The Gaia mission
arXiv:1609.04153 · doi:10.1051/0004-6361/201629272
Abstract
Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original interferometric concept was changed to a direct-imaging approach. Both the spacecraft and the payload were built by European industry. The involvement of the scientific community focusses on data processing for which the international Gaia Data Processing and Analysis Consortium (DPAC) was selected in 2007. Gaia was launched on 19 December 2013 and arrived at its operating point, the second Lagrange point of the Sun-Earth-Moon system, a few weeks later. The commissioning of the spacecraft and payload was completed on 19 July 2014. The nominal five-year mission started with four weeks of special, ecliptic-pole scanning and subsequently transferred into full-sky scanning mode. We recall the scientific goals of Gaia and give a description of the as-built spacecraft that is currently (mid-2016) being operated to achieve these goals. We pay special attention to the payload module, the performance of which is closely related to the scientific performance of the mission. We provide a summary of the commissioning activities and findings, followed by a description of the routine operational mode. We summarise scientific performance estimates on the basis of in-orbit operations. Several intermediate Gaia data releases are planned and the data can be retrieved from the Gaia Archive, which is available through the Gaia home page at http://www.cosmos.esa.int/gaia.
The Gaia Collaboration consists of 625 authors. Accepted by A&A in the Gaia Special Feature
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Cited by in corpus (412)
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- A low-mass triple system with a wide L/T transition brown dwarf component: NLTT 51469AB/SDSS 2131-0119
- GRAVITY spectro-interferometric study of the massive multiple stellar system HD 93 206 A
- Abundance analyses of the new R Coronae Borealis stars: ASAS-RCB-8 and ASAS-RCB-10
- The Belgian repository of fundamental atomic data and stellar spectra (BRASS) II. Quality assessment of atomic data for unblended lines in FGK stars
- Confronting expansion distances of planetary nebulae with Gaia DR2 measurements
- Investigation of the Globular Cluster NGC 2808 with the Ultra-Violet Imaging Telescope
- Coronal X-ray emission and planetary irradiation in HD 209458
- Recovering saturated images for high dynamic Kernel-Phase analysis Application to the determination of dynamical masses for the system Gl 494AB
- Spectroscopic confirmation of the low-latitude object FSR 1716 as an old globular cluster
- Young open cluster IC 4996 and its vicinity: multicolor photometry and Gaia DR2 astrometry
- The Measured Impact of Chromatic Atmospheric Effects on Barycentric Corrections: Results from the EXtreme PREcision Spectrograph
- ISPY -- NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring
- Opacity distribution functions for stellar spectra synthesis
- A multi-wavelength study of the debris disc around 49 Cet
- The intricate Galaxy disk: velocity asymmetries in Gaia-TGAS
- Magnetic field geometry and chemical abundance distribution of the He-strong star CPD -57 3509
- Gaia Data Release 1: The archive visualisation service
- YZ Phe: an active contact binary with variation of the O'Connell effect and orbital period change
- New binaries in the epsilon Cha association
- Collisions of Terrestrial Worlds: The Occurrence of Extreme Mid-Infrared Excesses around Low-Mass Field Stars
- Ultralow-amplitude RR Lyrae Stars in M4
- Proper Motions and Shock Wave Dynamics in the HH 7-11 Stellar Jet
- Unveiling the nature of the Gemini multiconjugate adaptive optics system distortions
- A massive nebula around the Luminous Blue Variable star RMC143 revealed by ALMA
- A compact gaseous accretion disk in Keplerian rotation around MWC147
- The ssos Pipeline: Identification of Solar System Objects in Astronomical Images
- RR Lyrae Stars in the Field of Sagittarius II
- Spot evolution in the eclipsing binary CoRoT 105895502
- Discovery of a Compact Companion to a Nearby Star
- A distortion solution for the Bok telescope with four CCD chips
- Variable Stars in Young Open Cluster NGC 2244
- Parameters of the Link between the Optical and Radio Frames from Gaia DR2 Data and VLBI Measurements
