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Record W1936097296 · doi:10.1088/0004-637x/814/1/32

DIRECT IMAGING OF AN ASYMMETRIC DEBRIS DISK IN THE HD 106906 PLANETARY SYSTEM

2015· article· en· W1936097296 on OpenAlexaff
Paul Kalas, Abhijith Rajan, Jason Wang, Maxwell A. Millar‐Blanchaer, Gaspard Duchêne, Christine Chen, Michael P. Fitzgerald, Ruobing Dong, James R. Graham, Jennifer Patience, Bruce Macintosh, Ruth Murray‐Clay, Brenda C. Matthews, Julien Rameau, Christian Marois, Jeffrey Chilcote, Robert J. De Rosa, René Doyon, Zachary H. Draper, Samantha Lawler, S. Mark Ammons, Pauline Arriaga, J. Bulger, Tara Cotten, Katherine B. Follette, Stephen J. Goodsell, Alexandra Z. Greenbaum, Pascale Hibon, Sasha Hinkley, Li-Wei Hung, Patrick Ingraham, Quinn Konapacky, David Lafreniére, James E. Larkin, Douglas Long, Jérôme Maîre, Franck Marchis, Stanimir Metchev, Katie M. Morzinski, E. Nielsen, Rebecca Oppenheimer, Marshall D. Perrin, Laurent Pueyo, Fredrik T. Rantakyrö, Jean-Baptiste Ruffio, Leslie Saddlemyer, Dmitry Savransky, Adam C. Schneider, Anand Sivaramakrishnan, Rémi Soummer, Inseok Song, Sandrine Thomas, Gautam Vasisht, Kimberly Ward-Duong, Sloane Wiktorowicz, Schuyler Wolff

Bibliographic record

VenueThe Astrophysical Journal · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsWestern UniversityUniversité de MontréalCanadian Institute for Theoretical AstrophysicsHerzberg Institute of AstrophysicsUniversity of Toronto
FundersScience Mission DirectorateComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationMinisterio de Ciencia, Tecnología e Innovación ProductivaNational Science Foundation
KeywordsPhysicsDebris diskPlanetAstrophysicsAstronomyDebrisPlanetary systemPrimary (astronomy)

Abstract

fetched live from OpenAlex

Here, we present the first scattered light detections of the HD 106906 debris disk using the Gemini/Gemini Planet Imager in the infrared and Hubble Space Telescope (HST)/Advanced Camera for Surveys in the optical. HD 106906 is a 13 Myr old F5V star in the Sco–Cen association, with a previously detected planet-mass candidate HD 106906b projected 650 AU from the host star. Our observations reveal a near edge-on debris disk that has a central cleared region with radius ~50 AU, and an outer extent >500 AU. The HST data show that the outer regions are highly asymmetric, resembling the "needle" morphology seen for the HD 15115 debris disk. The planet candidate is oriented ~21° away from the position angle of the primary's debris disk, strongly suggesting non-coplanarity with the system. We hypothesize that HD 106906b could be dynamically involved in the perturbation of the primary's disk, and investigate whether or not there is evidence for a circumplanetary dust disk or cloud that is either primordial or captured from the primary. In conclusion, we show that both the existing optical properties and near-infrared colors of HD 106906b are weakly consistent with this possibility, motivating future work to test for the observational signatures of dust surrounding the planet.

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)0.001
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 score0.056
Threshold uncertainty score0.363

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
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 head0.225
Teacher spread0.212 · 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

Citations104
Published2015
Admission routes1
Has abstractyes

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