The mass distribution and gravitational potential of the Milky Way

Abstract

We present mass models of the Milky Way created to fit observational constraints and to be consistent with expectations from theoretical modelling. The method used to create these models is that demonstrated in McMillan (2011), and we improve on those models by adding gas discs to the potential, considering the effects of allowing the inner slope of the halo density profile to vary, and including new observations of maser sources in the Milky Way amongst the new constraints. We provide a best fitting model, as well as estimates of the properties of the Milky Way. Under the assumptions in our main model, we find that the Sun is $R_0=(8.20\pm 0.09)\mathrm{kpc}$ from the Galactic Centre, with the circular speed at the Sun being $v_0=(232.8\pm 3.0)\mathrm{km}{\mathrm{s}}^{-1}$; that the Galaxy has a total stellar mass of $(54.3\pm 5.7)\times 10^9{\mathrm{M}}_{\odot }$, a total virial mass of $(1.30\pm 0.30)\times 10^{12}{\mathrm{M}}_{\odot }$ and a local dark-matter density of $0.38\pm 0.04{\mathrm{GeV}\mathrm{cm}}^{-3}$, where the quoted uncertainties are statistical. These values are sensitive to our choice of priors and constraints. We investigate systematic uncertainties, which in some cases may be larger. For example, if we weaken our prior on $R_0$, we find it to be $(7.97\pm 0.15)\mathrm{kpc}$ and that $v_0=(226.8\pm 4.2)\mathrm{km}{\mathrm{s}}^{-1}$. We find that most of these properties, including the local dark-matter density, are remarkably insensitive to the assumed power-law density slope at the centre of the dark-matter halo. We find that it is unlikely that the local standard of rest differs significantly from that found under assumptions of axisymmetry. We have made code to compute the force from our potential, and to integrate orbits within it, publicly available.

MNRAS accepted. Revised to correct local dark matter density unit conversion. Code to use the gravitational potential available at https://github.com/PaulMcMillan-Astro/GalPot

References in corpus (26)

• The Gaia mission
• Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
• The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars
• The RAVE Survey: Constraining the Local Galactic Escape Speed
• The Local Dark Matter Density
• The Milky Way's circular velocity curve between 4 and 14 kpc from APOGEE data
• Dynamical modelling of the Galactic bulge and bar: the Milky Way's bar pattern speed, stellar, and dark matter mass distribution
• An Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis
• "Skinny Milky Way, Please", says Sagittarius
• A First Constraint on the Thick Disk Scale Length: Differential Radial Abundances in K Giants at Galactocentric Radii 4, 8, and 12 kpc
• On the Shoulders of Giants: Properties of the Stellar Halo and the Milky Way Mass Distribution
• The old nuclear star cluster in the Milky Way: dynamics, mass, statistical parallax, and black hole mass
• Constraining the Galaxy's dark halo with RAVE stars
• Globular Cluster Streams as Galactic High-Precision Scales - The Poster Child Palomar 5
• On the Formation of Galactic Thick Disks
• The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures
• Galactic masers and the Milky Way circular velocity
• Made-to-Measure models of the Galactic Box/Peanut bulge: stellar and total mass in the bulge region
• A new determination of the local dark matter density from the kinematics of K dwarfs
• Kinematic modelling of the Milky Way using the RAVE and GCS stellar surveys
• Weighing the local dark matter with RAVE red clump stars
• The mechanics of tidal streams
• Dipping Our Toes in the Water: First Models of GD-1 as a Stream
• The power spectrum of the Milky Way: Velocity fluctuations in the Galactic disk
• The incorrect rotation curve of the Milky Way
• The Milky Way Tomography with SDSS. V. Mapping the Dark Matter Halo

Cited by in corpus (556)

• Formation of Double Neutron Star Systems
• The GALAH+ Survey: Third Data Release
• Evidence for Two Early Accretion Events That Built the Milky Way Stellar Halo
• Gaia EDR3 view on Galactic globular clusters
• Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure
• The second data release from the European Pulsar Timing Array I. The dataset and timing analysis
• Tango for three: Sagittarius, LMC, and the Milky Way
• Strong-field Gravity Tests with the Double Pulsar
• Markov Chain Monte Carlo Methods for Bayesian Data Analysis in Astronomy
• A Sun-like star orbiting a black hole
• Dark matter local density determination: recent observations and future prospects
• The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
• The Global Dynamical Atlas of the Milky Way mergers: Constraints from Gaia EDR3 based orbits of globular clusters, stellar streams and satellite galaxies
• Distances and parallax bias in Gaia DR2
• A red giant orbiting a black hole
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• The chemical characterisation of halo substructure in the Milky Way based on APOGEE
• 3D kinematics and age distribution of the Open Cluster population
• Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry
• The Hestia project: simulations of the Local Group
• Proper Motions, Orbits, and Tidal Influences of Milky Way Dwarf Spheroidal Galaxies
• Measuring the Mass of the Large Magellanic Cloud with Stellar Streams Observed by $S^5$
• Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry
• The last breath of the Sagittarius dSph
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Detection of the Milky Way reflex motion due to the Large Magellanic Cloud infall
• The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces
• $S^5$: Probing the Milky Way and Magellanic Clouds potentials with the 6-D map of the Orphan-Chenab stream
• The Chemical Compositions of Accreted and {\it in situ} Galactic Globular Clusters According to SDSS/APOGEE
• The Chemo-Dynamical Groups of Galactic Globular Clusters
• Detection of the LMC-induced sloshing of the Galactic halo
• Gaia Early Data Release 3: The Galactic anticentre
• Kinematics of Antlia 2 and Crater 2 from The Southern Stellar Stream Spectroscopic Survey (S5)
• $S^5$: The Orbital and Chemical Properties of One Dozen Stellar Streams
• A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes
• The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and $Gaia$ eDR3
• A Low-Mass Stellar-Debris Stream Associated with a Globular Cluster Pair in the Halo