- Determination of astrophysical parameters of quasars within the Gaia mission
- New powerful outburst of the unusual young star V1318 Cyg S (LkHα 225)
- The GALAH survey: unresolved triple Sun-like stars discovered by the Gaia mission
- A method to calculate the local density distribution of the Galaxy from the Tycho-Gaia Astrometric Solution data
- The young star population of L1188
- Two's a crowd? Characterising the effect of photometric contamination on the extraction of the global asteroseismic parameter in red-giant binaries
- SN 2016B a.k.a ASASSN-16ab: a transitional type II supernova
- Testing the distance scale of the Gaia TGAS catalogue by kinematic method
- Application of Time Transfer Functions to Gaia's global astrometry - Validation on DPAC simulated Gaia-like observations
- Comparison of Gaia and asteroseismic distances
- The GAPS Programme with HARPS-N at TNG XV. A substellar companion around a K giant star identified with quasi-simultaneous HARPS-N and GIANO measurements
- A catalogue of oxygen-rich pulsating giants in the galactic halo and the Sagittarius stream
- Detecting unresolved binary stars in Euclid VIS images
- Proper Motions of the Satellites of M31
- Pulsations and Period Variations of the Scuti Star AN Lyncis in a possible three-body system
- Helium-Star Models with Optically Thick Winds: Implications for the Internal Structures and Mass-Loss Rates of Wolf-Rayet Stars
- An analysis of binary microlensing event OGLE-2015-BLG-0060
- Understanding the evolution of Atira-class asteroid 2019 AQ3, a major step towards the future discovery of the Vatira population
- Astronomical distance scales in the Gaia era
- Vertical Distribution and Kinematics of Protoplanetary Nebulae in the Galaxy
- A revisit to the enigmatic variable star 21 Comae
- Calibrations of SITELLE's first data release
- The Case for a Large-Scale Occultation Network
- Gravitational wave effects on astrometric observables
- Open star clusters in the Milky Way - Comparison of photometric and trigonometric distance scales based on Gaia TGAS data
- Optimal extinction measurements - I. Single-object extinction inference
- The influence of dark matter halo on the stellar stream asymmetry via dynamical friction
- A new method of measuring center-of-mass velocities of radially pulsating stars from high-resolution spectroscopy
- Overall properties of the Gaia DR1 reference frame
- An astrometric and spectroscopic study of the Scuti variable HD21190 and its wide companion CPD -83 64B
- Relativistic Astronomy. II. In-Flight Solution of Motion and Test of Special Relativity Light Aberration
- Data-driven stellar parameters for southern TESS FGK targets
- A study of full space motions of outer Galactic disk A and F stars in two deep pencil-beams
- A catalogue of spectroscopic binary candidate stars derived from a comparison of Gaia DR2 with other radial velocity catalogues
- OGLE-2018-BLG-0022: First Prediction of an Astrometric Microlensing Signal from a Photometric Microlensing Event
- Gaia and VLT astrometry of faint stars: Precision of Gaia DR1 positions and updated VLT parallaxes of ultracool dwarfs
- The impact of geometric distortions in multiconjugate adaptive optics astrometric observations with future extremely large telescopes
- Differential Astrometric Framework for the Jupiter Relativistic Experiment with Gaia
- Variable Stars in Sagittarius Globular Clusters I. Arp~2
- Faint, high proper motion star candidates selected from the SDSS and PS1 catalogs
- A first view with GAIA on KIC 8462852 - distance estimates and a comparison to other F stars
- A test field for Gaia. Radial velocity catalogue of stars in the South Ecliptic Pole
- Constraints on HD113337 fundamental parameters and planetary system. Combining long-base visible interferometry, disk imaging and high-contrast imaging
- A deep staring campaign in the Sigma Orionis cluster. Variability in substellar members
- An improved solution to geometric distortion using an orthogonal method
- Search for Stellar Streams Based on Data from the RAVE5 and Gaia TGAS Catalogues
- Precision Time-series Photometry in the Thermal Infrared with a 'Wall-Eyed' Pointing Mode at the Large Binocular Telescope
- Sliced Inverse Regression for the inference of stellar fundamental parameters