Enabling science with Gaia observations of naked-eye stars
arXiv:1605.08347 · doi:10.1117/12.2231240
Abstract
ESA's Gaia space astrometry mission is performing an all-sky survey of stellar objects. At the beginning of the nominal mission in July 2014, an operation scheme was adopted that enabled Gaia to routinely acquire observations of all stars brighter than the original limit of G~6, i.e. the naked-eye stars. Here, we describe the current status and extent of those observations and their on-ground processing. We present an overview of the data products generated for G<6 stars and the potential scientific applications. Finally, we discuss how the Gaia survey could be enhanced by further exploiting the techniques we developed.
arXiv comment16 pages, 8 figures. Submitted for the proceedings of the 2016 SPIE Astronomical Instrumentation and Telescopes conference (SPIE 9904)
References in corpus (19)
- Astropy: A Community Python Package for Astronomy
- SB9: The Ninth Catalogue of Spectroscopic Binary Orbits
- The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample
- Gaia broad band photometry
- The Exoplanet Orbit Database
- Science performance of Gaia, ESA's space-astrometry mission
- Retired A Stars and Their Companions. III. Comparing the Mass-Period Distributions of Planets Around A-Type Stars and Sun-Like Stars
- Search for brown-dwarf companions of stars
- The TRENDS High-Contrast Imaging Survey. IV. The Occurrence Rate of Giant Planets around M-Dwarfs
- The HARPS-N Rocky Planet Search I. HD219134b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun
- Extrasolar planets and brown dwarfs around A-F type stars VI. High precision RV survey of early type dwarfs with HARPS
- High-contrast Imaging Search for Planets and Brown Dwarfs around the Most Massive Stars in the Solar Neighborhood
- The Mass of HD 38529 c from Hubble Space Telescope Astrometry and High-Precision Radial Velocities
- Gaia's potential for the discovery of circumbinary planets
- Detecting stars, galaxies, and asteroids with Gaia
- High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)
- HD 5388 b is a 69 M_Jup companion instead of a planet
- Analysis and interpretation of the Cramer-Rao lower-bound in astrometry: One dimensional case
- Enabling Gaia observations of naked-eye stars
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- The Gaia mission
- The Gemini Planet Imager Exoplanet Survey: Dynamical Mass of the Exoplanet beta Pictoris b from Combined Direct Imaging and Astrometry
- A detector interferometric calibration experiment for high precision astrometry
- A decade of radial-velocity monitoring of Vega and new limits on the presence of planets
- Precision Orbit of Delphini and Prospects for Astrometric Detection of Exoplanets
- Accurate Ground-based Astrometry of Naked-eye Stars: The United States Naval Observatory Bright-Star Astrometric Database
- Micro-arcsecond Astrometry Technology: Detector and Field Distortion Calibration