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.

51 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

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• The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars
• Star Clusters Across Cosmic Time
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• 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
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• LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) The survey science plan
• Near-Field Cosmology with Metal-Poor Stars
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• 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
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• The RAdial Velocity Experiment (RAVE): Fourth data release
• A New Mechanism for Radial Migration in Galactic Disks: Spiral-Bar Resonance Overlap
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• Galaxy Formation Theory
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• Stellar yields from metal-rich asymptotic giant branch models
• Galaxia: a code to generate a synthetic survey of the Milky Way
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• 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
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• 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
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• The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry and location
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• 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
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• Structure of Disk Dominated Galaxies: II. Color Gradients and Stellar Population Models
• Current Status of r-Process Nucleosynthesis
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• Galactic archaeology: mapping and dating stellar populations with asteroseismology of red-giant stars
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• 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
• From dawn till disk: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
• The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
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• Evolution of Galactic Discs: Multiple Patterns, Radial Migration and Disc Outskirts
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• 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
• 'Sculptor'-ing the Galaxy? The Chemical Compositions of Red Giants in the Sculptor Dwarf Spheroidal Galaxy
• Estimating stellar birth radii and the time evolution of the Milky Way's ISM metallicity gradient
• 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
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• The age of the oldest Open Clusters
• Structure Finding in Cosmological Simulations: The State of Affairs
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• SubHaloes going Notts: The SubHalo-Finder Comparison Project
• Planetary System Disruption by Galactic Perturbations to Wide Binary Stars
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• From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
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• 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
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• The Cosmic Evolution of Metallicity from the SDSS Fossil Record
• The Long-term Evolution of the Galactic Disk Traced by Dissolving Star Clusters
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• A Comparison of the Chemical Evolutionary Histories of the Galactic Thin Disk and Thick Disk Stellar Populations
• Prospects for chemically tagging stars in the Galaxy
• The Gaia-ESO Survey: calibration strategy
• The baryonic mass function of galaxies
• Carbon-Enhanced Metal-Poor Stars, the Cosmic Microwave Background, and the Stellar IMF in the Early Universe
• The velocity distribution of nearby stars from Hipparcos data II. The nature of the low-velocity moving groups
• Does the Milky Way Produce a Nuclear Galactic Wind?
• Action-space clustering of tidal streams to infer the Galactic potential
• Population synthesis to constrain Galactic and Stellar Physics- I- Determining age and mass of thin-disc red-giant stars
• The Stellar Populations of M33's Outer Regions III: Star Formation History
• Galactic Bulges from HST NICMOS Observations: Global Scaling Relations
• The Stellar Populations of M33's Outer Regions IV: Inflow History and Chemical Evolution
• 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
• Star Clusters in Evolving Galaxies
• Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
• Statistics of Stellar Variability from Kepler - I: Revisiting Quarter 1 with an Astrophysically Robust Systematics Correction
• The Pristine survey III: Spectroscopic confirmation of an efficient search for extremely metal-poor stars
• Orbital evolution of the Carina dwarf galaxy and self-consistent star formation history determination
• A Two Micron All-Sky Survey View of the Sagittarius Dwarf Galaxy: VI. s-Process and Titanium Abundance Variations Along the Sagittarius Stream
• Comprehensive abundance analysis of red giants in the open clusters NGC 2527, 2682, 2482, 2539, 2335, 2251 and 2266
• Chemically tagging the Hyades Supercluster: A homogeneous sample of F6-K4 kinematically selected northern stars
• 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
• An HST/ACS investigation of the spatial and chemical structure and sub-structure of NGC 891, a Milky Way analogue
• The impact of baryonic physics on the shape and radial alignment of substructures in cosmological dark matter haloes
• On the recent star formation history of the Milky Way disk
• 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
• Chemical abundances in giants stars of the tidally disrupted globular cluster NGC 6712 from high-resolution infrared spectroscopy
• Spectroscopy of Bright QUEST RR Lyrae Stars: Velocity Substructures toward Virgo
• The Spatial Distribution of the Galactic First Stars I: High-Resolution N-body Approach
• 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging
• Chemical evidence for planetary ingestion in a quarter of Sun-like stars
• Stellar ages, masses, extinctions and orbital parameters based on spectroscopic parameters of Gaia DR3
• Abundance-age relations with red clump stars in open clusters
• Chemical signatures of the first star clusters
• Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE
• The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way
• 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?
• Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk
• A comparison between the stellar and dynamical masses of six globular clusters
• The GALAH Survey: Verifying abundance trends in the open cluster M67 using non-LTE spectroscopy
• Simulations of minor mergers. II. The phase-space structure of thick discs
• Evidence of a thick disk rotation-metallicity correlation
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• The Sun was not born in M 67
• Microarcsecond Astrometry: Science Highlights from Gaia
• Elemental Abundances of Solar Sibling Candidates
• Streams in the Aquarius stellar haloes
• Star Formation Regulation and Self-Pollution by Stellar Wind Feedback
• The Chemical Evolution of Globular Clusters I. Reactive Elements and Non-Metals
• Effect of bars on the galaxy properties
• An HI survey of six Local Group analogs: I. Survey description and the search for high-velocity clouds
• Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars
• How Many Elements Matter?
• Identifying Contributions to the Stellar Halo from Accreted, Kicked-Out, and In Situ Populations
• Evidence of tidal debris from Omega Cen in the Kapteyn Group
• Quantitative chemical tagging, stellar ages and the chemo-dynamical evolution of the Galactic disc
• Stellar Abundance Maps of the Milky Way Disk
• 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 Galactic Thick Disc density profile traced with RR Lyrae stars
• The GALAH survey: Chemical Tagging of Star Clusters and New Members in the Pleiades
• Thick disk kinematics from RAVE and the solar motion
• Chemical abundances in bright giants of the globular cluster M62 (NGC 6266)
• Metal Mixing and Ejection in Dwarf Galaxies is Dependent on Nucleosynthetic Source
• Beyond the two-infall model I. Indications for a recent gas infall with Gaia DR3 chemical abundances
• The evolution of CNO elements in galaxies
• Cosmic phylogeny: reconstructing the chemical history of the solar neighbourhood with an evolutionary tree
• Science Programs for a 2 m-class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope
• Fundamental properties of five Kepler stars using global asteroseismic quantities and ground-based observations
• The chemistry of the most metal-rich damped Lyman $\alpha$ systems at z$\sim 2$ II. Context with the Local Group
• The stellar Initial Mass Function of the solar neighbourhood revealed by Gaia
• Chemical separation of disc components using RAVE
• Detection of a population of carbon-enhanced metal-poor stars in the Sculptor dwarf spheroidal galaxy
• Rotation and Lithium Confirmation of a 500 Parsec Halo for the Open Cluster NGC 2516
• Unmixing the Galactic Halo with RR Lyrae tagging
• Weighing the Galactic disk using phase-space spirals II. Most stringent constraints to a thin dark disk using Gaia EDR3
• Quantifying Chemical Tagging: Towards Robust Group Finding in the Galaxy
• Search for giant planets in M67 I. Overview
• Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
• The homogeneity of the star forming environment of the Milky Way disk over time
• 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
• 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
• 3D Spectrophotometry of Planetary Nebulae in the Bulge of M31
• Deep SDSS optical spectroscopy of distant halo stars II. Iron, calcium, and magnesium abundances
• The Pristine survey -- XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3
• 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
• On the 3 dimensional structure of edge-on disk galaxies
• A Disk Origin for the Monoceros Ring and A13 Stellar Overdensities
• 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 investigation of ELAIS field by Vega photometry: Absolute - magnitude dependent on the Galactic model parameters
• VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies
• Integrated Light Chemical Tagging Analyses of Seven M31 Outer Halo Globular Clusters from the Pan-Andromeda Archaeological Survey
• Renegade Subhaloes in the Local Group
• 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
• The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region
• Using APOGEE Wide Binaries to Test Chemical Tagging with Dwarf Stars
• The GALAH Survey and Gaia DR2: (Non)existence of five sparse high-latitude open clusters
• 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
• Metallicity Bias in the Kinematics of the Milky Way Stellar Halo
• Abundances in the Milky Way across five nucleosynthetic channels from 4 million LAMOST stars
• Reconstructing fossil sub-structures of the Galactic disk: clues from abundance patterns of old open clusters and moving groups
• The Stellar Populations of M33's Outer Regions II: Deep ACS Imaging
• 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
