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Record W3109078977

Two Young Planetary Systems around Field Stars with Ages between 20 and 320 Myr from TESS

2020· article· en· W3109078977 on OpenAlexaff
George Zhou, Samuel N. Quinn, Jonathan Irwin, Chelsea X. Huang, Karen A. Collins, Luke G. Bouma, Lamisha Khan, Anaka Landrigan, Andrew Vanderburg, Joseph E. Rodriguez, David W. Latham, Guillermo Torres, Stephanie T. Douglas, Allyson Bieryla, Gilbert A. Esquerdo, P. Berlind, M. Calkins, Lars A. Buchhave, David Charbonneau, Kevin I. Collins, John F. Kielkopf, R. Hart, Brad Carter, Chris Stockdale, Carl Ziegler, Nicholas M. Law, Andrew W. Mann, Steve B. Howell, Rachel A. Matson, Nicholas J. Scott, Elise Furlan, R. J. White, C. Hellier, D. R. Anderson, R. G. West, G. Ricker, R. Vanderspek, Sara Seager, Jon M. Jenkins, Joshua N. Winn, Ismael Mireles, Pamela Rowden, Daniel A. Yahalomi, Bill Wohler, C. E. Brasseur, Tansu Daylan, Knicole D. Colón

Bibliographic record

VenueUniversity of Southern Queensland ePrints (University of Southern Queensland) · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
Fundersnot available
KeywordsPhysicsmyrStarsPlanetary systemAstronomyAstrophysicsField (mathematics)Astrobiology
DOInot available

Abstract

fetched live from OpenAlex

Planets around young stars trace the early evolution of planetary systems. We report the discovery and validation of two planetary systems with ages ≲300 Myr from observations by the Transiting Exoplanet Survey Satellite (TESS). The Myr old G star TOI-251 hosts a mini-Neptune with a day period. The Myr old K star TOI-942 hosts a system of inflated Neptune-sized planets, with TOI-942b orbiting in a period of days with a radius of and TOI-942c orbiting in a period of days with a radius of . Though we cannot place either host star into a known stellar association or cluster, we can estimate their ages via their photometric and spectroscopic properties. Both stars exhibit significant photometric variability due to spot modulation, with measured rotation periods of ∼3.5 days. These stars also exhibit significant chromospheric activity, with age estimates from the chromospheric calcium emission lines and X-ray fluxes matching that estimated from gyrochronology. Both stars also exhibit significant lithium absorption, similar in equivalent width to well-characterized young cluster members. TESS has the potential to deliver a population of young planet-bearing field stars, contributing significantly to tracing the properties of planets as a function of their age.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.392
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.012
GPT teacher head0.171
Teacher spread0.160 · 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 teacher head, not a consensus.

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

Citations50
Published2020
Admission routes1
Has abstractyes

Explore more

Same venueUniversity of Southern Queensland ePrints (University of Southern Queensland)Same topicStellar, planetary, and galactic studiesFrench-language works237,207