Array programming with NumPy

2020/09/16 by Charles R. Harris, K. Jarrod Millman, Stéfan J. van der Walt +23 · 1231 citations
Computer Science · Decision Sciences · Materials Science · #Computational Physics and Python Applications #Machine Learning in Materials Science #Scientific Computing and Data Management

paper · pdf · doi:10.1038/s41586-020-2649-2

openalex created_date 2020/06/25 · openalex publication_date 2020/09/16 · openalex updated_date 2026/07/30

Abstract

Abstract Array programming provides a powerful, compact and expressive syntax for accessing, manipulating and operating on data in vectors, matrices and higher-dimensional arrays. NumPy is the primary array programming library for the Python language. It has an essential role in research analysis pipelines in fields as diverse as physics, chemistry, astronomy, geoscience, biology, psychology, materials science, engineering, finance and economics. For example, in astronomy, NumPy was an important part of the software stack used in the discovery of gravitational waves 1 and in the first imaging of a black hole 2 . Here we review how a few fundamental array concepts lead to a simple and powerful programming paradigm for organizing, exploring and analysing scientific data. NumPy is the foundation upon which the scientific Python ecosystem is constructed. It is so pervasive that several projects, targeting audiences with specialized needs, have developed their own NumPy-like interfaces and array objects. Owing to its central position in the ecosystem, NumPy increasingly acts as an interoperability layer between such array computation libraries and, together with its application programming interface (API), provides a flexible framework to support the next decade of scientific and industrial analysis.

Citations

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• CAJAL enables analysis and integration of single-cell morphological data using metric geometry
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• Deep Learning for Fluorescence Lifetime Predictions Enables High-Throughput In Vivo Imaging
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• Machine Learning Applications in Use-Wear Analysis: A Critical Review
• Divergent genomic trajectories predate the origin of animals and fungi
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• Galaxy as a gateway to bioinformatics: Multi-Interface Galaxy Hands-on Training Suite (MIGHTS) for scRNA-seq
• Grammar-constrained decoding for structured information extraction with fine-tuned generative models applied to clinical trial abstracts
• NeuroVar: an open-source tool for the visualization of gene expression and variation data for biomarkers of neurological diseases
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• 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
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• QCManyBody: A flexible implementation of the many-body expansion
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• VAMPyR—A high-level Python library for mathematical operations in a multiwavelet representation
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• Matrix decompositions in quantum optics: Takagi/Autonne, Bloch–Messiah/Euler, Iwasawa, and Williamson
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• MixtureMetrics: A comprehensive package to develop additive numerical features to describe complex materials for machine learning modeling
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• A Python Interface for Numerical Relativity Program AMSS-NCKU
• Talking Trees: Reasoning-Assisted Induction of Decision Trees for Tabular Data
• Efficient Digital Methods to Quantify Sensor Output Uncertainty
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• A New Precise Measurement of the Cosmic Microwave Background Radiation Temperature at z=0.89 Toward PKS1830-211
• Reconciling the Tension Between Light Curve Modeling of Type II Supernovae and Neutrino-Driven Core-Collapse Supernovae Models with Late-Phase Spectroscopy
• Guiding Application Users via Estimation of Computational Resources for Massively Parallel Chemistry Computations
• Exciting Stellar Eccentricity in Gaia BH3 via a Hidden Black Hole Binary
• d2: Improving Reasoning in Diffusion Language Models via Trajectory Likelihood Estimation
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• Examining the robustness of Physics-Informed Neural Networks to noise for Inverse Problems
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• The tangled warp of the Milky Way
• Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content
• Adaptive Approach to Enhance Machine Learning Scheduling Algorithms During Runtime Using Reinforcement Learning in Metascheduling Applications
• The periodicity of three-dimensional oscillatory reconnection
• NEXUS: A Search for Nuclear Variability with the First Two JWST NIRCam Epochs
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• Policy Gradient Steering: Interventions from Behavioral Objectives
• CDAE: Enhancing Perturbation Robustness in Pretrained Language Models with Contrastive Denoising
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• It's All Just Vectorization: einx, a Universal Notation for Tensor Operations
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• DrLungker: A Deep Ensemble Learning Framework for Predicting Anti‐Lung Cancer Compound Activity and Validating Multitarget Potency through WaterMap, DFT, MD Simulations, and MM‐GBSA Analysis