• A CCD Study of High Latitude Galactic Structure: Testing the Model Parameters
• Contrasting the chemical evolution of the Milky Way and Andromeda galaxies
• Strong chemical tagging with APOGEE: 21 candidate star clusters that have dissolved across the Milky Way disc
• Wide Binaries in Tycho-Gaia II: Metallicities, Abundances, and Prospects for Chemical Tagging
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
• Dynamics for Galactic Archaeology
• All quiet in the outer halo: chemical abundances in the globular cluster Pal 3
• Galaxy Genesis -- unravelling the epoch of dissipation in the early disk
• Disruption of a Dwarf Galaxy Under Strong Shocking: The Origin of omega Centauri
• The GALAH Survey: Chemical Clocks
• 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
• The detailed chemical abundance patterns of accreted halo stars from the optical to infrared
• High resolution elemental abundance analysis of the Hyades Supercluster
• The GALAH Survey: Accurate Radial Velocities and Library of Observed Stellar Template Spectra
• The chemical composition of globular clusters in the Local Group
• Stellar metallicity variations across spiral arms in disk galaxies with multiple populations
• BVI photometry of the very old open cluster Berkeley 17
• Chemo-kinematics of the Milky Way from the SDSS-III MARVELS Survey
• Scalar perturbations in $f(T)$ gravity using the $1+3$ covariant approach
• 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
• A variational encoder-decoder approach to precise spectroscopic age estimation for large Galactic surveys
• The Scaleheight of Giant Molecular Clouds is Less than that of Smaller Clouds
• The GALAH Survey: Stellar streams and how stellar velocity distributions vary with Galactic longitude, hemisphere and metallicity
• The Natural Science Underlying Big History
• Mixing of metals during star cluster formation: statistics and implications for chemical tagging
• The age-metallicity relation in the solar neighbourhood from a pilot sample of white dwarf-main sequence binaries
• Exploring the outskirts of globular clusters: the peculiar kinematics of NGC 3201
• The Abundances of Light Neutron-Capture Elements in Planetary Nebulae III. The Impact of New Atomic Data on Nebular Selenium and Krypton Abundance Determinations
• Streams Going Notts: The tidal debris finder comparison project
• The (im)possibility of strong chemical tagging
• Spectrum Syntheses of High Resolution Integrated Light Spectra of Galactic Globular Clusters
• The hunt for the Milky Way's accreted disc
• A Wide-Field View of Leo II -- A Structural Analysis Using the SDSS
• Properties of carbon stars in the Solar neighbourhood based on Gaia DR2 astrometry
• 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
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• Most "young" $\alpha$-rich stars have high masses but are actually old
• Yule-Simpson's paradox in Galactic Archaeology
• From giant clumps to clouds -- II. The emergence of thick disc kinematics from the conditions of star formation in high redshift gas rich galaxies
• 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
• Detailed abundance analysis of globular clusters in the Local Group: NGC 147, NGC 6822, and Messier 33
• The stellar metallicity distribution of disc galaxies and bulges in cosmological simulations
• 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
• Estimating stellar ages and metallicities from parallaxes and broadband photometry - successes and shortcomings
• Maximum Likelihood Fitting of Tidal Streams With Application to the Sagittarius Dwarf Tidal Tails
• Precise reddening and metallicity of NGC6752 from FLAMES spectra
• The dimensionality of stellar chemical space using spectra from the Apache Point Observatory Galactic Evolution Experiment
• The most ancient spiral galaxy: a 2.6-Gyr-old disk with a tranquil velocity field
• Iron-peak elements Sc, V, Mn, Cu and Zn in Galactic bulge globular clusters
• Migration and Mixing in the Galactic Disc from Encounters between Sagittarius and the Milky Way
• 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
• Insight Into the Formation of the Milky Way Through Cold Halo Substructure. II. The Elemental Abundances of ECHOS
• Reconstructing the Accretion History of the Galactic Stellar Halo from Chemical Abundance Ratio Distributions
• Chemical Abundances for Seven Giant Stars in M68 (NGC 4590) : A Globular Cluster with Abnormal Silicon and Titanium Abundances
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
• 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
• 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
• [Mg/Fe] ratios in the solar neighbourhood: stellar yields and chemical evolution scenarios
