The New Galaxy: Signatures of its Formation

Abstract

The formation and evolution of galaxies is one of the great outstanding problems of astrophysics. Within the broad context of hierachical structure formation, we have only a crude picture of how galaxies like our own came into existence. A detailed physical picture where individual stellar populations can be associated with (tagged to) elements of the protocloud is far beyond our current understanding. Important clues have begun to emerge from both the Galaxy (near-field cosmology) and the high redshift universe (far-field cosmology). Here we focus on the fossil evidence provided by the Galaxy. Detailed studies of the Galaxy lie at the core of understanding the complex processes involved in baryon dissipation. This is a necessary first step towards achieving a successful theory of galaxy formation.

arXiv comment51 pages (with figs embedded) + 4 colour plates. The interested reader is strongly encouraged to ignore the latex version and low res figures within; instead, download the properly typeset paper (6 Mby) and colour plates (3 Mby) from ftp://www.aao.gov.au/pub/local/jbh/araa/Galleys

References in corpus (127)

• Dark Matter Substructure in Galactic Halos
• Large scale bias and the peak background split
• Where are the missing galactic satellites?
• Dwarf Galaxies of the Local Group
• Observational evidence for self-interacting cold dark matter
• The Nucleosynthetic Signature of Population III
• Mass function of dark matter halos
• A Hipparcos census of the nearby OB associations
• GAIA: Composition, Formation and Evolution of the Galaxy
• Starburst-driven Mass Loss from Dwarf Galaxies: Efficiency and Metal Ejection
• Reionization and the abundance of galactic satellites
• A Recipe for Galaxy Formation Shaun Cole
• The Baryonic Tully-Fisher Relation
• The Ghost of Sagittarius and Lumps in the Halo of the Milky Way
• Old Stellar Populations. VI. Absorption-Line Spectra of Galaxy Nuclei and Globular Clusters
• Kinematics of Metal-Poor Stars in the Galaxy. III. Formation of the Stellar Halo and Thick Disk as Revealed from a Large Sample of Non-Kinematically Selected Stars
• Abundance Gradients and the Formation of the Milky Way
• The Stellar Population Histories of Local Early-Type Galaxies. I. Population Parameters
• Debris streams in the solar neighbourhood as relicts from the formation of the Milky Way
• A giant stream of metal-rich stars in the halo of the galaxy M31
• Neutron-Capture Elements in the Early Galaxy: Insights from a Large Sample of Metal-Poor Giants
• The Formation of Disk Galaxies
• The Effect of the Outer Lindblad Resonance of the Galactic Bar on the Local Stellar Velocity Distribution
• Detection of massive tidal tails around the globular cluster Pal 5 with SDSS commissioning data
• Great Circle tidal streams: evidence for a nearly spherical massive dark halo around the Milky Way
• Building up the Stellar Halo of the Galaxy
• Hydrodynamic Simulations of Galaxy Formation. II. Photoionization and the Formation of Low Mass Galaxies
• Quantifying the Fragility of Galactic Disks in Minor Mergers
• The 2dF Galaxy Redshift Survey: Luminosity dependence of galaxy clustering
• The Galactic Thick Disk Stellar Abundances
• Evolution of the Hubble Sequence in Hierarchical Models for Galaxy Formation
• Substructure and halo density profiles in a Warm Dark Matter Cosmology
• Elemental Abundances in QSOs: Star Formation and Galactic Nuclear Evolution at High Redshifts
• High Velocity Clouds: Building Blocks of the Local Group
• The Ages of Elliptical Galaxies in a Merger Model
• Measurement of stellar age from uranium decay
• Massive star formation in 100,000 years from turbulent and pressurized molecular clouds
• Some Revised Observational Constraints on the Formation and Evolution of the Galactic Disk
• Sagittarius: The Nearest Dwarf Galaxy
• Multiple Stellar Populations in the Globular Cluster omega Centauri as Tracers of a Merger Event
• The Kinematics, Orbit, and Survival of the Sagittarius Dwarf Spheroidal Galaxy
• The stellar populations of spiral galaxies
• 2MASS Observations of the Perseus, Orion A, Orion B, and Monoceros R2 Molecular Clouds
• NON-AXISYMMETRIC STRUCTURES IN THE STELLAR DISKS OF GALAXIES
• Fossil Signatures of Ancient Accretion Events in the Halo
• Ages of Globular Clusters from Hipparcos Parallaxes of Local Subdwarfs
• The Age Of Globular Clusters In Light Of Hipparcos: Resolving the Age Problem?
• The r-Process Enriched Low Metallicity Giant HD 115444
• A Prescription for Building the Milky Way's Halo from Disrupted Satellites
• Galactic chemical evolution of heavy elements: from Barium to Europium
• Evidence for a non-zero Lambda and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and Cosmic Microwave Background Anisotropies
• Galactic Halo substructure in the Sloan Digital Sky Survey: the ancient tidal stream from the Sagittarius dwarf galaxy
• Evidence for Secular Evolution in Late-Type Spirals
• Measuring non-axisymmetry in spiral galaxies
• The dearth of halo dwarf galaxies: is there power on short scales?
• Evidence of Multiple r-Process Sites in the Early Galaxy: New Observations of CS 22892-052
• Photoionization and the Formation of Dwarf Galaxies
• The QUEST RR Lyrae Survey: Confirmation of the Clump at 50 kpc and Other Over-Densities in the Outer Halo
• How Lumpy is the Milky Way's Dark Matter Halo?
• Probing Dark Matter Substructure in Lens Galaxies
• On the galactic disc age-metallicity relation
• Effects of Tidal Shocks on the Evolution of Globular Clusters
• The Mass of the Milky Way Galaxy
• Halo Cores and Phase Space Densities: Observational Constraints on Dark Matter Physics and Structure Formation
• The Merging History of the Milky Way
• Cosmology from large-scale structure: Constraining $\Lambda$CDM with BOSS
• The Ursa Major Cluster of Galaxies. I. Cluster Definition and Photometric Data
• Disk Galaxies and Galaxy Disks
• The solar neighbourhood age-metallicity relation - does it exist?
• Photometry and the Metallicity Distribution of the Outer Halo of M31
• The local space density of Sb-Sdm galaxies as function of their scalesize, surface brightness and luminosity
• Thickening of galactic disks through clustered star formation
• On the Destruction and Over-Merging of Dark Halos in Dissipationless N-body Simulations
• Galaxy Disruption as the Origin of Intracluster Light in the Coma Cluster
• The first generation of stars: first steps towards chemical evolution of galaxies
• A Determination of the Thick Disk Chemical Abundance Distribution: Implications for Galaxy Evolution
• Exploring Halo Substructure with Giant Stars: I. Survey Description and Calibration of the Photometric Search Technique
• The Colour-Magnitude Relation as a Constraint on the Formation of Rich Cluster Galaxies
• Globular Cluster Ages and the Formation of the Galactic Halo
• The Ages and Metallicities of Early Type Galaxies in the Fornax Cluster
• Fossil Imprints of the First Generation Supernova Ejecta in Extremely Metal-Deficient Stars
• Ring structure and warp of NGC5907 -- Interaction with dwarf galaxies
• Galaxy mapping with the SAURON integral-field spectrograph: The star formation history of NGC 4365
• Dark matter in Draco and the Local Group: Implications for direct detection experiments
• Interpreting Debris from Satellite Disruption In External Galaxies
• Galactic Indigestion: Numerical Simulations of the Milky Way's Closest Neighbor
• Th Ages for Metal-Poor Stars
• The two-point correlation function and morphological segregation in the Optical Redshift Survey
• The geometry of phase mixing
• Delayed Recombination
• The Luminosity-Metallicity Relation for Bulges of Spiral Galaxies
• The Smith Cloud: HI associated with the Sgr dwarf?
• High-Resolution Abundance Analysis of Very Metal-Rich Stars in the Solar Neighborhood
• Halo Substructure and Disk Heating in a Lambda CDM Universe
• A refurbished convergent point method for finding moving groups in the Hipparcos Catalogue
• The G Dwarf Problem Exists in Other Galaxies
• Star Formation Histories of Nearby Dwarf Galaxies
• Actinides: How well do we know their stellar production?
