GAIA: Composition, Formation and Evolution of the Galaxy

Abstract

The GAIA astrometric mission has recently been approved as one of the next two `cornerstones' of ESA's science programme, with a launch date target of not later than mid-2012. GAIA will provide positional and radial velocity measurements with the accuracies needed to produce a stereoscopic and kinematic census of about one billion stars throughout our Galaxy (and into the Local Group), amounting to about 1 per cent of the Galactic stellar population. GAIA's main scientific goal is to clarify the origin and history of our Galaxy, from a quantitative census of the stellar populations. It will advance questions such as when the stars in our Galaxy formed, when and how it was assembled, and its distribution of dark matter. The survey aims for completeness to V=20 mag, with accuracies of about 10 microarcsec at 15 mag. Combined with astrophysical information for each star, provided by on-board multi-colour photometry and (limited) spectroscopy, these data will have the precision necessary to quantify the early formation, and subsequent dynamical, chemical and star formation evolution of our Galaxy. Additional products include detection and orbital classification of tens of thousands of extra-Solar planetary systems, and a comprehensive survey of some 10^5-10^6 minor bodies in our Solar System, through galaxies in the nearby Universe, to some 500,000 distant quasars. It will provide a number of stringent new tests of general relativity and cosmology. The complete satellite system was evaluated as part of a detailed technology study, including a detailed payload design, corresponding accuracy assesments, and results from a prototype data reduction development.

Accepted by A&A: 25 pages, 8 figures

References in corpus (6)

• The Kinematics, Orbit, and Survival of the Sagittarius Dwarf Spheroidal Galaxy
• Galactic Bulges
• Extra-Solar Planets
• The recent star formation history of the Hipparcos solar neighbourhood
• Space-borne global astrometric surveys: the hunt for extra-solar planets
• Stellar Structure and Evolution: Deductions from Hipparcos

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• A Gaia Survey for Young Stars Associated with the Lupus Clouds
• Asteroseismic properties of solar-type stars observed with the NASA K2 mission: results from Campaigns 1-3 and prospects for future observations
• Kinematic parameters and membership probabilities of open clusters in the Bordeaux PM2000 catalogue
• Photo-centric variability of quasars caused by variations in their inner structure: Consequences on Gaia measurements
• M dwarf luminosity, radius, and $\alpha$-enrichment from $I$-band spectral features
• Abundances and kinematics for ten anticentre open clusters
• Mapping the Local Halo: Statistical Parallax Analysis of SDSS Low-Mass Subdwarfs
• Analytical Derivation of Second-Order Deflection in Equatorial Plane of a Radially Moving Kerr-Newman Black Hole
• A New M Dwarf Debris Disk Candidate in a Young Moving Group Discovered with Disk Detective
• Distance and extinction determination for APOGEE stars with Bayesian method
• Numerical Simulations of the Light Propagation in the Gravitational Field of Moving Bodies
• Towards automatic classification of all WISE sources
• Narrow-Angle Astrometry with the Space Interferometry Mission: The Search for Extra-solar Planets. I. Detection and Characterization of Single Planets
• First Light for GRAVITY Wide: Large Separation Fringe Tracking for the Very Large Telescope Interferometer
• Using Galactic Cepheids to verify Gaia parallaxes
• Signatures of Dark Matter Halo Expansion in Galaxy Populations
• Tracing the Hercules stream around the Galaxy
• Impact of basic angle variations on the parallax zero point for a scanning astrometric satellite
• Dispersal of tidal debris in a Milky-Way-sized dark matter halo
• SDSS J074511.56+194926.5: Discovery of a Metal-Rich and Tidally Distorted Extremely Low Mass White Dwarf
• "Orphan" afterglows in the Universal Structured Jet Model for gamma-ray bursts
• Vertical Oscillations of Fluid and Stellar Disks
• Predicted microlensing events from analysis of Gaia Data Release 2
• Stellar Population Astrophysics (SPA) with TNG. The old open clusters Collinder 350, Gulliver 51, NGC 7044, and Ruprecht 171
• Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
• A Census of Stars and Disks in Corona Australis
• Astrometric observations of X-ray binaries using very long baseline interferometry
• The Gold Standard: Accurate Stellar and Planetary Parameters for Eight Kepler M dwarf Systems Enabled by Parallaxes
• Revised Exoplanet Radii and Habitability Using Gaia Data Release 2
• The HARPS search for southern extra-solar planets. XX. Planets around the active star BD-08:2823
• Astrometrically Registered Simultaneous Observations of the 22 GHz H${}_2$O and the 43GHz SiO masers towards R Leonis Minoris using KVN and Source/Frequency Phase Referencing