• 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
• StePar: an automatic code to infer stellar atmospheric parameters
• Know thy star, know thy planet: Chemo-kinematically characterizing TESS targets
• Tracing the anemic stellar halo of M101
• The case for high precision in elemental abundances of stars in the era of large spectroscopic surveys
• Constraining the Galactic potential via action-based distribution functions for mono-abundance stellar populations
• 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
• Stellar Population Astrophysics (SPA) with TNG Atmospheric parameters of members of 16 unstudied open clusters
• Reliability and limitations of inferring birth radii in the Milky Way disk
• Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
• The Quest for the Sun's Siblings: an Exploratory Search in the Hipparcos Catalogue
• Four-hundred Very Metal-poor Stars studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency
• Kinematic structures of the Solar neighbourhood revealed by Gaia DR1/TGAS and RAVE
• The radial metallicity gradient and the history of elemental enrichment in M81 through emission-line probes
• On the correlation between the recent star formation rate in the Solar Neighbourhood and the glaciation period record on Earth
• Orbital Torus Imaging: Using Element Abundances to Map Orbits and Mass in the Milky Way
• The Stellar Halo Metallicity - Luminosity Relationship for Spiral Galaxies
• APOGEE chemical tagging constraint on the maximum star cluster mass in the $\alpha$-enhanced Galactic disk
• Constructing Polynomial Spectral Models for Stars
• Timing the Milky Way bar formation and the accompanying radial migration episode
• Chemical compositions of stars in two stellar streams from the Galactic thick disk
• Study of the stellar population properties in the discs of ten spiral galaxies
• Reading the CARDs: the Imprint of Accretion History in the Chemical Abundances of the Milky Way's Stellar Halo
• Detailed Chemical Abundances of Four Stars in the Unusual Globular Cluster, Palomar 1
• NGC 5694: another foster son of the Galactic Halo
• A homogeneous spectroscopic analysis of a Kepler legacy sample of dwarfs for gravity-mode asteroseismology
• Mapping the Galactic Halo with blue horizontal branch stars from the 2dF quasar redshift survey
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• Elemental Abundances in M31: Gradients in the Giant Stellar Stream
• The extended structure of the remote cluster B514 in M31. Detection of extra-tidal stars
• The metallicity distributions in high-latitudes with SDSS
• Age Determination of Galaxy Merger Remnant Stars using Asteroseismology
• Stellar over-densities in the halo: the extent of the Virgo over-density
• Effects of the selection function on metallicity trends in spectroscopic surveys of the Milky Way
• Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes
• Vertical and radial metallicity gradients in high latitude galactic fields with SDSS
• A Two-Point Correlation Function For Galactic Halo Stars
• Slicing The Monoceros Overdensity with Suprime-Cam
• The GALAH Survey and Symbiotic Stars. I. Discovery and follow-up of 33 candidate accreting-only systems
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Combined APOGEE-GALAH stellar catalogues using the Cannon
• The horizontal branch luminosity vs metallicity in M31 globular clusters
• Hunting the Parent of the Orphan Stream II: The First High-Resolution Spectroscopic Study
• APOGEE spectroscopic evidence for chemical anomalies in dwarf galaxies: The case of M~54 and Sagittarius
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Origin of chemical and dynamical properties of the Galactic thick disk
• The Galactic Stellar Disc
• Chemical tagging of the Ursa Major moving group: A northern selection of FGK stars
• The radial alignment of dark matter subhalos: from simulations to observations
• Jurassic: A Chemically Anomalous Structure in the Galactic Halo
• Cosmic Renaissance: The First Sources of Light
• Multiwavelength Absolute Magnitudes and Colours of Red Clump Stars in {\it Gaia} Era
• STREAMFINDER II: A possible fanning structure parallel to the GD-1 stream in Pan-STARRS1
• The GALAH Survey: Chemically tagging the Fimbulthul stream to the globular cluster $\omega$ Centauri
• The $Gaia$-ESO Survey: the inner disk intermediate-age open cluster NGC 6802
• Stars on the run: escaping from stellar clusters
• The velocity ellipsoid in the Galactic disc using Gaia DR1
• The Sextet Arcs: a Strongly Lensed Lyman Break Galaxy in the ACS Spectroscopic Galaxy Survey towards Abell 1689
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• 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
• 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 ?
• Residual Abundances in GALAH DR3: Implications for Nucleosynthesis and Identification of Unique Stellar Populations
• A metallicity study of F, G, K and M dwarfs in the Coma Berenices open cluster from the APOGEE survey
• Chemical Signature Indicating A Lack of Massive Stars in Dwarf Galaxies
• The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk
• Accelerated Fitting of Stellar Spectra
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• A Recommendation Algorithm to Predict Giant Exoplanet Host Stars Using Stellar Elemental Abundances
• The intrinsic ellipticity of dwarf spheroidal galaxies: constraints from the Andromeda system
• 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
• On the Identification of Wide Binaries in the Kepler Field
• Towards a better understanding of the distance scale from RR Lyrae variable stars: A case study for the inner halo globular cluster NGC 6723
• Hot Jupiters, cold kinematics: High phase space densities of host stars reflect an age bias
• The high velocity stars in the Local Stellar Halo from Gaia and LAMOST
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• Three new bricks in the wall: Berkeley 23, Berkeley 31, and King 8
• A phylogenetic approach to chemical tagging. Reassembling open cluster stars
• The metallicity distribution of F/G dwarfs derived from BATC survey data
• From birth associations to field stars: mapping the small-scale orbit distribution in the Galactic disc
• The nature of the Milky Way's stellar halo revealed by the three integrals of motion
• The Sloan digital sky survey data release 7 spectroscopic m dwarf catalog iii: The spatial dependence of magnetic activity in the galaxy
• The GALAH Survey: Accreted stars also inhabit the Spite Plateau
• The AMBRE Project: Solar neighbourhood chemodynamical constraints on Galactic disc evolution
• Chemically peculiar A and F stars with enhanced s-process and iron-peak elements: stellar radiative acceleration at work
• The substructures in the local stellar halo from Gaia and LAMOST
• New Signatures of the Milky Way Formation in the Local Halo and Inner Halo Streamers in the Era of Gaia
• The Kapteyn moving group is not tidal debris from $\omega$ Centauri
• The Outskrits of Spiral Galaxies: Evidence for Multiple Stellar Populations
• Binary fractions of G and K dwarf stars based on the Gaia EDR3 and LAMOST DR5: impacts of the chemical abundances
• On the Chemical and Kinematic Consistency Between N-rich Metal-poor Field Stars and Enriched Populations in Globular Clusters
• SMHASH: Anatomy of the Orphan Stream using RR Lyrae stars
• The stellar metallicity distribution in intermediate latitude fields with BATC and SDSS data
• Optimal Integrated Abundances for Chemical Tagging of Extragalactic Globular Clusters
• Detection of Satellite Remnants in the Galactic Halo with Gaia - II. A modified Great Circle Cell Method
• Quest for finding the lost siblings of the Sun
• Comprehensive abundance analysis of red giants in the open clusters Stock 2, NGC 2168, 6475, 6991 and 7762
• 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
• An old, metal-rich accreted stellar component in the Milky Way stellar disk
• Super-Earth ingestion can explain the anomalously high metal abundances of M67 Y2235
• Machine learning in APOGEE: Identification of stellar populations through chemical abundances
• Disentangled Representation Learning for Astronomical Chemical Tagging
• 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
• VISTA's view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge
• A kinematic calibration of the O-rich Mira variable period-age relation from Gaia
• Age-metallicity dependent stellar kinematics of the Milky Way disc from LAMOST and Gaia
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• The Gaia-ESO Survey: The inner disc, intermediate-age open cluster Pismis 18
• Self-consistent simulations of star cluster formation from gas clouds under the influence of galaxy-scale tidal fields
• Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
• The GALAH survey: Co-orbiting stars and chemical tagging
• The Orbit and Origin of the Ultra-faint Dwarf Galaxy Segue 1
• A revisited study of Cepheids in open clusters in the Gaia era
• Triggering the Formation of Halo Globular Clusters with Galaxy Outflows
• Velocity and abundance precisions for future high-resolution spectroscopic surveys: a study for 4MOST
• The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS) I: A Pilot Study of the stellar populations in NGC 2298 and NGC 3201
• A new set of chisels for Galactic archaeology: Sc, V and Zn as taggers of accreted globular clusters
• The GALAH+ Survey: A New Library of Observed Stellar Spectra Improves Radial Velocities and Hints at Motions within M67
• On the relevance of chaos for halo stars in the solar neighbourhood II
• Stellar Signatures of Inhomogeneous Big Bang Nucleosynthesis
• The Gaia-ESO Survey: Separating disk chemical substructures with cluster models
• 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
• A data-driven model of nucleosynthesis with chemical tagging in a lower-dimensional latent space
• Cardinal kinematics: I. Rotation fields of the APOGEE Survey
• 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
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• Origin of a massive hyper-runaway subgiant star LAMOST-HVS1 -- implication from Gaia and follow-up spectroscopy
