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Record W2146081406 · doi:10.1088/0004-637x/769/1/77

MOA-2010-BLG-311: A PLANETARY CANDIDATE BELOW THE THRESHOLD OF RELIABLE DETECTION

2013· article· en· W2146081406 on OpenAlexaff
Jennifer C. Yee, L.W. Hung, I. A. Bond, William H. Allen, L. A. G. Monard, Michael D. Albrow, P. Fouqué, M. Dominik, Y. Tsapras, A. Udalski, Andrew Gould, Robert T. Zellem, M. Bos, G. W. Christie, D. L. DePoy, Subo Dong, J. Drummond, B. S. Gaudi, E. Gorbikov, Cheongho Han, S. Kaspi, N. Klein, Chung‐Uk Lee, Dan Maoz, J. McCormick, D. Moorhouse, T. Natusch, M. Nola, B.-G. Park, Richard W. Pogge, David Polishook, Avi Shporer, Yossi Shvartzvald, J. Skowron, G. Thornley, F. Abe, D. P. Bennett, C. S. Botzler, P. Chote, M. Freeman, Akihiko Fukui, K. Furusawa, P. Harris, Y. Itow, C. H. Ling, K. Masuda, Y. Matsubara, N. Miyake, Koji Ohnishi, Nicholas J. Rattenbury, To. Saito, D. J. Sullivan, T. Sumi, Daisuke Suzuki, W. L. Sweatman, P. J. Tristram, K. Wada, P. C. M. Yock, M. K. Szymański, I. Soszyński, M. Kubiak, R. Poleski, K. Ulaczyk, G. Pietrzyński, Ł. Wyrzykowski, E. Bachelet, V. Batista, Thomas G. Beatty, Jean‐Philippe Beaulieu, C. S. Bennett, Rachel Bowens-Rubin, S. Brillant, J. A. R. Caldwell, A. Cassan, Andrew A. Cole, E. Corrales, C. Coutures, S. Dieters, D. Dominis Prester, J. Donatowicz, J. Greenhill, Calen B. Henderson, D. Kubas, J. B. Marquette, Roland Martín, J. W. Menzies, B. J. Shappee, A. Williams, D. Wouters, Jennifer L. van Saders, M. Zub, R. A. Street, K. Horne, D. M. Bramich, I. A. Steele, K. A. Alsubai, V. Bozza, P. Browne, M. Burgdorf, S. Calchi Novati, P. Dodds, F. Finet, T. Gerner, S. Hardis, K. Harpsøe, F. V. Hessman, T. C. Hinse, M. Hundertmark, U. G. Jørgensen, N. Kains, E. Kerins, C. Liebig, L. Mancini, M. Mathiasen, Matthew T. Penny, S. Proft, S. Rahvar, D. Ricci, K. C. Sahu, G. Scarpetta, Sebastian Schäfer, F. Schönebeck, C. Snodgrass, J. Southworth, J. Surdej, J. Wambsganß

Bibliographic record

VenueThe Astrophysical Journal · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsPerimeter Institute
FundersNational Research Foundation of KoreaCalifornia Institute of TechnologyEuropean CommissionQatar National Research FundKorea Research Council of Fundamental Science and TechnologyQatar FoundationKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationFonds pour la Formation à la Recherche dans l’Industrie et dans l’AgricultureDeutsche ForschungsgemeinschaftScience and Technology Facilities CouncilNational Research FoundationSpace Telescope Science InstituteAlfred P. Sloan FoundationNational Geographic SocietyNational Science Foundation
KeywordsGravitational microlensingPhysicsPlanetPlanetary systemAstrophysicsEvent (particle physics)Lens (geology)MagnificationAstronomyStarsOptics

Abstract

fetched live from OpenAlex

We analyze MOA-2010-BLG-311, a high magnification ( A max > 600) microlensing event with complete data coverage over the peak, making it very sensitive to planetary signals. We fit this event with both a point lens and a two-body lens model and find that the two-body lens model is a better fit but with only Δχ 2 ∼ 80. The preferred mass ratio between the lens star and its companion is q = 10 −3.7 ± 0.1 , placing the candidate companion in the planetary regime. Despite the formal significance of the planet, we show that because of systematics in the data the evidence for a planetary companion to the lens is too tenuous to claim a secure detection. When combined with analyses of other high-magnification events, this event helps empirically define the threshold for reliable planet detection in high-magnification events, which remains an open question.

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 score0.011
Threshold uncertainty score0.036

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 studies0.0020.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0110.003

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 head0.008
GPT teacher head0.197
Teacher spread0.189 · 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

Citations23
Published2013
Admission routes1
Has abstractyes

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