• Evaluating GAIA performances on eclipsing binaries. I. Orbits and stellar parameters for V505 Per, V570 Per and OO Peg
• The Variable Sky of Deep Synoptic Surveys
• Gaia eclipsing binary and multiple systems. Two-Gaussian models applied to OGLE-III eclipsing binary light curves in the Large Magellanic Cloud
• Searching for Failed Supernovae With Astrometric Binaries
• Filtration of atmospheric noise in narrow-field astrometry with very large telescopes
• Stellar atmosphere parameters with MAx, a MAssive compression of x^2 for spectral fitting
• Kinematics of RHB stars to trace the structure of the galaxy
• Atmospheric stellar parameters for large surveys using FASMA, a new spectral synthesis package
• The white dwarf luminosity function. I. Statistical errors and alternatives
• Spitzer, Gaia, and the Potential of the Milky Way
• Tidal disruption events from massive black hole binaries: predictions for ongoing and future surveys
• The imprint of satellite accretion on the chemical and dynamical properties of disc galaxies
• The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses
• Strong Constraints to the Putative Planet Candidate around VB 10 using Doppler spectroscopy
• Long-term stability of the HR 8799 planetary system without resonant lock
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• The evolution of streams in a time-dependent potential
• Open clusters and associations in the Gaia era
• The Most Distant Stars in the Milky Way
• Astrometric detection of exoplanets from the ground
• Dark impact and galactic star formation: Origin of the Gould belt
• Gaia astrometry for stars with too few observations - a Bayesian approach
• Catalogue of exoplanets accessible in reflected starlight to the Nancy Grace Roman Space Telescope. A population study and prospects for phase-curve measurements
• Proper motion survey and kinematic analysis of the Rho Ophiuchi embedded cluster
• Supernovae with "Super-Hipparcos"
• Action-based Dynamical Modelling for the Milky Way Disk
• Estimating cosmological parameters from future gravitational lens surveys
• A bimodal dust grain distribution in the IC 434 HII region
• The high velocity stars in the Local Stellar Halo from Gaia and LAMOST
• The Pan-Pacific Planet Search III: Five companions orbiting giant stars
• A novel method to bracket the corotation radius in galaxy disks: vertex deviation maps
• 3D Galactic dust extinction mapping with multi-band photometry
• Extending the first-order post-Newtonian scheme in multiple systems to the second-order contributions to light propagation
• The Gaia spectrophotometric standard stars survey -- V. Preliminary flux tables for the calibration of Gaia DR2 and (E)DR3
• Stellar Open Clusters' Membership Probabilities: an N-Dimensional Geometrical Approach
• A resolved, au-scale gas disk around the B[e] star HD 50138
• The membership of stars, density profile and mass segregation in open clusters using a new machine learning-based method
• A gap in the double white dwarf separation distribution caused by the common-envelope evolution: astrometric evidence from Gaia
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• Modelling radiation damage to ESA's Gaia satellite CCDs
• SDSS/SEGUE Spectral Feature Analysis For Stellar Atmospheric Parameter Estimation
• The Gaia spectrophotometric standard stars survey -II. Instrumental effects of six ground-based observing campaigns
• HALO7D I: The Line of Sight Velocities of Distant Main Sequence Stars in the Milky Way Halo
• The Late-Type Extension to MoVeRS (LaTE-MoVeRS): Proper motion verified low-mass stars and brown dwarfs from SDSS, 2MASS, and WISE
• Climbing the cosmic ladder with stellar twins
• New Signatures of the Milky Way Formation in the Local Halo and Inner Halo Streamers in the Era of Gaia
• An extremely fast halo hot subdwarf star in a wide binary system
• Fine structure of the age-chromospheric activity relation in solar-type stars I: The Ca II infrared triplet: Absolute flux calibration
• The impact of CCD radiation damage on Gaia astrometry: I. Image location estimation in the presence of radiation damage
• A new line on the wide binary test of gravity
• Detection of satellite remnants in the Galactic Halo with Gaia III. Detection limits for Ultra Faint Dwarf Galaxies
• Incorporating Streams into Milky Way Models
• Digging supplementary buried channels: investigating the notch architecture within the CCD pixels on ESA's Gaia satellite
• On the distances of planetary nebulae
• Pushing the limits of the Gaia space mission by analyzing galaxy morphology
• Implications of a wavelength dependent PSF for weak lensing measurements
• A semi-empirical library of galaxy spectra for Gaia classification based on SDSS data and PEGASE models
• Stellar ages from asteroseismology
• Kinematics of symmetric Galactic longitudes to probe the spiral arms of the Milky Way with Gaia
• The O- and B-Type Stellar Population in W3: Beyond the High-Density Layer
• Can Cosmic Parallax Distinguish Between Anisotropic Cosmologies?
