SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

Abstract

SciPy is an open source scientific computing library for the Python programming language. SciPy 1.0 was released in late 2017, about 16 years after the original version 0.1 release. SciPy has become a de facto standard for leveraging scientific algorithms in the Python programming language, with more than 600 unique code contributors, thousands of dependent packages, over 100,000 dependent repositories, and millions of downloads per year. This includes usage of SciPy in almost half of all machine learning projects on GitHub, and usage by high profile projects including LIGO gravitational wave analysis and creation of the first-ever image of a black hole (M87). The library includes functionality spanning clustering, Fourier transforms, integration, interpolation, file I/O, linear algebra, image processing, orthogonal distance regression, minimization algorithms, signal processing, sparse matrix handling, computational geometry, and statistics. In this work, we provide an overview of the capabilities and development practices of the SciPy library and highlight some recent technical developments.

Article source data is available here: https://github.com/scipy/scipy-articles

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• Classical variational simulation of the Quantum Approximate Optimization Algorithm
• The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
• Inverse Kohn-Sham Density Functional Theory: Progress and Challenges
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• Spatially Resolved Properties of High Redshift Galaxies in the SMACS0723 JWST ERO Field
• The Neutrino Fast Flavor Instability in Three Dimensions
• No peaks without valleys: The stable mass transfer channel for gravitational-wave sources in light of the neutron star-black hole mass gap
• High-redshift radio galaxies: a potential new source of 21-cm fluctuations
• Predicting Aqueous Solubility of Organic Molecules Using Deep Learning Models with Varied Molecular Representations
• Ultra-fast interpretable machine-learning potentials
• POSEIDON: A Multidimensional Atmospheric Retrieval Code for Exoplanet Spectra
• Bilby-MCMC: An MCMC sampler for gravitational-wave inference
• AGNIFS survey of local AGN: GMOS-IFU data and outflows in 30 sources
• The Upper Edge of the Neptune Desert Is Stable Against Photoevaporation
• Supernova Model Discrimination with Hyper-Kamiokande
• The Sparkler: Evolved High-Redshift Globular Clusters Captured by JWST
• The Three Hundred Project: Dynamical state of galaxy clusters and morphology from multi-wavelength synthetic maps
• Morphologies of Galaxies at $z\gtrsim 9$ Uncovered by JWST/NIRCam Imaging: Cosmic Size Evolution and an Identification of an Extremely Compact Bright Galaxy at $z\sim 12$
• RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow
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• No Such Thing as a Simple Flare: Substructure and QPPs Observed in a Statistical Sample of 20 Second Cadence TESS Flares
• CEERS Key Paper IV: Galaxies at $4<z<9$ are Bluer than They Appear -- Characterizing Galaxy Stellar Populations from Rest-Frame $\sim 1$ micron Imaging
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• Awesome SOSS: Transmission Spectroscopy of WASP-96b with NIRISS/SOSS
• A unique hot Jupiter spectral sequence with evidence for compositional diversity
• EvryFlare III: Temperature Evolution and Habitability Impacts of Dozens of Superflares Observed Simultaneously by Evryscope and TESS
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• Ideal refocusing of an optically active spin qubit under strong hyperfine interactions
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• Mitigation of LEO Satellite Brightness and Trail Effects on the Rubin Observatory LSST
• Evidence of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters
• Analysis of Early Science observations with the CHaracterising ExOPlanets Satellite (CHEOPS) using pycheops
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• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of $z>6.5$ Quasars Using JWST
• Quasar Feedback Survey: Multi-phase outflows, turbulence and evidence for feedback caused by low power radio jets inclined into the galaxy disk
• The DECam Local Volume Exploration Survey Data Release 2
• ExoClock Project III: 450 new exoplanet ephemerides from ground and space observations
• zeus: A Python implementation of Ensemble Slice Sampling for efficient Bayesian parameter inference
• Analysis of a JWST NIRSpec Lab Time Series: Characterizing Systematics, Recovering Exoplanet Transit Spectroscopy, and Constraining a Noise Floor
• Deep learning-based surrogate model for 3-D patient-specific computational fluid dynamics
• Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
• ARES I: WASP-76 b, A Tale of Two HST Spectra
• pyFIT3D and pyPipe3D -- The new version of the Integral Field Spectroscopy data analysis pipeline
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Observable-to-Mass-and-Redshift Relations of Galaxy Clusters and Groups with Weak-Lensing Mass Calibration from the Hyper Suprime-Cam Subaru Strategic Program Survey
• Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock images
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• Dissecting the Local Environment of FRB 190608 in the Spiral Arm of its Host Galaxy
• Robustness of dark energy phenomenology across different parameterizations
• Chemo-dynamics of outer halo dwarf stars, including \textit{Gaia}-Sausage and \textit{Gaia}-Sequoia candidates
