Ultracool dwarf benchmarks with \emph{Gaia} primaries

F. Marocco; D. J. Pinfield; N. J. Cook; M. R. Zapatero Osorio; D. Montes; J. A. Caballero; M. C. Gálvez-Ortiz; M. Gromadzki; H. R. A. Jones; R. Kurtev; R. L. Smart; Z. Zhang; A. L. Cabrera Lavers; D. García Álvarez; Z. X. Qi; M. J. Rickard; L. Dover

doi:10.1093/mnras/stx1500

Ultracool dwarf benchmarks with \emph{Gaia} primaries

F. Marocco, D. J. Pinfield, N. J. Cook, M. R. Zapatero Osorio, D. Montes, J. A. Caballero, M. C. Gálvez-Ortiz, M. Gromadzki, H. R. A. Jones, R. Kurtev, R. L. Smart, Z. Zhang, A. L. Cabrera Lavers, D. García Álvarez, Z. X. Qi, M. J. Rickard, L. Dover

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Abstract

We 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}\,

Original language	English
Pages (from-to)	4885–4907
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	470
Issue number	4
Early online date	16 Jun 2017
DOIs	https://doi.org/10.1093/mnras/stx1500
Publication status	Published - 1 Oct 2017

Keywords

astro-ph.SR

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1706 - 1
© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Accepted author manuscript, 4.96 MBLicence: Other

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Marocco, 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 (MNRAS), 470(4), 4885–4907. https://doi.org/10.1093/mnras/stx1500

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title = "Ultracool dwarf benchmarks with \textbackslash{}emph\{Gaia\} primaries",

abstract = "We explore the potential of \textbackslash{}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 \textbackslash{}emph\{Gaia\} primary stars is generated and assessed. Of order \$\textbackslash{}sim\$24,000 companions should be identifiable outside of the Galactic plane (\$|b| > 10\textbackslash{},\$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 \textbackslash{}le M/M\_\{\textbackslash{}odot\} \textbackslash{}le 0.1\$, \$0.1 \textbackslash{}le \{\textbackslash{}rm age/Gyr\} \textbackslash{}le 14\$, and \$-2.5 \textbackslash{}le \{\textbackslash{}rm [Fe/H]\} \textbackslash{}le 0.5\$, with systems required to have a false alarm probability \$ \$0.6\textbackslash{}, kau\}\textbackslash{},",

keywords = "astro-ph.SR",

author = "F. Marocco and Pinfield, \{D. J.\} and Cook, \{N. J.\} and Osorio, \{M. R. Zapatero\} and D. Montes and Caballero, \{J. A.\} and G{\'a}lvez-Ortiz, \{M. C.\} and M. Gromadzki and Jones, \{H. R. A.\} and R. Kurtev and Smart, \{R. L.\} and Z. Zhang and Lavers, \{A. L. Cabrera\} and {\'A}lvarez, \{D. Garc{\'i}a\} and Qi, \{Z. X.\} and Rickard, \{M. J.\} and L. Dover",

note = "This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. {\textcopyright} 2017 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. ",

year = "2017",

month = oct,

day = "1",

doi = "10.1093/mnras/stx1500",

language = "English",

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pages = "4885–4907",

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Marocco, F, Pinfield, DJ, Cook, NJ, Osorio, MRZ, Montes, D, Caballero, JA, Gálvez-Ortiz, MC, Gromadzki, M, Jones, HRA, Kurtev, R, Smart, RL, Zhang, Z, Lavers, ALC, Álvarez, DG, Qi, ZX, Rickard, MJ & Dover, L 2017, 'Ultracool dwarf benchmarks with \emph{Gaia} primaries', Monthly Notices of the Royal Astronomical Society (MNRAS), vol. 470, no. 4, pp. 4885–4907. https://doi.org/10.1093/mnras/stx1500

TY - JOUR

T1 - Ultracool dwarf benchmarks with \emph{Gaia} primaries

AU - Marocco, F.

AU - Pinfield, D. J.

AU - Cook, N. J.

AU - Osorio, M. R. Zapatero

AU - Montes, D.

AU - Caballero, J. A.

AU - Gálvez-Ortiz, M. C.

AU - Gromadzki, M.

AU - Jones, H. R. A.

AU - Kurtev, R.

AU - Smart, R. L.

AU - Zhang, Z.

AU - Lavers, A. L. Cabrera

AU - Álvarez, D. García

AU - Qi, Z. X.

AU - Rickard, M. J.

AU - Dover, L.

N1 - This 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.

PY - 2017/10/1

Y1 - 2017/10/1

N2 - We 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}\,

AB - We 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}\,

KW - astro-ph.SR

U2 - 10.1093/mnras/stx1500

DO - 10.1093/mnras/stx1500

M3 - Article

SN - 0035-8711

VL - 470

SP - 4885

EP - 4907

JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

IS - 4

ER -

Ultracool dwarf benchmarks with \emph{Gaia} primaries

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