• Narrow-Angle Astrometry with the Space Interferometry Mission: The Search for Extra-Solar Planets. II. Detection and Characterization of Planetary Systems
• Transit Probabilities in Secularly Evolving Planetary Systems
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• Radial velocities of early-type stars in the Perseus OB2 association
• Searching transients in large-scale surveys. A method based on the Abbe value
• Gravitational lensing of massive particles by a black-bounce-Schwarzschild black hole
• Hyades dynamics from N-body simulations: Accuracy of astrometric radial velocities from Hipparcos
• Predictions for the detection of Tidal Streams with Gaia using Great Circle Methods
• Evidence of the $Gaia$--VLBI position differences being related to radio source structure
• Electrode level Monte Carlo model of radiation damage effects on astronomical CCDs
• A Census of the 32 Ori Association with Gaia
• The Gaia-ESO Survey: N-body modelling of the Gamma Velorum cluster
• Astrometric planet search around southern ultracool dwarfs II: Astrometric reduction methods and a deep astrometric catalogue
• The slowly pulsating B-star 18 Peg: A testbed for upper main sequence stellar evolution
• Survey for Distant Stellar Aggregates in Galactic Disk: Detecting Two Thousand Star Clusters and Candidates, along with the Dwarf Galaxy IC10
• Astrobiological Complexity with Probabilistic Cellular Automata
• Detection and Characterization of Planetary Systems with $\mu$as Astrometry
• Optical Spectra of Candidate Southern Hemisphere International Celestial Reference Frame (ICRF) radio sources
• Astrometry and Exoplanets: the Gaia Era, and Beyond
• Automatic Observation Rendering (AMORE) I. On a synthetic stellar population's colour-magnitude diagram
• The Gaia spectrophotometric standard stars survey -- IV. Results of the absolute photometry campaign
• The Distances to Open Clusters from Main-Sequence Fitting. V. Extension of Color Calibration and Test using Cool and Metal-Rich Stars in NGC 6791
• Dissecting galaxy formation models with Sensitivity Analysis -- A new approach to constrain the Milky Way formation history
• Spectroscopic Survey of G and K Dwarfs in the Hipparcos Catalog. I. Comparison between the Hipparcos and Photometric Parallaxes
• A Global Correction to PPMXL Proper Motions
• On the relevance of chaos for halo stars in the solar neighbourhood II
• Velocity and abundance precisions for future high-resolution spectroscopic surveys: a study for 4MOST
• 3D hydrodynamical model atmospheres: a tool to correct radial velocities and parallaxes for Gaia
• Reconsidering the galactic coordinate system
• Very Low-Mass Stellar and Substellar Companions to Solar-like Stars From MARVELS VI: A Giant Planet and a Brown Dwarf Candidate in a Close Binary System HD 87646
• ANTARES: Progress towards building a `Broker' of time-domain alerts
• Chromaticity in all-reflective telescopes for astrometry
• Milky Way type galaxies in a LCDM cosmology
• Determination of stellar parameters with GAIA
• The stellar metallicity distribution of the Milky Way from the BATC survey
• Second Order Kerr-Newman Time Delay
• New detections of embedded clusters in the Galactic halo
• Electromagnetic signals from planetary collisions
• Motion Verified Red Stars (MoVeRS): A Catalog of Proper Motion Selected Low-mass Stars from WISE, SDSS, and 2MASS
• Relativistic gravitational deflection of light and its impact on the modeling accuracy for the Space Interferometry Mission
• Analysis of the Kinematic Structure of the Cygnus OB1 association
• The 4 Pi Sky Transient Alerts Hub
• Gaia: a Window to Large Scale Flows
• Gaia predicted brown dwarf detection rates around FGK stars in astrometry, radial velocity, and photometric transits
• Dynamical invariants and diffusion of merger substructures in time-dependent gravitational potentials
• The TEMPO Survey I: Predicting Yields of the Transiting Exosatellites, Moons, and Planets from a 30-day Survey of Orion with the Nancy Grace Roman Space Telescope
• Directly testing gravity with Proxima Centauri
• GS-TEC: the Gaia Spectrophotometry Transient Events Classifier