• A 5% measurement of the Hubble constant from Type II supernovae
• Survey of Surveys I: The largest catalogue of radial velocities for the Galaxy
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• ARES II: Characterising the Hot Jupiters WASP-127 b, WASP-79 b and WASP-62 b with HST
• The Hubble Space Telescope Survey of M31 Satellite Galaxies I. RR Lyrae-based Distances and Refined 3D Geometric Structure
• Properties and characteristics of the WFIRST H4RG-10 detectors
• ZTF Early Observations of Type Ia Supernovae II: First Light, the Initial Rise, and Time to Reach Maximum Brightness
• Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
• First Detection of Hydroxyl Radical Emission from an Exoplanet Atmosphere: High-dispersion Characterization of WASP-33b using Subaru/IRD
• Detection of Atmospheric Escape from Four Young Mini Neptunes
• Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged Inside the Debris Disk of the Young Star AF Lep
• Diving Beneath the Sea of Stellar Activity: Chromatic Radial Velocities of the Young AU Mic Planetary System
• A Feasible Approach for Automatically Differentiable Unitary Coupled-Cluster on Quantum Computers
• Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3
• Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
• One qubit as a Universal Approximant
• Stellar Collapse Diversity and the Diffuse Supernova Neutrino Background
• Recovering the star formation histories of recently-quenched galaxies: the impact of model and prior choices
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
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• TRIDENT: A Rapid 3D Radiative Transfer Model for Exoplanet Transmission Spectra
• Ram pressure stripping candidates in the Coma Cluster: Evidence for enhanced star formation
• Molecules with ALMA at Planet-forming Scales (MAPS) VI: Distribution of the small organics HCN, C2H, and H2CO
• p-winds: an open-source Python code to model planetary outflows and upper atmospheres
• PHANGS-JWST First Results: A statistical view on bubble evolution in NGC628
• TESS-Gaia Light Curve: a PSF-based TESS FFI light curve product
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• A Shock Flash Breaking Out of a Dusty Red Supergiant
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• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• Quaia, the Gaia-unWISE Quasar Catalog: An All-Sky Spectroscopic Quasar Sample
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• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
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• Strong Superexchange in a $d^{9-\delta }$ Nickelate Revealed by Resonant Inelastic X-Ray Scattering
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• Perceval: A Software Platform for Discrete Variable Photonic Quantum Computing
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• Direct Imaging Discovery and Dynamical Mass of a Substellar Companion Orbiting an Accelerating Hyades Sun-like Star with SCExAO/CHARIS
• Gas Dynamics in the Galaxy: Total Mass Distribution and the Bar Pattern Speed
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• STRIDES: Automated uniform models for 30 quadruply imaged quasars
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• Modeling protoplanetary disk SEDs with artificial neural networks: Revisiting the viscous disk model and updated disk masses
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
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• Overlap-ADAPT-VQE: Practical Quantum Chemistry on Quantum Computers via Overlap-Guided Compact Ansätze
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• The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
• Andromeda XXI -- a dwarf galaxy in a low density dark matter halo
• Reinforcement learning approach to non-equilibrium quantum thermodynamics
• Pre-Common-Envelope Mass Loss from Coalescing Binary Systems
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Molecules with ALMA at Planet-forming Scales (MAPS) XI: CN and HCN as Tracers of Photochemistry in Disks
• Constraining mornings & evenings on distant worlds: a new semi-analytical approach and prospects with transmission spectroscopy
• Cataloging the radio-sky with unsupervised machine learning: a new approach for the SKA era
• The Optical Two and Three-Dimensional Fundamental Plane Correlations for Nearly 180 Gamma-Ray Burst Afterglows with Swift/UVOT, RATIR, and the SUBARU Telescope
• Determining the proton content with a quantum computer
• Limitations on sharing Bell nonlocality between sequential pairs of observers
• Rates and delay times of type Ia supernovae in the Dark Energy Survey
• LIGOs Quantum Response to Squeezed States
• The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies
• Limits on Millimeter Continuum Emission from Circumplanetary Material in the DSHARP Disks
• Stellar Rotation in the K2 Sample: Evidence for Modified Spindown
• Steady-state accretion in magnetized protoplanetary disks
• Linear Viscoelastic Properties of the Vertex Model for Epithelial Tissues
• A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329
• Variational quantum eigensolver for the Heisenberg antiferromagnet on the kagome lattice
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• The multiwavelength properties of red QSOs -- Evidence for dusty winds as the origin of QSO reddening
• Correlation-consistent Gaussian basis sets for solids made simple
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• TOI-1452 b: SPIRou and TESS reveal a super-Earth in a temperate orbit transiting an M4 dwarf
• Masses and radiative decay widths of S- and P-wave singly-, doubly- and triply-heavy charm and bottom baryons