• A dark-matter-sensitive orientation clock near rotating black holes
• THOR and HAMRR
• Cryopreservation and post-thaw differentiation of monocytes enabled by macromolecular cryoprotectants which restrict intracellular ice formation
• Sensitive detection of structural dynamics using a statistical framework for comparative crystallography
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• Menger_Curvature : a MDAKit implementation to decipher the dynamics, curvatures and flexibilities of polymeric backbones at the residue level
• Application of MobileNet and Xception neural networks to identify Sillago sihama populations in Vietnam's coastal waters based on otolith morphology
• Reproducible Brain Charts: An open data resource for mapping brain development and its associations with mental health
• Regulation Ratio: A Singular Multi-Omic Measurement of Gene Regulatory Mechanisms
• Characterizing developmental changes in infant habituation using functional change point detection
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• Flower Visitation through the Lens: Exploring the Foraging Behaviour of Bombus terrestris with a Computer Vision-Based Application
• Fantastic stewards and where to find them: a descriptive study of the heterogeneous disparity in physician–pharmacist–nurse distribution among the infectious disease workforce
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• Turing instabilities in two-layer networks
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• Multimodal integration using a machine learning approach facilitates risk stratification in HR+/HER2− breast cancer
• Unlocking the specificity of antimicrobial peptide interactions for membrane-targeted therapies
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• Leveraging large language models for accurate classification of liver lesions from MRI reports
• An evaluation of rectum contours generated by artificial intelligence automatic contouring software using geometry, dosimetry and predicted toxicity
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• Enhancing decision-making and patient comprehension in complex rectal cancer surgery through personalized three-dimensional imaging: randomized feasibility study
• DoliClock: a lipid-based aging clock reveals accelerated aging in neurological disorders
• Impact of drugs and environmental contaminants on amine production by gut bacteria
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• Accounting for contact tracing in epidemiological birth-death models
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• Distinct genomic contexts predict gene presence–absence variation in different pathotypes of Magnaporthe oryzae
• Defining the limits of plant chemical space: challenges and estimations
• Predicting biomolecule adsorption on nanomaterials: a hybrid framework of molecular simulations and machine learning
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• Spatial structure could explain the maintenance of alternative reproductive tactics in tree cricket males
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• Functional Hierarchy of the Human Neocortex from Cradle to Grave
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• Neural networks reveal emergent properties of collective learning in democratic but not despotic groups
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• The binding of the salvianolic acid A to the citrullinating enzyme PADI4 as a potential treatment for cancer
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• D-LIM: A neural network for interpretable gene–gene interactions
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• Col-OSSOS: Investigating the Origins of Different Surfaces in the Primordial Kuiper Belt
• Reduction of Residence Time of Air in the Arctic Since the 1980s
• A Late-time Radio Survey of Type Ia-CSM Supernovae with the Very Large Array
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• Precise Constraints on the Energy Budget of WASP-121 b from its JWST NIRISS/SOSS Phase Curve
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• The JWST EXCELS survey: Insights into the nature of quenching at cosmic noon
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• Deep Learning the Functional Renormalization Group
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• DESI DR1 Lyα 1D power spectrum: Validation of estimators
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• From virtual Z gates to virtual Z pulses
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• Hybrid Active-Passive Galactic Cosmic Ray Simulator: in-silico design and optimization
• JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b
• Multivariate Low-Rank State-Space Model with SPDE Approach for High-Dimensional Data
• The impact of Alfvenic shear flow on magnetic reconnection and turbulence
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• TESS Subgiant and Lower Red Giant Asteroseismology in the Continuous Viewing Zones
• DELVE Milky Way Satellite Census I: Satellite Population and Survey Selection Function
• WIYN Open Cluster Study. XCVII. An Extended Radial-Velocity Survey and Spectroscopic Binary Orbits in the Open Cluster NGC 188