• Galaxy destruction and diffuse light in clusters
• The Shape and Figure Rotation of NGC 2915's Dark Halo
• Deep CCD Surface Photometry of the Edge-On Spiral NGC 4244
• Radially truncated galactic discs
• Diffuse Stellar Light at 100 kpc Scales in M87
• The Relative Age of the Thin and Thick Galactic Disks
• Is Dark Matter in Spiral Galaxies Cold Gas? I. Observational Constraints and Dynamical Clues About Galaxy Evolution
• Stellar Archaeology: a Keck Pilot Program on Extremely Metal-Poor Stars From the Hamburg/ESO Survey. I Stellar Parameters
• The distribution of nearby stars in phase space mapped by Hipparcos: I. The potential well and local dynamical mass
• Sensitive Radio Observations of High Redshift Dusty QSOs
• Constraints on the evolution of S0 galaxies in rich clusters at moderate redshifts
• Suppressing Linear Power on Dwarf Galaxy Halo Scales
• The Age of the Universe
• Mapping the Galactic Halo III. Simulated Observations of Tidal Streams
• A Younger Age for the Universe
• Evolution of Galaxies in Clusters
• Probing the Site for r-Process Nucleosyntheis with Abundances of Barium and Magnesium in Extremely Metal-Poor Stars
• The scatter in the near-infrared colour-magnitude relation in spiral galaxies
• Low-Luminosity Early-Type Galaxies in the Coma Cluster: Variations in Spectral Properties
• Global star formation history: A Local Group perspective
• Chemical enrichment and star formation in the Milky Way disk; II. Star formation history
• Evolution of the Abundance of CO, O2, and Dust in the Early Universe
• Chemical abundance patterns -- fingerprints of nucleosynthesis in the first stars
• Spectral Variations in Early-Type Galaxies as a Function of Mass
• The Kinematic and Spatial Deployment of Compact, Isolated High-Velocity Clouds
• Searching for Machos (and other Dark Matter Candidates) in a Simulated Galaxy
• Canaries in a Coal Mine: Using Globular Clusters to Place Limits on Massive Black Holes in the Galactic Halo
• Detecting Dark Matter in High Velocity Clouds
• Nuclear Chronometers

Cited by in corpus (789)

• SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
• The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
• The Galaxy in Context: Structural, Kinematic and Integrated Properties
• The Geneva-Copenhagen survey of the Solar neighbourhood: Ages, metallicities, and kinematic properties of 14,000 F and G dwarfs
• The merger that led to the formation of the Milky Way's inner stellar halo and thick disk
• Star Formation Histories, Abundances and Kinematics of Dwarf Galaxies in the Local Group
• Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood
• The First Stars
• The Radial Velocity Experiment (RAVE): first data release
• Elemental Abundance Survey of The Galactic Thick Disk
• The GALAH Survey: Scientific Motivation
• The s Process: Nuclear Physics, Stellar Models, Observations
• Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions
• Multiple populations in globular clusters. Lessons learned from the Milky Way globular clusters
• The Chemical Compositions of Galactic Disk F and G Dwarfs
• Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
• The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars
• Star Clusters Across Cosmic Time
• From rings to bulges: evidence for rapid secular galaxy evolution at z~2 from integral field spectroscopy in the SINS survey
• The GALAH+ Survey: Third Data Release
• A Survey of Star-Forming Galaxies in the z=1.4-2.5 `Redshift Desert': Overview
• The Milky Way Tomography with SDSS: II. Stellar Metallicity
• Galactic stellar haloes in the CDM model
• LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) The survey science plan
• Near-Field Cosmology with Metal-Poor Stars
• Asteroseismology of Solar-Type and Red-Giant Stars
• The First Galaxies
• Measuring the rotation period distribution of field M-dwarfs with Kepler
• A Spectroscopic Study of the Ancient Milky Way: F- and G-Type Stars in the Third Data Release of the Sloan Digital Sky Survey
• The Haunted Halos of Andromeda and Triangulum: A panorama of galaxy formation in action
• The Emergence of the Thick Disk in a CDM Universe
• Streams, substructures and the early history of the Milky Way
• The RAdial Velocity Experiment (RAVE): Fourth data release
• A New Mechanism for Radial Migration in Galactic Disks: Spiral-Bar Resonance Overlap
• The Geneva-Copenhagen Survey of the Solar neighbourhood II. New uvby calibrations and rediscussion of stellar ages, the G dwarf problem, age-metallicity diagram, and heating mechanisms of the disk
• Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure
• The GALAH Survey: Second Data Release
• The formation and assembly history of the Milky Way revealed by its globular cluster population
• What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
• Formation of the First Stars
• Galaxy Formation Theory
• Formation of globular clusters in hierarchical cosmology
• Stellar yields from metal-rich asymptotic giant branch models
• Galaxia: a code to generate a synthetic survey of the Milky Way
• Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
• Distances and ages of NGC 6397, NGC 6752 and 47 Tuc
• The Large-scale Bipolar Wind in the Galactic Center
• Thin, thick and dark discs in LCDM
• Stars beyond Galaxies: The Origin of Extended Luminous Halos around Galaxies
• Galaxy Disks
• The Milky Way has no thick disk
• A Comparison of Elemental Abundance Ratios in Globular Clusters, Field Stars, and Dwarf Spheroidal Galaxies
• Angular momentum and galaxy formation revisited
• VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies: II. Implications for Understanding Galaxy Evolution
• Oxygen Abundances in Nearby FGK Stars and the Galactic Chemical Evolution of the Local Disk and Halo
• The stellar halo of the Galaxy
• Chemodynamical evolution of the Milky Way disk II: Variations with Galactic radius and height above the disk plane
• The Milky Way's Stellar Disk
• Probing the Outer Galactic halo with RR Lyrae from the Catalina Surveys
• The Gaia-ESO Survey: the Galactic Thick to Thin Disc transition
• The NIR Ca II triplet at low metallicity - Searching for extremely low-metallicity stars in classical dwarf galaxies
• The Influence of Sagittarius and the Large Magellanic Cloud on the Milky Way Galaxy
• The nucleus of the Sagittarius dSph galaxy and M54: a window on the process of galaxy nucleation
• Globular clusters, satellite galaxies and stellar haloes from early dark matter peaks
• The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry and location
• Light Curve Templates and Galactic Distribution of RR Lyrae Stars from Sloan Digital Sky Survey Stripe 82
• Chemical Abundance Distributions of Galactic Halos and their Satellite Systems in a Lambda CDM Universe
• The Galaxy and its stellar halo: insights on their formation from a hybrid cosmological approach
• Thin disc, Thick Disc and Halo in a Simulated Galaxy
• Current Status of r-Process Nucleosynthesis
• Structure of Disk Dominated Galaxies: II. Color Gradients and Stellar Population Models
• Using chemical tagging to redefine the interface of the Galactic disk and halo
• Galactic archaeology: mapping and dating stellar populations with asteroseismology of red-giant stars
• The GALAH Survey: Observational Overview and Gaia DR1 companion
• Three Epochs of Star Formation in the High Redshift Universe
• Comparing the properties of local globular cluster systems: implications for the formation of the Galactic halo
• Chemodynamics of the Milky Way. I. The first year of APOGEE data
• Chemodynamical history of the Galactic Bulge
• The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
• From dawn till disk: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
• The evolution of the C/O ratio in metal-poor halo stars
• Stellar Population gradients in galaxy discs from the CALIFA survey
• Oxygen Abundances in Nearby Stars. Clues to the formation and evolution of the Galactic disk
• Evolution of Galactic Discs: Multiple Patterns, Radial Migration and Disc Outskirts
• Chemical tagging with APOGEE: Discovery of a large population of N-rich stars in the inner Galaxy
• On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk
• STEllar Content and Kinematics from high resolution galactic spectra via Maximum A Posteriori
• Estimating stellar birth radii and the time evolution of the Milky Way's ISM metallicity gradient
• 'Sculptor'-ing the Galaxy? The Chemical Compositions of Red Giants in the Sculptor Dwarf Spheroidal Galaxy
• Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way
• Chemical Evolution in Hierarchical Models of Cosmic Structure II: The Formation of the Milky Way Stellar Halo and the Distribution of the Oldest Stars
• The age of the oldest Open Clusters
• Structure Finding in Cosmological Simulations: The State of Affairs
• Chemical Evolution in Hierarchical Models Of Cosmic Structure I: Constraints on the Early Stellar Initial Mass Function
• SubHaloes going Notts: The SubHalo-Finder Comparison Project
• Planetary System Disruption by Galactic Perturbations to Wide Binary Stars
• From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
• Star formation history of barred disc galaxies
• Two distinct halo populations in the solar neighborhood. II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
• Accuracy and precision of industrial stellar abundances
• Radial Migration in Disk Galaxies I: Transient Spiral Structure and Dynamics
• Kinematics of the stellar halo and the mass distribution of the Milky Way using BHB stars
• Pieces of the puzzle: Ancient substructure in the Galactic disk
• The Cosmic Evolution of Metallicity from the SDSS Fossil Record
• The Long-term Evolution of the Galactic Disk Traced by Dissolving Star Clusters
• On the origin of the chemical bimodality of disk stars: A tale of merger and migration
• Pre-galactic metal enrichment - The chemical signatures of the first stars
• Chemical abundances of the Milky Way thick disk and stellar halo II.: sodium, iron-peak and neutron-capture elements
• Observations of Thick Disks in the Hubble Space Telescope Ultra Deep Field
• Elemental Abundance Ratios in Stars of the Outer Galactic Disk. IV. A New Sample of Open Clusters
• VINTERGATAN I: The origins of chemically, kinematically and structurally distinct discs in a simulated Milky Way-mass galaxy
• Verifying asteroseismically determined parameters of Kepler stars using hipparcos parallaxes: self-consistent stellar properties and distances
• Simultaneous calibration of spectro-photometric distances and the Gaia DR2 parallax zero-point offset with deep learning
• The Global Dynamical Atlas of the Milky Way mergers: Constraints from Gaia EDR3 based orbits of globular clusters, stellar streams and satellite galaxies
• The QUEST RR Lyrae Survey II: The Halo Overdensities in the First Catalog
• The influence of atomic diffusion on stellar ages and chemical tagging
• The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- II: Stellar Atmospheric Parameters, Chemical Abundances and Distances
• Reconstructing the Last Major Merger of the Milky Way with the H3 Survey
• The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- I: Survey Description, Spectra and Radial Velocities
• Spectroscopy of Red Giants in the LMC Bar: Abundances, Kinematics, and the Age-Metallicity Relation
• Measuring Radial Orbit Migration in the Milky Way Disk
• The evolution of CNO isotopes: a new window on cosmic star-formation history and the stellar IMF in the age of ALMA
• Abundances in giant stars of the globular cluster NGC 6752
• Evidence for an Intermediate-Mass Milky Way from Gaia DR2 Halo Globular Cluster Motions
• Building the Galactic halo from globular clusters: evidence from chemically unusual red giants
• Where are the most ancient stars in the Milky Way?