• Quasar variability limits on cosmological density of cosmic strings
• Liverpool Telescope 2: a new robotic facility for rapid transient follow-up
• Reliability of the measured velocity anisotropy of the Milky Way stellar halo
• A new algorithm for optimizing the wavelength coverage for spectroscopic studies: Spectral Wavelength Optimization Code (SWOC)
• Deep Extragalactic VLBI-Optical Survey (DEVOS): I. Pilot MERLIN and VLBI observations
• Using Action Space Clustering to Constrain the Accretion History of Milky Way like Galaxies
• Gravitational Deflection of Massive Particles by a Schwarzschild Black Hole in Radiation Gauge
• Astrometric Interferometry
• The CoRoT-GES Collaboration. Improving Red Giants spectroscopic surface gravity and abundances with asteroseismology
• Limits in astrometric accuracy induced by surface brightness asymmetries in red supergiant stars
• The astrometric Gaia-FUN-SSO observation campaign of 99 942 Apophis
• Quasars can be used to verify the parallax zero-point of the Tycho-Gaia Astrometric Solution
• Towards a library of synthetic galaxy spectra and preliminary results of classification and parametrization of unresolved galaxies for Gaia - II
• Velocity-space substructure from nearby RAVE and SDSS stars
• Detection of Galaxies with Gaia
• Astrometric Reverberation Mapping
• Gaia on-board metrology: basic angle and best focus
• The proper motion of HV2112: A TŻO candidate in the SMC
• Dynamical inference from a kinematic snapshot: The force law in the Solar System
• Ages of 70 dwarfs of three populations in the solar neighborhood: considering O and C abundances in stellar models
• Enabling Gaia observations of naked-eye stars
• An efficient PSF construction method
• Application of Time Transfer Function to McVittie Spacetime: Gravitational Time Delay and Secular Increase in Astronomical Unit
• Aberration in proper motions for stars in our Galaxy
• Gaia Eclipsing Binary and Multiple Systems. A study of detectability and classification of eclipsing binaries with Gaia
• Characterisation of a candidate dual AGN
• Evaluating GAIA performances on eclipsing binaries. III. Orbits and stellar parameters for UW LMi, V432 Aur and CN Lyn
• Simulated Galactic methanol maser distribution to constrain Milky Way parameters
• Observable Predictions from Perturber-coupled High-eccentricity Tidal Migration of Warm Jupiters
• Asymmetric metallicity patterns in the stellar velocity space with RAVE
• The MAVERIC survey: A catalogue of radio sources in southern globular clusters from the Australia Telescope Compact Array
• Mass estimators in the Gaia era
• M dwarfs in the b201 tile of the VVV survey: Colour-based Selection, Spectral Types and Light Curves
• Testing gravity with interstellar precursor missions
• Secular Behavior of Exoplanets: Self-Consistency and Comparisons with the Planet-Planet Scattering Hypothesis
• Detecting the Orbital Motion of Nearby Supermassive Black Hole Binaries with Gaia
• Imprints of Zero-Age Velocity Dispersions and Dynamical Heating on the Age-Velocity dispersion Relation
• Searching for the first stars with the Gaia mission
• Building the cosmic distance scale: from Hipparcos to Gaia
• Evolutionary design of photometric systems and its application to Gaia
• Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters II. Berkeley 23, King 1, NGC 559, NGC 6603 and NGC 7245
• Milky Way chemo-dynamics in the era of Gaia
• Leading-order deflection of particles by a moving Schwarzschild lens with a two-dimensional velocity
• Connecting HL Tau to the Observed Exoplanet Sample
• Microlensing Neutron Stars
• Weighted statistical parameters for irregularly sampled time series
• Kerr-Newman black hole lensing of relativistic massive particles in the weak field limit
• Structure of the nucleus of 1928+738
• Non-Parametric Spherical Jeans Mass Estimation with B-splines
• A radiation transfer model for the Milky Way. II The global properties and large scale structure
• The tilting rate of the Milky Way's disc
• Drivers of disc tilting I: Correlations and possible drivers for Milky Way analogues
• The Araucaria Project. Precise physical parameters of the eclipsing binary IO Aqr
• Collisions of Terrestrial Worlds: The Occurrence of Extreme Mid-Infrared Excesses around Low-Mass Field Stars
• Potential asteroid discoveries by the ESA Gaia mission: Results from follow-up observations
• A conjugate gradient algorithm for the astrometric core solution of Gaia
• Measuring the microlensing parallax from various space observatories
• Determination of robust metallicities for metal-rich red giant branch stars
• Masses and luminosities for 342 stars from the PennState-Toruń Centre for Astronomy Planet Search
• An application of Galactic parallax: the distance to the tidal stream GD-1
• Characterization of Exoplanet-Host Stars
• Gaia transient detection efficiency: hunting for nuclear transients
• The tightening of wide binaries in dSph galaxies through dynamical friction as a test of the Dark Matter hypothesis
• Optical Spectra of Candidate International Celestial Reference Frame (ICRF) Flat-Spectrum Radio Sources. III
• 3D maps of the local interstellar medium: searching for the imprints of past events
• SNGuess: A method for the selection of young extragalactic transients
• Local Group(s)
• The Influence of the Galactic Bar on the Dynamics of Globular Clusters
• Stellar substructures in the solar neighbourhood IV. Kinematic Group 1 in the Geneva-Copenhagen survey
• The potential of sparse photometric data in asteroid shape modeling
• Determination of astrophysical parameters of quasars within the Gaia mission
• 10 Years of Archival High-Resolution NIR Spectra: The Raw and Reduced IGRINS Spectral Archive (RRISA)
• GAIA accuracy on radial velocities assessed from a synthetic spectra database
• The Photo-Astrometric Vertical Tracer Density of the Milky Way I: The Method
• Photometric constraints on white dwarfs and the identification of extreme objects
• Some aspects of Relativistic Astrometry from within the Solar System
• Light propagation in 2PN approximation in the monopole and quadrupole field of a body at rest: Initial value problem
• Evaluating Gaia performances on eclipsing binaries. IV. Orbits and stellar parameters for SV Cam, BS Dra and HP Dra
• Detectability of GRB optical afterglows with Gaia satellite
• On the influence of radio extended structures on offsets between the optical and VLBI positions of sources in the ICRF2
• Inferring the Galactic potential with Gaia and friends: synergies with other surveys
• Spectroscopy of Candidate Members of the Sco-Cen Complex
• A direct probe of cosmological power spectra of the peculiar velocity field and the gravitational lensing magnification from photometric redshift surveys
• Gaia: the Galaxy in six (and more) dimensions
• Application of Time Transfer Functions to Gaia's global astrometry - Validation on DPAC simulated Gaia-like observations
• Spatial distribution of stellar populations in the Magellanic Clouds: Implementation to Gaia
• Variability search in M 31 using Principal Component Analysis and the Hubble Source Catalog
• The white dwarf luminosity function --II. The effect of the measurement errors and other biases
• Characterisation of close visual binaries from the AstraLux Large M Dwarf Survey
• Constraining MOND Using the Vertical Motion of Stars in the Solar Neighborhood
• Gaia: 3-dimensional census of the Milky Way Galaxy
• Ensemble age inversions for large spectroscopic surveys
• The post-linear Schwarzschild solution in harmonic coordinates: elimination of structure-dependent terms
• Astronomical distance scales in the Gaia era
• Hypercompact stellar clusters: morphological renditions and spectro-photometric models
• Intrapixel effects of CCD and CMOS detectors
• Neural network correction of astrometric chromaticity
• Opening a new window to other worlds with spectropolarimetry
• Kerr-Schild Form of the Exact Metric for a Constantly Moving Kerr Black Hole and Null Gravitational Deflection
• Spot and Facula Activity Variations of the Eccentric Detached Eclipsing Binary KIC 8098300 Based on the Time-series Orbital Solutions
• Quasars in the Galactic Anti-Center Area from the LAMOST DR3
• Obliquities of Exoplanet Host Stars from Precise Distances and Stellar Angular Diameters
• Are the Ultra-Faint Dwarf Galaxies Just Cusps?
• Using Java for distributed computing in the Gaia satellite data processing
• Comparative Planetology and the Search for Life Beyond the Solar System
• Astrometric effects of non-uniform telescope throughput
• Liverpool Telescope 2: a new robotic facility for time domain astronomy in 2020+
• A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources II: Update to the PS1 Point Source Catalog
• Influence of interstellar and atmospheric extinction on light curves of eclipsing binaries
• Satellite galaxies as better tracers of the Milky Way halo mass
• Automated Determination of Stellar Parameters from Simulated Dispersed Images for DIVA
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Total light deflection in the gravitational field of an axisymmetric body at rest with full mass and spin multipole structure
• Using microlensed quasars to probe the structure of the Milky Way
• Building Blocks of the Milky Way's Accreted Spheroid
• Perspectives of a visible instrument on the VLTI
• Connecting VLBI and Gaia celestial reference frames
• Formalism and quality of a proper motion link with extragalactic objects for astrometric satellite missions
• On the behaviour of streams in angle and frequency spaces in different potentials
• Four New Delta Scuti Pulsators from a Variability Survey of 131 Stars
• Astrometric mock observations for determining the local dark matter density
• Gravitational deflection of light in polar-axis plane of a moving Kerr-Newman black hole
• ACCESS: Enabling an Improved Flux Scale for Astrophysics
• A lower bound on the Milky Way mass from general phase-space distribution function models
• Observing the PTPS Sample of Evolved Exoplanet Host Candidates Using the NPOI
• Observational dynamics of low-mass stellar systems
• Improving LSST Photometric Calibration with Gaia Data
• Redshift determination through weighted phase correlation: a linearithmic implementation
• Chemodynamics of the Milky Way and disc formation history: insight from the RAVE and Gaia-ESO surveys
• Angular distances in metric theories
• V773 Cas, QS Aql, and BR Ind: Eclipsing Binaries as Parts of Multiple Systems
• Astrometric tests of General Relativity in the Solar System: mathematical and computational scenarios
• Improving the astrometric performance of VLTI-PRIMA
• GAIA Galaxy Survey: a multi-colour galaxy survey with GAIA
• The validation of made-to-measure method for reconstruction of phase space distribution functions
• GAVIP: A Platform for Gaia Data Analysis
• A Gaia successor with NIR Sensors
• SDSS, LSST, and Gaia: Lessons and Synergies
• Modelling the chemical evolution of the Milky Way
• Resonant Effects of a Bar on the Galactic Disk Kinematics Perpendicular to Its Plane
• Testing Planet Formation Models with Gaia $\mu$as Astrometry
• Detecting New Planets in Transiting Systems
• Parameterized second post-Newtonian framework with conservation Laws
• Benchmark stars, benchmark spectrographs: Detailed spectroscopic comparison of ESPRESSO, PEPSI, and HARPS data for Gaia benchmark stars
• The Gaia Basic angle: measurement and variations
• Asteroseismology of red giants & galactic archaeology
• The on-board data handling concept for the LOFT Large Area Detector
• Mapping the three-dimensional multi-band extinction and diffuse interstellar bands in the Milky Way with LAMOST
• The Sloan Digital Sky Survey DR7 Spectroscopic M Dwarf Catalog II: Statistical Parallax Analysis
• Light deflection in binary stars
• Low-Resolution Near-infrared Stellar Spectra Observed by the Cosmic Infrared Background Experiment (CIBER)
• Alpha-process elements in the Galaxy: a possible GAIA contribution
• Leading-order gravitational time delay of massive particles by a moving Schwarzschild lens
• Stars in the age of micro-arc-second astrometry
• Low-Mass Stars in the Sloan Digital Sky Survey: Galactic Structure, Kinematics, and the Luminosity Function
• On the loss of telemetry data in full-sky surveys from space
• Breaking the degeneracy in stellar spectral classification from single wide-band images
• Upper limits on the gravitational mass loss of the Galaxy and the LIGO burst searches
• GAIA: AGB stars as tracers of star formation histories in the Galaxy and beyond
• Testing General Relativity with Binary Lens Microlensing Events
• Radiation effects on the Gaia CCDs after 30 months at L2
• Crowding in the GAIA spectrograph focal plane
• The interferometric baselines and GRAVITY astrometric error budget
• A Vlbi Survey of Weak Extragalactic Radio Sources for the Alignment of the Icrf and the Future Gaia Frame
• Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole