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Following the TraCS of exoplanets with Pan-Planets: Wendelstein-1b and Wendelstein-2b

2020· article· en· W3101686356 on OpenAlexfundno aff
Christian Obermeier, Jana Steuer, H. Kellermann, R. P. Saglia, Th. Henning, A. Riffeser, U. Hopp, Guðmundur Stefánsson, Caleb I. Cañas, Joe P. Ninan, Suvrath Mahadevan, Howard Isaacson, Andrew W. Howard, John H. Livingston, J. Koppenhoefer, R. Bender

Bibliographic record

VenueSpringer Link (Chiba Institute of Technology) · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersPlanetary Science DivisionOffice of Advanced CyberinfrastructureStrongScience Mission DirectorateLudwig-Maximilians-Universität MünchenInstitute for Computational and Data Sciences, Pennsylvania State UniversitySmithsonian Astrophysical ObservatoryNASA HeadquartersMax-Planck-Institut für AstronomiePennsylvania Space Grant ConsortiumNational Central UniversityNuclear Safety and Security CommissionGeorg-August-Universität GöttingenQueen's UniversitySpace Telescope Science InstituteUniversity of Texas at AustinJohns Hopkins UniversityQueen's University BelfastNASA Astrobiology InstituteNational Aeronautics and Space AdministrationEötvös Loránd TudományegyetemCalifornia Institute of TechnologyDurham UniversitySmithsonian InstitutionNational Science Foundation
KeywordsExoplanetPlanetHot JupiterPhysicsTransit (satellite)AstronomyJupiter (rocket family)AstrophysicsWendelstein 7-XPhotometry (optics)StarsAstrobiologySpace explorationPlasmaStellarator

Abstract

fetched live from OpenAlex

Hot Jupiters seem to get rarer with decreasing stellar mass. The goal of the Pan-Planets transit survey was the detection of such planets and a statistical characterization of their frequency. Here, we announce the discovery and validation of two planets found in that survey, Wendelstein-1b and Wendelstein-2b, which are two short-period hot Jupiters that orbit late K host stars. We validated them both by the traditional method of radial velocity measurements with the HIgh Resolution Echelle Spectrometer and the Habitable-zone Planet Finder instruments and then by their Transit Color Signature (TraCS). We observed the targets in the wavelength range of 4000−24 000 Å and performed a simultaneous multiband transit fit and additionally determined their thermal emission via secondary eclipse observations. Wendelstein-1b is a hot Jupiter with a radius of 1.0314<sub>−0.0061</sub> <sup>+0.0061</sup> R<sub>J</sub> and mass of 0.592<sub>−0.129</sub> <sup>+0.0165</sup> M<sub>J</sub>, orbiting a K7V dwarf star at a period of 2.66 d, and has an estimated surface temperature of about 1727<sub>−90</sub> <sup>+78</sup> K. Wendelstein-2b is a hot Jupiter with a radius of 1.1592<sub>−0.0210</sub> <sup>+0.0204</sup> R<sub>J</sub> and a mass of 0.731<sub>−0.311</sup> <sup>+0.0541</sup> M<sub>J</sub>, orbiting a K6V dwarf star at a period of 1.75 d, and has an estimated surface temperature of about 1852<sub>−140</sub> <sup>+120</sup> K. With this, we demonstrate that multiband photometry is an effective way of validating transiting exoplanets, in particular for fainter targets since radial velocity follow-up becomes more and more costly for those targets.

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.424
Threshold uncertainty score0.860

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 head0.013
GPT teacher head0.210
Teacher spread0.197 · 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.

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

Citations5
Published2020
Admission routes1
Has abstractyes

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