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Record W4408128577 · doi:10.1093/mnras/staf360

Unveiling the infrared excess of SIPS J2045–6332: evidence for a young stellar object with potential low-mass companion

2025· article· en· W4408128577 on OpenAlexaff
Michiharu Hyogo, Thomas P. Bickle, Joseph R. Biggs, Adam J. Burgasser, Dan Caselden, S. L. Casewell, Sergio Dieterich, Hugo A. Durantini Luca, Jacqueline K. Faherty, Daniella C. Bardalez Gagliuffi, Jonathan Gagné, J. Davy Kirkpatrick, Marc J. Kuchner, C. M. Lisse, Federico Marocco, Aaron Meisner, Austin Rothermich, Adam C. Schneider, Steven M. Silverberg

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversité de MontréalRio Tinto (Canada)Espace pour la vie
FundersLos Alamos National LaboratoryAustralian Research CouncilJet Propulsion LaboratoryUniversity of MelbourneUniversity of EdinburghSpace Telescope Science InstituteDurham UniversityAstronomy Australia LimitedNational Computational InfrastructureNational Aeronautics and Space AdministrationEötvös Loránd TudományegyetemCurtin University of TechnologyCalifornia Institute of TechnologySwinburne University of TechnologyUniversity of Hawai'iGordon and Betty Moore FoundationUniversity of CaliforniaUniversity of Western AustraliaUniversity of QueenslandNational Science Foundation
KeywordsPhysicsInfraredAstronomyAstrophysicsYoung stellar objectInfrared excessStellar massBrown dwarfObject (grammar)Star formationStars

Abstract

fetched live from OpenAlex

ABSTRACT The Disc Detective project, a citizen science initiative, aims to identify circumstellar discs around stars by detecting objects with infrared (IR) excess using data from the Wide-field Infrared Survey Explorer (WISE). In this study, we investigate SIPS J2045–6332, a potential brown dwarf with significant IR excess in WISE and Two Micron All Sky Survey (2MASS) bands, initially identified by project volunteers. Despite early indicators of a circumstellar disc, discrepancies between observed brightness and expected spectral energy distribution (SED) models suggested unusual properties. To explore potential explanations, we created SED templates for spectral types M9 to L4 and compared them with SIPS J2045–6332’s photometric data, revealing an excess brightness that points to either an unresolved low-mass companion or a young, inflated primary star. Further analysis of IR spectral features and surface gravity indicators supports a youthful classification, estimating the object’s age at 26–200 million years. Observations also suggest the presence of a mid L-type companion at a projected distance of 6.7 au. This study highlights SIPS J2045–6332 as an intriguing system with unique IR characteristics and recommends follow-up observations with high-resolution telescopes to confirm the companion hypothesis and further characterize the system.

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)0.000
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 score0.001
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.228
Teacher spread0.217 · 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

Citations2
Published2025
Admission routes1
Has abstractyes

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