• Quasinormal modes and their overtones at the common horizon in a binary black hole merger
• Simulating periodic systems on quantum computer
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• The CARMENES search for exoplanets around M dwarfs. Three temperate to warm super-Earths
• Square Kilometre Array Science Data Challenge 1: analysis and results
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• TIC 168789840: A Sextuply-Eclipsing Sextuple Star System
• Quantum variational optimization: The role of entanglement and problem hardness
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• The Pan-STARRS1 z>5.6 quasar survey II: Discovery of 55 Quasars at 5.6<z<6.5
• Molecular Gas Properties and CO-to-H2 Conversion Factors in the Central Kiloparsec of NGC 3351
• New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood
• Lattice continuum-limit study of nucleon quasi-PDFs
• Stellar Disruption of Axion Miniclusters in the Milky Way
• Jet collimation and acceleration in the giant radio galaxy NGC 315
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Reducing qubit requirements while maintaining numerical precision for the Variational Quantum Eigensolver: A Basis-Set-Free Approach
• The Nominal Range of Rocky Planet Masses, Radii, Surface Gravities and Bulk Densities
• The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models
• Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations
• TheHaloMod: An online calculator for the halo model
• In-situ extreme mass ratio inspirals via sub-parsec formation and migration of stars in thin, gravitationally unstable AGN discs
• ARES III: Unveiling the Two Faces of KELT-7 b with HST WFC3
• Eigenpulses of dispersive time-varying media
• PySME -- Spectroscopy Made Easier
• Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour
• Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF
• Outflows Driven by Direct and Reprocessed Radiation Pressure in Massive Star Clusters
• Solar Flare Effects on the Earth's Lower Ionosphere
• Quantum algorithms for quantum dynamics: A performance study on the spin-boson model
• Dynamically cold disks in the early Universe: myth or reality?
• Speckle Observations of TESS Exoplanet Host Stars: Understanding the Binary Exoplanet Host Star Orbital Period Distribution
• Ultraviolet spectra of extreme nearby star-forming regions: evidence for an overabundance of very massive stars
• The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5
• Constraints on the assembly history of the Milky Way's smooth, diffuse stellar halo from the metallicity-dependent, radially-dominated velocity anisotropy profiles probed with K giants and BHB stars using LAMOST, SDSS/SEGUE, and Gaia
• Gas-phase metallicity gradients in galaxies at $z\sim 6-8$
• YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-Loop
• Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
• The Ariel Target List: The Impact of TESS and the Potential for Characterising Multiple Planets Within a System
• EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802
• A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67
• The Physical Drivers and Observational Tracers of CO-to-H2 Conversion Factor Variations in Nearby Barred Galaxy Centers
• Optimizing a DIscrete Loss (ODIL) to solve forward and inverse problems for partial differential equations using machine learning tools
• Assessing the data-analysis impact of LISA orbit approximations using a GPU-accelerated response model
• The GCE in a New Light: Disentangling the $\gamma$-ray Sky with Bayesian Graph Convolutional Neural Networks
• tax2vec: Constructing Interpretable Features from Taxonomies for Short Text Classification
• Quartz Clouds in the Dayside Atmosphere of the Quintessential Hot Jupiter HD 189733 b
• Observations of the Crab Nebula and Pulsar with the Large-Sized Telescope Prototype of the Cherenkov Telescope Array
• Two temperate Earth-mass planets orbiting the nearby star GJ1002
• Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results
• An ALMA study of hub-filament systems I. On the clump mass concentration within the most massive cores
• Double-, triple-line spectroscopic candidates in the LAMOST Medium-Resolution Spectroscopic Survey
• Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks
• Automated galaxy-galaxy strong lens modelling: no lens left behind
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Long-term Evolution of Tightly-Packed Stellar Black Holes in AGN Disks: Formation of Merging Black-Hole Binaries via Close Encounters
• Bound entanglement from randomized measurements
• The GALAH survey: A census of lithium-rich giant stars
• Detection of the tidal deformation of WASP-103b at $3\sigma$ with CHEOPS
• Phase-resolved spectroscopy of a quasi-periodic oscillation in the black hole X-ray binary GRS 1915+105 with NICER and NuSTAR
• JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b
• A population of heavily reddened, optically missed novae from Palomar Gattini-IR: Constraints on the Galactic nova rate
• The Two-Dimensional Metallicity Distribution and Mixing Scales of Nearby Galaxies
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the $TESS$ Continuous Viewing Zones and beyond
• The Spectacular Ultraviolet Flash From the Peculiar Type Ia Supernova 2019yvq
• Formation of an extended stellar halo around an ultra-faint dwarf galaxy following one of the earliest mergers from galactic building blocks
• "Look! It's a Computer Program! It's an Algorithm! It's AI!": Does Terminology Affect Human Perceptions and Evaluations of Algorithmic Decision-Making Systems?
