The Three-Dimensional Universe with Gaia

By C. Turon, K. O'flaherty, M. Perryman. 2005

385 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/964dc56fec28a58e51ded714d66987f64a1a785c

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Citations in the corpus

Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A Grid of 200,000 YSO Model SEDs (2006, methodology): “For stellar temperatures below 10, 000K, we used model stellar photospheres from Brott & Hauschildt (2005), while for stellar temperatures above 10, 000K we used model stellar photospheres from Kurucz (1993).”
Outer structure of the Galactic warp and flare: explaining the Canis Major over-density (2006, methodology): “However, the new model (Drimmel 2005) indicates that the far infrared DIRBE 240µm data, are sensitive to at least ∼ 7 kpc from the Sun, and possibly beyond.”
The Variation of Integrated Star Initial Mass Functions among Galaxies (2005, background): “Subject headings: galaxies: abundances — galaxies: evolution — galaxies: general — galaxies: star clusters — galaxies: stellar content — galaxies: structure”
Physics, Astrophysics and Cosmology with Gravitational Waves (2009, background): “vitational and electromagnetic observations, with applications in the observations of isolated neutrons stars, binary systems, etc. And would lead to synergies, for example, between the LISA and Gaia [289] missions. 7.2 Black hole astrophysics Black holes are the most relativistic systems possible. ”
The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from the Kinematics of ~2400 SDSS Blue Horizontal-Branch Stars (2008, background): “The planned or alreadyunderway kinematically unbiased surveys, such as the European Space Agency’s astrometric mission Gaia (Turon et al. 2005), the Space Interferometry Mission (SIM; Unwin et al. 2000), the RAdial Velocity Experiment (RAVE; Steinmetz et al. 2006), the Sloan Digital Sky Survey (SDSS”
Validation of the new Hipparcos reduction (2007, methodology): “Key words. space vehicles: instruments – methods: data analysis – catalogs – astrometry – instrumentation: miscellaneous”
Chemodynamics of the Milky Way - I. The first year of APOGEE data (2013, background): “…one billion (mostly disc) stars with unprecedented accuracy (σ(π) ∼ 20µas and σ(µ) ∼ 20µas at magnitude G ∼ 15 – providing a distance accuracy of 1–2% at 1 kpc; see Turon et al. 2005), but it also provides medium-resolution spectra in the CaII triplet region (the 848 . . . 874 nm wavelength range)…”
New Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets (2006, methodology): “However, with an accurate determination of each star’s effective temperature and with more advanced stellar models (PHOENIX; Brott & Hauschildt 2005), T. N. Gautier et al. (2006, in preparation) were able to fit the 24 m colors of M stars.”
The stellar halo of the Galaxy (2008, background): “Therefore, and for many other reasons (Lindegren 2005), astrometric space missions with wide field angle capabilities are an absolute necessity.”