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Record W2144022483 · doi:10.1088/0004-637x/768/2/129

MICROLENSING DISCOVERY OF A POPULATION OF VERY TIGHT, VERY LOW MASS BINARY BROWN DWARFS

2013· article· en· W2144022483 on OpenAlexaff
J.-Y. Choi, Cheongho Han, A. Udalski, T. Sumi, B. Scott Gaudi, Andrew Gould, D. P. Bennett, M. Dominik, Jean‐Philippe Beaulieu, Y. Tsapras, V. Bozza, F. Abe, I. A. Bond, C. S. Botzler, P. Chote, M. Freeman, Akihiko Fukui, K. Furusawa, Y. Itow, C. H. Ling, K. Masuda, Y. Matsubara, N. Miyake, Y. Muraki, Koji Ohnishi, Nicholas J. Rattenbury, To. Saito, D. J. Sullivan, K. Suzuki, W. L. Sweatman, Daisuke Suzuki, S. Takino, P. J. Tristram, K. Wada, P. C. M. Yock, M. K. Szymański, M. Kubiak, G. Pietrzyński, I. Soszyński, J. Skowron, S. Kozłowski, R. Poleski, K. Ulaczyk, Ł. Wyrzykowski, P. Pietrukowicz, L. A. Almeida, D. L. DePoy, Subo Dong, E. Gorbikov, F. Jablonski, Calen B. Henderson, Kyu‐Ha Hwang, J. Janczak, Youn Kil Jung, S. Kaspi, Chung‐Uk Lee, Uri Malamud, D. Maoz, D. McGregor, J. A. Muñoz, B.-G. Park, H. Park, Richard W. Pogge, Yossi Shvartzvald, In-Gu Shin, Jennifer C. Yee, K. A. Alsubai, P. Browne, M. Burgdorf, S. Calchi Novati, P. Dodds, X.-S. Fang, F. Finet, M. Glitrup, F. Grundahl, S.-H. Gu, S. Hardis, K. Harpsøe, T. C. Hinse, A. Hornstrup, M. Hundertmark, J. Jessen‐Hansen, U. G. Jrgensen, N. Kains, E. Kerins, C. Liebig, Mikkel N. Lund, M. Lundkvist, G. Maier, L. Mancini, M. Mathiasen, Matthew T. Penny, S. Rahvar, D. Ricci, G. Scarpetta, J. Skottfelt, C. Snodgrass, J. Southworth, J. Surdej, J. Tregloan-Reed, J. Wambsganß, O. Wertz, F. Zimmer, Michael D. Albrow, E. Bachelet, V. Batista, S. Brillant, A. Cassan, Andrew A. Cole, C. Coutures, S. Dieters, D. Dominis Prester, J. Donatowicz, P. Fouqué, J. Greenhill, D. Kubas, J. B. Marquette, J. W. Menzies, K. C. Sahu, M. Zub, D. M. Bramich, K. Horne, I. A. Steele, R. A. Street

Bibliographic record

VenueThe Astrophysical Journal · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsPerimeter Institute
FundersJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilFédération Wallonie-BruxellesChungbuk National UniversityFonds National de la Recherche LuxembourgQatar National Research FundQatar FoundationKorea Research Council of Fundamental Science and TechnologyFonds pour la Formation à la Recherche dans l’Industrie et dans l’AgricultureDeutsche ForschungsgemeinschaftLeverhulme TrustCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationKorea Astronomy and Space Science InstituteNational Science Foundation
KeywordsGravitational microlensingBrown dwarfPhysicsAstrophysicsLow MassAstronomyBinary numberPopulationStellar massStarsStar formation

Abstract

fetched live from OpenAlex

Although many models have been proposed, the physical mechanisms responsible for the formation of low-mass brown dwarfs (BDs) are poorly understood. The multiplicity properties and minimum mass of the BD mass function provide critical empirical diagnostics of these mechanisms. We present the discovery via gravitational microlensing of two very low mass, very tight binary systems. These binaries have directly and precisely measured total system masses of 0.025 M ☉ and 0.034 M ☉ , and projected separations of 0.31 AU and 0.19 AU, making them the lowest-mass and tightest field BD binaries known. The discovery of a population of such binaries indicates that BD binaries can robustly form at least down to masses of ∼0.02 M ☉ . Future microlensing surveys will measure a mass-selected sample of BD binary systems, which can then be directly compared to similar samples of stellar binaries.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation 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 score0.002
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.007
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 source (direct Gemma or distilled Codex), 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

Citations51
Published2013
Admission routes1
Has abstractyes

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