• Anisotropic momentum broadening in the 2+1D Glasma: analytic weak field approximation and lattice simulations
• Quantum-classical simulation of two-site dynamical mean-field theory on noisy quantum hardware
• HETDEX Public Source Catalog 1: 220K Sources Including Over 50K Lyman Alpha Emitters from an Untargeted Wide-area Spectroscopic Survey
• Discovery of post-mass-transfer helium-burning red giants using asteroseismology
• TOI-5205 b: A Short-period Jovian Planet Transiting a Mid-M Dwarf
• Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
• To cool is to keep: Residual H/He atmospheres of super-Earths and sub-Neptunes
• The Thousand-Pulsar-Array program on MeerKAT -- IX. The time-averaged properties of the observed pulsar population
• Systematically Measuring Ultra-Diffuse Galaxies (SMUDGes). III. The Southern SMUDGes Catalog
• Evidence for disequilibrium chemistry from vertical mixing in hot Jupiter atmospheres. A comprehensive survey of transiting close-in gas giant exoplanets with warm-Spitzer/IRAC
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• The role of galaxies and AGN in reionising the IGM -- III : IGM-galaxy cross-correlations at z~6 from 8 quasar fields with DEIMOS and MUSE
• Interpreting High-Resolution Spectroscopy of Exoplanets Using Cross-Correlations and Supervised Machine Learning
• Linear and Nonlinear Dimensionality Reduction from Fluid Mechanics to Machine Learning
• Machine Learning Quantum Reaction Rate Constants
• Constraints on the Faint End of the Galaxy Stellar Mass Function at z ~ 4-8 from Deep JWST Data
• Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
• Interactive Dimensionality Reduction for Comparative Analysis
• A Deep Learning Approach for Active Anomaly Detection of Extragalactic Transients
• TETRIS-ADAPT-VQE: An adaptive algorithm that yields shallower, denser circuit ansätze
• A Spectral Survey of WASP-19b with ESPRESSO
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
• Appreciating mergers for understanding the non-linear $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ and $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{galaxy}}$ relations, updated herein, and the implications for the (reduced) role of AGN feedback
• Atmospheres as windows into sub-Neptune interiors: coupled chemistry and structure of hydrogen-silane-water envelopes
• BAFFLES: Bayesian Ages for Field Lower-Mass Stars
• TOI-2109b: An Ultrahot Gas Giant on a 16 hr Orbit
• Mapping the exo-Neptunian landscape. A ridge between the desert and savanna
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• A Machine Learning Based Source Property Inference for Compact Binary Mergers
• The Hills Mechanism and the Galactic Center S-stars
• Inference of the cosmic rest-frame from supernovae Ia
• The Thousand-Pulsar-Array programme on MeerKAT: -- VI. Pulse widths of a large and diverse sample of radio pulsars
• The Value of Progenitor Radius Measurements for Explosion Modeling of Type II-Plateau Supernovae
• Gamma rays as probes of cosmic-ray propagation and interactions in galaxies
• Keck/NIRSPEC studies of He I in the atmospheres of two inflated hot gas giants orbiting K dwarfs: WASP-52b and WASP-177b
• Propagating Speed of Primordial Gravitational Waves
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• Statistical properties of the nebular spectra of 103 stripped envelope core collapse supernovae
• Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars
• Evidence for Metallicity-Dependant Spin Evolution in the Kepler field
• First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\ge 5$
• Black Hole Accretion Correlates with Star Formation Rate and Star Formation Efficiency in Nearby Luminous Type 1 Active Galaxies
• Using deep learning to understand and mitigate the qubit noise environment
• Fast simulations of highly-connected spiking cortical models using GPUs
• Alkaline Exospheres of Exoplanet Systems: Evaporative Transmission Spectra
• Stacking fault energy prediction for austenitic steels: thermodynamic modeling vs. machine learning