• JWST/NIRSpec Observations of Salacia-Actaea and Máni: Exploring Population-level Trends among Water-ice-rich Kuiper Belt Objects
• Tidy simulation: Designing robust, reproducible, and scalable Monte Carlo simulations
• Towards estimating the number of strains that make up a natural bacterial population
• A Meshing Framework for Digital Twins for Extrusion based Additive Manufacturing
• Enabling stable preservation of ML algorithms in high-energy physics with petrifyML
• The Polar Orbit of TOI-2374 b, a Planet in the Neptunian Ridge
• The Orbits of Isolated Dwarfs in the Local Group from New 3D Kinematics: Constraints on First Infall, Backsplash, and Quenching Mechanisms
• Maximum diversity and weighting for invariants of periodic time series
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• Probing small-scale dark matter clumping with the large-scale 21-cm power spectrum
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• CityAQVis: Integrated ML-Visualization Sandbox Tool for Pollutant Estimation in Urban Regions Using Multi-Source Data (Software Article)
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• gmx_MMPBSA: A New Tool to Perform End-State Free Energy Calculations with GROMACS
• LEO-Vetter: Fully Automated Flux- and Pixel-Level Vetting of TESS Planet Candidates to Support Occurrence Rates
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• Spatial transcriptomics reveals expression gradients in developing wheat inflorescences at cellular resolution
• Unraveling the emission mechanism powering long period radio transients from interacting white dwarf binaries via kinetic plasma simulations
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• Supernovae drive large-scale, incompressible turbulence through small-scale instabilities
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• Probing the Cosmological Principle with CMB lensing and cosmic shear
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• Why Cosmic Voids Matter: Pristine Evolution
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• The Lyα and Continuum Origins Survey. III. Investigating the link between galaxy morphology, merger properties and LyC escape
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• H-alpha as a Tracer of Star Formation in the SPHINX Cosmological Simulations
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• Shape spectra of elastic shells with surface-adsorbed semiflexible polymers
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• Madness, Cannibalism, and Traditional Fiction between Lu Xun and Mo Yan
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• Resolving Emission from Small Dust Grains in the Blue Compact Dwarf II Zw 40 with JWST
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way–mass Galaxies
• High Resolution ALMA Data of the Fomalhaut Debris Disk Confirms Apsidal Width Variation
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• treeX: Unsupervised Tree Instance Segmentation in Dense Forest Point Clouds
• Breaking Down the \textsfCosmoGEMS: Toward Modeling and Understanding Globular Cluster Stellar Streams in a Fully Cosmological Context
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• Crowning the Queen: Membership, Age, Rotation, and Activity for the Open Cluster Coma Berenices
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• Cellpose: a generalist algorithm for cellular segmentation
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• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
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• Exoplanet Atmospheric Refraction Effects in the Kepler Sample
• Uniform Reanalysis of JWST MIRI 15μm Exoplanet Eclipse Observations using Frame-Normalized Principal Component Analysis
• Analyzing Common Electronic Structure Theory Algorithms for Distributed Quantum Computing
• The Rapid ASKAP Continuum Survey IV: continuum imaging at 1367.5 MHz and the first data release of RACS-mid
• Catalytic Quantum Error Correction: Theory, Efficient Catalyst Preparation, and Numerical Benchmarks
• An Algorithm for Automated Extraction of Resonance Parameters from the Stabilization Method
• Parsimonious Gaussian mixture models with piecewise-constant eigenvalue profiles
• More sophisticated is not always better: comparison of similarity measures for unsupervised learning of pathways in biomolecular simulations
• NOCTIS: Novel Object Cyclic Threshold based Instance Segmentation
• The TESS Grand Unified Hot Jupiter Survey. III. Thirty More Giant Planets
• Investigating the physical properties of dusty star-forming galaxies at z>=1.5 in the GOODS-South field using JWST
• Soliton Synchronization with Randomness: Rogue Waves and Universality
• Evaluation of acoustic Green's function in rectangular rooms with general surface impedance walls
• The BoRG-JWST Survey: Analogs at z∼8 to the UV-luminous Galaxy Population at z\gtrsim10
• SPARSE: Scattering Poles and Amplitudes from Radial Schrödinger Equations
• Extreme Forward Scattering Observed in Disk-Averaged Near-Infrared Phase Curves of Titan
• A hyperboloidal method for numerical simulations of multidimensional nonlinear wave equations: nonlinear tails
• Heavy element nucleosynthesis in rotating proto-magnetar winds
• Characterization of the Cherenkov Photon Background for Low-Noise Silicon Detectors in Space
• Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results
• Mid-Infrared Dust Evolution and Late-time Circumstellar Medium Interaction in SN 2017eaw
• Functional Renormalization for Signal Detection: Dimensional Analysis and Dimensional Phase Transition for Nearly Continuous Spectra Effective Field Theory
• Sparse grids vs. random points for high-dimensional polynomial approximation
• A Structured Proximal Stochastic Variance Reduced Zeroth-order Algorithm
• The NEID Earth Twin Survey. III. Survey Performance After Three Years on Sky
• Black Hole Supernovae, Their Equation of State Dependence, and Ejecta Composition
• High-definition imaging of a filamentary connection between a close quasar pair at z=3
• Jet stream poleward migration leads to marine primary production decrease
• Improved Particle Spray Algorithm for Modeling Globular Cluster Streams
• Unified reconstruction of the Lyman-alpha power spectrum with Hamiltonian Monte Carlo
• Magnetic Diagnostics of Prominence Eruptions through the Hanle Effect of the He i 1083 nm Line
• DSSP 4: FAIR annotation of protein secondary structure
• Rust vs. C for Python Libraries: Evaluating Rust-Compatible Bindings Toolchains
• Bridging taxonomic gaps in microbial community profiling with LSTM-generated synthetic full-length 16S rRNA sequences
• Variability-finding in Rubin Data Preview 1 with LSDB
• Anchoring Stellar Age Indicators: A Cross-Calibration of [C/N] and Gyrochronology Ages via the Age-Velocity-Dispersion Relation
• Impostor Among νs: Dark Radiation Masquerading as Self-Interacting Neutrinos
• Neutrino masses, matter-antimatter asymmetry, dark matter, and supermassive black hole formation explained with Majorons
• Attribution assignment for deep-generative sequence models enables interpretability analysis using positive-only data
• Mathematical Computation on High-dimensional Data via Array Programming and Parallel Acceleration
• Probing foreground residuals in cleaned CMB temperature maps from Planck
• QTurbo: A Robust and Efficient Compiler for Analog Quantum Simulation
• Double Compact Binary Merger Rate Density in Open Star Clusters: Black Holes, Neutron Stars, and White Dwarfs
• Surface curvature and secondary vortices in steady dense shallow granular flows
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• Basement membranes are crucial for proper olfactory placode shape, position and boundary with the brain, and for olfactory axon development
• Modeling the Mass Distribution and Gravitational Potential of Nearby Disk Galaxies: Implications for the ISM Dynamical Equilibrium
• Binary black holes in the heat of merger
• A Gaussian jump process formulation of the reaction–diffusion master equation enables faster exact stochastic simulations
• Microscopic approach to the quantized light-matter interaction in semiconductor nanostructures: Complex coupled dynamics of excitons, biexcitons, and photons
• KnotDLO: Toward Interpretable Knot Tying
• Explainable anomaly detection for sound spectrograms using pooling statistics with quantile differences
• Glitches far from transient gravitational-wave events do not bias inference
• rodeo: Probabilistic Methods of Parameter Inference for Ordinary Differential Equations
• Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
• REBELS-MOSFIRE: Weak CIII] Emission is Typical Among Extremely UV-bright, Massive Galaxies at z∼7
• Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities
• The Relation between Solar Spicules and Magnetohydrodynamic Shocks
• Inferring Host-galaxy Properties of LIGO–Virgo–KAGRA’s Black Holes
• 3D tomography of the giant Lyα nebulae of z ≈ 3–5 radio-loud AGN
• Analysis-ready VCF at Biobank scale using Zarr
• Galaxy Cluster Mass Estimation Through The Splashback Radius
• A Ground-Based Transit Observation of the Long-Period Extremely Low-Density Planet HIP 41378 f
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• The Low Mass Dwarf Host Galaxy of Non-Repeating FRB 20230708A
• Engineering Precise and Robust Effective Hamiltonians
• Interior dynamics of super-Earth 55 Cancri e
• Consequences of Non-Gaussian Instrumental Noise in Perturbed Nulling Interferometers
• Behavioral Traits as Dynamical Systems: Utilizing Entropy to Analyze Longitudinal Psychometric Data in Coupled Ordinary Differential Equations
• An Earth-like Density for the Temperate Earth-sized Planet GJ 12b
• PlaceFM: A Training-free Geospatial Foundation Model of Places using Large-Scale Point of Interest Data
• STable AutoCorrelation Integral Estimator (STACIE): Robust and accurate transport properties from molecular dynamics simulations
• Asteroseismology with PBjam 2.0: measuring dipole mode frequencies in coupling regimes from main sequence to low-luminosity red giant stars
• Compact Ionized Gas Region Surrounded by Porous Neutral Gas in a Dusty Lyman Break Galaxy at Redshift z=8.312
• TESSERA: Temporal Embeddings of Surface Spectra for Earth Representation and Analysis
• rd-spiral: An open-source Python library for learning 2D reaction-diffusion dynamics through pseudo-spectral method
• A hybrid approach for the dynamic routing of police patrols
• Speeding up thermalization and quantum state preparation through engineered quantum collisions
• Permutation Equivariant Neural Controlled Differential Equations for Dynamic Graph Representation Learning
• Investigating silicate, carbon, and water in the diffuse interstellar medium: the first shots from WISCI
• Galaxy Morphology Classification: Are Stellar Circularities Enough?
• Follow-Up Exploration of the TWA 7 Planet-Disk System with JWST NIRCam
• Gravity-sensitive Spectral Indices in Ultracool Dwarfs: Investigating Correlations with Metallicity and Planet Occurrence using SpeX and FIRE Observations
• Anti-Phishing Training (Still) Does Not Work: A Large-Scale Reproduction of Phishing Training Inefficacy Grounded in the NIST Phish Scale
• Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf
• BRAiSE: synthetic polarisation in RMHD AGN jet simulations
• The Hα line as a probe of chromospheric magnetic fields
• The HST-Gaia Near-Infrared Astrometric Reference Frame near the Milky Way Galactic Center
• Ancient DNA reveals diverse community organizations in the 5th millennium BCE Carpathian Basin
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• 100-Day Analysis of USD/IDR Exchange Rate Dynamics Around the 2025 U.S. Presidential Inauguration
• Denoising the Future: Top-p Distributions for Moving Through Time
• Fast Capture of Cell-Level Provenance in Numpy
• Simulated impact on LSST data of Starlink V1.5 and V2 satellites
• Binsparse: A Specification for Cross-Platform Storage of Sparse Matrices and Tensors
• Adapting Vision-Language Models for Evaluating World Models
• Testing Cosmic Distance Duality Relation and Transparency with DESI DR2
• JAX-LaB: A High-Performance, Differentiable, Lattice Boltzmann Library for Modeling Multiphase Fluid Dynamics in Geosciences and Engineering
• Two Types of 1/f Range in Solar Wind Turbulence
• X-ray emission signatures of galactic feedback in the hot circumgalactic medium: predictions from cosmological hydrodynamical simulations
• Magnetic Hysteresis Experiments Performed on Quantum Annealers
• Transformers for Stratified Spectropolarimetric Inversion: Proof of Concept
• Disentangling Metallicity Effects in Hot Jupiter Occurrence Across Galactic Birth Radius and Phase-Space Density
• Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
• BLADE: An Automated Framework for Classifying Light Curves from the Center for Near-Earth Object Studies (CNEOS) Fireball Database
• SO emission in the dynamically perturbed protoplanetary disks around CQ Tau and MWC 758
• Wavelet-based Global Orientation and Surface Reconstruction for Point Clouds
• Systematic non-thermal velocity increase preceding soft X-ray flare onset: A large-scale Hinode/EIS study
• A System Level Compiler for Massively-Parallel, Spatial, Dataflow Architectures
• Synthesizer: Synthetic Observables For Modern Astronomy
• Dense SAE Latents Are Features, Not Bugs
• cAST: Enhancing Code Retrieval-Augmented Generation with Structural Chunking via Abstract Syntax Tree
• Stable Gradients for Stable Learning at Scale in Deep Reinforcement Learning
• Over-squashing in Spatiotemporal Graph Neural Networks
• Cosmological constraints on 4-dimensional Einstein-Gauss-Bonnet gravity
• MoR: Better Handling Diverse Queries with a Mixture of Sparse, Dense, and Human Retrievers
• What is a good use case for quantum computers?
• Low-metallicity nova explosions: a site for weak rp-process nucleosynthesis
• Zero-Shot Reinforcement Learning Under Partial Observability
• Procedures for Constraining Robotic Fiber Positioning for Highly Multiplexed Spectroscopic Surveys: The Case of FPS for SDSS-V
• Optimal alignment of Lorentz orientation and generalization to matrix Lie groups
• Vacuum Instability and False Vacuum Decay Induced by Domain Walls in the N2HDM
• Black hole ringdown spectroscopy of curvature-coupled scalar and pseudoscalar fields
• ODIN: The LAE Lyα Luminosity Function over Cosmic Time and Environmental Density
• VLBA astrometry of PSRs B0329+54 and B1133+16: Improved pulsar distances and comparison of global ionospheric models
• JWST Reveals a Candidate Jellyfish Galaxy at z=1.156
• Thermal and Optical Characterization of Near-Earth Objects: Science Commissioning of the Recently Upgraded Mid-Infrared Camera MIRSI on the NASA Infrared Telescope Facility
• NIR filter transformations across the HR diagram: JWST, Roman, and Euclid
• Sub-Parsec Acceleration and Collimation of NGC 4261's Twin Jets
• Limits to Extracting Neutron-Star Physics Constraints from NICER Pulse Profiles
• lcpy: an open-source python package for parametric and dynamic Life Cycle Assessment and Life Cycle Costing
• The Courage to Stop: Overcoming Sunk Cost Fallacy in Deep Reinforcement Learning
• Kinetic theory of coupled binary-fluid-surfactant systems
• CGBack: Diffusion Model for Backmapping Large-Scale and Complex Coarse-Grained Molecular Systems
• Tides Tighten the Hycean Habitable Zone
• The Software Landscape for the Density Matrix Renormalization Group
• The population of NuSTAR Black Hole X-ray Binaries
• Spatial autocorrelation in machine learning for modelling soil organic carbon
• Impacts of UV Radiation from an AGN on Planetary Atmospheres and Consequences for Galactic Habitability
• Hi-GDT: A Hi-C-based 3D gene domain analysis tool for analyzing local chromatin contacts in plants
• Media Capture, Survival of the Corruptest and Journalistic Agency: The Case of Bulgaria
• Graphene edge method for three‐dimensional probing of Raman microscopes focal volumes
• Enhanced prediction of ionic liquid toxicity using a meta-ensemble learning framework with data augmentation
• Real-Time High-Accuracy Digital Wireless Time, Frequency, and Phase Calibration For Coherent Distributed Antenna Arrays
• Gas-Poor Hosts and Gas-Rich Companions of z≈3.5 Radio Active Galactic Nuclei: ALMA Insights into Jet Triggering and Feedback
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): VIII. The impact of external photoevaporation on disk masses and radii in Upper Scorpius
• On the Mass Budget Problem of Protoplanetary Disks: Streaming Instability and Optically Thick Emission
• On the calculation of p-values for quadratic statistics in Pulsar Timing Arrays
• The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): XI. Beam-corrected gas disk sizes from fitting 12CO moment zero maps
• Discovery of a 21 cm absorption system at z=2.327 with CHIME
• Identifiability Challenges in Sparse Linear Ordinary Differential Equations
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• Tryptoline Stereoprobe Elaboration Identifies Inhibitors of the GRPEL1-HSPA9 Chaperone Complex
• Label-semantics Aware Generative Approach for Domain-Agnostic Multilabel Classification
• Demystifying Topological Message-Passing with Relational Structures: A Case Study on Oversquashing in Simplicial Message-Passing
• Mapping the Spatial Distribution of Fast Radio Bursts within their Host Galaxies
• Multi-band, Multi-epoch Photometry of the Spot-crossing System TOI-3884: Refined System Geometry and Spot Properties
• Searching for Historical Extragalactic Optical Transients Associated with Fast Radio Bursts
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• How to craft a deep reinforcement learning policy for wind farm flow control
• Dynamical mass distribution and velocity structure of the Galactic centre
• Testing OH Megamaser Identification Methods in HI Surveys: Updated Source-Flagging Algorithms and New Detections in ALFALFA
• Optimizing entanglement distribution via noisy quantum channels
• Stochastic elastohydrodynamics of contact and coarsening during membrane adhesion
• PyGemini: Unified Software Development towards Maritime Autonomy Systems
• 3DFlowAction: Learning Cross-Embodiment Manipulation from 3D Flow World Model
• A Detection of Helium in the Bright Superluminous Supernova SN 2024rmj
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• The Hourglass Simulation: A Catalog for the Roman High-Latitude Time-Domain Core Community Survey
• Modern approaches to building interpretable models of the property market using machine learning on the base of mass cadastral valuation
• Toward Better SSIM Loss for Unsupervised Monocular Depth Estimation
• UnHiPPO: Uncertainty-aware Initialization for State Space Models
• The TESS Ten Thousand Catalog: 10,001 uniformly-vetted and -validated Eclipsing Binary Stars detected in Full-Frame Image data by machine learning and analyzed by citizen scientists
• LFA applied to CNNs: Efficient Singular Value Decomposition of Convolutional Mappings by Local Fourier Analysis
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• Dr Wenowdis: Specializing Dynamic Language C Extensions using Type Information
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• Initial Characterization of Stellar Photometry of Roman images from the OpenUniverse Simulations
• Use the 4S (Signal-Safe Speckle Subtraction): Explainable Machine Learning Reveals the Giant Exoplanet AF Lep b in High-contrast Imaging Data from 2011

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