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dc.contributor.authorMarocco, F.
dc.contributor.authorPinfield, D. J.
dc.contributor.authorCook, N. J.
dc.contributor.authorOsorio, M. R. Zapatero
dc.contributor.authorMontes, D.
dc.contributor.authorCaballero, J. A.
dc.contributor.authorGálvez-Ortiz, M. C.
dc.contributor.authorGromadzki, M.
dc.contributor.authorJones, H. R. A.
dc.contributor.authorKurtev, R.
dc.contributor.authorSmart, R. L.
dc.contributor.authorZhang, Z.
dc.contributor.authorLavers, A. L. Cabrera
dc.contributor.authorÁlvarez, D. García
dc.contributor.authorQi, Z. X.
dc.contributor.authorRickard, M. J.
dc.contributor.authorDover, L.
dc.date.accessioned2018-09-12T00:12:03Z
dc.date.available2018-09-12T00:12:03Z
dc.date.issued2017-10-01
dc.identifier.citationMarocco , F , Pinfield , D J , Cook , N J , Osorio , M R Z , Montes , D , Caballero , J A , Gálvez-Ortiz , M C , Gromadzki , M , Jones , H R A , Kurtev , R , Smart , R L , Zhang , Z , Lavers , A L C , Álvarez , D G , Qi , Z X , Rickard , M J & Dover , L 2017 , ' Ultracool dwarf benchmarks with \emph{Gaia} primaries ' , Monthly Notices of the Royal Astronomical Society , vol. 470 , no. 4 , pp. 4885–4907 . https://doi.org/10.1093/mnras/stx1500
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/1706.06038v1
dc.identifier.urihttp://hdl.handle.net/2299/20557
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2017 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.description.abstractWe explore the potential of \emph{Gaia} for the field of benchmark ultracool/brown dwarf companions, and present the results of an initial search for metal-rich/metal-poor systems. A simulated population of resolved ultracool dwarf companions to \emph{Gaia} primary stars is generated and assessed. Of order $\sim$24,000 companions should be identifiable outside of the Galactic plane ($|b| > 10\,$deg) with large-scale ground- and space-based surveys including late M, L, T, and Y types. Our simulated companion parameter space covers $0.02 \le M/M_{\odot} \le 0.1$, $0.1 \le {\rm age/Gyr} \le 14$, and $-2.5 \le {\rm [Fe/H]} \le 0.5$, with systems required to have a false alarm probability $ $0.6\, kau}\,en
dc.format.extent5201793
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.SR
dc.titleUltracool dwarf benchmarks with \emph{Gaia} primariesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/mnras/stx1500
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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