• Predicting the Mechanical Properties of Biopolymer Gels Using Neural Networks Trained on Discrete Fiber Network Data
• Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at $z=4.5-11.5$
• COSMOS2020: Exploring the dawn of quenching for massive galaxies at 3 < z < 5 with a new colour selection method
• The Low-redshift Lyman-continuum Survey: [S II]-deficiency and the leakage of ionizing radiation
• The First Dynamical Mass Measurement in the HR 8799 System
• The K2 Galactic Archaeology Program Data Release 3: Age-abundance patterns in C1-C8 and C10-C18
• A Population-Informed Mass Estimate for Pulsar J0740+6620
• The Formation of a Stellar Association in the NGC 7000/IC 5070 Complex: Results from Kinematic Analysis of Stars and Gas
• Recovery of TESS Stellar Rotation Periods Using Deep Learning
• Confirmation of Iron Emission Lines and Non-detection of TiO on the Dayside of KELT-9b with MAROON-X
• Gauge-equivariant flow models for sampling in lattice field theories with pseudofermions
• WISDOM Project -- X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
• Hyperuniformity and phase enrichment in vortex and rotor assemblies
• Gaia Data Release 3: Properties of the line broadening parameter derived with the Radial Velocity Spectrometer (RVS)
• The mass and size of Herbig disks as seen by ALMA
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Importance nested sampling with normalising flows
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA
• On the origin of the mass-metallicity gradient relation in the local Universe
• Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST
• Interpreting deep learning models for weak lensing
• The importance of silicate vapor in determining the structure, radii, and envelope mass fractions of sub-Neptunes
• Is the expansion of the universe accelerating? All signs still point to yes a local dipole anisotropy cannot explain dark energy
• Two-dimensional topological insulator state in cadmium arsenide thin films
• Enhanced Lidov-Kozai migration and the formation of the transiting giant planet WD1856+534b
• Flowsheet synthesis through hierarchical reinforcement learning and graph neural networks
• Alignment between Initial State and Mixer Improves QAOA Performance for Constrained Optimization
• Liquid demixing in elastic networks: cavitation, permeation, or size selection?
• DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power Spectra
• GHOST: Using Only Host Galaxy Information to Accurately Associate and Distinguish Supernovae
• A trend in the effective spin distribution of LIGO binary black holes with mass
• Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
• Quantum optimization via four-body Rydberg gates
• The phase spiral in Gaia DR3
• Artificial intelligence discovery of a charging protocol in a micromaser quantum battery
• A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing
• Deep embedded clustering of coral reef bioacoustics
• Optimized Low-Depth Quantum Circuits for Molecular Electronic Structure using a Separable Pair Approximation
• Classical Cepheid period-Wesenheit-metallicity relation in the Gaia bands
• X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• How robustly can we constrain the low-mass end of the $z\sim 6-7$ stellar mass function? -- The limits of lensing models and stellar population assumptions in the Hubble Frontier Fields
• ULYSSES: Universal LeptogeneSiS Equation Solver
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• The Milky Way tomography with APOGEE: intrinsic density distribution and structure of mono-abundance populations
• The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of $z\sim 2.3$ Star-forming Galaxies
• The Fifth Catalogue of Nearby Stars (CNS5)
• A Complex Luminosity Function for the Anomalous Globular Clusters in NGC1052-DF2 and NGC1052-DF4
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• How runaway stars boost galactic outflows
• Few-mode Field Quantization for Multiple Emitters
• Weighing the Galactic disk using phase-space spirals II. Most stringent constraints to a thin dark disk using Gaia EDR3
• Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift
• Formation of the Hub-Filament System G33.92+0.11: Local Interplay between Gravity, Velocity, and Magnetic Field
• An Automated Scanning Transmission Electron Microscope Guided by Sparse Data Analytics
• Nucleon D-term in holographic QCD
• Detecting stochastic gravitational waves with binary resonance
• Mid-to-Late M Dwarfs Lack Jupiter Analogs
• A tight angular-momentum plane for disc galaxies
• 2D Retrieval Frameworks for Hot Jupiter Phase Curves
• Element abundance patterns in stars indicate fission of nuclei heavier than uranium
• Dynamical ejecta synchrotron emission as possible contributor to the changing behaviour of GRB170817A
• PtyLab.m/py/jl: a cross-platform, open-source inverse modeling toolbox for conventional and Fourier ptychography
• Removing degeneracy and multimodality in gravitational wave source parameters
• Molecules with ALMA at Planet-forming Scales (MAPS) XIII: HCO${}^{+}$ and disk ionization structure
• Runaway OB Stars in the Small Magellanic Cloud: Dynamical Versus Supernova Ejections
• Flares, jets and quasi-periodic outbursts from neutron star merger remnants
• Infrared Excesses around Bright White Dwarfs from Gaia and unWISE I
• Metastable Helium Reveals an Extended Atmosphere for the Gas Giant HAT-P-18b
• Predicting the Exoplanet Yield of the TESS Prime and Extended Missions Through Years 1-7
• The Sandwich Mode for Vertical Shear Instability in Protoplanetary Disks
• Substructure in the stellar halo near the Sun. I. Data-driven clustering in Integrals of Motion space
• The New Generation Planetary Population Synthesis (NGPPS). VI. Introducing KOBE: Kepler Observes Bern Exoplanets. Theoretical perspectives on the architecture of planetary systems: Peas in a pod
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies
• On the Application of Bayesian Leave-One-Out Cross-Validation to Exoplanet Atmospheric Analysis
• Thermodynamic uncertainty relations for coherently driven open quantum systems
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Chemo-kinematics of the Milky Way spiral arms and bar resonances: connection to ridges and moving groups in the Solar vicinity
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation
• A significant mutual inclination between the planets within the $\pi$ Mensae system
• Rejuvenated accretors have less bound envelopes: Impact of Roche lobe overflow on subsequent common envelope events
• CO or no CO? Narrowing the CO abundance constraint and recovering the H2O detection in the atmosphere of WASP-127 b using SPIRou
• Non-intrusive reduced-order models for parametric partial differential equations via data-driven operator inference
• A Closer Look at Exoplanet Occurrence Rates: Considering the Multiplicity of Stars Without Detected Planets
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• A Quantum Algorithm to Calculate Band Structure at the EOM Level of Theory
• A new lepto-hadronic model applied to the first simultaneous multiwavelength data set for Cygnus X--1
• The Galaxy Progenitors of Stellar Streams around Milky Way-mass Galaxies in the FIRE Cosmological Simulations
• TOI-1235 b: a keystone super-Earth for testing radius valley emergence models around early M dwarfs
• Observational Inference on the Delay Time Distribution of Short Gamma-ray Bursts
• Mapping the Complex Kinematic Substructure in the TW Hya Disk
• A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models
• Stellar Escape from Globular Clusters. I. Escape Mechanisms and Properties at Ejection
• Exploring dark matter spike distribution around the Galactic centre with stellar orbits
• The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveys
• A Rosetta Stone for eccentric gravitational waveform models
• The Hawaii Infrared Parallax Program. V. New T-Dwarf Members and Candidate Members of Nearby Young Moving Groups
• Gemini/GMOS Optical Transmission Spectroscopy of WASP-121b: signs of variability in an ultra-hot Jupiter?