• Peeking beneath the precision floor I: metallicity spreads and multiple elemental dispersions in the globular clusters NGC 288 and NGC 362
• 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
• Properties of galaxies with ring structures
• A geostatistical analysis of multiscale metallicity variations in galaxies [II]: Predicting the metallicities of Hii and diffuse ionised gas regions via universal kriging
• Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO) II. t-SNE Portrait of Local Fossil Relics and Structures
• HE 0017+0055 : A probable pulsating CEMP-rs star and long-period binary
• Remarkable migration of the solar system from the innermost Galactic disk; a wander, a wobble, and a climate catastrophe on the Earth
• The HR 1614 moving group is not a dissolving cluster
• Chemo-Dynamical Clustering applied to APOGEE data: Re-Discovering Globular Clusters
• Ghosts of Milky Way's past: the globular cluster ESO 37-1 (E 3)
• Inference of stellar parameters from brightness variations
• Kinematics of the Galactic disk from LAMOST Dwarf sample
• Investigating the amplitude and rotation of the phase spiral in the Milky Way outer disc
• A Unified Exploration of the Chronology of the Galaxy
• The horizontal branch morphology of M31 globular clusters. Extreme second parameter effect in outer halo clusters
• A new algorithm for optimizing the wavelength coverage for spectroscopic studies: Spectral Wavelength Optimization Code (SWOC)
• The Parent Populations of 6 groups identified from Chemical Tagging in the Solar neighborhood
• Abundance ties: Nephele and the globular cluster population accreted with $\omega$ Cen. Based on APOGEE DR17 and Gaia EDR3
• Exploring the chemodynamics of metal-poor stellar populations
• Simulating a White Dwarf-dominated Galactic Halo
• Searching for Solar Siblings in APOGEE and $Gaia$ DR2 with N-body Simulations
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• The Gaia-ESO Survey: Chemical tagging in the thin disk. Open clusters blindly recovered in the elemental abundance space
• Tracing birth properties of stars with abundance clustering
• Galactic Archaeology with CoRoT and APOGEE: Creating mock observations from a chemodynamical model
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Possible Streams of the Globular Clusters in the Galaxy
• High Velocity Stars in SDSS/APOGEE DR17
• 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
• 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
• 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
• Stellar Over-densities in the Outer Halo of the Milky Way
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Holistic spectroscopy: Complete reconstruction of a wide-field, multi-object spectroscopic image using a photonic comb
• Chemical abundance analysis of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy
• Implications of the spectroscopic abundances in α Centauri A and B
• A high fidelity Milky Way simulation with Kraken, Gaia-Enceladus, and Sequoia analogues: clues to their accretion histories
• Metallicities and ages of stellar populations at a high Galactic latitude field
• Structure and Evolution of the Milky Way
• Kinematically Detected Halo Streams
• Old open clusters and the Galactic metallicity gradient: Berkeley 20, Berkeley 66, and Tombaugh 2
• Asymmetric metallicity patterns in the stellar velocity space with RAVE
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Towards Studying Hierarchical Assembly in Real Time: A Milky Way Progenitor Galaxy at z = 2.36 under the Microscope
• 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
• Clustering in the Stellar Abundances Space
• Prospecting for chemical tags among open clusters
• A high resolution, multi-epoch spectral atlas of peculiar stars including RAVE, GAIA and HERMES wavelength ranges
• The heavy-elements heritage of the falling sky
• Exploring the origin of the extended main sequence turn off in M37 through the white dwarf cooling sequence
• Using heritability of stellar chemistry to reveal the history of the Milky Way
• Booms and Busts: the Burstiness of Star Formation in Nearby Dwarf Galaxies
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• The Gaia-ESO Survey: α-abundances of metal-poor stars
• Local Stellar Kinematics from RAVE data -- VIII. Effects of the Galactic Disc Perturbations on Stellar Orbits of Red Clump Stars
• High-resolution near-infrared spectroscopy of globular cluster and field stars toward the Galactic bulge
• Imprints of Zero-Age Velocity Dispersions and Dynamical Heating on the Age-Velocity dispersion Relation
• The structure of the Galactic halo: SDSS versus SuperCOSMOS
• Spatial and Kinematic Clustering of Stars in the Galactic Disk
• Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
• Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• Mass and Age determination of the LAMOST data with different Machine Learning methods
• Galaxy archaeology for wet mergers: Globular cluster age distributions in the Milky Way and nearby galaxies
• The in situ origin of the globular cluster NGC 6388 from abundances of Sc, V, and Zn of a large sample of stars
• Tidal debris from Omega Centauri discovered with unsupervised machine learning
• The 300km/s stellar stream near Segue 1: Insights From high-resolution spectroscopy of its brightest star
• Exploring Hydrodynamic Instabilities along the Infalling High-Velocity Cloud Complex A
• 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
• The Aquarius Co-Moving Group is Not a Disrupted Classical Globular Cluster
• Reliable stellar abundances of individual stars with the MUSE integral-field spectrograph
• The GALAH Survey: Dependence of elemental abundances on age and metallicity for stars in the Galactic disc
• A high-resolution spectroscopic study of two new Na- and Al-rich field giants -- likely globular cluster escapees in the Galactic halo
• A GALAH View of the Chemical Homogeneity and Ages of Stellar Strings Identified in Gaia
• How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
• An optimized Method to Identify RR Lyrae stars in the SDSS X Pan-STARRS1 Overlapping Area Using a Bayesian Generative Technique
• Internal calibration of LAMOST and Gaia DR3 GSP-Spec stellar abundances
• From light to mass: accessing the initial and present-day Galactic globular cluster mass functions
• A Hierarchical Model for the Ages of Galactic Halo White Dwarfs
• More pieces of the puzzle: Chemistry and substructures in the Galactic thick disk
• Traits for chemical evolution in solar twins: Trends of neutron-capture elements with stellar age
• First Light Results from the Hermes Spectrograph at the AAT
• Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
• RR Lyrae stars as probes of the outer Galactic halo: Chemical and kinematic analysis of a pilot sample
• Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages
• Chemodynamic evolution of Sun-like stars in nearby moving groups
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• The GALAH Survey: Stellar parameters and abundances for 800,000 Gaia RVS spectra using GALAH DR4 and The Cannon
• 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
• Local Group(s)
• Candidate List of Edge-on Galaxies with Substantial Extraplanar Dust
• Elemental abundances of intermediate age open cluster NGC 3680
• Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
• NGC 765 - A disturbed H I giant
• Chemical evolution of star clusters
• 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
• The Lives of Stars: Insights From the TGAS-RAVE-LAMOST Dataset
• The Radial Distribution of Mono-Metallicity Populations in the Galactic Disk as Evidence for Two-Phase Disk Formation
• Origins and Interpretation of Tidal Debris
• Two substructures in the nearby stellar halo found in Gaia and RAVE
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• Resolved Stellar Populations as Tracers of Outskirts
• Metallicity Calibration and Photometric Parallax Estimation: II. SDSS photometry
• Towards 21st Century Stellar Models: Star Clusters, Supercomputing, and Asteroseismology
• A spectroscopic survey of faint, high-galactic latitude red clump stars. II. The medium resolution sample
• Bar-spiral interaction produces radial migration and star formation bursts
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Turbulent gas-rich discs at high redshift: origin of thick stellar discs through 3D 'baryon sloshing'
• Mapping the Distant and Metal-Poor Milky Way with SDSS-V
• Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF
• Spectroscopic Observations of Obscured Populations in the Inner Galaxy: 2MASS-GC02, Terzan 4, and the 200 km/s stellar peak
• Automatic line selection for abundance determination in large stellar spectroscopic surveys
• Studying stellar populations in Omega Centauri with phylogenetics
• Detection of Open Cluster Members Inside and Beyond Tidal Radius by Machine Learning Methods Based on Gaia DR3
• Outer Spiral Disks as Clues to Galaxy Formation and Evolution
• Chemodynamics of metal-poor wide binaries in the Galactic halo: Association with the Sequoia event
• From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
• Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
• The Impact of Inelastic Collisions with Hydrogen on NLTE Copper Abundances in Metal-Poor Stars
• Nearby stellar substructures in the Galactic halo from DESI Milky Way Survey Year 1 Data Release
• The GALAH survey: Multiple stars and our Galaxy. I. A comprehensive method for deriving properties of FGK binary stars
• Galactic Archeology with 4MOST
• Tracing the origin of moving groups I. The γ Leo moving group with high resolution spectra from the Subaru Telescope
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
• The Astrophysical Variance in Gaia-RVS Spectra
• Blue Straggler Stars: Early Observations that Failed to Solve the Problem
• Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs
• The Gaia-ESO Survey astrophysical calibration
• 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
• The Chemodynamical Nature of the Triangulum-Andromeda Overdensity
• Introduction to Tidal Streams
• Omega Centauri: weak MgH-band in red giants directly trace the helium content
• Galactic Stellar Populations from Photometric Metallicity Distribution Functions
• Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
• Tracking Cluster Debris (TraCD)- I. Dissolution of clusters and searching the solar cradle
• GALAH Survey: Chemically Tagging the Thick Disk
• The K2 Galactic Archaeology Program: Overview, target selection and survey properties
• Tomography of stellar halos: what does anisotropy in a stellar halo tell us?