• Reconstructing the Disrupted Dwarf Galaxy $Gaia$-Sausage/Enceladus Using its Stars and Globular Clusters
• Tree-ring structure of Galactic bar resonance
• Elevated r-process enrichment in Gaia Sausage and Sequoia
• An extended halo around an ancient dwarf galaxy
• Measuring the Milky Way mass distribution in the presence of the LMC
• The Accreted Nuclear Clusters of the Milky Way
• All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• The mass of the Milky Way out to 100 kpc using halo stars
• The Gaia DR3 view of dynamical substructure in the stellar halo near the Sun
• $R$-process enhancements of Gaia-Enceladus in GALAH DR3
• GASTRO library I: the simulated chemodynamical properties of several GSE-like stellar halos
• An improved test of the strong equivalence principle with the pulsar in a triple star system
• Discovery of a Gamma-ray Black Widow Pulsar by GPU-accelerated Einstein@Home
• The extended halo of NGC 2682 (M 67) from Gaia DR2
• A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations
• Handling the Uncertainties in the Galactic Dark Matter Distribution for Particle Dark Matter Searches
• The star formation history of Upper Scorpius and Ophiuchus
• Gaia Data Release 3: Chemical cartography of the Milky Way
• Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys
• The large-scale ionization cones in the Galaxy
• Gravothermal evolution of dark matter halos with differential elastic scattering
• Evidence of a dwarf galaxy stream populating the inner Milky Way Halo
• A guided map to the Spiral arms in the galactic disk of the Milky Way
• Co-formation of the thin and thick discs revealed by APOGEE-DR16 and Gaia-DR2
• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• Breakdown of the Newton-Einstein Standard Gravity at Low Acceleration in Internal Dynamics of Wide Binary Stars
• Uncertainties in the Galactic dark matter distribution: an update
• Stellar ages, masses, extinctions and orbital parameters based on spectroscopic parameters of Gaia DR3
• The stellar mass distribution of the Milky Way's bar: an analytic model
• CMZoom: Survey Overview and First Data Release
• Abundance and temperature of the outer hot circum-Galactic medium: The SRG/eROSITA view of the soft X-ray background in the eFEDS field
• The tidal remnant of an unusually metal-poor globular cluster
• Eryn : A multi-purpose sampler for Bayesian inference
• Strong constraints on the gravitational law from $Gaia$ DR3 wide binaries
• PSR J2222--0137. I. Improved physical parameters for the system
• The R-Process Alliance: Chemo-Dynamically Tagged Groups of Halo $r$-Process-Enhanced Stars Reveal a Shared Chemical-Evolution History
• Recent advances in the determination of some Galactic constants in the Milky Way
• Exploring the Galaxy's halo and very metal-weak thick disk with SkyMapper and Gaia DR2
• Radialization of satellite orbits in galaxy mergers
• The Atari Disk, a Metal-Poor Stellar Population in the Disk System of the Milky Way
• Towards Robust Constraints on Axion Dark Matter using PSR J1745-2900
• Gravity experiments with radio pulsars
• A population of heavily reddened, optically missed novae from Palomar Gattini-IR: Constraints on the Galactic nova rate
• A measurement of the Galactic plane mass density from binary pulsar accelerations
• The Kinematic Properties of Milky Way Stellar Halo Populations
• Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-Faint Dwarf Galaxy in the Constellation Pegasus
• Beyond the two-infall model I. Indications for a recent gas infall with Gaia DR3 chemical abundances
• The phase spiral in Gaia DR3
• LAMOST meets Gaia: The Galactic Open Clusters
• A Search for Axionic Dark Matter Using the Magnetar PSR J1745-2900
• Weighing the Galactic disk using phase-space spirals II. Most stringent constraints to a thin dark disk using Gaia EDR3
• The origin and fate of the Gaia phase-space snail
• Median Statistics Estimate of the Distance to the Galactic Center
• A model for a dark matter core at the galactic center
• Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
• Exploring dark matter spike distribution around the Galactic centre with stellar orbits
• Substructure in the stellar halo near the Sun. I. Data-driven clustering in Integrals of Motion space
• Milky Way total Mass derived by Rotation Curve and Globular Cluster kinematics from Gaia EDR3
• Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds
• Deep Subaru Hyper Suprime-Cam observations of Milky Way satellites Columba I and Triangulum II
• Simulating the Fermi Bubbles as Forward Shocks Driven by AGN Jets
• Kinematics and dynamics of Gaia red clump stars
• Testing kinematic distances under a realistic Galactic potential
• Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
• A revisit of PSR J1909$-$3744 with 15-year high-precision timing
• Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator
• Intermediate- and high-velocity clouds in the Milky Way II: evidence for a Galactic fountain with collimated outflows and diffuse inflows
• The volumetric star formation law in the Milky Way
• High-precision chemical abundances of Galactic building blocks. The distinct chemical abundance sequence of Sequoia
• The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO
• Dynamically Tagged Groups of Metal-Poor Stars from the Best \& Brightest Survey
• "Super-Kilonovae" from Massive Collapsars as Signatures of Black-Hole Birth in the Pair-instability Mass Gap
• A Comparative Analysis of the Chemical Compositions of Gaia-Enceladus/Sausage and Milky Way Satellites using APOGEE
• Action-based distribution function modelling for constraining the shape of the Galactic dark matter halo
• Lithium and Beryllium in the Gaia-Enceladus Galaxy
• Galactic Bar Resonances Inferred from Kinematically Hot Stars in Gaia EDR3
• The R-Process Alliance: The Peculiar Chemical Abundance Pattern of RAVE J183013.5-455510
• 3D hydrodynamic simulations for the formation of the Local Group satellite planes
• Mass models of the Milky Way and estimation of its mass from the GAIA DR3 data-set
• Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
• The Radcliffe Wave is Oscillating
• The global stability of M33 in MOND
• Evidence for sub-Chandrasekhar Type Ia supernovae from the last major merger
• On the stability of tidal streams in action space
• Vertical motion in the Galactic disc: unwinding the Snail
• Probing the Milky Way's Dark Matter Halo for the 3.5 keV Line
• Tidally induced spiral arm wraps encoded in phase space
• Did Sgr cause the vertical waves in the solar neighbourhood?
• New minimal, median, and maximal propagation models for dark matter searches with Galactic cosmic rays
• A self-consistent dynamical model of the Milky Way disc adjusted to Gaia data
• Icarus: a Flat and Fast Prograde Stellar Stream in the Milky Way disk
• Dynamical model of the Milky Way using APOGEE and Gaia data
• The Gaia-ESO Survey: Carbon abundance in the Galactic thin and thick disks
• Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS
• Finding the remnants of the Milky Way's last neutron star mergers
• Constraining the mass of the Local Group
• Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
• High-precision chemical abundances of Galactic building blocks. II. Revisiting the chemical distinctness of the Helmi streams
• Neutrino clustering in the Milky Way and beyond
• Radial halo substructure in harmony with the Galactic bar
• Exotic Compact Objects: The Dark White Dwarf
• DESI Early Data Release Milky Way Survey Value-Added Catalogue
• Milky Way Accelerometry via Millisecond Pulsar Timing
• An artificial neural network to discover Hypervelocity stars: Candidates in Gaia DR1/TGAS
• Clues to the origin of Fermi Bubbles from OVIII/OVII line ratio
• The Flattening Metallicity Gradient in the Milky Way's Thin Disk
• Elemental abundances of nearby M dwarfs based on high-resolution near-infrared spectra obtained by the Subaru/IRD survey: Proof of concept
• Abundance Patterns of $\alpha$ and Neutron-capture Elements in the Helmi Stream
• Chemo-Dynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-$s$ and CEMP-no Stars
• The structural evolution of galaxies with both thin and thick discs
• Mapping the anisotropic Galactic stellar halo with Blue Horizontal Branch stars
• The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA
• Kinematic structures of the Solar neighbourhood revealed by Gaia DR1/TGAS and RAVE
• The impact of a massive Sagittarius dSph on GD-1-like streams
• The R-Process Alliance: Chemo-Dynamically Tagged Groups II. An Extended Sample of Halo $r$-Process-Enhanced Stars
• Search for Gamma-ray Spectral Lines from Dark Matter Annihilation up to 100 TeV towards the Galactic Center with MAGIC
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• Revealing the Ionization Properties of the Magellanic Stream using Optical Emission
• Spiral-like features in the disc revealed by Gaia DR3 radial actions
• Orbital dynamics and histories of satellite galaxies around Milky Way-mass galaxies in the FIRE simulations
• A transiting brown dwarf in a 2 hour orbit
• Age Determination of Galaxy Merger Remnant Stars using Asteroseismology
• Dynamically Tagged Groups of Metal-Poor Stars II. The Radial Velocity Experiment Data Release 6
• A Swing of the Pendulum: The Chemodynamics of the Local Stellar Halo Indicate Contributions from Several Radial Merger Events
• Prompt cusps and the dark matter annihilation signal
• Magnetized High Velocity Clouds in the Galactic Halo: A New Distance Constraint
• Mapping Milky Way disk perturbations in stellar number density and vertical velocity using Gaia DR3
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• The Unmixed Debris of Gaia-Sausage/Enceladus in the Form of a Pair of Halo Stellar Overdensities
• The Imprint of Spiral Arms on the Galactic Rotation Curve
• Weighing the Galactic disk using phase-space spirals I. Tests on one-dimensional simulations
• The Life Cycle of the Central Molecular Zone. II: Distribution of atomic and molecular gas tracers
• Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor ($[Fe/H]\lesssim -3$) Regime
• Modeling the kinematics of globular cluster systems
• Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer
• Mapping Dark Matter in the Milky Way using Normalizing Flows and Gaia DR3
• The Cetus-Palca stream: A disrupted small dwarf galaxy. A prequel to the science possible with WEAVE with precise spectro-photometric distances
• Weighing the Galactic disk using phase-space spirals III. Probing distant regions of the disk using the Gaia EDR3 proper motion sample
• A 62-minute orbital period black widow binary in a wide hierarchical triple
• A first estimate of the Milky Way dark matter halo spin
• The energy distribution of the first supernovae
• Weighing the Galactic disk in sub-regions of the solar neighbourhood using Gaia DR2
• The oblateness of the Milky Way dark matter halo from the stellar streams of NGC 3201, M68, and Palomar 5
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars
• 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
• The Kick Velocity Distribution of Isolated Neutron Stars
• Dynamical age of the Tucana-Horologium young stellar association
• Gliese 12 b: A temperate Earth-sized planet at 12 pc ideal for atmospheric transmission spectroscopy
• Most nearby young star clusters formed in three massive complexes
• Chronology of the chemical enrichment of the old Galactic stellar populations
• Probing black holes in a dark matter spike of M87 using quasinormal modes
• Observational Evidence for a Thick Disk of Dark Molecular Gas in the Outer Galaxy
• Age dissection of the vertical breathing motions in Gaia DR2: evidence for spiral driving
• The AMBRE Project: Solar neighbourhood chemodynamical constraints on Galactic disc evolution
• Self-interacting dark matter interpretation of Crater II
• The Far-Away Blues: Exploring the Furthest Extents of the Boötes I Ultra Faint Dwarf Galaxy
• The GALAH Survey: Accreted stars also inhabit the Spite Plateau
• The substructures in the local stellar halo from Gaia and LAMOST
• Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar
• Cosmic flow around local massive galaxies
• Young giants of intermediate mass Evidence of rotation and mixing
• Constraining scalarization in scalar-Gauss-Bonnet gravity through binary pulsars
• The GALAH survey: Tracing the Milky Way's formation and evolution through RR Lyrae stars
• DELVE-ing into the Jet: a thin stellar stream on a retrograde orbit at 30 kpc
• A-SLOTH reveals the nature of the first stars
• The structure of the Milky Way based on unWISE 3.4$\mu$m integrated photometry
• Classifying globular clusters and applying them to estimate the mass of the Milky Way
• Taking the Milky Way for a spin: disc formation in the ARTEMIS simulations
• Improved particle spray algorithm for modeling globular cluster streams
• Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties
• Spectroscopic analysis of Milky Way outer halo satellites: Aquarius II and Bootes II
• The origin of a distributed stellar population in the star-forming region W4
• Photometric metallicity for 694233 Galactic giant stars from Gaia DR3 synthetic Stromgren photometry. Metallicity distribution functions of halo sub-structures
• A dense $0.1{\mathbf{M}}_{\odot }$ star in a 51-minute orbital period eclipsing binary
• Tracing the Milky Way's Vestigial Nuclear Jet
• New type II Cepheids from VVV data towards the Galactic center
• Candidate Members of the VMP/EMP Disk System of the Galaxy from the SkyMapper and SAGES Surveys
• The MPIfR-MeerKAT Galactic Plane Survey II. The eccentric double neutron star system PSR J1208-5936 and a neutron star merger rate update
• A panoramic view of the Local Group dwarf galaxy NGC 6822
• Tracing stars in Milky Way satellites with A-SLOTH
• Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data
• Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
• A new resonance-like feature in the outer disc of the Milky Way
• First estimate of the local value of the baryonic streaming velocity
• Radial migration and vertical action in N-body simulations
• The role of radial migration in open cluster and field star populations with Gaia dr3
• A kinematic calibration of the O-rich Mira variable period-age relation from Gaia
• Extended reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and gravitational waves
• Gaia-Sausage-Enceladus star formation history as revealed by detailed elemental abundances
• The M31/M33 tidal interaction: A hydrodynamic simulation of the extended gas distribution
• Predicting the Yield of Small Transiting Exoplanets around Mid-M and Ultra-Cool Dwarfs in the Nancy Grace Roman Space Telescope Galactic Bulge Time Domain Survey
• Strong limits on keV-scale galactic sterile neutrino dark matter with stray light from NuSTAR after 11 years of operation
• Robustness of dark matter constraints and interplay with collider searches for New Physics
• Linking nearby stellar streams to more distant halo overdensities
• Can ultralight dark matter explain the age-velocity dispersion relation of the Milky Way disc: A revised and improved treatment
• The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• The Age-Metallicity-Specific Orbital Energy Relation for the Milky Way's Globular Cluster System Confirms the Importance of Accretion for Its Formation
• Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way
• 60 candidate high-velocity stars originating from the Sagittarius dwarf spheroidal galaxy in Gaia EDR3
• Typhon: a polar stream from the outer halo raining through the Solar neighborhood
• Substructures, Resonances and debris streams
• Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*
• An enquiry on the origins of N-rich stars in the inner Galaxy basedon APOGEE chemical compositions
• Investigating the detection of dark matter subhalos as extended sources with Fermi-LAT
• Two channels for the formation of compact dwarf galaxies in clusters of galaxies
• Testing the weak equivalence principle by differential measurements of fundamental constants in the Magellanic Clouds
• GalactICS with Gas
• Gaia DR2 orbital properties for field stars with globular cluster-like CN band strengths
• The orbital evolution of UFDs and GCs in an evolving Galactic potential
• The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
• The metal-poor end of the Spite plateau. II. Detailed chemical investigation
• Discovery and Timing of Millisecond Pulsars in the Globular Cluster M5 (NGC 5904) with FAST and Arecibo
• Gravitational focusing effects on streaming dark matter as a new detection concept
• Unveiling the past evolution of the progenitor of the Helmi streams
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
• Probability of forming gaps in the GD-1 stream by close encounters of globular clusters
• A purely acceleration-based measurement of the fundamental Galactic parameters
• Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
• Constructing the Milky Way Stellar Halo in the Galactic Center by Direct Orbit Integration
• On the metal-poor edge of the Milky Way "thin disc"
• The effect of stellar encounters on the dark matter annihilation signal from prompt cusps
• The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy
• Improved bounds on the bosonic dark matter with pulsars in the Milky Way
• Antaeus: a retrograde group of tidal debris in the Milky Way's disk plane
• Directly testing gravity with Proxima Centauri
• The giants that were born swiftly -- Implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters
• VVV-WIT-08: the giant star that blinked
• Stellar encounters with giant molecular clouds
• A halo of trapped interstellar matter surrounding the solar system
• PBH assisted search for QCD axion dark matter
• How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
• Investigating the amplitude and rotation of the phase spiral in the Milky Way outer disc
• New constraints on the kinematic, relativistic and evolutionary properties of the PSR J1757$-$1854 double neutron star system
• Mass measurements and 3D orbital geometry of PSR J1933$-$6211
• Chrono-chemodynamical analysis of the globular cluster NGC 6355: Looking for the fundamental bricks of the Bulge
• The Spectacular Tidal Tails of Globular Cluster M3 (NGC 5272)
• 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
• Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.S
• Dark Matter Substructure under the Electron Scattering Lamppost
• The longevity of the oldest open clusters: Structural parameters of NGC 188, NGC 2420, NGC 2425, NGC 2682, NGC 6791, NGC 6819
• On the Galactic rotation curve inferred from the Jeans equations Assessing its robustness using Gaia DR3 and cosmological simulations
• Ripples spreading across the Galactic disc. Interplay of direct and indirect effects of the Sagittarius dwarf impact
• Deceleration of kicked objects due to the Galactic potential
• SDSS-IV MaNGA: the "G-dwarf problem" revisited
• Synthetic observations of spiral arm tracers of a simulated Milky Way analog
• Finding $r$-II sibling stars in the Milky Way with the Greedy Optimistic Clustering algorithm
• The LMC impact on the kinematics of the Milky Way satellites: clues from the running solar apex
• The orbital-decay test of general relativity to the 2% level with 6-year VLBA astrometry of the double neutron star PSR J1537+1155
• Discovery of an $[Fe/H]\sim -4.8$ Star in $Gaia$ XP Spectra
• High Velocity Stars in SDSS/APOGEE DR17
• Virial Clumps in Central Molecular Zone Clouds
• Mass-loss and composition of wind ejecta in type I X-ray bursts
• Constraints on the electron-to-proton mass ratio variation at the epoch of reionization
• Searching for Milky Way twins: Radial abundance distribution as a strict criterion
• Evidence For Multiple Accretion Events in the $Gaia$-Sausage/Enceladus Structures
• Constrained cosmological simulations of the Local Group using Bayesian hierarchical field-level inference
• Kinematic constraints on the ages and kick velocities of Galactic neutron star binaries
• Frequencies, chaos and resonances: a study of orbital parameters of nearby thick disc and halo stars
• The historical record of massive star formation in Cygnus
• Characterisation of local halo building blocks: Thamnos and Sequoia
• On $N$-body simulations of globular cluster stream
• Efficient and accurate force replay in cosmological-baryonic simulations
• Searching Accretion-Enhanced Dark Matter Annihilation Signals in the Galactic Centre
• The shapes and alignments of the satellites of the Milky Way and Andromeda
• Accurate Computation of the Screening of Scalar Fifth Forces in Galaxies
• Multi-TeV dark matter density in the inner Milky Way halo: spectral and dynamical constraints
• Fermi bubbles: the collimated outburst needed to explain forward-shock edges
• Moons Are Planets: Scientific Usefulness Versus Cultural Teleology in the Taxonomy of Planetary Science
• The FAST Globular Cluster Pulsar Survey (GC FANS)
• Weighing the Galactic disk using phase-space spirals IV. Tests on a three-dimensional galaxy simulation
• Efficient radial migration by giant molecular clouds in the first several hundred Myr after the stellar birth
• Using heritability of stellar chemistry to reveal the history of the Milky Way
• Connecting the local stellar halo and its dark matter density to dwarf galaxies via blue stragglers
• The Pristine survey: XXV. The very metal-poor Galaxy: Chemodynamics through the follow-up of the Pristine-Gaia synthetic catalogue
• The GALAH Survey: No chemical evidence of an extragalactic origin for the Nyx stream
• NGC 307 and the Effects of Dark-Matter Haloes on Measuring Supermassive Black Holes in Disc Galaxies
• LMC-driven anisotropic boosts in stream--subhalo interactions
• Constraining Sterile Neutrino Dark Matter in the Milky Way Halo with Swift-XRT
• Testing gravity with interstellar precursor missions
• Important stellar perturbers found during the StePPeD database update based on Gaia EDR3 data
• Inhomogeneity in the early Galactic chemical enrichment exposed by beryllium abundances in extremely metal-poor stars
• $S^5$: New insights from deep spectroscopic observations of the tidal tails of the globular clusters NGC 1261 and NGC 1904
• The earliest phases of CNO enrichment in galaxies
• A Preferential Attachment Model for the Stellar Initial Mass Function
• Comparing bulge RR Lyrae stars with bulge giants -- Insight from 3D kinematics
• Could very low-metallicity stars with rotation-dominated orbits have been shepherded by the bar?
• Limits on dark matter annihilation in prompt cusps from the isotropic gamma-ray background
• Characterization and dynamics of the peculiar stream Jhelum, A tentative role for the Sagittarius dwarf galaxy
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models
• New stellar velocity substructures from Gaia DR3 proper motions
• Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field
• Hidden deep in the halo: selection of a reduced proper motion halo catalogue and mining retrograde streams in the velocity space
• Non-Parametric Spherical Jeans Mass Estimation with B-splines
• Searching for Extragalactic Exoplanetary Systems: the Curious Case of BD+20 2457
• Prospects for Detecting Gaps in Globular Cluster Stellar Streams in External Galaxies with the Nancy Grace Roman Space Telescope
• G112-43/44: A metal-poor binary star with a unique chemical composition and kinematics like the Helmi streams
• Absence of obvious tidal tails around the globular cluster NGC 6397
• Untangling the Sources of Abundance Dispersion in Low-Metallicity Stars
• Cosmic Ray Antihelium from a Strongly Coupled Dark Sector
• Li distribution, kinematics and detailed abundance analysis among very metal-poor stars in the Galactic halo from the HESP-GOMPA survey
• On Detecting Interstellar Scintillation in Narrowband Radio SETI
• Populating The Milky Way: Characterising Planet Demographics by Combining Galaxy Formation Simulations and Planet Population Synthesis Models
• Metallicity and $\alpha$-abundance for 48 million stars in low-extinction regions in the Milky Way
• Equilibrium axisymmetric halo model for the Milky Way and its implications for direct and indirect DM searches
• Dynamically Forming Extremely Low-Mass White Dwarf Binaries in Wide Orbits
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• The vertical structure of the spiral galaxy NGC 3501: first stages of the formation of a thin metal-rich disc
• Peeking beneath the precision floor -- II. Probing the chemo-dynamical histories of the potential globular cluster siblings, NGC 288 and NGC 362
• Gaia DR 2 data and the evolutionary status of eight high velocity hot post-AGB candidates
• How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
• The dynamics of Galactic centre pulsars: constraining pulsar distances and intrinsic spin-down
• Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
• First spiral arm detection using dynamical mass measurements of the Milky Way disk
• Element abundance analysis of the metal-rich stellar halo and high-velocitythick disk in the galaxy
• The Likelihood of Undiscovered Globular Clusters in the Outskirts of the Milky Way
• Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
• The $Hubble$ Missing Globular Cluster Survey. I. Survey overview and the first precise age estimate for ESO452-11 and 2MASS-GC01
• Radial and azimuthal gradients of the moving groups in Gaia DR3: The slow/fast bar degeneracy problem
• Existence of the Metal-Rich Stellar Halo and High-velocity Thick Disk in the Galaxy
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78
• Evidence for Co-rotation Origin of Super Metal Rich Stars in LAMOST-Gaia: Multiple Ridges with a Similar Slope in phi versus Lz Plane
• Europium, we have a problem. Modelling r-process enrichment across Local Group galaxies
• Chemodynamical Properties and Ages of Metal-Poor Stars in S-PLUS
• Limitations and rotation of the two-armed phase spiral in the Milky Way stellar disc
• Study of Jupiter's Interior with Quadratic Monte Carlo Simulations
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• The Influence of the Galactic Bar on the Dynamics of Globular Clusters
• Can Planet 9 be an Axion Star?
• Chemodynamic evolution of Sun-like stars in nearby moving groups
• Rediscovering the Milky Way with orbit superposition approach and APOGEE data I. Method validation
• Quantifying torque from the Milky Way bar using Gaia DR2
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• A particle's perspective on screening mechanisms
• Nearby open clusters with tidal features: golden sample selection and 3D structure
• $G$ Objects and primordial black holes
• On the chaos induced by the Galactic bar on the orbits of nearby halo stars
• New Constraints on Decaying Dark Matter from INTEGRAL/SPI
• Revisit NGC 5466 Tidal Stream with $Gaia$, SDSS/SEGUE and LAMOST
• Weakly-Supervised Anomaly Detection in the Milky Way
• A kinematically constrained kick distribution for isolated neutron stars
• A Pristine-UNIONS view on the Galaxy: Kinematics of the distant spur feature of the Sagittarius stream traced by Blue Horizontal Branch stars
• The Solar System's passage through the Radcliffe wave during the middle Miocene
• Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary
• Two substructures in the nearby stellar halo found in Gaia and RAVE
• Tidal Suppression of Fuzzy Dark Matter Heating in Milky Way Satellite Galaxies
• Revisiting Pulsar Velocities Using Gaia Data Release 2
• Young stars raining through the Galactic Halo: the nature and orbit of Price-Whelan 1
• Probing the Halo Gas Distribution in the Inner Galaxy with Fermi Bubble Observations
• Exploring the ex-situ components within Gaia DR3
• Chemodynamics of metal-poor wide binaries in the Galactic halo: Association with the Sequoia event
• Gaps in stellar streams as a result of globular cluster fly-bys
• Prospects for probing small-scale dark matter models with pulsars around Sagittarius A*
• Discovery of a pair of very metal-poor stars enriched in neutron-capture elements: The proto-disk r-II star BPS CS 29529-0089 and the Gaia-Sausage-Enceladus r-I star TYC 9219-2422-1
• Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
• A chemodynamical analysis of bright metal-poor stars from the HESP-GOMPA survey -- Indications of a non-prevailing site for light r-process elements
• Supernova-Neutrino-Boosted Dark Matter from All Galaxies
• Proper Motions of the Satellites of M31
• Existence of Tidal Tails for the Globular Cluster NGC 5824
• No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
• The double neutron star PSR J1946+2052 I. Masses and tests of general relativity
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• The oldest stars with low neutron-capture element abundances and origins in ancient dwarf galaxies
• Can tides explain the low dark matter density in Fornax?
• First measurement of the triaxiality of the inner dark matter halo of the Milky Way
• A Gaia based photometric and kinematic analysis of the old open cluster King 11
• On the Galactic radio signal from stimulated decay of axion dark matter
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal) -- III. Age and metallicity distribution of Gaia-Sausage-Enceladus stars near the Sun
• Dynamical streams in the local stellar halo
• Pushing the boundaries of asteroseismic individual frequency modelling: unveiling two evolved very-low metallicity red giants
• An Actinide-boost Star Discovered in the Gaia-Sausage-Enceladus
• Dynamical mirages: how bar-induced resonant trapping can mimic substructure clustering in dynamical parameter spaces
• Determination of Sodium Abundance Ratio from Low-Resolution Stellar Spectra and Its Applications
• Radio and gamma-ray timing of TRAPUM L-band Fermi pulsar survey discoveries
• Local dark matter density from Gaia DR3 K-dwarfs using Gaussian processes
• Nearby stellar substructures in the Galactic halo from DESI Milky Way Survey Year 1 Data Release
• A Simulation Based Inference Approach to the Dynamics of the MW-LMC System -- Validation
• Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
• AMS-02 antiprotons and dark matter: Trimmed hints and robust bounds
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• The Pristine Survey -- XXVII. Journey to the Galactic outskirts -- Mapping the outer halo red giant stars down to the very metal-poor end
• Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• NGC 1851A: Revealing an ongoing three-body encounter in a dense globular cluster
• The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
• Rotation Curve of the Milky Way and the Dark Matter Density
• Dark sector domain walls could explain the observed planes of satellites
• Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream
• SDSS-IV MaNGA: Ionization sources of diffuse extra-planar galactic medium
• A Vertically Orientated Dark Matter Halo Marks a Flip of the Galactic Disk
• Dark matter spiral arms in Milky Way-like halos
• Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool
• Destruction of the central black hole gas reservoir through head-on galaxy collisions
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• A Dwarf Galaxy Debris Stream Associated with Palomar 1 and the Anticenter Stream
• A study of full space motions of outer Galactic disk A and F stars in two deep pencil-beams
• Unveiling VVV/WISE Mira variables on the far side of the Galactic disk: Distances, kinematics and a new extinction law
• Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars
• A new understanding of the Gemini-Monoceros X-ray enhancement from discoveries with eROSITA
• Globular clusters in \textsc{OrbIT}: complete dynamical characterisation of the globular cluster population of the Milky Way through updated orbital reconstruction
• The Chemodynamical Nature of the Triangulum-Andromeda Overdensity
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• On the Use of Field RR Lyrae as Galactic Probes -- VIII. Early Formation of the Galactic Spheroid
• Open cluster members in APOGEE DR17 I. Dynamics and star members
• Searching for new Hypervelocity Stars with Gaia DR3 and VLT/FORS2 Spectroscopy
• The R-Process Alliance: Hunting for gold in the near-UV spectrum of 2MASS J05383296-5904280
• Detecting dilute axion stars constrained by fast radio bursts in the Solar System via stimulated decay
• Using dust to constrain dark matter models
• Constraints on the parameters of keV-scale mass annihilating Dark Matter obtained with SRG/ART-XC observations
• The R-Process Alliance: Exploring the cosmic scatter among ten r-process sites with stellar abundances
• Lost Sisters Found: TESS and Gaia Reveal a Dissolving Pleiades Complex
• Investigating the vertical distribution of the disk as a function of radial action
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• J01020100-7122208: an accreted evolved blue straggler that wasn't ejected from a supermassive black hole
• Very metal-poor stars in the solar vicinity: kinematics and abundance analysis
• 3D Kinematics of Stellar SiO Masers in the Galactic Center
• Comparing simulated Milky Way satellite galaxies with observations using unsupervised clustering
• M dwarf spectral indices at moderate resolution: accurate $T_{\mathrm{eff}}$ and [Fe/H] for 178 southern stars
• Galactic Orbital Effects on Pulsar Timing
• The K supergiant runaway star HD 137071
• Dark matter effect attributed to the inherent structure of cosmic space
• Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• Possible tidal dissipation in millisecond pulsar binaries
• Influence of the Galactic gravitational field on the positional accuracy of extragalactic sources. II Observational appearances and detectability
• Consistencies and inconsistencies in redshift-independent distances
• Partitioning the Galactic Halo with Gaussian Mixture Models
• Main-sequence Turnoff Stars as Probes of the Ancient Galactic Relic: Chemo-dynamical Analysis of a Pilot Sample
• The metal-poorest tail of the Galactic halo: hypothesis on its origin from precise spectral analysis
• The Spheroidal Bulge of the Milky Way: Chemodynamically Distinct from the Inner-Thick Disc and Bar
• The Nephele ecosystem: stars, globular clusters, and stellar streams associated with the progenitor galaxy of $\omega$ Centauri
• Testing the predictions of axisymmetric distribution functions of galactic dark matter with hydrodynamical simulations
• Deciphering the Milky Way's star formation at cosmic noon with high proper-motion stars: A precursor to the merger-driven starburst
• Co-evolution of Nuclear Star Clusters and Massive Black Holes: Extreme Mass-Ratio Inspirals
• Can supernova from runaway stars mimic the signs of absorbing `super-virial' gas?
• Machine Learning the Dark Matter Halo Mass of Milky Way-Like Systems
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• Bulgeless Evolution And the Rise of Discs (BEARD) II. The role of mergers in shaping the Milky Way analogues in TNG50
• On the baryon budget in the X-ray-emitting circumgalactic medium of Milky Way-mass galaxies
• Minimum-entropy constraints on galactic potentials
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits
• The First Star-by-star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model
• Signatures of simulated spiral arms on radial actions
• Gaia DR2 and EDR3 data and evolutionary status of post-AGB stars with high radial velocities
• Stellar substructures in the Galactic disc and halo: Properties, origins, and evolution
• Discovery of Galactic center ejected star in DESI DR1
• PSR J1227$-$6208 and its massive white dwarf companion: pulsar emission analysis, timing update and mass measurements
• The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates
• Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
• Resonant Effects of a Bar on the Galactic Disk Kinematics Perpendicular to Its Plane
• Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number
• Numerical solutions of the complete two-body system in QUMOND
• Retuning radio astronomy for axion dark matter with neutron stars
• Observing Double White Dwarfs with the Lunar GW Antenna
• Not all nitrogen-rich field stars originate from globular clusters
• The angular momentum of stars reflects the relationship between star-forming environment and galactic evolution history
• Tidal disruption events as the origin of the eROSITA and Fermi bubbles
• Neutrinos from stars in the Milky Way
• GSE vs. LMC: reshaping of radially biased stellar haloes by satellites
• Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars
• Searching for stars ejected from the Galactic Centre in DESI
• The odd bunch: chrono-chemo-dynamics of sixteen unusual stars from Kepler
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• Undetected past contacts with technological species: implications for technosignature science
• The metal-poor tail of the APOGEE survey I. Uncovering [Fe/H] < -2.5 stars from the inner Galaxy to the Magellanic Clouds
• Gravitational waves from primordial black holes passing by neutron stars: observational prospects for the Galactic center
• Comparing radial migration in dark matter and MOND regimes
• Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests
• Search for a photon peak from keV-scale dark matter annihilation with NuSTAR: Constraints on $⟨\sigma v⟩$ after 11 years of observations
• On the connection between nitrogen-enhanced field stars and the Galactic globular clusters
• Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
• HE0144-4657: A Carbon-Enhanced Ultra Metal-Poor Star ([Fe/H] ~ -4.1) from the Helmi Stream Disrupted Dwarf Galaxy
• First large scale spatial and velocity patterns of local metal-rich stars in the Milky Way
• Orbital dynamics in galactic potentials under mass transfer
• Insights into the structure and kinematics of a Milky Way-like galaxy
• Radio timing constraints on the mass of the binary pulsar PSR J1528-3146
• The cosmic journey of dust grains -- from nucleation to planetary system
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• A search for stellar structures around nine outer halo globular clusters in the Milky Way
• Improving the spin-down limits of the continuous gravitational waves emitted from rotating triaxial pulsars
• Detectability of compact intermediate-mass black hole binaries as low-frequency gravitational wave sources: the influence of dynamical friction of dark matter
• Three Models of the Gravitational Potential of the Milky Way
• Globular clusters of the Gaia Enceladus/Sausage -- I. Orbital and dynamical evolution on cosmological timescales
• Unit conversions and collected numbers in cosmology
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• From the Fire: A Deeper Look at the Phoenix Stream
• Galactic Electron-Positron Annihilation Emission from X-Ray Binaries with Transient and Persistent Jets
• The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models
• Photo-chemo-dynamical analysis and the origin of the bulge globular cluster Palomar 6
• The multiple corrugations in the Galactic disk derived from the LAMOST and Gaia survey data
• IY Lyr: A Thick-Disk first-overtone RR Lyrae Star with a Possible Neutron Star Companion
• The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter
• First evidence of a collision between two unrelated open clusters in the Milky Way
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• Probing the Milky Way Halo with RR Lyrae Stars from Gaia Data Release 3
• A new member of the Milky Way's family tree: Characterizing the Pontus merger of our Galaxy
• The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios
• Infrared photometry and CaT spectroscopy of the most metal-poor in-situ globular cluster VVV-CL001
• Signatures of Galactic Expansion in Gaia DR3: Implications for the JWST Early-Galaxy Puzzle
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• Redshifted civilizations, galactic empires, and the Fermi paradox
• Dark matter and LHC: Complementarities and limitations
• Constraints on extended axion structures from the lensing of fast radio bursts
• Dynamical Models of the Milky Way in Action Space with LAMOST DR8 and GAIA EDR3
• Antinuclei from Primordial Black Holes
• Constraining Fermionic Dark Matter with Galactic Neutron Stars
• Mapping the evolution of supernova-neutrino-boosted dark matter within the Milky Way
• Most dwarf spheroidal galaxies surrounding the Milky Way cannot be dark-matter dominated satellites
• On the most reliable value of the Galactic aberration constant
• Testing MOND using the dynamics of nearby stellar streams
• The disturbed outer Milky Way disc