• Growth and evolution of secondary volcanic atmospheres: I. Identifying the geological character of hot rocky planets
• Disk structure around the Class I protostar L1489 IRS revealed by ALMA: a warped disk system
• High [OIII]/[CII] surface brightness ratios trace early starburst galaxies
• Matrix-free multigrid solvers for phase-field fracture problems
• AU Microscopii in the FUV: Observations in Quiescence, During Flares, and Implications for AU Mic b and c
• A framework for the architecture of exoplanetary systems. I. Four classes of planetary system architecture
• Probing the Nature of High Redshift Weak Emission Line Quasars: A Young Quasar with a Starburst Host Galaxy
• The Mantis Network III: Expanding the limits of chemical searches within ultra hot-Jupiters. New detections of Ca I, V I, Ti I, Cr I, Ni I, Sr II, Ba II, and Tb II in KELT-9 b
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Precision Machine Learning
• A neural simulation-based inference approach for characterizing the Galactic Center $\gamma$-ray excess
• Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey
• ZTF20aajnksq (AT2020blt): A Fast Optical Transient at $z\approx 2.9$ With No Detected Gamma-Ray Burst Counterpart
• TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on $H_0$
• High-resolution atmospheric retrievals of WASP-121b transmission spectroscopy with ESPRESSO: Consistent relative abundance constraints across multiple epochs and instruments
• Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R${}_{\odot }$
• Modeling Dark Photon Oscillations in Our Inhomogeneous Universe
• Discovery of a directly imaged planet to the young solar analog YSES 2
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Dynamically constraining the length of the Milky Way bar
• pymia: A Python package for data handling and evaluation in deep learning-based medical image analysis
• Self-lensing flares from black hole binaries I: general-relativistic ray tracing of black hole binaries
• The nucleation fraction of Local Volume galaxies
• Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
• Adorym: A multi-platform generic x-ray image reconstruction framework based on automatic differentiation
• Non-linear black hole dynamics and Carrollian fluids
• An efficient adaptive variational quantum solver of the Schrodinger equation based on reduced density matrices
• Relaxation Runge-Kutta Methods for Hamiltonian Problems
• PeriPy -- A High Performance OpenCL Peridynamics Package
• UV Exoplanet Transmission Spectral Features as Probes of Metals and Rainout
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• PBjam: A Python package for automating asteroseismology of solar-like oscillators
• Scattered Light Imaging: Resolving the substructure of nerve fiber crossings in whole brain sections with micrometer resolution
• Warm Jupiters in TESS Full-Frame Images: A Catalog and Observed Eccentricity Distribution for Year 1
• Superradiant Production of Heavy Dark Matter from Primordial Black Holes
• After The Fall: Resolving the Molecular Gas in Post-Starburst Galaxies
• True masses of the long-period companions to HD 92987 and HD 221420 from Hipparcos-Gaia astrometry
• On the treatment of boundary conditions for bond-based peridynamic models
• A SModelS interface for pyhf likelihoods
• Autonomous synthesis of thin film materials with pulsed laser deposition enabled by in situ spectroscopy and automation
• Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores
• Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488)
• Chemodynamics of Green Pea galaxies -- I. Outflows and turbulence driving the escape of ionising photons and chemical enrichment
• JWST near-infrared spectroscopy of the Lucy Jupiter Trojan flyby targets: Evidence for OH absorption, aliphatic organics, and CO${}_2$
• Classification of Magnetohydrodynamic Simulations using Wavelet Scattering Transforms
• VERTICO II: effects of HI-identified environmental mechanisms on molecular gas
• Properties of the jet in M87 revealed by its helical structure imaged with the VLBA at 8 and 15 GHz
• Tracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253
• Stellar Metallicities from SkyMapper Photometry II: Precise photometric metallicities of $\sim$280,000 giant stars with [Fe/H] $<-0.75$ in the Milky Way
• Differentiable quantum chemistry with PySCF for molecules and materials at the mean-field level and beyond
• Drag, lift and torque correlations for axi-symmetric non-spherical particles in locally non-uniform flows
• The Hubble WFC3 Emission Spectrum of the Extremely-Hot Jupiter, KELT-9b
• Double-Weak Decays of ${}^{124}$Xe and ${}^{136}$Xe in the XENON1T and XENONnT Experiments
• A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation
• The bursty star formation history of the Fornax dwarf spheroidal galaxy revealed with the HST
• Quantifying Dynamic Tilting in Halide Perovskites: Chemical Trends and Local Correlations
• On the Stellar Kinematics and Mass of the Virgo Ultra-Diffuse Galaxy VCC 1287
• Dark Matter Deficient Galaxies And Their Member Star Clusters Form Simultaneously During High-velocity Galaxy Collisions In 1.25 pc Resolution Simulations
• 3D spectroscopic analysis of helium-line white dwarfs
• APPLESOSS: A Producer of ProfiLEs for SOSS. Application to the NIRISS SOSS Mode
• First SETI Observations with China's Five-hundred-meter Aperture Spherical radio Telescope (FAST)
• An Inverse Procedural Modeling Pipeline for SVBRDF Maps
