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Record W3103517891

OGLE-2016-BLG-1190Lb: The First <i>Spitzer</i> Bulge Planet Lies Near the Planet/Brown-dwarf Boundary

2018· article· en· W3103517891 on OpenAlexaff
Yoon-Hyun Ryu, Jennifer C. Yee, A. Udalski, I. A. Bond, Yossi Shvartzvald, Weicheng Zang, R. Figuera Jaimes, U. G. Jørgensen, Wei Zhu, Chelsea X. Huang, Youn Kil Jung, Michael D. Albrow, Sun‐Ju Chung, Andrew Gould, Cheongho Han, Kyu‐Ha Hwang, In-Gu Shin, Sang-Mok Cha, Dong-Jin Kim, Hyoun-Woo Kim, Seung‐Lee Kim, Chung‐Uk Lee, D.-J. Lee, Yongseok Lee, B.-G. Park, Richard W. Pogge, S. Calchi Novati, S. Carey, Calen B. Henderson, C. Beichman, B. Scott Gaudi, P. Mróz, R. Poleski, J. Skowron, M. K. Szymański, I. Soszyński, S. Kozłowski, P. Pietrukowicz, K. Ulaczyk, M. Pawlak, F. Abe, Y. Asakura, Richard Barry, D. P. Bennett, Aparna Bhattacharya, M. Donachie, Phil Evans, Akihiko Fukui, Yuki Hirao, Y. Itow, K. Kawasaki, Naoki Koshimoto, M. C. A. Li, C. H. Ling, K. Masuda, Y. Matsubara, Shota Miyazaki, Y. Muraki, M. Nagakane, Koji Ohnishi, ‪Clément Ranc, Nicholas J. Rattenbury, To. Saito, A. Sharan, D. J. Sullivan, T. Sumi, Daisuke Suzuki, P. J. Tristram, Tōru Yamada, A. Yonehara, G. Bryden, S. B. Howell, Savannah Jacklin, Matthew T. Penny, Shude Mao, P. Fouqué, T. Wang, R. A. Street, Y. Tsapras, M. Hundertmark, E. Bachelet, M. Dominik, Zhexing Li, S. Cross, A. Cassan, K. Horne, R. W. Schmidt, J. Wambsganß, S. K. Ment, D. Maoz, C. Snodgrass, I. A. Steele, V. Bozza, M. Burgdorf, S. Ciceri, G. D’Ago, D. F. Evans, T. C. Hinse, E. Kerins, Rosita Kokotanekova, P. Longã, Jasmine MacKenzie, A. Popovas, M. Rabus, S. Rahvar, Sedighe Sajadian, J. Skottfelt, J. Southworth, C. von Essen

Bibliographic record

VenueOpen Research Online (The Open University) · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsCanadian Institute for Theoretical AstrophysicsThe Scarborough HospitalUniversity of Toronto
Fundersnot available
KeywordsGravitational microlensingPhysicsPlanetAstronomyBrown dwarfAstrophysicsExoplanetPlanetary systemBulgeStars
DOInot available

Abstract

fetched live from OpenAlex

We report the discovery of OGLE-2016-BLG-1190Lb, which is likely to be the first <i>Spitzer</i> microlensing planet in the Galactic bulge/bar, an assignation that can be confirmed by two epochs of high-resolution imaging of the combined source–lens baseline object. The planet's mass, <i>M</i><sub>p</sub> = 13.4 ± 0.9 <i>M<sub>J</sub></i> , places it right at the deuterium-burning limit, i.e., the conventional boundary between "planets" and "brown dwarfs." Its existence raises the question of whether such objects are really "planets" (formed within the disks of their hosts) or "failed stars" (low-mass objects formed by gas fragmentation). This question may ultimately be addressed by comparing disk and bulge/bar planets, which is a goal of the <i>Spitzer</i> microlens program. The host is a G dwarf, M<sub>host</sub> = 0.89 ± 0.07 <i>M</i> ⊙, and the planet has a semimajor axis a ~ 2.0 au. We use <i>Kepler K2</i> Campaign 9 microlensing data to break the lens-mass degeneracy that generically impacts parallax solutions from Earth–<i>Spitzer</i> observations alone, which is the first successful application of this approach. The microlensing data, derived primarily from near-continuous, ultradense survey observations from OGLE, MOA, and three KMTNet telescopes, contain more orbital information than for any previous microlensing planet, but not quite enough to accurately specify the full orbit. However, these data do permit the first rigorous test of microlensing orbital-motion measurements, which are typically derived from data taken over <1% of an orbital period.

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)0.002
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow), Science and technology studies, Scholarly communication, Open science, Insufficient payload (model declined to judge)
Consensus categoriesScience and technology studies, Insufficient payload (model declined to judge)
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Other · Consensus signal: none
Teacher disagreement score0.772
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0020.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.001
Science and technology studies0.0080.003
Scholarly communication0.0020.001
Open science0.0070.005
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0050.002

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 head0.045
GPT teacher head0.294
Teacher spread0.249 · 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; both teacher heads agree on what is shown here.

Study designNot applicable
Domainnot available
GenreOther

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

Citations30
Published2018
Admission routes1
Has abstractyes

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