MétaCan
Menu
← Back to cohort
Record W2154208465 · doi:10.1088/0004-637x/760/2/116

MICROLENSING BINARIES WITH CANDIDATE BROWN DWARF COMPANIONS

2012· article· en· W2154208465 on OpenAlexaff
In-Gu Shin, Cheongho Han, Andrew Gould, A. Udalski, T. Sumi, M. Dominik, Jean‐Philippe Beaulieu, Y. Tsapras, V. Bozza, M. K. Szymański, M. Kubiak, I. Soszyński, G. Pietrzyński, R. Poleski, K. Ulaczyk, P. Pietrukowicz, S. Kozłowski, J. Skowron, Ł. Wyrzykowski, F. Abe, D. P. Bennett, I. A. Bond, C. S. Botzler, M. Freeman, Akihiko Fukui, K. Furusawa, F. Hayashi, J. B. Hearnshaw, S. Hosaka, Y. Itow, K. Kamiya, P. M. Kilmartin, S. Kobara, A. Korpela, C. H. Ling, S. Makita, K. Masuda, Y. Matsubara, N. Miyake, Y. Muraki, M. Nagaya, K. Nishimoto, Koji Ohnishi, Teppei Okumura, K. Omori, Y. C. Perrott, Nicholas J. Rattenbury, To. Saito, L. Skuljan, D. J. Sullivan, Daisuke Suzuki, W. L. Sweatman, P. J. Tristram, K. Wada, P. C. M. Yock, G. W. Christie, D. L. DePoy, Subo Dong, A. Gal‐Yam, B. Scott Gaudi, Li-Wei Hung, J. Janczak, S. Kaspi, Dan Maoz, J. McCormick, D. McGregor, D. Moorhouse, J. A. Muñoz, T. Natusch, C. Nelson, Richard W. Pogge, Thiam-Guan Tan, David Polishook, Yossi Shvartzvald, Avi Shporer, G. Thornley, Uri Malamud, Jennifer C. Yee, J.-Y. Choi, Youn Kil Jung, H. Park, Chung‐Uk Lee, B.-G. Park, J.-R. Koo, David Bajek, D. M. Bramich, P. Browne, K. Horne, С. И. Ипатов, C. Snodgrass, I. A. Steele, R. A. Street, K. A. Alsubai, M. Burgdorf, S. Calchi Novati, P. Dodds, S. Dreizler, X.-S. Fang, F. Grundahl, Chengyu Gu, S. Hardis, K. Harpsøe, T. C. Hinse, M. Hundertmark, J. Jessen‐Hansen, Ulrik Jørgensen, N. Kains, E. Kerins, C. Liebig, Mikkel N. Lund, M. Lundkvist, L. Mancini, M. Mathiasen, A. Hornstrup, Matthew T. Penny, S. Proft, S. Rahvar, D. Ricci, G. Scarpetta, J. Skottfelt, J. Southworth, J. Surdej, J. Tregloan-Reed, O. Wertz, F. Zimmer, Michael D. Albrow, V. Batista, S. Brillant, J. A. R. Caldwell, J. J. Calitz, A. Cassan, Andrew A. Cole, K. H. Cook, E. Corrales, C. Coutures, S. Dieters, D. Dominis Prester, J. Donatowicz, P. Fouqué, J. Greenhill, K. Hill, M. Hoffman, Stephen R. Kane, D. Kubas, J. B. Marquette, Roland Martín, P. J. Meintjes, J. W. Menzies, K. R. Pollard, K. C. Sahu, J. Wambsganß, A. Williams, C. Vinter, M. Zub

Bibliographic record

VenueThe Astrophysical Journal · 2012
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsPerimeter Institute
FundersMarsden FundJapan Society for the Promotion of ScienceNational Research Foundation of KoreaFonds 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 ForschungsgemeinschaftScience and Technology Facilities CouncilNational Research FoundationCalifornia Institute of TechnologyEuropean CommissionFédération Wallonie-BruxellesNational Aeronautics and Space AdministrationKorea Astronomy and Space Science InstituteNational Science Foundation
KeywordsPhysicsGravitational microlensingBrown dwarfAstrophysicsAstronomyBinary starCircumbinary planetStars

Abstract

fetched live from OpenAlex

Brown dwarfs are important objects because they may provide a missing link between stars and planets, two populations that have dramatically different formation histories. In this paper, we present the candidate binaries with brown dwarf companions that are found by analyzing binary microlensing events discovered during the 2004–2011 observation seasons. Based on the low mass ratio criterion of q < 0.2, we found seven candidate events: OGLE-2004-BLG-035, OGLE-2004-BLG-039, OGLE-2007-BLG-006, OGLE-2007-BLG-399/MOA-2007-BLG-334, MOA-2011-BLG-104/OGLE-2011-BLG-0172, MOA-2011-BLG-149, and MOA-201-BLG-278/OGLE-2011-BLG-012N. Among them, we are able to confirm that the companions of the lenses of MOA-2011-BLG-104/OGLE-2011-BLG-0172 and MOA-2011-BLG-149 are brown dwarfs by determining the mass of the lens based on the simultaneous measurement of the Einstein radius and the lens parallax. The measured masses of the brown dwarf companions are 0.02 ± 0.01 M ☉ and 0.019 ± 0.002 M ☉ for MOA-2011-BLG-104/OGLE-2011-BLG-0172 and MOA-2011-BLG-149, respectively, and both companions are orbiting low-mass M dwarf host stars. More microlensing brown dwarfs are expected to be detected as the number of lensing events with well-covered light curves increases with new-generation searches.

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 score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.000

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 head0.011
GPT teacher head0.219
Teacher spread0.208 · 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

Citations22
Published2012
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical Journal→Same topicStellar, planetary, and galactic studies→French-language works237,207→