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dc.contributor.authorBaig, Sayan
dc.contributor.authorSmart, R. L.
dc.contributor.authorJones, Hugh R. A.
dc.contributor.authorGagné, Jonathan
dc.contributor.authorPinfield, D. J.
dc.contributor.authorCheng, Gemma
dc.contributor.authorMoranta, Leslie
dc.date.accessioned2024-09-23T15:45:02Z
dc.date.available2024-09-23T15:45:02Z
dc.date.issued2024-08-20
dc.identifier.citationBaig , S , Smart , R L , Jones , H R A , Gagné , J , Pinfield , D J , Cheng , G & Moranta , L 2024 , ' The Gaiaultracool dwarf sample – V: the ultracool dwarf companion catalogue ' , Monthly Notices of the Royal Astronomical Society , vol. 533 , no. 4 , pp. 3784-3810 . https://doi.org/10.1093/mnras/stae2005
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/2408.07024v1
dc.identifier.urihttp://hdl.handle.net/2299/28215
dc.description© 2024 The Authors. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
dc.description.abstractWe present the Ultracool Dwarf Companion Catalogue of 278 multiple systems, 32 of which are newly discovered, each with at least one spectroscopically confirmed Ultracool Dwarf, within a 100 pc volume-limited sample. This catalogue is compiled using the Gaia Catalogue of Nearby Stars for stellar primaries and the Gaia Ultracool Dwarf Sample for low-mass companions and includes 241 doubles, 33 triples, and 4 higher-order systems established from positional, proper motion, and parallax constraints. The catalogue seeks to identify probable benchmark systems within 100 pc to obtain model-independent astrophysical parameters of Ultracool Dwarfs. Chance alignment probabilities are calculated to evaluate the physical nature of each system. Astrometric and photometric data from Gaia Data Release 3 and the Two Micron All Sky Survey are included for all objects. We identify potential unseen companions using a combination of the renormalized unit weight error, image parameter determination statistics, non-single star solutions, and photometric blending as provided by Gaia, identifying hierarchical Ultracool triple systems. Our catalogue includes 17 White Dwarf - Ultracool Dwarf systems, whose ages are determined using cooling models. We also use the Gaia FLAME results and the BANYAN ς procedures to age 40 and 34 systems, respectively, and derive mass estimates from evolutionary models.en
dc.format.extent27
dc.format.extent3095989
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.SR
dc.subjectastro-ph.EP
dc.subjectastro-ph.GA
dc.subjectbrown dwarfs
dc.subjectbinaries: general
dc.subjectstars: low-mass
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.titleThe Gaiaultracool dwarf sample – V: the ultracool dwarf companion catalogueen
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionSchool of Health and Social Work
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85203850948&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1093/mnras/stae2005
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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