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Record W2598539591 · doi:10.3847/1538-3881/aa63e9

1–2.4 μm Near-IR Spectrum of the Giant Planet β Pictoris b Obtained with the Gemini Planet Imager

2017· article· en· W2598539591 on OpenAlexafffund
Jeffrey Chilcote, Laurent Pueyo, Robert J. De Rosa, Jeffrey Vargas, Bruce Macintosh, Vanessa P. Bailey, Travis Barman, Brian Bauman, Sebastian Bruzzone, J. Bulger, Adam Burrows, Andrew Cardwell, Christine Chen, Tara Cotten, Daren Dillon, René Doyon, Zachary H. Draper, Gaspard Duchêne, Jennifer Dunn, Darren Erikson, Michael P. Fitzgerald, Katherine B. Follette, Donald T. Gavel, Stephen J. Goodsell, James R. Graham, Alexandra Z. Greenbaum, Markus Hartung, Pascale Hibon, Li-Wei Hung, Patrick Ingraham, Paul Kalas, Quinn Konopacky, James E. Larkin, Jérôme Maîre, Franck Marchis, Mark S. Marley, Christian Marois, Stanimir Metchev, Maxwell A. Millar‐Blanchaer, Katie M. Morzinski, E. Nielsen, Andrew Norton, Rebecca Oppenheimer, D. M. Palmer, Jennifer Patience, Marshall D. Perrin, Lisa Poyneer, Abhijith Rajan, Julien Rameau, Fredrik T. Rantakyrö, Naru Sadakuni, Leslie Saddlemyer, Dmitry Savransky, Adam C. Schneider, Andrew Serio, Anand Sivaramakrishnan, Inseok Song, Rémi Soummer, Sandrine Thomas, J. Kent Wallace, Jason Wang, Kimberly Ward-Duong, Sloane Wiktorowicz, Schuyler Wolff

Bibliographic record

VenueThe Astronomical Journal · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of VictoriaUniversité de MontréalWestern UniversityCanadian Institute for Theoretical AstrophysicsHerzberg Institute of AstrophysicsUniversity of Toronto
FundersLawrence Livermore National LaboratoryScience Mission DirectorateScience and Technology Facilities CouncilUniversity of TorontoUniversity of California, Santa CruzNASA Exoplanet Science InstituteJet Propulsion LaboratorySpace Telescope Science InstituteNational Aeronautics and Space AdministrationU.S. Department of EnergyCalifornia Institute of TechnologyOffice of the President, University of CaliforniaNational Science Foundation
KeywordsSurface gravityPhysicsPlanetBrown dwarfAstrophysicsRADIUSEffective temperatureLuminosityGiant planetExoplanetInfraredPlanetary systemStarsAstronomy

Abstract

fetched live from OpenAlex

Abstract Using the Gemini Planet Imager located at Gemini South, we measured the near-infrared (1.0–2.4 μ m) spectrum of the planetary companion to the nearby, young star β Pictoris. We compare the spectrum obtained with currently published model grids and with known substellar objects and present the best matching models as well as the best matching observed objects. Comparing the empirical measurement of the bolometric luminosity to evolutionary models, we find a mass of 12.9 ± 0.2 , an effective temperature of 1724 ± 15 K, a radius of 1.46 ± 0.01 , and a surface gravity of [dex] (cgs). The stated uncertainties are statistical errors only, and do not incorporate any uncertainty on the evolutionary models. Using atmospheric models, we find an effective temperature of 1700–1800 K and a surface gravity of –4.0 [dex] depending upon the model. These values agree well with other publications and with “hot-start” predictions from planetary evolution models. Further, we find that the spectrum of β Pic b best matches a low surface gravity L2 ± 1 brown dwarf. Finally, comparing the spectrum to field brown dwarfs, we find the the spectrum best matches 2MASS J04062677–381210 and 2MASS J03552337+1133437.

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 categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.032
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.001
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
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 head0.008
GPT teacher head0.205
Teacher spread0.198 · 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

Citations99
Published2017
Admission routes2
Has abstractyes

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