• 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
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Chemodynamics of the Milky Way and disc formation history: insight from the RAVE and Gaia-ESO surveys
• Solar twins in Gaia DR3 GSP-Spec I. Building a large catalog of Solar twins with ages
• Chemical abundances of field halo stars -- Implications for the building blocks of the Milky Way
• Identifying substructure associations in the Milky Way halo using chemo-kinematic tagging
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Dissecting stellar populations with manifold learning I. Validation of the method on a synthetic Milky Way-like galaxy
• The broadening of the main sequence in the open cluster M38
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Radial Mixing due to Spiral-Bar Resonance Overlap: Implications to the Milky Way
• Quantifying chemical and kinematical properties of Galactic disks
• iota Horologii is unlikely to be an evaporated Hyades star
• The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates
• Milky Way's Metal-Poor Stars display Chemical Transition near the Solar Radius
• A Universal Vertical Stellar Density Distribution Law for the Galaxy
• Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns
• Chemical tagging experiment with the Gaia-ESO open clusters
• The odd bunch: chrono-chemo-dynamics of sixteen unusual stars from Kepler
• On the connection between nitrogen-enhanced field stars and the Galactic globular clusters
• What will Gaia tell us about the Galactic disk?
• A new moving group in the Local Arm
• Caveats about measuring carbon abundances in stars using the CH band
• 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
• Two faces of Gaia-Sausage-Enceladus: Mining the chemical abundance space with graph attention networks
• Low mass variable stars in the globular cluster NGC 6397
• Asteroseismology of red giants & galactic archaeology
• New families in our Solar neighborhood: applying Gaussian Mixture models for objective classification of structures in the Milky Way and in simulations
• Radial Migration in Spiral Galaxies
• Studying Young Stars with Large Spectroscopic Surveys
• 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
• The metal-poor tail of the APOGEE survey I. Uncovering [Fe/H] < -2.5 stars from the inner Galaxy to the Magellanic Clouds
• Parametrization of the Galactic Structure by two exponentials
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• What can the outskirts of galaxies tell us about dark matter?
• Galaxy simulations in the Gaia era
• Chemical Abundance Analysis of Moving Group W11450 (Latham 1)
• Globular Clusters in the Sagittarius stream. Revising members and candidates with Gaia DR2
• A relic from a past merger event in the Large Magellanic Cloud
• Functional Data Analysis for Extracting the Intrinsic Dimensionality of Spectra: Application to Chemical Homogeneity in the Open Cluster M67
• Observational Comparison of Star Formation in Different Galaxy Types
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• An ancient system hidden in the Galactic plane?
• Chemical Tagging of FGK Stars: Testing Membership to Young Stellar Kinematics Groups
• Searching for and characterizing halo substructures with the GALAH DR4 survey
• Kolmogorov complexity in the Milky Way and its reduction with warm dark matter
• Evolution of action-space coherence in a Milky Way-like simulation
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• Deep chemical tagging -- Identifying open clusters and moving groups in chemical space with graph attention networks
• A Compact Spectrograph to Search for Extrasolar Planets
• Do open clusters have distinguishable chemical signatures?
• The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
• 3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations