The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package^*

2018/08/23 by A. M. Price-Whelan, Adrian M. Price-Whelan, B. M. Sipőcz +200 · 746 citations
Computer Science · Physics and Astronomy · #Computational Physics and Python Applications #Astronomy and Astrophysical Research #Advanced Data Storage Technologies

paper · pdf · doi:10.3847/1538-3881/aabc4f

Abstract

Abstract The Astropy Project supports and fosters the development of open-source and openly developed Python packages that provide commonly needed functionality to the astronomical community. A key element of the Astropy Project is the core package astropy , which serves as the foundation for more specialized projects and packages. In this article, we provide an overview of the organization of the Astropy project and summarize key features in the core package, as of the recent major release, version 2.0. We then describe the project infrastructure designed to facilitate and support development for a broader ecosystem of interoperable packages. We conclude with a future outlook of planned new features and directions for the broader Astropy Project.

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• Characterizing TESS-Identified Quadruple and Higher Order Eclipsing Binaries: I. Speckle Imaging with DSSI and HRCam
• Clouds and Clarity: Revisiting Atmospheric Feature Trends in Neptune-size Exoplanets
• The Calibration of Short Wavelength Polycyclic Aromatic Hydrocarbon Emission as Star Formation Rate Indicators with JWST
• ALMASOP: Inner-Envelope Structures of Protostars Driving Nascent Jets
• The Evolution in Coma Molecular Composition of Comet C/2017 K2 (PanSTARRS) Across the H₂O Sublimation Zone: ALMA Imaging of an H₂O-Dominated Coma
• The Triple System V1371 Tau: An Eclipsing Binary with an Outer Be Star
• Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth τ
• The Apache Point Observatory extra-Galactic Evolution Experiment (APOeGEE): Chemical Abundance Trends for Seven Dwarf Spheroidal Galaxies in the APOGEE Survey
• Discovery of a 9.67-s pulsar in an ultraluminous X-ray source in NGC 4631 with XMM-Newton
• SOFIA FEEDBACK Survey: The Eagle Nebula in [C II] and Molecular Lines
• ALMA and JWST Imaging of z &gt; 6 Quasars: No Spatial Position Offset Observed Between Quasars and Their Host Galaxies
• X-Ray Observations of Old Nearby Supernovae: Constraints on Compact Object Populations and Late Interaction
• Convolutional Neural Networks for classifying galaxy mergers: Can faint tidal features aid in classifying mergers?
• Discovery of the First Five Carbon-Enhanced Metal-Poor Stars in the LMC
• A New High-latitude H <scp>i</scp> Cloud Complex Entrained in the Northern Fermi Bubble
• Profiling Near-surface Winds on Mars Using Attitude Data from Mars 2020 Ingenuity
• Benchmarking differential reddening in front of globular clusters
• Stellar Birth Radii in the LMC: Insights into Chemodynamics, Radial Migration, and Star Formation Across the Disk
• A Correlation Between the Final Separation and Mass Ratio from Common Envelope Simulations
• A JWST Transit of a Jupiter Analog I: Constraints on the Oblateness of Kepler-167e
• Quasars acting as Strong Lenses Found in DESI DR1
• Star Formation Histories and Stellar Dynamics in the Central Galaxies of RX J0820.9+0752, A1835, and PKS 0745-191
• A Possible "Too-Many-Satellites" Problem in the Isolated Dwarf Galaxy DDO 161
• 52 Eclipsing Quadruple Star Candidates Discovered in TESS Full Frame Images
• AGN--Host Galaxy Image Decomposition with JWST
• Deconvolution for Large Astronomical Surveys: A Study of the Scaled Gradient Projection Method on Zwicky Transient Facility Data
• Figuring Out Gas &amp; Galaxies In Enzo (FOGGIE). XIII. On the Observability of Extended HI Disks and Warps
• Disk Formation and the Size-sSFR Relation of Dwarf Galaxies
• The Library of Exoplanet Atmospheric Composition Measurements: Population Level Trends in Exoplanet Composition with ExoComp
• The ODYSSEUS Survey. Spatial correlation of magnetospheric inclinations points to parsec-scale star-cloud connection
• The magnetic fields of the dusty nuclei and molecular outflows of Arp 220
• The N_H Distribution of Hard X-ray Selected AGN in the NEP Field
• oMEGACat. VIII. A Subpopulation Census of ω Centauri
• Mitigating gain calibration errors from EoR observations with SKA1-Low AA*
• Figuring Out Gas &amp; Galaxies In Enzo (FOGGIE) XI: Circumgalactic O VI Emission Traces Clumpy Inflowing Recycled Gas
• The <i>JWST</i> Emission Line Survey (JELS): the sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• A giant planet transiting a 3-Myr protostar with a misaligned disk
• Limits on the flux of nuclearites and other heavy compact objects from\n the "Pi of the Sky" project
• The Discovery and Evolution of a Possible New Epoch of Cometary Activity by the Centaur (2060) Chiron
• Morphological Classification of Galaxies in S-PLUS using an Ensemble of Convolutional Networks
• An Updated SynthPop Model for Microlensing Simulations I: Model Description & Evaluation
• Inferring Stellar Densities with Flexible Models I: The Distribution of RR Lyrae in the Milky Way with Gaia DR3
• The Barnard’s Star planetary system: stability, composition, and evolution of four sub-Earth exoplanets
• Toward an open‐source 3D‐printable laboratory
• A Mid-Infrared Spectroscopic Study of Young Stellar Objects in the SMC Region NGC 346: JWST Detects Dust, Accretion, Ices and Outflows
• <scp>fink</scp>, a new generation of broker for the LSST community
• Ray-tracing a small orbital mission for soft-X-ray polarimetry
• Generalization from Low- to Moderate-Resolution Spectra with Neural Networks for Stellar Parameter Estimation: A Case Study with DESI
• RV-exoplanet eccentricities: Good, Beta, and Best
• Towards a measurement of the primordial helium isotope ratio
• Emerging Diversity Among the Main-Belt Comets: Insights from JWST and Ground-Based Observations of 457P/Lemmon-PANSTARRS
• White Dwarf Merger Remnants with Cooling Delays on the Q Branch Lack Strong Magnetism
• BE Lyncis is not a Black Hole Binary: Lessons From Gaia and Hipparcos Astrometry
• Probing the Physical and Chemical Characteristics of an Extremely Early Class 0 Protostar in G204.4-11.3A2-NE
• A Systematic Search for Gaseous Debris Disks in DESI Early Data Release White Dwarfs
• XRISM/Resolve reveals the complex iron structure of NGC 7213: Evidence for radial stratification between inner disk and broad-line region
• The White Dwarf Initial-Final Mass Relation from Open Clusters in Gaia DR3
• JWST-TST DREAMS: Quartz Clouds in the Atmosphere of WASP-17b
• Galaxy Spin Alignment with Tidal Fields in the SDSS-IV MaNGA Survey
• AT2025ulz and S250818k: Deep X-ray and radio limits on off-axis afterglow emission and prospects for future discovery
• Sensitivity to Sub-Io-sized Exosatellite Transits in the MIRI LRS Lightcurve of the Nearest Substellar Worlds
• Discovery of SN 2025wny: a Strongly Gravitationally Lensed Superluminous Supernova at z = 2.01
• The Near-Ultraviolet Spectra of FU Orionis Accretion Disks
• Validating Open Cluster Candidates with Photometric Bayesian Evidence
• SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z &gt; 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit
• The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5
• Ultracool dwarf Science with MachIne LEarning (USMILE). I. Scalable Tree-Based Models for Photometric Spectral Classification and New Discoveries from LSST Data Preview 1 and Euclid Quick Data Release 1
• Do Young Suns Produce Frequent, Massive CMEs? Results from Five-year Dedicated Optical Observations of EK Draconis and V889 Hercules
• The Solar Neighborhood. LV. M Dwarf Twin Binaries -- One in Five Twin Sibling Pairs Are Mismatched in Activity and/or Rotation
• Earth Analogs in Reflected Light: Insights from Early Spectral Characterization in Unconstrained Orbits
• SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations
• The velocity dispersion profile of nine open clusters in the solar neighborhood
• Exploring the statistical properties of double radio relics in the TNG-Cluster and TNG300 simulations
• Aiming for Proxima Centauri b: Gravitational effects on relativistic spacecraft trajectories
• The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
• Discovery of a Debris Disk Around TWA 20
• SPHEREx: Aromatics, Aliphatics and PAH Size across the Iris Nebula
• Discovery of 79 δ Scuti Stars in NGC 3532 Suggests a Decrease of Pulsator Occurrence with Age
• A Census of Chemically Peculiar Stars in Stellar Associations
• A Compact Multi-Planet System of Three Transiting Giant Planets Around TIC118798035
• XRISM/Resolve Spectroscopy of the Central Engine in the Seyfert-1 AGN Mrk 279
• The \mathttWebSky [CII] Forecasts and the search for primordial intermittent non-Gaussianity
• Milky Way Mass Through Escape Velocity Curve from LAMOST K Giants
• AT2025ulz and S250818k: zooming in with the Hubble Space Telescope
• Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered Via UV Excess
• A spectral library and census of near-infrared stellar large-amplitude variables from Palomar Gattini-IR
• Rise of the forsaken relics: connecting present-day stellar streams and phase-mixed galaxies to the Epoch of Reionization
• A High-Resolution Spectroscopic Survey of Directly Imaged Companion Hosts: II. Diversity in C/O Ratios among Host Stars
• Increased molecular gas velocity dispersion and star formation efficiency in barred galaxy centres
• Optimizing Kilonova Searches: A Case Study of the Type IIb SN 2025ulz in the Localization Volume of the Low-Significance Gravitational Wave Event S250818k
• Extending the [C/N]-Age Calibration: Using Globular Clusters to Explore Older and Metal-Poor Populations
• Investigating the Effects of Point Source Injection Strategies on KMTNet Real/Bogus Classification
• Compact vs. Scattered: Suitability of Southern 6.7GHz Methanol Masers for VLBI astrometry
• Contribution from Nonlinear Quasi-normal Modes in GW250114
• PAH Emission Spectra and Band Ratios for Arbitrary Radiation Fields with the Single Photon Approximation
• Unbound Tails and Compressed Heads: A JCMT Study of the SFO 38 Cloud
• CHIME-o-Grav: Wideband Timing of Four Millisecond Pulsars from the NANOGrav 15-yr dataset
• Spectroscopic Follow-up of Young High-α Dwarf Star Candidates: Still Likely Genuinely Young
• The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-Sequence Galaxies at z=4-6
• What is the True HI Gas Content in Massive Quiescent Galaxies in the Local Universe?
• StarStream: Automatic detection algorithm for stellar streams
• StarStream on Gaia: Stream discovery and mass loss rate of globular clusters
• Eclipsing Stellar Flare on the Demon Star Algol Binary System Observed during the MAXI-NICER Follow-up Campaign in 2018
• Polarization Dynamics of X-Ray Synchrotron Emission from a Multi-Zone Blazar Jet
• Galaxy Protoclusters as Drivers of Cosmic Reionization: I. Bubble Overlap at Redshift z ~ 7 in LAGER-z7OD1
• Investigating the Formation of Planets Interior to in situ Hot Jupiters
• ALMAGAL VIII. Cataloging Hierarchical Mass Structure from Cores to Clumps across the Galactic Disk
• A 50-min coronal kink oscillation and its possible photospheric counterpart
• The rings of (2060) Chiron: Evidence of an evolving system
• Strategy for identifying Vera C. Rubin Observatory kilonova candidates for targeted gravitational-wave searches
• Hubble reveals complex multi-scale structure in the edge-on protoplanetary disk IRAS 23077+6707
• The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape
• Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
• JWST/MIRI-MRS view of the metal-poor galaxy CGCG 007-025: the spatial location of PAHs and very highly ionized gas
• NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists
• Reanalysis of the eclipses of LHS 1140 c: No evidence of an atmosphere and implications for the internal structure of the planet
• Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
• The Green Bank Ammonia Survey: Data Release 2
• Dark gaps and resonances in barred galaxies
• Environmental Regulation of Dust and Star Formation Unveiled by Subaru Dual Narrow-band Imaging: Degree-scale Balmer Decrement Mapping across a z = 0.9 Supercluster
• New Synoptic Observations of the Cosmic Optical Background with New Horizons
• Discovery of an Accretion Burst in a Free-Floating Planetary-Mass Object
• The influence of tight binaries on proto-planetary disk masses
• A complex structure of escaping helium spanning more than half the orbit of the ultra-hot Jupiter WASP-121 b
• GMIMS-DRAGONS: A Faraday Depth Survey of the Northern Sky Covering 350 to 1030 MHz
• Measuring the Temperature of Extremely Hot Shock-Heated Gas in the Major Merger MACS~J0717.5+3745 With Relativistic Corrections to the Sunyaev-Zel'dovich Effect
• LATIS Data Release: ∼4200 Spectra of z ∼ 2-3 Galaxies, Redshifts, and Intergalactic Medium Tomography Maps
• The Distribution of Quenched Galaxies in the Massive z = 0.87 Galaxy Cluster El Gordo
• Direct Spectroscopy of 51 Eridani b with JWST NIRSpec
• Classification for 969 double-mode RR Lyrae stars from Zwicky Transient Facility
• An automated probabilistic asteroid prediscovery pipeline
• Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys
• Machine Learning for Radial Velocity Analysis I: Vision Transformers as a Robust Alternative for Detecting Planetary Candidates
• Machine Learning Techniques to Distinguish Giant Stars from Dwarf Stars Using Only Photometry -- Pushing Redwards
• In-flight performance of the IXPE telescopes
• A Sample of HeII λ4686 "Changing-Look" Quasars
• Mapping the Cloud-Driven Atmospheric Dynamics &amp; Chemistry of an Isolated Exoplanet Analog with Harmonic Signatures
• Study of HI Turbulence in the SMC Using Multi-point Structure Functions
• A Link Between Rocky Planet Density and Host Star Chemistry
• Methanol emission tracing ice chemistry and dust evolution in the TW Hya protoplanetary disk
• Mapping the Stellar Kinematics in the Central 240 Parsecs of M87 with the James Webb Space Telescope
• Signatures of Galactic Expansion in Gaia DR3: Implications for the JWST Early-Galaxy Puzzle
• SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604
• Threading the Magellanic Needle: Hypervelocity Stars Trace the Past Location of the LMC
• JWST Observations of Starbursts: PAHs Closely Trace the Cool Phase of M82's Galactic Wind
• Pan-STARRS follow-up of the gravitational-wave event S250818k and the lightcurve of SN 2025ulz
• Forecasting the Observable Rates of Gravitationally Lensed Supernovae for the PASSAGES Dusty Starbursts
• Searching for Ultra-light Dark Matter in Spatial Correlations of White Dwarf Structure
• A Cold and Super-Puffy Planet on a Prograde Orbit
• An Efficient Shift-and-Stack Algorithm Applied to Detection Catalogs
• FIELDMAPS Data Release: Far-Infrared Polarization in the "Bones" of the Milky Way
• The Hourglass-shaped Magnetic Fields and Dust Filaments in the HH 211 Protostellar Envelope
• SN 2025coe: A Multiple-Peaked Calcium-Strong Transient from A White-Dwarf Progenitor
• Second-timescale Glints from Satellites and Space Debris Detected with Tomo-e Gozen
• Automated Modeling with AAP-Imfit: Astrometry and Photometry via CASA
• oMEGACat. VII. Tracing Interstellar and Intracluster Medium of ω Centauri using Sodium Absorptions
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• [C/N] Ages for Red Giants and their Implications for Galactic Archaeology
• Planets larger than Neptune have elevated eccentricities
• JWST/MIRI Imaging of the Warm Dust Component of the <i>ϵ</i> Eridani Debris Disk
• Diffusion-based Galaxy Simulations for the Nancy Grace Roman Space Telescope High Latitude Survey
• The Orbital Eccentricities of Planets in the Kinematic Thin and Thick Galactic Disks
• Unveiling a 36 billion solar mass black hole at the centre of the Cosmic Horseshoe gravitational lens
• Probing the origin of the X-ray and optical emission in the z=3.1 strongly lensed radio-quiet quasar GraL J065904.1+162909 to milliarcsecond resolution
• Comprehensive X-ray Observations of the Exceptional Ultra-long X-ray and Gamma-ray Transient GRB 250702B with Swift, NuSTAR, and Chandra: Insights from the X-ray Afterglow Properties
• Optical/infrared observations of the extraordinary GRB 250702B: a highly obscured afterglow in a massive galaxy consistent with multiple possible progenitors
• Detection of HI filament: Pair Stacking vs. Filament Stacking
• The impact of cosmic filaments on the abundance of satellite galaxies
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z&gt;6 JWST Results? CMB Experiments can discover the Origin in Near Future
• Masses, Star-Formation Efficiencies, and Dynamical Evolution of 18,000 HII Regions
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• A Two-Stage Kick Scenario for the Peculiar LMXB GX 1+4
• Unveiling Central ortho-H2D+ Depletion at Sub-kau Scales in Prestellar Core G205.46-14.56M3: The First Interferometric Evidence and Implications for Deuterium Chemistry
• Reconciling the Tension Between Light Curve Modeling of Type II Supernovae and Neutrino-Driven Core-Collapse Supernovae Models with Late-Phase Spectroscopy
• Millisecond Pulsar Discoveries in an Image-based MeerKAT Survey of the Galactic Bulge
• Fitting the Shadows: Star Formation Scaling Relations in the Low Surface Brightness Regime
• On the formation of star-forming galaxies having anomalously low-metallicity regions: the role of galaxy interaction and CGM/IGM accretion
• Constraints on the Orbit of the Young Substellar Companion GQ Lup B from High-Resolution Spectroscopy and VLTI/GRAVITY Astrometry
• Discovery of Two Highly Scattered Pulsars from Image-Based Circular Polarization Searches with the Australian SKA Pathfinder
• NEXUS: A Search for Nuclear Variability with the First Two JWST NIRCam Epochs
• A High-Precision, Differentiable Code for Solar System Ephemerides
• Neptune’s inner moons and rings are exposed icy body interiors
• JWST Spectra Indicate a Large Mass of Postshock Dust Formed by SN 2010jl
• Orbital and Atmospheric Modeling of H <scp>ii</scp> 1348B: An Eccentric Young Substellar Companion in the Pleiades
• Refined rotational state and shape model of (98943) Torifune ahead of the Hayabusa2# flyby
• THOR and HAMRR
• Seasonal Changes in the Atmosphere of HD 80606 b Observed with JWST’s NIRSpec/G395H
• Quantifying the Contamination of TESS Ecliptic-Plane Light Curves by Minor Planets
• The impact of glitches on young pulsar rotational evolution
• Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys
• The Discovery of an Active Wind from the Milky Way’s Central Black Hole
• A Study of HH 270 with the James Webb Space Telescope
• Spectroscopic Confirmation of a Large and Luminous Galaxy with Weak Emission Lines at <i>z</i> = 13.53
• Traces of Helium Detected in Type Ic Supernova 2014L
• UGC 2369S: A Kiloparsec-scale Triple Merger Candidate Identified in a Nearby Luminous Infrared Galaxy
• Excavating the Ruins: An Ancient <i>z</i> = 2.675 Galaxy Which Formed in the First 500 Myr
• ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791
• Hidden in Plain Sight: Searching for Globular Clusters within JWST Observations of the PLCK G165.7+67.0 Galaxy Cluster
• Evidence for a Delayed Ultraviolet Counterpart to X-Ray Quasiperiodic Eruptions in Ansky
• Can the Dust Eclipses in WR 104 Provide Constraints on the System’s Inclination?
• HD 164604 c: A Second Giant Planet on a 15 Yr Orbit and Constraints on the Planet–Planet Mutual Inclination*
• Exomoons and Exorings with the Habitable Worlds Observatory. II. Finding “Endor” with Lunar Eclipses
• A Protoplanet Candidate in the PDS 66 Disk Indicated by Silicon Sulfide Isotopologues
• MINDS. Anatomy of a Water-rich, Inclined, Brown Dwarf Disk: Lack of Abundant Hydrocarbons
• Intertwined Birth and Death: A Herbig–Haro Outflow Resolves the Distance to Vela Junior
• Planetary Habitability Under the Light of a Rapidly Changing Star
• A Characterization of JWST MIRI Detector Persistence and Implications for High-contrast Imaging
• Searching for Extragalactic Exoplanets: A Survey of the Sagittarius Dwarf Galaxy Stream with TESS
• Earliest Galaxy Evolution in the CANUCS+Technicolor fields: Galaxy Properties at z∼10-16 seen with the Full NIRCam Medium and Broad Band Filters
• The Death of Vulcan: NEID Reveals That the Planet Candidate Orbiting HD 26965 Is Stellar Activity*
• Precise Constraints on the Energy Budget of WASP-121 b from its JWST NIRISS/SOSS Phase Curve
• Searching for GEMS: TOI-5349b is a Saturn-like planet orbiting a metal-rich early M-dwarf
• The Platonic Universe: Do Foundation Models See the Same Sky?
• TOI-2155b: a high-mass brown dwarf near the hydrogen burning mass limit from the TESS mission
• Recalibration of the Hα surface brightness-radius relation for planetary nebulae using Gaia DR3: new distances and the Milky Way oxygen radial gradient
• The Timescales of Embedded Star Formation as Observed in STARFORGE
• CECILIA: Gas-Phase Physical Conditions and Multi-Element Chemistry at Cosmic Noon
• A Decade of Transit-Timing Measurements Confirm Resonance in the K2-19 System
• The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30-day Orbit and a More Massive Outer World
• Simulating Image Coaddition with the Nancy Grace Roman Space Telescope. IV. Hyperparameter Optimization and Experimental Features
• The JWST EXCELS survey: Insights into the nature of quenching at cosmic noon
• Multi-spacecraft Measurements of the Evolving Geometry of the Solar Alfvén Surface Over Half a Solar Cycle
• Europa’s H₂O₂: Temperature Insensitivity and a Correlation with CO₂
• Population-Dependent r-process Scatter in the Globular Cluster M15
• Atomic and molecular gas in the Milky Way. I. Structure decomposition
• Overdispersed radio source counts and excess radio dipole detection
• A New Way to Discover Strong Gravitational Lenses: Pair-wise Spectroscopic Search from DESI DR1
• ExoIris: fast exoplanet transmission spectroscopy in Python
• Absence of Radio Emission Reveals an Exceptionally Weak Explosion of the Putative Historical Supernova Pa 30
• Hubble Space Telescope Imaging of Three Isolated Faint Dwarf Galaxies Beyond the Local Group: Pavo, Corvus A, and Kamino
• DingshanDeng/DiskMINT: DiskMINT v1.7.0 Release
• FindPOTATOs: Minor Planet Observation Linking Software
• Modeling the JWST MIRI Counts, Insights Into the Source Properties and Role of Dust-Obscured AGN
• Dynamical Analysis of the HD 169142 Planet-Forming Disk: Twelve Years of High-Contrast Polarimetry
• The Importance of Standardizing Spectra in the Era of Large Spectroscopic Surveys: A Case Study of M Dwarfs in SDSS-V
• Kinematics of Stellar Streams from Globular Clusters Depend on Black Hole Retention and Star Mass: A Selection Effect for Dark Matter Inference
• Measuring the Two-Dimensional Thermal Structures of Protoplanetary Disks
• Constraining Cosmology with Double-source-plane Strong Gravitational Lenses from the AGEL Survey
• Tidal Disruption of Super Star Clusters as the origin of Bluish Light at the inner region of the Perseus Cluster Central Galaxy
• Dichotomy in Long-Lived Radio Emission from Tidal Disruption Events AT 2020zso and AT 2021sdu: Multi-Component Outflows vs. Host Contamination
• Possible Evidence for the Presence of Volatiles on the Warm Super-Earth TOI-270 b
• A simple, flexible method for timing cross-calibration of space missions
• DESI DR1 Lyα 1D power spectrum: Validation of estimators
• SuNeRF-CME: Physics-Informed Neural Radiance Fields for Tomographic Reconstruction of Coronal Mass Ejections
• Vanishing Refractories: Tracing Dust Evolution in the BP Tau Protoplanetary Disk
• Characterizing the Time Variability of 2M1207 A+b with JWST NIRSpec/PRISM
• Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts
• JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b
• The impact of Alfvenic shear flow on magnetic reconnection and turbulence
• TESS Subgiant and Lower Red Giant Asteroseismology in the Continuous Viewing Zones
• SN 2024aecx: a fast-evolving Type IIb supernova with a prominent shock-cooling peak
• DELVE Milky Way Satellite Census I: Satellite Population and Survey Selection Function
• Characterization of Two Cool Galaxy Outflow Candidates Using Mid-Infrared Emission from Polycyclic Aromatic Hydrocarbons
• JWST/NIRSpec Observations of Salacia-Actaea and Máni: Exploring Population-level Trends among Water-ice-rich Kuiper Belt Objects
• JWST's first view of the most vigorously star-forming cloud in the Galactic center -- Sagittarius B2
• Molecular Jets from an Evolved Protostar: Insights from JWST-ALMA Synergy
• A Candidate Dual QSO at Cosmic Noon
• The Polar Orbit of TOI-2374 b, a Planet in the Neptunian Ridge
• Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1^*
• The Orbits of Isolated Dwarfs in the Local Group from New 3D Kinematics: Constraints on First Infall, Backsplash, and Quenching Mechanisms
• Hydrocarbon Hazes on Temperate sub-Neptune K2-18b supported by data from the James Webb Space Telescope
• Evidence of Galactic Center Expansion from Gaia DR3 Stars along the South North Axis: Implications for the JWST Early Galaxy Problem
• The CHARA Array Polarization Model and Prospects for Spectropolarimetry
• Scaling K2. VII. Evidence For a High Occurrence Rate of Hot Sub-Neptunes at Intermediate Ages
• Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation
• Spatially Offset Active Galactic Nuclei in the Very Large Array Sky Survey: Tracers of Galaxy Mergers and Wandering Massive Black Holes
• Detection of a Deeply Embedded Protocluster Candidate in NGC 602 with JWST
• Exploring the History of Stellar Mergers with Chemistry: Examining the Origins of Massive α-Enriched Stars using Carbon Isotope Ratios
• Ground-Based Mid-IR Direct Imaging: The Origin of the Thermal Background on the Keck II Telescope and Correcting Instrumental Systematics
• Searching for GEMS: The Occurrence of Giant Planets orbiting M-dwarfs within 100 pc
• Quaia, the Gaia-unWISE Quasar Catalog: An All-sky Spectroscopic Quasar Sample
• Black Hole Spectroscopy and Tests of General Relativity with GW250114
• High-Pass Filtering and Gaussian Process Regularization: Stellar Activity Characterization Techniques Applied to the 55 Cancri Planetary System
• Early warning for lensed gravitational wave counterparts from time delays of their host galaxies observed in the optical
• Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
• A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666
• 3I/ATLAS: In Search of the Witnesses to Its Voyage
• spherical: A Comprehensive Database and Automated Pipeline for VLT/SPHERE High-Contrast Imaging
• The redshift distribution of Einstein Probe transients supports their relation to gamma-ray bursts
• Constraining Baryon Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger
• What's the Buzz About GX 13+1? Constraining Coronal Geometry with QUEEN-BEE: A Bayesian Nested Sampling Framework for X-ray Polarization Rotation Analysis
• The Lyα and Continuum Origins Survey. III. Investigating the link between galaxy morphology, merger properties and LyC escape
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen
• Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b
• Direct Detection of Known Exoplanets in Reflected Light: Predicting Sky Position with Literature Orbit Solutions
• Revealing the Two `Horns' of Taurus with GAIA DR2
• Simulations of Flare Chemistry in Brown Dwarf Companions to Active M Dwarfs
• The first radio view of a type Ibn supernova in SN 2023fyq: Understanding the mass-loss history in the last decade before the explosion
• Optical Spectroscopy Reveals Hidden Neutron-capture Elemental Abundance Differences among APOGEE-identified Chemical Doppelgängers
• On the origin of super-global spin-up trends of X-ray pulsars in HMXB systems
• Enhancements in velocity-dependent dark matter annihilation in Galactic subhalos
• The Open mulTiwavelength Transient Event Repository (OTTER): Infrastructure Release and Tidal Disruption Event Catalog
• X-ray investigation of possible super-Eddington accretion in a radio-loud quasar at z=6.13
• Generation of Lognormal Synthetic Lyman-α Forest Spectra for P_1D Analysis
• Resolving Emission from Small Dust Grains in the Blue Compact Dwarf II Zw 40 with JWST
• The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars
• New Interpretation for the Orientation of the LMC's Gaseous Arms B and E using ULLYSES
• SN 2019hnl: A Type IIP Supernova with a Partially Stripped, Low Mass Progenitor
• Breaking Down the \textsfCosmoGEMS: Toward Modeling and Understanding Globular Cluster Stellar Streams in a Fully Cosmological Context
• Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey. III. Detectability of Giant Exomoons of Wide Separation Giant Planets
• VLA FRAMEx. III. Circumnuclear Radio Emission Mechanisms in Hard X-ray Selected Active Galactic Nuclei
• Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations
• Extended and Compact Ortho-H₂D⁺ Structures Close to the Moment of Star-Formation: Evidence from ALMA-ACA Observations in Taurus
• Double White Dwarf Binaries in SDSS-V DR19 : A catalog of DA white dwarf binaries and constraints on the binary population
• Synchronous Rotation in the (120347) Salacia-Actaea System
• Investigations of MWISP Clumps: 13CO Clump Source Catalog and Physical Properties
• Radiative Transfer Modeling of a Shadowed Protoplanetary Disk assisted by a Neural Network
• GRB 250704B: An Off-axis Short GRB with a Long-Lived Afterglow Plateau
• The Interstellar Medium in I Zw 18 seen with JWST/MIRI: II. Warm Molecular Hydrogen and Warm Dust
• Onset of CN Emission in 3I/ATLAS: Evidence for Strong Carbon-Chain Depletion
• Unveiling Stellar Feedback and Cloud Structure in the ρ Ophiuchi A Region with ALMA and JWST: Discovery of Substellar Cores, C¹⁸O Striations, and Protostellar Outflows
• The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-rays and Radio
• The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the Ultraviolet to the Near-Infrared
• Terrestrial Exoplanet Internal Structure Constraints Enabled by Comprehensive Host Star Characterization Reveal that Terrestrial Planets in Mean-motion Resonances are Water Rich
• HostSubGP: Precise Galaxy Background Subtraction in Transient Spectroscopy with Gaussian Processes
• SQuIGGLE: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, z∼0.7 post-starburst galaxies
• Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
• Cosmo-Learn: code for learning cosmology using different methods and mock data
• Glimmers in the Cosmic Dawn. III. On the Photometrically Determined Black Hole Mass to Stellar Mass Relation Across Cosmic Time
• Massive extended streamers feed high-mass young stars
• How does feedback affect the star formation histories of galaxies?
• Stringent Upper Bounds on Atmospheric Mass Loss from Three Neptune-Sized Planets in the TOI-4010 System
• The BlueDOG at Cosmic Noon: A Possible Analog to Little Red Dots?
• Asteroseismology of Carbon-Deficient Red Giants: Merger Products of Hierarchical Triple Systems?
• Exploring the Relationship Between Swift Short Gamma-Ray Burst Afterglows and their Host Galaxy Properties
• Wide Separation Planets In Time (WISPIT): Discovery of a Gap Hα Protoplanet WISPIT 2b with MagAO-X
• WIde Separation Planets In Time (WISPIT): A Gap-clearing Planet in a Multi-ringed Disk around the Young Solar-type Star WISPIT 2
• STCTM: a forward modeling and retrieval framework for stellar contamination and stellar spectra
• The Missing Hard Photons of Little Red Dots: Their Incident Ionizing Spectra Resemble Massive Stars
• In Search of Decay: An Analysis of Transit Times of Hot Jupiters in Main Sequence and Post-Main Sequence Systems
• Transiting Planetary Debris near the Roche Limit of a White Dwarf on a 4.97 hr Orbit -- and its Vanishing
• VLT/MUSE Detection of the AB Aurigae b Protoplanet with H _{\rm α} Spectroscopy
• Inferring Mbh-Mbulge Evolution from the Gravitational Wave Background
• TrES-1 b: A Case Study in Detecting Secular Evolution of Exoplanet Orbits
• The Fraction of Clumpy Galaxies in JWST Surveys over 2
• A Spectroscopic Hunt for Post-Red Supergiants in the Large Magellanic Cloud II: Turbulent Line Broadening in the Spectra of LMC Yellow Supergiants
• Spatially Resolved [O III] Emission Line Kinematics of Reverberation-Mapped AGNs with the Keck Cosmic Web Imager
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• A Near-Infrared Spectral Library of Very Young Brown Dwarfs and Planetary-Mass Objects in the Orion Nebula Cluster
• Searching for continuous gravitational waves in the Parkes Pulsar Timing Array Data Release 3
• A Catalog of M&amp;M Eclipsing Binaries with TESS
• Prospects for the formation of GW231123 from the AGN channel
• Real-time prediction of two geomagnetic storms using Solar Orbiter as a far upstream solar wind monitor
• Development of Turbulence in Post-shock Regions
• The New Status Qvo? SN 2021qvo is Another 2003fg-like Type Ia Supernova with a Rising Light-Curve Bump
• MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
• Aligned Stellar Obliquities for Two Hot Jupiter-hosting M Dwarfs Revealed by MAROON-X: Implications for Hot Jupiter Formation
• Spatially and Dynamically Extended Molecular Gas in Stephan's Quintet Revealed by ALMA CO(1-0) Total Power Mapping
• Mass Loss and Subsequent Thermal Evolution of Surviving Helium White Dwarfs Shocked by Thermonuclear Supernovae
• Cosmology-informed Neural Networks to infer dark energy equation-of-state
• Late-time Hubble Space Telescope Ultraviolet Spectra of SN 2023ixf and SN 2024ggi Show Ongoing Interaction with Circumstellar Material
• The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance
• SN 2021aaev: a Hydrogen-Rich Superluminous Supernova with Early Flash and Long-Lived Circumstellar Interaction in an Unusual Host Environment
• Discovery of Hα Emission from a Protoplanet Candidate Around the Young Star 2MASS J16120668-3010270 with MagAO-X
• First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b
• Pulsations change the structures of massive stars before they explode: interpreting the nearby supernova SN 2023ixf
• An Ultraviolet Study of CO Chemistry in the Magellanic Clouds
• The Type II SN 2025pht in NGC 1637: A Red Supergiant with Carbon-rich Circumstellar Dust as the First JWST Detection of a Supernova Progenitor Star
• The Dark Energy Bedrock All-Sky Supernova Program: Cross Calibration, Simulations, and Cosmology Forecasts
• Cosmic cascades: How disk substructure regulates the flow of water to inner planetary systems
• The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey -- III. A census of millisecond pulsars at 154 MHz
• Optimizing Convolution Direction and Template Selection for Difference Image Analysis
• Strong NUV Refractory Absorption and Dissociated Water in the Hubble Transmission Spectrum of the Ultra Hot Jupiter KELT-20 b
• The watery atmosphere of HD~209458~b revealed by joint K- and L-band high-resolution spectroscopy
• Classifying Cool Dwarfs: Comprehensive Spectral Typing of Field and Peculiar Dwarfs Using Machine Learning
• The Interstellar Medium in IZw18 seen with JWST/MIRI: I. Highly Ionized Gas
• Leonessa: An Extremely Metal-poor Galaxy Undergoing Secular Chemical Evolution
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from \mathbf2
• On the Origin of Neutron-capture Elements in r-I and r-II Stars: A Differential-abundance Analysis
• Orbits and Masses for 156 Companions from Combined Astrometry and Radial Velocities, and A Validation of Gaia Non-Single Star Solutions
• White dwarfs in wide binaries: the strong effects of stellar evolution and mass loss
• MAGAZ3NE: Far-IR and Radio Insights into the Nature and Properties of Ultramassive Galaxies at z\gtrsim3
• SKYSURF VIII -- Modeling SKYSURF Completeness Data for Comparison to the Hubble Space Telescope Exposure Time Calculator
• The Impact of External Radiation on the Inner Disk Chemistry of Planet Formation
• Enhanced Pebble Drift across Planet-opened Gaps in Windy Protoplanetary Disks
• Smart Source Detection Framework for Lobster Eye Telescopes
• LAMOST Medium-resolution Spectroscopic Survey of the Rosette Nebula
• Characterizing Temperatures of Flares on the M Dwarf Wolf 359 from Simultaneous Multiband Optical Observations
• JWST Spectroscopy of a Blue Binary Cold Classical Kuiper Belt Object
• Stellar CoRGI in MaNGA: Stellar Counterrotating Galaxies Identified in the MaNGA Survey
• Spectral Characteristics of Interstellar Object 3I/ATLAS from SOAR Observations
• Revisiting the Gas Dynamics of Henize 2-10: Possible Drivers of the Starburst
• A Deep VLA Search for a Persistent Radio Counterpart to the One-off FRB 20250316A
• Combined tracer analysis for DESI 2024 BAO
• Hubble constant constraint using 117 FRBs with a more accurate probability density function for \rm DM_{\rm diff}
• Resolution-Corrected White Dwarf Gravitational Redshifts Validate SDSS-V Wavelength Calibration and Enable Accurate Mass-Radius Tests
• A second-generation star in a relic dwarf galaxy
• A Systematic Search for Main-Sequence Dipper Stars Using the Zwicky Transient Facility
• Utilizing Maximum Variability to Discern TDE Emission from AGN Flares
• Globular Clusters in the Galaxy Cluster MACS0416 at z = 0.397
• Profiling Dark Matter Spikes with Gravitational Waves from Accelerated Binaries
• Prospects of a New L₅ Trojan Flyby Target for the Lucy Mission
• JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum
• A New Approach to Compiling Exoatmospheric Target Lists And Quantifying the Ground-Based Resources Needed to Vet Them
• The Diversity of Metal-Enrichment and Abundance Patterns at High Redshift: A Magellan Survey of Gas-rich Galaxies Traced by Damped Lyman-alpha Absorbers at z~5
• The X-ray Variability and Luminosity Function of High Mass X-ray Binaries in the Dwarf Starburst Galaxy IC 10
• Testing Dark Matter with Generative Models for Extragalactic Stellar Streams
• A shock flash breaking out of a dusty red supergiant
• Pre-discovery TESS Observations of Interstellar Object 3I/ATLAS
• Using Faded Changing-Look Quasars to Unveil the Spectral Energy Distribution Evolution of Low-Luminosity Active Galactic Nuclei
• SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis
• A Nitrogen-rich AGN Powering a Large Ionizing Bubble at z=8.63
• Estimate of Current Mass of the Large Magellanic Cloud from the Orphan-Chenab Tidal Stream
• Mapping the Distant and Metal-Poor Milky Way with SDSS-V
• A Novel Formation Channel for Supermassive Black Hole Binaries in the Early Universe via Primordial Black Holes
• A 50 s quasi-periodic oscillation in the early X-ray afterglow of GRB 220711B
• Challenges to the Two-Infall Scenario by Large Stellar Age Catalogs
• Star formation histories and gas content limits of three ultra-faint dwarfs on the periphery of M31
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• A Melody in the Noise: Modeling Echoes of the Crab Nebula
• Echoes in Different Tempo: Long-Term Monitoring of Crab Echoes with CHIME
• A MaNGA about the Legacy I: Connecting the Assembly of Stellar Halo with the Average Star Formation History in Low-Redshift Massive Galaxies
• The Impact of Foregrounds on Dark Ages Measurements with the Highly Redshifted 21 cm Line
• Enabling Early Transient Discovery in LSST via Difference Imaging with DECam
• Radio Variability in Recently-Quenched Galaxies: The Impact of TDE or AGN Driven Outflows
• When the Wall Fell: Study of Polycyclic Aromatic Hydrocarbons in T Chamaeleontis using JWST
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Quenching Through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of z ~ 0.7 Post-Starburst Galaxies
• Radio Emission from a Nearby M dwarf Binary
• Thick Disks around White Dwarfs viewed 'Edge-off': Effects on Transit Properties and Infrared Excess
• A Classification Scheme for X-ray Bright Type Ia Supernova Remnants Based on Their Circumstellar Interaction
• A New Inner Heliosphere Proton Parameter Dataset from the Helios Mission. [europepmc]
• Social networks predict the life and death of honey bees. [europepmc]
• A modular platform for automated cryo-FIB workflows. [europepmc]
• Single Vesicle Fluorescence-Bleaching Assay for Multi-Parameter Analysis of Proteoliposomes by Total Internal Reflection Fluorescence Microscopy. [europepmc]
• Towards super-resolved terahertz microscopy for cellular imaging. [europepmc]
• Identification of carbon dioxide in an exoplanet atmosphere. [europepmc]
• Quantum wake dynamics in Heisenberg antiferromagnetic chains. [europepmc]
• Trait mindful awareness predicts inter-brain coupling but not individual brain responses during naturalistic face-to-face interactions. [europepmc]
• ReCSAI: recursive compressed sensing artificial intelligence for confocal lifetime localization microscopy. [europepmc]
• Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM. [europepmc]
• Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H. [europepmc]
• Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. [europepmc]
• Spatial consistency of cell growth direction during organ morphogenesis requires CELLULOSE SYNTHASE INTERACTIVE1. [europepmc]
• Carbonaceous dust grains seen in the first billion years of cosmic time. [europepmc]
• Outflows from the youngest stars are mostly molecular. [europepmc]
• Qudi-HiM: an open-source acquisition software package for highly multiplexed sequential and combinatorial optical imaging. [europepmc]
• The photometric variability of massive stars due to gravity waves excited by core convection. [europepmc]
• Retrospective Motion Artifact Reduction by Spatial Scaling of Liver Diffusion-Weighted Images. [europepmc]
• Sulfur dioxide in the mid-infrared transmission spectrum of WASP-39b. [europepmc]
• Spectroscopic confirmation of two luminous galaxies at a redshift of 14. [europepmc]
• Strong Lensing by Galaxies. [europepmc]
• Nitric oxide modulates contrast suppression in a subset of mouse retinal ganglion cells. [europepmc]
• Photometric detection at 7.7 μm of a galaxy beyond redshift 14 with JWST/MIRI. [europepmc]
• A complex structure of escaping helium spanning more than half the orbit of the ultra-hot Jupiter WASP-121 b. [europepmc]
• Little red dots as young supermassive black holes in dense ionized cocoons. [europepmc]

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