• On the estimation of the Local Dark Matter Density using the rotation curve of the Milky Way
• Overview of the DESI Milky Way Survey
• The origin and evolution of r- and s-process elements in the Milky Way stellar disk
• NGC 300: an extremely faint, outer stellar disk observed to 10 scale lengths
• Isochrone ages for ~3 million stars with the second Gaia data release
• Accretion relicts in the solar neighbourhood: debris from omegaCen's parent galaxy
• The chemical homogeneity of open clusters
• Deep Hubble Space Telescope Imaging of IC 1613 II. The Star Formation History
• Abundances for metal-poor stars with accurate parallaxes II. alpha-elements in the halo
• The influence of residual gas expulsion on the evolution of the Galactic globular cluster system and the origin of the Population II halo
• Chemical Homogeneity in Collinder 261 and Implications for Chemical Tagging
• Chemical Homogeneity in the Hyades
• Galactic Stellar Populations in the Era of SDSS and Other Large Surveys
• The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products
• The Dawes Review 8: Measuring the Stellar Initial Mass Function
• Phase-Space Distributions of Chemical Abundances in Milky Way-type Galaxy Halos
• Abundance Analysis of Turn-Off and Early Subgiant Stars in the Globular Cluster 47 Tuc (NGC 104)
• The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co in the Milky Way stellar disk
• Antitruncated Stellar Disks via Minor Mergers
• The Bologna Open Cluster Chemical Evolution (BOCCE) Project: midterm results from the photometric sample
• Chemically Tagging the HR1614 Moving Group
• Chemical Abundances and Kinematics in Globular Clusters and Local Group Dwarf Galaxies and Their Implications for Formation Theories of the Galactic Halo
• The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS
• The Southern Stellar Stream Spectroscopic Survey ($S^5$): Overview, Target Selection, Data Reduction, Validation, and Early Science
• The Poor Old Heart of the Milky Way
• Two distinct halo populations in the solar neighborhood. III. Evidence from stellar ages and orbital parameters
• The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?
• The Caterpillar Project: A Large Suite of Milky Way Sized Halos
• Tracing the formation of the Milky Way through ultra metal-poor stars
• The origin of the Milky Way globular clusters
• Stellar Chemical Abundances: In Pursuit of the Highest Achievable Precision
• The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
• A Study of Edge-On Galaxies with the Hubble Space Telescope's Advanced Camera for Surveys. II. Vertical distribution of the resolved stellar population
• The GALAH survey: tracing the Galactic disk with Open Clusters
• The $R$-Process Alliance: Fourth Data Release from the Search for $r$-Process-Enhanced Stars in the Galactic Halo
• Tightly Correlated X-ray/H$\alpha$ Emitting Filaments in the Superbubble and Large-Scale Superwind of NGC 3079
• Reconstructing Galaxy Histories from Globular Clusters
• A new perspective on globular clusters, their initial mass function, and their contribution to the stellar halo and to cosmic reionisation
• Exploring the Variable Sky with LINEAR. II. Halo Structure and Substructure Traced by RR Lyrae Stars to 30 kpc
• Galactic seismology: the evolving "phase spiral" after the Sagittarius dwarf impact
• 18 Sco: a solar twin rich in refractory and neutron-capture elements. Implications for chemical tagging
• Chemical Enrichment and Radial Migration in the Galactic Disk -- the origin of the [$\alpha /\mathrm{Fe}]$ Double Sequence
• Constraining the primordial initial mass function with stellar archaeology
• Evidence for a Milky Way Tidal Stream Reaching Beyond 100 kpc
• Discovery of $\sim$ 9,000 new RR Lyrae in the Southern Catalina Surveys
• An accurate and self-consistent chemical abundance catalogue for the APOGEE/Kepler sample
• High-precision stellar abundances of the elements - methods and applications
• StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
• The Inside-out Growth of the Galactic Disk
• Open clusters as key tracers of Galactic chemical evolution. III. Element abundances in Berkeley 20, Berkeley 29, Collinder 261, and Melotte 66
• PLATO as it is: a legacy mission for Galactic archaeology
• Galactic Archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE
• The mass-metallicity relation of interacting galaxies
• The origin of diverse $\alpha$-element abundances in galaxy discs
• Halo Star Streams in the Solar Neighborhood
• The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system
• Selecting accreted populations: metallicity, elemental abundances, and ages of the Gaia-Sausage-Enceladus and Sequoia populations
• The SAMI Galaxy Survey: Global stellar populations on the size-mass plane
• A Wide-Field Survey of the Fornax Dwarf Spheroidal Galaxy
• Chemical evolution of galaxies. I. A composition-dependent SPH model for chemical evolution and cooling
• On the identification of merger debris in the {\it Gaia} Era
• Elemental Abundances in Milky Way-like Galaxies from a Hierarchical Galaxy Formation Model
• $S^5$: The Orbital and Chemical Properties of One Dozen Stellar Streams
• The Hyades open cluster is chemically inhomogeneous
• Stellar Abundances for Galactic Archaeology Database IV - Compilation of Stars in Dwarf Galaxies
• Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
• Identical or fraternal twins? : The chemical homogeneity of wide binaries from Gaia DR2
• The Chemical Properties of Milky Way and M31 Globular Clusters: I. A Comparative Study
• The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and $Gaia$ eDR3
• TESS reveals that the nearby Pisces-Eridanus stellar stream is only 120 Myr old
• The Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk
• On the age heterogeneity of the Pleiades, Hyades and Sirius moving groups
• Disassembling the Galaxy with angle-action coordinates
• The Rich Are Different: Evidence from the RAVE Survey for Stellar Radial Migration
• Principal Component Analysis on Chemical Abundances Spaces
• Galactic Doppelganger: The chemical similarity among field stars and among stars with a common birth origin
• Reconstructing the Disrupted Dwarf Galaxy $Gaia$-Sausage/Enceladus Using its Stars and Globular Clusters
• The Southern Stellar Stream Spectroscopic Survey (S5): Chemical Abundances of Seven Stellar Streams
• Chemical tagging in the SDSS-III/APOGEE survey: new identifications of halo stars with globular cluster origins
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• Kronos & Krios: Evidence for accretion of a massive, rocky planetary system in a comoving pair of solar-type stars
• A panoramic view of the Milky Way analogue NGC 891
• Early turbulent mixing as the origin of chemical homogeneity in open star clusters
• In the Galactic disk, stellar [Fe/H] and age predict orbits and precise [X/Fe]
• Globular cluster number density profiles using Gaia DR2
• Revealing Substructure in the Galactic Halo - The SEKBO RR Lyrae Survey
• The vertical motion history of disk stars throughout the Galaxy
• Kinematics of Highly R-Process-Enhanced Field Stars: Evidence for an Accretion Origin and Detection of Several Groups from Disrupted Satellites
• Metallicity Fluctuation Statistics in the Interstellar Medium and Young Stars. I. Variance and Correlation
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• The chemical compositions of solar twins in the open cluster M67
• Signatures of unresolved binaries in stellar spectra: implications for spectral fitting
• The minimum stellar metallicity observable in the Galaxy
• The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
• The fraction of globular cluster second-generation stars in the Galactic halo
• Inside the whale: the structure and dynamics of the isolated Cetus dwarf spheroidal
• The Kinematics of Thick Disks in Nine External Galaxies
• Impact of radial migration on stellar and gas radial metallicity distribution
• The Stellar Content of Galaxy Halos: A Comparison between LambdaCDM Models and Observations of M31
• Whiting 1: the youngest globular cluster associated with the Sgr dSph
• Fundamental relations for the velocity dispersion of stars in the Milky Way
• High-precision abundances of elements in Kepler LEGACY stars. Verification of trends with stellar age
• The RAVE catalogue of stellar elemental abundances: first data release
• The physics of gas phase metallicity gradients in galaxies
• The Kinematics of Thick Disks in External Galaxies
• Identifying the best iron-peak and $\alpha$-capture elements for chemical tagging: The impact of the number of lines on measured scatter
• The Local Group as a time machine: studying the high-redshift Universe with nearby galaxies
• Further Evidence for a Merger Origin for the Thick Disk: Galactic Stars Along Lines-of-sight to Dwarf Spheroidal Galaxies
• The Galah Survey: Classification and diagnostics with t-SNE reduction of spectral information
• The Gaia-ESO Survey: Characterisation of the [alpha/Fe] sequences in the Milky Way discs
• An N-body/SPH Study of Isolated Galaxy Mass Density Profiles
• Two chemically similar stellar overdensities on opposite sides of the plane of the Galaxy
• Signatures of minor mergers in Milky Way-like disc kinematics: Ringing revisited
• Mining the Galactic Halo for Very Metal-Poor Stars
• Galactic halo stellar structures in the Triangulum-Andromeda region
• Search for Associations Containing Young stars (SACY): Chemical tagging IC 2391 & the Argus association
• $R$-process enhancements of Gaia-Enceladus in GALAH DR3
• The H alpha Galaxy Survey VII. The spatial distribution of star formation within disks and bulges
• Phylogeny of the Milky Way's inner disk and bulge populations: Implications for gas accretion, (the lack of) inside-out thick disk formation, and quenching
• Testing the chemical tagging technique with open clusters
• A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE
• Galaxy And Mass Assembly (GAMA): In Search of Milky-Way Magellanic Cloud Analogues
• Metal-Poor Stars and the Chemical Enrichment of the Universe
• Spectroscopic Survey of the Galaxy with Gaia II. The expected science yield from the Radial Velocity Spectrometer
• Chemical tagging can work: Identification of stellar phase-space structures purely by chemical-abundance similarity
• The evolution of the Milky Way: New insights from open clusters
• Halos of Spiral Galaxies. I. The Tip of the Red Giant Branch as a Distance Indicator
• Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
• Dark Shards: velocity substructure from Gaia and direct searches for dark matter
• The Abundance Gradient in the Extremely Faint Outer Disk of NGC 300
• Chemical gradients in the Milky Way from the RAVE data. II. Giant stars
• Clues for the origin of the fundamental metallicity relations. I: The hierarchical building up of the structure
• The Origin of the Gaussian Initial Mass Function of Old Globular Cluster Systems
• Chemical (in)homogeneity and atomic diffusion in the open cluster M67
• How magnetic activity alters what we learn from stellar spectra
• Chemically tagging the Hyades stream: Does it partly originate from the Hyades cluster?
• Galactic Chemical Evolution
• Local Surface Density of the Galactic Disk from a 3-D Stellar Velocity Sample
• The GALAH Survey: Chemodynamics of the Solar Neighbourhood
• The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc
• Prospects for chemically tagging stars in the Galaxy
• A Comparison of the Chemical Evolutionary Histories of the Galactic Thin Disk and Thick Disk Stellar Populations
• The Gaia-ESO Survey: calibration strategy
• Carbon-Enhanced Metal-Poor Stars, the Cosmic Microwave Background, and the Stellar IMF in the Early Universe
• The baryonic mass function of galaxies
• The velocity distribution of nearby stars from Hipparcos data II. The nature of the low-velocity moving groups
• Population synthesis to constrain Galactic and Stellar Physics- I- Determining age and mass of thin-disc red-giant stars
• Does the Milky Way Produce a Nuclear Galactic Wind?
• Action-space clustering of tidal streams to infer the Galactic potential
• The Stellar Populations of M33's Outer Regions IV: Inflow History and Chemical Evolution
• The Stellar Populations of M33's Outer Regions III: Star Formation History
• Galactic Bulges from HST NICMOS Observations: Global Scaling Relations
• Chemical Abundances of new member stars in the Tucana II dwarf galaxy
• Carbon-Enhanced Hyper-metal-poor Stars and the Stellar IMF at Low Metallicity
• Exploring the origin of low-metallicity stars in Milky Way-like galaxies with the NIHAO-UHD simulations
• The Stellar Halo of the Galaxy is Tilted & Doubly Broken
• Statistics of Stellar Variability from Kepler - I: Revisiting Quarter 1 with an Astrophysically Robust Systematics Correction
• A Two Micron All-Sky Survey View of the Sagittarius Dwarf Galaxy: VI. s-Process and Titanium Abundance Variations Along the Sagittarius Stream
• Orbital evolution of the Carina dwarf galaxy and self-consistent star formation history determination
• Star Clusters in Evolving Galaxies
• Comprehensive abundance analysis of red giants in the open clusters NGC 2527, 2682, 2482, 2539, 2335, 2251 and 2266
• Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
• Chemically tagging the Hyades Supercluster: A homogeneous sample of F6-K4 kinematically selected northern stars
• The Pristine survey III: Spectroscopic confirmation of an efficient search for extremely metal-poor stars
• An HST/ACS investigation of the spatial and chemical structure and sub-structure of NGC 891, a Milky Way analogue
• The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies
• Stellar mass distribution and star formation history of the Galactic disk revealed by mono-age stellar populations from LAMOST
• The impact of baryonic physics on the shape and radial alignment of substructures in cosmological dark matter haloes
• A New View of the Super Star Clusters in the Low-Metallicity Galaxy SBS 0335-052
• Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy
• On the recent star formation history of the Milky Way disk
• Chemical abundances in giants stars of the tidally disrupted globular cluster NGC 6712 from high-resolution infrared spectroscopy
• Stellar ages, masses, extinctions and orbital parameters based on spectroscopic parameters of Gaia DR3
• 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging
• Spectroscopy of Bright QUEST RR Lyrae Stars: Velocity Substructures toward Virgo
• Chemical evidence for planetary ingestion in a quarter of Sun-like stars
• Abundance-age relations with red clump stars in open clusters
• The Spatial Distribution of the Galactic First Stars I: High-Resolution N-body Approach
• Butterfly in a Cocoon, Understanding the origin and morphology of Globular Cluster Streams: The case of GD-1
• The Gaia-ESO Survey: Evidence of atomic diffusion in M67?
• The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way
• Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE
• Chemical signatures of the first star clusters
• The GALAH Survey: Verifying abundance trends in the open cluster M67 using non-LTE spectroscopy
• Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk
• Simulations of minor mergers. II. The phase-space structure of thick discs
• A comparison between the stellar and dynamical masses of six globular clusters
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• Streams in the Aquarius stellar haloes
• The Sun was not born in M 67
• Elemental Abundances of Solar Sibling Candidates
• Microarcsecond Astrometry: Science Highlights from Gaia
• Evidence of a thick disk rotation-metallicity correlation
• Star Formation Regulation and Self-Pollution by Stellar Wind Feedback
• Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars
• How Many Elements Matter?
• An HI survey of six Local Group analogs: I. Survey description and the search for high-velocity clouds
• The Chemical Evolution of Globular Clusters I. Reactive Elements and Non-Metals
• Effect of bars on the galaxy properties
• Stellar Abundance Maps of the Milky Way Disk
• Identifying Contributions to the Stellar Halo from Accreted, Kicked-Out, and In Situ Populations
• Quantitative chemical tagging, stellar ages and the chemo-dynamical evolution of the Galactic disc
• Evidence of tidal debris from Omega Cen in the Kapteyn Group
• Prospects for Measuring Abundances of >20 Elements with Low-resolution Stellar Spectra
• Red thick disks of nearby galaxies
• Carbon-Rich Mira Variables: Kinematics and Absolute Magnitudes
• The GALAH survey: Chemical Tagging of Star Clusters and New Members in the Pleiades
• The Galactic Thick Disc density profile traced with RR Lyrae stars
• Chemical abundances in bright giants of the globular cluster M62 (NGC 6266)
• Thick disk kinematics from RAVE and the solar motion
• Metal Mixing and Ejection in Dwarf Galaxies is Dependent on Nucleosynthetic Source
• The evolution of CNO elements in galaxies
• Beyond the two-infall model I. Indications for a recent gas infall with Gaia DR3 chemical abundances
• Science Programs for a 2 m-class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope
• Cosmic phylogeny: reconstructing the chemical history of the solar neighbourhood with an evolutionary tree
• The chemistry of the most metal-rich damped Lyman $\alpha$ systems at z$\sim 2$ II. Context with the Local Group
• Unmixing the Galactic Halo with RR Lyrae tagging
• Fundamental properties of five Kepler stars using global asteroseismic quantities and ground-based observations
• Weighing the Galactic disk using phase-space spirals II. Most stringent constraints to a thin dark disk using Gaia EDR3
• Rotation and Lithium Confirmation of a 500 Parsec Halo for the Open Cluster NGC 2516
• Detection of a population of carbon-enhanced metal-poor stars in the Sculptor dwarf spheroidal galaxy
• The stellar Initial Mass Function of the solar neighbourhood revealed by Gaia
• Chemical separation of disc components using RAVE
• The homogeneity of the star forming environment of the Milky Way disk over time
• Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
• Quantifying Chemical Tagging: Towards Robust Group Finding in the Galaxy
• Search for giant planets in M67 I. Overview
• Chemical Abundances of the Outer Halo Stars in the Milky Way
• On the Predicted and Observed Color Boundaries of the RR Lyrae Instability Strip as a Function of Metallicity
• Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
• The UK Infrared Telescope M33 monitoring project. V. The star formation history across the galactic disc
• Radial Migration of the Sun in the Milky Way: a Statistical Study
• Deep SDSS optical spectroscopy of distant halo stars II. Iron, calcium, and magnesium abundances
• A Disk Origin for the Monoceros Ring and A13 Stellar Overdensities
• Identifying Sagittarius Stream Stars By Their APOGEE Chemical Abundance Signatures
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• High Velocity Cloud Complex H: A Satellite of the Milky Way in a Retrograde Orbit?
• The INT/WFC survey of the Monoceros Ring: Accretion origin or Galactic Anomaly?
• The Pristine survey -- XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3
• 3D Spectrophotometry of Planetary Nebulae in the Bulge of M31
• On the 3 dimensional structure of edge-on disk galaxies
• The investigation of ELAIS field by Vega photometry: Absolute - magnitude dependent on the Galactic model parameters
• The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region
• Integrated Light Chemical Tagging Analyses of Seven M31 Outer Halo Globular Clusters from the Pan-Andromeda Archaeological Survey
• VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies
• Star Formation in the Most Distant Molecular Cloud in the Extreme Outer Galaxy: A Laboratory of Star Formation in an Early Epoch of the Galaxy's Formation
• Renegade Subhaloes in the Local Group
• Reconstructing fossil sub-structures of the Galactic disk: clues from abundance patterns of old open clusters and moving groups
• The GALAH Survey and Gaia DR2: (Non)existence of five sparse high-latitude open clusters
• Metallicity Bias in the Kinematics of the Milky Way Stellar Halo
• The Gaia-ESO Survey: Properties of the intermediate age open cluster NGC 4815
• Comprehensive abundance analysis of red giants in the open clusters NGC 1342, 1662, 1912, 2354 and 2447
• Using APOGEE Wide Binaries to Test Chemical Tagging with Dwarf Stars
• The Stellar Populations of M33's Outer Regions II: Deep ACS Imaging
• Abundances in the Milky Way across five nucleosynthetic channels from 4 million LAMOST stars
• A CCD Study of High Latitude Galactic Structure: Testing the Model Parameters
• Thin disk kinematics from RAVE and the solar motion
• New Light on the Initial Mass Function of the Galactic Halo Globular Clusters
• The Gaia-ESO Survey: the selection function of the Milky Way field stars
• Contrasting the chemical evolution of the Milky Way and Andromeda galaxies
• Galaxy Genesis -- unravelling the epoch of dissipation in the early disk
• Disruption of a Dwarf Galaxy Under Strong Shocking: The Origin of omega Centauri
• Strong chemical tagging with APOGEE: 21 candidate star clusters that have dissolved across the Milky Way disc
• All quiet in the outer halo: chemical abundances in the globular cluster Pal 3
• The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• Dynamics for Galactic Archaeology
• Wide Binaries in Tycho-Gaia II: Metallicities, Abundances, and Prospects for Chemical Tagging
• The GALAH Survey: Accurate Radial Velocities and Library of Observed Stellar Template Spectra
• High resolution elemental abundance analysis of the Hyades Supercluster
• The GALAH Survey: Chemical Clocks
• The detailed chemical abundance patterns of accreted halo stars from the optical to infrared
• Open Cluster Chemical Homogeneity Throughout the Milky Way
• Detection of satellite remnants in the Galactic Halo with Gaia - I. The effect of the Galactic background, observational errors and sampling
• Observational constraints on the origin of the elements. VII. NLTE analysis of Y II lines in spectra of cool stars and implications for Y as a Galactic chemical clock
• The Scaleheight of Giant Molecular Clouds is Less than that of Smaller Clouds
• BVI photometry of the very old open cluster Berkeley 17
• The Natural Science Underlying Big History
• Mixing of metals during star cluster formation: statistics and implications for chemical tagging
• Stellar metallicity variations across spiral arms in disk galaxies with multiple populations
• The GALAH Survey: Stellar streams and how stellar velocity distributions vary with Galactic longitude, hemisphere and metallicity
• The chemical composition of globular clusters in the Local Group
• Scalar perturbations in $f(T)$ gravity using the $1+3$ covariant approach
• A variational encoder-decoder approach to precise spectroscopic age estimation for large Galactic surveys
• Chemo-kinematics of the Milky Way from the SDSS-III MARVELS Survey
• The (im)possibility of strong chemical tagging
• The age-metallicity relation in the solar neighbourhood from a pilot sample of white dwarf-main sequence binaries
• Streams Going Notts: The tidal debris finder comparison project
• Exploring the outskirts of globular clusters: the peculiar kinematics of NGC 3201
• Spectrum Syntheses of High Resolution Integrated Light Spectra of Galactic Globular Clusters
• The Abundances of Light Neutron-Capture Elements in Planetary Nebulae III. The Impact of New Atomic Data on Nebular Selenium and Krypton Abundance Determinations
• The hunt for the Milky Way's accreted disc
• A Wide-Field View of Leo II -- A Structural Analysis Using the SDSS
• The [α/Fe]-[Fe/H] relation in the E-MOSAICS simulations: its connection to the birth place of globular clusters and the fraction of globular cluster field stars in the bulge
• Most "young" $\alpha$-rich stars have high masses but are actually old
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• From giant clumps to clouds -- II. The emergence of thick disc kinematics from the conditions of star formation in high redshift gas rich galaxies
• Yule-Simpson's paradox in Galactic Archaeology
• Properties of carbon stars in the Solar neighbourhood based on Gaia DR2 astrometry
• The Pristine survey XIII: Uncovering the very metal-poor tail of the thin disc
• The Vertical Metallicity Gradient of the Milky Way Disk: Transitions in [a/Fe] Populations
• The dimensionality of stellar chemical space using spectra from the Apache Point Observatory Galactic Evolution Experiment
• Precise reddening and metallicity of NGC6752 from FLAMES spectra
• Maximum Likelihood Fitting of Tidal Streams With Application to the Sagittarius Dwarf Tidal Tails
• Blind chemical tagging with DBSCAN: prospects for spectroscopic surveys
• On the relation between radial alignment of dark matter subhalos and host mass in cosmological simulations
• The stellar metallicity distribution of disc galaxies and bulges in cosmological simulations
• Detailed abundance analysis of globular clusters in the Local Group: NGC 147, NGC 6822, and Messier 33
• The most ancient spiral galaxy: a 2.6-Gyr-old disk with a tranquil velocity field
• Estimating stellar ages and metallicities from parallaxes and broadband photometry - successes and shortcomings
• Migration and Mixing in the Galactic Disc from Encounters between Sagittarius and the Milky Way
• Insight Into the Formation of the Milky Way Through Cold Halo Substructure. II. The Elemental Abundances of ECHOS
• The K2 Galactic Caps Project -- Going Beyond the \textit{Kepler} Field and Ageing the Galactic Disc
• The stellar population content of the thick disk and halo of the Milky Way analogue NGC 891
• Iron-peak elements Sc, V, Mn, Cu and Zn in Galactic bulge globular clusters
• [Mg/Fe] ratios in the solar neighbourhood: stellar yields and chemical evolution scenarios
• The Pristine Inner Galaxy Survey (PIGS) V: a chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge
• Chemical Abundances for Seven Giant Stars in M68 (NGC 4590) : A Globular Cluster with Abnormal Silicon and Titanium Abundances
• Reconstructing the Accretion History of the Galactic Stellar Halo from Chemical Abundance Ratio Distributions
• Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• The RAdial Velocity Experiment (RAVE): Parameterisation of RAVE spectra based on convolutional neural networks
• The innate origin of radial and vertical gradients in a simulated galaxy disc
• StePar: an automatic code to infer stellar atmospheric parameters
• On the Red Giant Branch: Ambiguity in the Surface Boundary Condition Leads to ~100 K Uncertainty in Model Effective Temperatures
• High-resolution elemental abundance analysis of the open cluster IC 4756
• Chemical inhomogeneities in the Pleiades: signatures of rocky-forming material in stellar atmospheres
• Deciphering the evolution of the Milky Way discs: Gaia APOGEE Kepler giant stars and the Besançon Galaxy Model
• Stellar Population Astrophysics (SPA) with TNG Atmospheric parameters of members of 16 unstudied open clusters
• Tracing the anemic stellar halo of M101
• Know thy star, know thy planet: Chemo-kinematically characterizing TESS targets
• Reliability and limitations of inferring birth radii in the Milky Way disk
• The case for high precision in elemental abundances of stars in the era of large spectroscopic surveys
• RR Lyrae in XSTPS: The halo density profile in the North Galactic Cap
• Chromospherically Active Stars in the RAVE Survey. II. Young dwarfs in the Solar neighborhood
• Constraining the Galactic potential via action-based distribution functions for mono-abundance stellar populations
• On the correlation between the recent star formation rate in the Solar Neighbourhood and the glaciation period record on Earth
• Four-hundred Very Metal-poor Stars studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency
• Orbital Torus Imaging: Using Element Abundances to Map Orbits and Mass in the Milky Way
• The Quest for the Sun's Siblings: an Exploratory Search in the Hipparcos Catalogue
• The radial metallicity gradient and the history of elemental enrichment in M81 through emission-line probes
• Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
• APOGEE chemical tagging constraint on the maximum star cluster mass in the $\alpha$-enhanced Galactic disk
• The Stellar Halo Metallicity - Luminosity Relationship for Spiral Galaxies
• Kinematic structures of the Solar neighbourhood revealed by Gaia DR1/TGAS and RAVE
• The metallicity distributions in high-latitudes with SDSS
• The extended structure of the remote cluster B514 in M31. Detection of extra-tidal stars
• Timing the Milky Way bar formation and the accompanying radial migration episode
• Reading the CARDs: the Imprint of Accretion History in the Chemical Abundances of the Milky Way's Stellar Halo
• Elemental Abundances in M31: Gradients in the Giant Stellar Stream
• A homogeneous spectroscopic analysis of a Kepler legacy sample of dwarfs for gravity-mode asteroseismology
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• Constructing Polynomial Spectral Models for Stars
• Study of the stellar population properties in the discs of ten spiral galaxies
• NGC 5694: another foster son of the Galactic Halo
• Chemical compositions of stars in two stellar streams from the Galactic thick disk
• Detailed Chemical Abundances of Four Stars in the Unusual Globular Cluster, Palomar 1
• Mapping the Galactic Halo with blue horizontal branch stars from the 2dF quasar redshift survey
• The horizontal branch luminosity vs metallicity in M31 globular clusters
• Vertical and radial metallicity gradients in high latitude galactic fields with SDSS
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Effects of the selection function on metallicity trends in spectroscopic surveys of the Milky Way
• APOGEE spectroscopic evidence for chemical anomalies in dwarf galaxies: The case of M~54 and Sagittarius
• Origin of chemical and dynamical properties of the Galactic thick disk
• Combined APOGEE-GALAH stellar catalogues using the Cannon
• Age Determination of Galaxy Merger Remnant Stars using Asteroseismology
• Slicing The Monoceros Overdensity with Suprime-Cam
• Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes
• Stellar over-densities in the halo: the extent of the Virgo over-density
• A Two-Point Correlation Function For Galactic Halo Stars
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Hunting the Parent of the Orphan Stream II: The First High-Resolution Spectroscopic Study
• The GALAH Survey and Symbiotic Stars. I. Discovery and follow-up of 33 candidate accreting-only systems
• Multiwavelength Absolute Magnitudes and Colours of Red Clump Stars in {\it Gaia} Era
• Stars on the run: escaping from stellar clusters
• The Galactic Stellar Disc
• The radial alignment of dark matter subhalos: from simulations to observations
• Chemical tagging of the Ursa Major moving group: A northern selection of FGK stars
• STREAMFINDER II: A possible fanning structure parallel to the GD-1 stream in Pan-STARRS1
• The $Gaia$-ESO Survey: the inner disk intermediate-age open cluster NGC 6802
• Cosmic Renaissance: The First Sources of Light
• Jurassic: A Chemically Anomalous Structure in the Galactic Halo
• The GALAH Survey: Chemically tagging the Fimbulthul stream to the globular cluster $\omega$ Centauri
• The velocity ellipsoid in the Galactic disc using Gaia DR1
• Chemical Abundance Study of One Red Giant Star in NGC 5694 : A Globular Cluster with Dwarf Spheroidals' Chemical Signature?
• The thick disk rotation-metallicity correlation as a fossil of an "inverse chemical gradient" in the early Galaxy
• The Sextet Arcs: a Strongly Lensed Lyman Break Galaxy in the ACS Spectroscopic Galaxy Survey towards Abell 1689
• Residual Abundances in GALAH DR3: Implications for Nucleosynthesis and Identification of Unique Stellar Populations
• Optical Imaging and Spectroscopy of the Edge-On Sbc Galaxy UGC10043: Evidence for a Galactic Wind and a Peculiar Triaxial Bulge
• When was the Large Magellanic Cloud accreted onto the Galaxy ?
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Chemical Signature Indicating A Lack of Massive Stars in Dwarf Galaxies
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk
• Accelerated Fitting of Stellar Spectra
• A metallicity study of F, G, K and M dwarfs in the Coma Berenices open cluster from the APOGEE survey
• Titans metal-poor reference stars. I. Accurate effective temperatures and surface gravities for dwarfs and subgiants from 3D non-LTE H$\alpha$ profiles and Gaia parallaxes
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• The intrinsic ellipticity of dwarf spheroidal galaxies: constraints from the Andromeda system
• On the Identification of Wide Binaries in the Kepler Field
• The high velocity stars in the Local Stellar Halo from Gaia and LAMOST
• Hot Jupiters, cold kinematics: High phase space densities of host stars reflect an age bias
• Towards a better understanding of the distance scale from RR Lyrae variable stars: A case study for the inner halo globular cluster NGC 6723
• A Recommendation Algorithm to Predict Giant Exoplanet Host Stars Using Stellar Elemental Abundances
• The nature of the Milky Way's stellar halo revealed by the three integrals of motion
• A phylogenetic approach to chemical tagging. Reassembling open cluster stars
• Three new bricks in the wall: Berkeley 23, Berkeley 31, and King 8
• The Sloan digital sky survey data release 7 spectroscopic m dwarf catalog iii: The spatial dependence of magnetic activity in the galaxy
• The metallicity distribution of F/G dwarfs derived from BATC survey data
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• From birth associations to field stars: mapping the small-scale orbit distribution in the Galactic disc
• The AMBRE Project: Solar neighbourhood chemodynamical constraints on Galactic disc evolution
• New Signatures of the Milky Way Formation in the Local Halo and Inner Halo Streamers in the Era of Gaia
• The GALAH Survey: Accreted stars also inhabit the Spite Plateau
• The substructures in the local stellar halo from Gaia and LAMOST
• Chemically peculiar A and F stars with enhanced s-process and iron-peak elements: stellar radiative acceleration at work
• Binary fractions of G and K dwarf stars based on the Gaia EDR3 and LAMOST DR5: impacts of the chemical abundances
• The Outskrits of Spiral Galaxies: Evidence for Multiple Stellar Populations
• SMHASH: Anatomy of the Orphan Stream using RR Lyrae stars
• Optimal Integrated Abundances for Chemical Tagging of Extragalactic Globular Clusters
• On the Chemical and Kinematic Consistency Between N-rich Metal-poor Field Stars and Enriched Populations in Globular Clusters
• The Kapteyn moving group is not tidal debris from $\omega$ Centauri
• The stellar metallicity distribution in intermediate latitude fields with BATC and SDSS data
• Comprehensive abundance analysis of red giants in the open clusters Stock 2, NGC 2168, 6475, 6991 and 7762
• Quest for finding the lost siblings of the Sun
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• A prescription and fast code for the long-term evolution of star clusters - II. Unbalanced and core evolution
• Detection of Satellite Remnants in the Galactic Halo with Gaia - II. A modified Great Circle Cell Method
• VISTA's view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge
• Age-metallicity dependent stellar kinematics of the Milky Way disc from LAMOST and Gaia
• Super-Earth ingestion can explain the anomalously high metal abundances of M67 Y2235
• Disentangled Representation Learning for Astronomical Chemical Tagging
• Machine learning in APOGEE: Identification of stellar populations through chemical abundances
• Self-consistent simulations of star cluster formation from gas clouds under the influence of galaxy-scale tidal fields
• An old, metal-rich accreted stellar component in the Milky Way stellar disk
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• A kinematic calibration of the O-rich Mira variable period-age relation from Gaia
• Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors
• Dark matter substructures affect dark matter-electron scattering in xenon-based direct detection experiments
• The Gaia-ESO Survey: The inner disc, intermediate-age open cluster Pismis 18
• Triggering the Formation of Halo Globular Clusters with Galaxy Outflows
• On the relevance of chaos for halo stars in the solar neighbourhood II
• The GALAH survey: Co-orbiting stars and chemical tagging
• Stellar Signatures of Inhomogeneous Big Bang Nucleosynthesis
• A revisited study of Cepheids in open clusters in the Gaia era
• The GALAH+ Survey: A New Library of Observed Stellar Spectra Improves Radial Velocities and Hints at Motions within M67
• The Orbit and Origin of the Ultra-faint Dwarf Galaxy Segue 1
• A new set of chisels for Galactic archaeology: Sc, V and Zn as taggers of accreted globular clusters
• The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS) I: A Pilot Study of the stellar populations in NGC 2298 and NGC 3201
• Velocity and abundance precisions for future high-resolution spectroscopic surveys: a study for 4MOST
• Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
• Origin of a massive hyper-runaway subgiant star LAMOST-HVS1 -- implication from Gaia and follow-up spectroscopy
• The contribution of halo red giant mass loss to the high-velocity gas falling onto the Milky Way disk
• The consistency of chemical clocks among coeval stars
• Cardinal kinematics: I. Rotation fields of the APOGEE Survey
• Peeking beneath the precision floor I: metallicity spreads and multiple elemental dispersions in the globular clusters NGC 288 and NGC 362
• The Gaia-ESO Survey: Separating disk chemical substructures with cluster models
• A data-driven model of nucleosynthesis with chemical tagging in a lower-dimensional latent space
• Correlations between age, kinematics, and chemistry as seen by the RAVE survey
• One Star to Tag Them All (OSTTA): I. Radial velocities and chemical abundances for 20 poorly studied open clusters
• Star Cluster Ages in the Gaia Era
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• Properties of galaxies with ring structures
• The HR 1614 moving group is not a dissolving cluster
• HE 0017+0055 : A probable pulsating CEMP-rs star and long-period binary
• A geostatistical analysis of multiscale metallicity variations in galaxies [II]: Predicting the metallicities of Hii and diffuse ionised gas regions via universal kriging
• Remarkable migration of the solar system from the innermost Galactic disk; a wander, a wobble, and a climate catastrophe on the Earth
• The Implications of Local Fluctuations in the Galactic Midplane for Dynamical Analysis in the Gaia Era
• The kinematics of the Local Group in a cosmological context
• Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO) II. t-SNE Portrait of Local Fossil Relics and Structures
• Inference of stellar parameters from brightness variations
• Chemo-Dynamical Clustering applied to APOGEE data: Re-Discovering Globular Clusters
• Searching for Solar Siblings in APOGEE and $Gaia$ DR2 with N-body Simulations
• A new algorithm for optimizing the wavelength coverage for spectroscopic studies: Spectral Wavelength Optimization Code (SWOC)
• Ghosts of Milky Way's past: the globular cluster ESO 37-1 (E 3)
• The Parent Populations of 6 groups identified from Chemical Tagging in the Solar neighborhood
• Tracing birth properties of stars with abundance clustering
• The Gaia-ESO Survey: Chemical tagging in the thin disk. Open clusters blindly recovered in the elemental abundance space
• Investigating the amplitude and rotation of the phase spiral in the Milky Way outer disc
• The horizontal branch morphology of M31 globular clusters. Extreme second parameter effect in outer halo clusters
• A Unified Exploration of the Chronology of the Galaxy
• Exploring the chemodynamics of metal-poor stellar populations
• Abundance ties: Nephele and the globular cluster population accreted with $\omega$ Cen. Based on APOGEE DR17 and Gaia EDR3
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Kinematics of the Galactic disk from LAMOST Dwarf sample
• Simulating a White Dwarf-dominated Galactic Halo
• High Velocity Stars in SDSS/APOGEE DR17
• Galactic Archaeology with CoRoT and APOGEE: Creating mock observations from a chemodynamical model
• Chemical Evolution of R-process Elements in Stars (CERES): IV. An observational run-up of the third r-process peak with Hf, Os, Ir, and Pt
• Possible Streams of the Globular Clusters in the Galaxy
• On the origin of the radial mass density profile of the Galactic halo Globular Cluster System
• Testing the chemical homogeneity of chemically tagged dissolved birth clusters
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Stellar Over-densities in the Outer Halo of the Milky Way
• Absorption Lines in the 0.91-1.33 $\mu$m Spectra of Red Giants for Measuring Abundances of Mg, Si, Ca, Ti, Cr, and Ni
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Metallicities and ages of stellar populations at a high Galactic latitude field
• Old open clusters and the Galactic metallicity gradient: Berkeley 20, Berkeley 66, and Tombaugh 2
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Kinematically Detected Halo Streams
• Chemical abundance analysis of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy
• A high fidelity Milky Way simulation with Kraken, Gaia-Enceladus, and Sequoia analogues: clues to their accretion histories
• Structure and Evolution of the Milky Way
• Implications of the spectroscopic abundances in α Centauri A and B
• Holistic spectroscopy: Complete reconstruction of a wide-field, multi-object spectroscopic image using a photonic comb
• Asymmetric metallicity patterns in the stellar velocity space with RAVE
• Exploring the origin of the extended main sequence turn off in M37 through the white dwarf cooling sequence
• Prospecting for chemical tags among open clusters
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• The structure of the Galactic halo: SDSS versus SuperCOSMOS
• Booms and Busts: the Burstiness of Star Formation in Nearby Dwarf Galaxies
• Clustering in the Stellar Abundances Space
• Imprints of Zero-Age Velocity Dispersions and Dynamical Heating on the Age-Velocity dispersion Relation
• Local Stellar Kinematics from RAVE data -- VIII. Effects of the Galactic Disc Perturbations on Stellar Orbits of Red Clump Stars
• The Gaia-ESO Survey: α-abundances of metal-poor stars
• The heavy-elements heritage of the falling sky
• The GALAH Survey: No chemical evidence of an extragalactic origin for the Nyx stream
• The chemical enrichment of the Milky Way disk evaluated using conditional abundances
• High-resolution near-infrared spectroscopy of globular cluster and field stars toward the Galactic bulge
• Towards Studying Hierarchical Assembly in Real Time: A Milky Way Progenitor Galaxy at z = 2.36 under the Microscope
• Using heritability of stellar chemistry to reveal the history of the Milky Way
• Spatial and Kinematic Clustering of Stars in the Galactic Disk
• A high resolution, multi-epoch spectral atlas of peculiar stars including RAVE, GAIA and HERMES wavelength ranges
• The in situ origin of the globular cluster NGC 6388 from abundances of Sc, V, and Zn of a large sample of stars
• Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field
• Mass and Age determination of the LAMOST data with different Machine Learning methods
• Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal) II. Unveiling the formation and evolution of the kinematically selected Thick and Thin Discs
• Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
• The 300km/s stellar stream near Segue 1: Insights From high-resolution spectroscopy of its brightest star
• Tidal debris from Omega Centauri discovered with unsupervised machine learning
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• Galaxy archaeology for wet mergers: Globular cluster age distributions in the Milky Way and nearby galaxies
• Exploring Hydrodynamic Instabilities along the Infalling High-Velocity Cloud Complex A
• First Light Results from the Hermes Spectrograph at the AAT
• From light to mass: accessing the initial and present-day Galactic globular cluster mass functions
• How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
• Internal calibration of LAMOST and Gaia DR3 GSP-Spec stellar abundances
• Reliable stellar abundances of individual stars with the MUSE integral-field spectrograph
• A Hierarchical Model for the Ages of Galactic Halo White Dwarfs
• More pieces of the puzzle: Chemistry and substructures in the Galactic thick disk
• An optimized Method to Identify RR Lyrae stars in the SDSS X Pan-STARRS1 Overlapping Area Using a Bayesian Generative Technique
• A high-resolution spectroscopic study of two new Na- and Al-rich field giants -- likely globular cluster escapees in the Galactic halo
• The Aquarius Co-Moving Group is Not a Disrupted Classical Globular Cluster
• A GALAH View of the Chemical Homogeneity and Ages of Stellar Strings Identified in Gaia
• Traits for chemical evolution in solar twins: Trends of neutron-capture elements with stellar age
• The GALAH Survey: Dependence of elemental abundances on age and metallicity for stars in the Galactic disc
• Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc
• High-Resolution Chemical Abundances of the Nyx Stream
• RR Lyrae stars as probes of the outer Galactic halo: Chemical and kinematic analysis of a pilot sample
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages
• Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Local Group(s)
• Candidate List of Edge-on Galaxies with Substantial Extraplanar Dust
• The GALAH Survey: Stellar parameters and abundances for 800,000 Gaia RVS spectra using GALAH DR4 and The Cannon
• Elemental abundances of intermediate age open cluster NGC 3680
• Chemodynamic evolution of Sun-like stars in nearby moving groups
• A spectroscopic survey of faint, high-galactic latitude red clump stars. II. The medium resolution sample
• NGC 765 - A disturbed H I giant
• Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
• Chemical evolution of star clusters
• The Radial Distribution of Mono-Metallicity Populations in the Galactic Disk as Evidence for Two-Phase Disk Formation
• Origins and Interpretation of Tidal Debris
• Bar-spiral interaction produces radial migration and star formation bursts
• Measuring Dwarf Galaxy Intrinsic Abundance Scatter with Mid-resolution Spectroscopic Surveys: Calibrating APOGEE Abundance Errors
• Spectroscopic analysis of the bulge Globular Cluster ESO~456-SC38
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• Towards 21st Century Stellar Models: Star Clusters, Supercomputing, and Asteroseismology
• Two substructures in the nearby stellar halo found in Gaia and RAVE
• Resolved Stellar Populations as Tracers of Outskirts
• Metallicity Calibration and Photometric Parallax Estimation: II. SDSS photometry
• The Lives of Stars: Insights From the TGAS-RAVE-LAMOST Dataset
• Outer Spiral Disks as Clues to Galaxy Formation and Evolution
• Detection of Open Cluster Members Inside and Beyond Tidal Radius by Machine Learning Methods Based on Gaia DR3
• Chemodynamics of metal-poor wide binaries in the Galactic halo: Association with the Sequoia event
• Mapping the Distant and Metal-Poor Milky Way with SDSS-V
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Spectroscopic Observations of Obscured Populations in the Inner Galaxy: 2MASS-GC02, Terzan 4, and the 200 km/s stellar peak
• Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF
• Studying stellar populations in Omega Centauri with phylogenetics
• Automatic line selection for abundance determination in large stellar spectroscopic surveys
• Turbulent gas-rich discs at high redshift: origin of thick stellar discs through 3D 'baryon sloshing'
• The Astrophysical Variance in Gaia-RVS Spectra
• The GALAH survey: Multiple stars and our Galaxy. I. A comprehensive method for deriving properties of FGK binary stars
• The Impact of Inelastic Collisions with Hydrogen on NLTE Copper Abundances in Metal-Poor Stars
• Galactic Archeology with 4MOST
• From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
• Nearby stellar substructures in the Galactic halo from DESI Milky Way Survey Year 1 Data Release
• Blue Straggler Stars: Early Observations that Failed to Solve the Problem
• Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• Tracing the origin of moving groups I. The γ Leo moving group with high resolution spectra from the Subaru Telescope
• Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
• Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• A baseline on the relation between chemical patterns and birth stellar cluster
• Tracking Cluster Debris (TraCD)- I. Dissolution of clusters and searching the solar cradle
• Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs
• Introduction to Tidal Streams
• Omega Centauri: weak MgH-band in red giants directly trace the helium content
• The Chemodynamical Nature of the Triangulum-Andromeda Overdensity
• GALAH Survey: Chemically Tagging the Thick Disk
• Galactic Stellar Populations from Photometric Metallicity Distribution Functions
• The Gaia-ESO Survey astrophysical calibration
• Tomography of stellar halos: what does anisotropy in a stellar halo tell us?
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• The K2 Galactic Archaeology Program: Overview, target selection and survey properties
• A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5<z<2.5$
• Metallicity distributions in and around galaxies
• Chemodynamics of the Milky Way and disc formation history: insight from the RAVE and Gaia-ESO surveys
• Quantifying chemical and kinematical properties of Galactic disks
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Milky Way's Metal-Poor Stars display Chemical Transition near the Solar Radius
• iota Horologii is unlikely to be an evaporated Hyades star
• Dissecting stellar populations with manifold learning I. Validation of the method on a synthetic Milky Way-like galaxy
• Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Identifying substructure associations in the Milky Way halo using chemo-kinematic tagging
• Solar twins in Gaia DR3 GSP-Spec I. Building a large catalog of Solar twins with ages
• Radial Mixing due to Spiral-Bar Resonance Overlap: Implications to the Milky Way
• The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates
• The broadening of the main sequence in the open cluster M38
• A Universal Vertical Stellar Density Distribution Law for the Galaxy
• Chemical abundances of field halo stars -- Implications for the building blocks of the Milky Way
• Radial Migration in Spiral Galaxies
• Parametrization of the Galactic Structure by two exponentials
• Studying Young Stars with Large Spectroscopic Surveys
• New families in our Solar neighborhood: applying Gaussian Mixture models for objective classification of structures in the Milky Way and in simulations
• What will Gaia tell us about the Galactic disk?
• Low mass variable stars in the globular cluster NGC 6397
• The odd bunch: chrono-chemo-dynamics of sixteen unusual stars from Kepler
• Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions
• A new moving group in the Local Arm
• Asteroseismology of red giants & galactic archaeology
• The metal-poor tail of the APOGEE survey I. Uncovering [Fe/H] < -2.5 stars from the inner Galaxy to the Magellanic Clouds
• Two faces of Gaia-Sausage-Enceladus: Mining the chemical abundance space with graph attention networks
• Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
• HR-GO II: chemical abundances of low-$E$ retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
• On the connection between nitrogen-enhanced field stars and the Galactic globular clusters
• Chemical tagging experiment with the Gaia-ESO open clusters
• Caveats about measuring carbon abundances in stars using the CH band
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• Evolution of action-space coherence in a Milky Way-like simulation
• Searching for and characterizing halo substructures with the GALAH DR4 survey
• Double Trouble: How Unresolved Spectroscopic Binary Stars Skew GALAH DR4 Stellar Parameters
• Kolmogorov complexity in the Milky Way and its reduction with warm dark matter
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• A Compact Spectrograph to Search for Extrasolar Planets
• Deep chemical tagging -- Identifying open clusters and moving groups in chemical space with graph attention networks
• Globular Clusters in the Sagittarius stream. Revising members and candidates with Gaia DR2
• Do open clusters have distinguishable chemical signatures?
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• 3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations
• The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
• An ancient system hidden in the Galactic plane?
• Chemical Tagging of FGK Stars: Testing Membership to Young Stellar Kinematics Groups
• Observational Comparison of Star Formation in Different Galaxy Types
• Functional Data Analysis for Extracting the Intrinsic Dimensionality of Spectra: Application to Chemical Homogeneity in the Open Cluster M67
• A relic from a past merger event in the Large Magellanic Cloud
• Chemical Abundance Analysis of Moving Group W11450 (Latham 1)
• What can the outskirts of galaxies tell us about dark matter?
• Galaxy simulations in the Gaia era