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Record W3190009545 · doi:10.1093/mnras/stab2313

TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet

2021· article· en· W3190009545 on OpenAlexaff
Ares Osborn, D. J. Armstrong, Bryson Cale, Rafael Brahm, Robert A. Wittenmyer, Fei Dai, Ian J. M. Crossfield, Edward M. Bryant, V. Adibekyan, Ryan Cloutier, Karen A. Collins, E. Delgado Mena, M. Fridlund, C. Hellier, Steve B. Howell, George W. King, J. Lillo-Box, Jon Otegi, S. G. Sousa, Keivan G. Stassun, Elisabeth C. Matthews, Carl Ziegler, G. Ricker, R. Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Jack S Acton, Brett Addison, D. R. Anderson, Sarah Ballard, D. Barrado, S. C. C. Barros, Natalie M. Batalha, Daniel Bayliss, Thomas Barclay, Björn Benneke, John Berberian, F. Bouchy, Brendan P. Bowler, César Briceño, Christopher J. Burke, M. R. Burleigh, S. L. Casewell, David R. Ciardi, Kevin I. Collins, Benjamin F Cooke, O. D. S. Demangeon, R. F. Díaz, Caroline Dorn, Diana Dragomir, Courtney D. Dressing, X. Dumusque, Néstor Espinoza, P. Figueira, Benjamin J. Fulton, Elise Furlan, Eric Gaidos, Claire Geneser, Samuel Gill, M. R. Goad, Erica J. Gonzales, Varoujan Gorjian, Maximilian N. Günther, Ravit Helled, Beth A Henderson, Thomas Henning, Aleisha Hogan, S. Hojjatpanah, Jonathan Horner, Andrew W. Howard, S. Hoyer, Daniel Huber, Howard Isaacson, J. S. Jenkins, Eric L. N. Jensen, Andrés Jordán, Stephen R. Kane, Richard C. Kidwell, John F. Kielkopf, Nicholas M. Law, M. Lendl, Mikkel N. Lund, Rachel A. Matson, Andrew W. Mann, J. McCormac, Matthew W. Mengel, Farisa Y. Morales, Louise D. Nielsen, Jack Okumura, H. P. Osborn, Erik A. Petigura, Peter Plavchan, D. Pollacco, Elisa V. Quintana, Liam Raynard, Paul Robertson, Mark E. Rose, Arpita Roy, Michael Reefe, A. Santerne, N. C. Santos, P. Sarkis, Joshua E. Schlieder, Richard P. Schwarz, Nicholas J. Scott, Avi Shporer, A. M. S. Smith, C. Stibbard, Chris Stockdale, P. A. Wilson, Joseph D. Twicken, Thiam-Guan Tan, Angelle Tanner, Johanna Teske, Rosanna H Tilbrook, C. G. Tinney, S. Udry, J. Villaseñor, José I Vines, Sharon X. Wang, Lauren M. Weiss, R. G. West, P. J. Wheatley, D. J. Wright, Hui Zhang, Farzaneh Zohrabi

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversité de MontréalCanadian Institute for Theoretical AstrophysicsUniversity of TorontoBanting Research Foundation
FundersFondo Nacional de Desarrollo Científico y TecnológicoNuclear Fuel Cycle and Supply ChainScience and Technology Facilities CouncilJet Propulsion LaboratoryAmes Research CenterGeorge Mason UniversityFederación Española de Enfermedades RarasAgencia Nacional de Investigación y DesarrolloNanjing UniversityFundação para a Ciência e a TecnologiaCentre National d’Etudes SpatialesNuclear Safety and Security CommissionUniversity of Southern QueenslandAustralian Research CouncilKorea Astronomy and Space Science InstituteUniversity of LouisvilleEuropean Southern ObservatorySpace Telescope Science InstituteUniversity of Hawai'iUniversity of Texas at AustinMichigan State UniversityCollege of Engineering, Michigan State UniversityEuropean Space AgencyNational Science FoundationUniversity of North Carolina at Chapel HillNational Research Council Sri LankaMinistério da Ciência, Tecnologia e InovaçãoComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyAgencia Estatal de InvestigaciónUniversity of New South WalesSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungUniversity of Florida
KeywordsPhysicsNeptunePlanetAstronomyAstrobiologySuper-EarthAstrophysicsEarth (classical element)Exoplanet

Abstract

fetched live from OpenAlex

ABSTRACT We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and radial velocities (RVs). We estimate the stellar rotation period to be 30.5 ± 0.7 d using archival photometry and RVs. Transiting Exoplanet Survey Satellite (TESS) objects of Interest (TOI)-431 b is a super-Earth with a period of 0.49 d, a radius of 1.28 ± 0.04 R⊕, a mass of 3.07 ± 0.35 M⊕, and a density of 8.0 ± 1.0 g cm−3; TOI-431 d is a sub-Neptune with a period of 12.46 d, a radius of 3.29 ± 0.09 R⊕, a mass of $9.90^{+1.53}_{-1.49}$ M⊕, and a density of 1.36 ± 0.25 g cm−3. We find a third planet, TOI-431 c, in the High Accuracy Radial velocity Planet Searcher RV data, but it is not seen to transit in the TESS light curves. It has an Msin i of $2.83^{+0.41}_{-0.34}$ M⊕, and a period of 4.85 d. TOI-431 d likely has an extended atmosphere and is one of the most well-suited TESS discoveries for atmospheric characterization, while the super-Earth TOI-431 b may be a stripped core. These planets straddle the radius gap, presenting an interesting case-study for atmospheric evolution, and TOI-431 b is a prime TESS discovery for the study of rocky planet phase curves.

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 score0.010
Threshold uncertainty score0.019

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 head0.007
GPT teacher head0.177
Teacher spread0.170 · 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

Citations45
Published2021
Admission routes1
Has abstractyes

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