University of Hertfordshire

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From the same journal

By the same authors

Ultracool dwarf benchmarks with \emph{Gaia} primaries

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Ultracool dwarf benchmarks with \emph{Gaia} primaries. / Marocco, F.; Pinfield, D. J.; Cook, N. J.; Osorio, M. R. Zapatero; 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. Cabrera; Álvarez, D. García; Qi, Z. X.; Rickard, M. J.; Dover, L.

In: Monthly Notices of the Royal Astronomical Society, Vol. 470, No. 4, 01.10.2017, p. 4885–4907.

Research output: Contribution to journalArticlepeer-review

Harvard

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, vol. 470, no. 4, pp. 4885–4907. https://doi.org/10.1093/mnras/stx1500

APA

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

Vancouver

Author

Marocco, F. ; Pinfield, D. J. ; Cook, N. J. ; Osorio, M. R. Zapatero ; 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. Cabrera ; Álvarez, D. García ; Qi, Z. X. ; Rickard, M. J. ; Dover, L. / Ultracool dwarf benchmarks with \emph{Gaia} primaries. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 470, No. 4. pp. 4885–4907.

Bibtex

@article{64193f50038b4d44bb12ecb5983da95a,
title = "Ultracool dwarf benchmarks with \emph{Gaia} primaries",
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}\,",
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",
volume = "470",
pages = "4885–4907",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "4",

}

RIS

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

VL - 470

SP - 4885

EP - 4907

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -