiro, Virgilio Gonano, Pete Hermes, John S. Langley, S. M. Lim, Graham Mitchell, Nolan Reket, Jeanne Riethmiller, Juergen Saeftel, Arttu Sainio, Christopher Tanner, Ivan A. Terentev, Ernest Jude P. Tiu, Sergey Y. Tumanov, Marciniak Urszula, Pia Vahlenkamp, Femke de Vroome, Paweł Wantuch

Bibliographic record

VenueThe Astronomical Journal · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersAustralian Astronomical Optics-MacquarieScience and Technology Facilities CouncilAgencia Estatal de InvestigaciónScience Mission DirectorateUniversity of California, Los AngelesJet Propulsion LaboratoryAgencia Nacional de Investigación y DesarrolloMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesSpace Telescope Science InstituteKorea Astronomy and Space Science InstituteEuropean Southern ObservatoryQueen's University BelfastSwinburne University of TechnologyNational Cancer InstituteNuclear Safety and Security CommissionMonash UniversityQueen's UniversityAustralian GovernmentNASA Exoplanet Science InstituteNational Computational InfrastructureGoddard Space Flight CenterEuropean Space AgencyAlfred P. Sloan FoundationAustralian National Data ServiceAstronomy Australia LimitedAustralian National UniversityNational Aeronautics and Space AdministrationAmes Research CenterCurtin University of TechnologyCalifornia Institute of TechnologyNational Science FoundationUK Research and InnovationUniversity of WarwickInstitute of Museum and Library Services
KeywordsBalmer seriesStarsPlanetBinary starTransit (satellite)Binary numberFlareLine (geometry)

Abstract

fetched live from OpenAlex

Abstract We report the identification and characterization of a new binary system composed of two near-equal mass M-dwarfs. The binary NGTS-EB-8 was identified as a planet candidate in data from the Next Generation Transit Survey (NGTS) by citizen scientists participating in the Planet Hunters NGTS project. High-resolution spectroscopic observations reveal the system to be a double-lined binary. By modeling the photometric and radial velocity observations, we determine an orbital period of 4.2 days and the masses and radii of both stars to be M A = 0.25 0 − 0.004 + 0.005 M ⊙ , M B = 0.20 8 − 0.004 + 0.005 M ⊙ , and R A = 0.25 5 − 0.005 + 0.004 R ⊙ , R B = 0.23 3 − 0.005 + 0.006 R ⊙ , respectively. We detect Balmer line emission from at least one of the stars but no significant flare activity. We note that both components lie in the fully convective regime of low-mass stars (≲0.35 M ⊙ ); therefore, they can be a valuable test for stellar evolutionary models. We demonstrate that the photometric observations, speckle imaging, and initial radial velocity measurements were unable to identify the true nature of this system and highlight that high-resolution spectroscopic observations are crucial in determining whether systems such as this are in fact binaries.

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 score0.003
Threshold uncertainty score0.010

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)0.0030.001

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 head0.010
GPT teacher head0.251
Teacher spread0.240 · 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
Published2025
Admission routes1
Has abstractyes

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