• Local classical MAX-CUT algorithm outperforms $p=2$ QAOA on high-girth regular graphs
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• The approximately universal shapes of epidemic curves in the Susceptible-Exposed-Infectious-Recovered (SEIR) model
• Gravitational wave population inference with deep flow-based generative network
• Reheating ACTs on Starobinsky and Higgs inflation
• Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: I. Period-Fourier-Metallicity Relations for Fundamental Mode RR Lyrae
• The frequency of extreme X-ray variability of radio-quiet quasars
• Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-Dwarf Companion in the Hyades
• Observing the Sun as a star: Design and early results from the NEID solar feed
• SMARPs and SHARPs: Two Solar Cycles of Active Region Data
• BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE
• Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
• Chemical Cartography with LAMOST and Gaia Reveal Azimuthal and Spiral Structure in the Galactic Disk
• Testing new physics models with global comparisons to collider measurements: the Contur toolkit
• Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk
• Pre-merger localization of compact-binary mergers with third generation observatories
• The Spectroscopic Classification of Astronomical Transients (SCAT) Survey: Overview, Pipeline Description, Initial Results, and Future Plans
• Stochastic Low Frequency Variability in 3-Dimensional Radiation Hydrodynamical Models of Massive Star Envelopes
• HST/WFC3 H$\alpha$ Direct-Imaging Detection of a Point-like Source in the Disk Cavity of AB Aur
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• Mining the Ultra-Hot Skies of HAT-P-70b: Detection of a Profusion of Neutral and Ionized Species
• A Transient "Changing-look'' Active Galactic Nucleus Resolved on Month Timescales from First-year Sloan Digital Sky Survey V Data
• Machine learning classification of CHIME fast radio bursts -- I. Supervised methods
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• The challenge of simulating the star cluster population of dwarf galaxies with resolved interstellar medium
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• Correlations between Triaxial Shapes and Formation History of Dark Matter Haloes
• Black Hole Polarimetry I: A Signature of Electromagnetic Energy Extraction
• ALMA Detection of Dust Trapping around Lagrangian Points in the LkCa 15 Disk
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• Machine-learning classification of astronomical sources: estimating F1-score in the absence of ground truth
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• QRnet: optimal regulator design with LQR-augmented neural networks
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• PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• Gaia DR3 in 6D: The search for fast hypervelocity stars and constraints on the Galactic Centre environment
• A quasar-based supermassive black hole binary population model: implications for the gravitational-wave background
• The KBSS-KCWI Survey: The connection between extended Ly$\alpha$ halos and galaxy azimuthal angle at $z\sim 2-3$
• Outflows from Super Star Clusters in the Central Starburst of NGC253
• Reweighting of molecular simulations with explicit-solvent SAXS restraints elucidates ion-dependent RNA ensembles
• Transmission spectroscopy for the warm sub-Neptune HD3167c: evidence for molecular absorption and a possible high metallicity atmosphere
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• Long-term Evolution of Binary Orbits Induced by Circumbinary Disks
• Dynamical Evidence of a Spiral Arm--Driving Planet in the MWC 758 Protoplanetary Disk
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• The XQR-30 Metal Absorber Catalog: 778 Absorption Systems Spanning 2 < z < 6.5
• Microcanonical and finite temperature ab initio molecular dynamics simulations on quantum computers
• Restoring isotropy in a three-dimensional lattice model: The Ising universality class
• The Most Metal-poor Stars in the Magellanic Clouds are $r$-process Enhanced
• Interpreting high spatial resolution line observations of planet-forming disks with gaps and rings -- The case of HD 163296
• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
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• The Pan-STARRS1 $\mathbf{z}>5.6$ Quasar Survey: III. The $\mathbf{z}\approx 6$ Quasar Luminosity Function
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• Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum
• The first large catalogue of spectroscopic redshifts in Webb's First Deep Field, SMACS J0723.3$-$7327
• JWST Noise Floor II: Systematic Error Sources in JWST NIRCam Time Series
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• Black-Box Optimization Revisited: Improving Algorithm Selection Wizards through Massive Benchmarking
• The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
• Photometric variability as a proxy for magnetic activity and its dependence on metallicity
• Cosmological Fast Optical Transients with the Zwicky Transient Facility: A Search for Dirty Fireballs
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• The GAPS Programme at TNG XXXIX -- Multiple molecular species in the atmosphere of the warm giant planet WASP-80 b unveiled at high resolution with GIANO-B
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• Swift J1727.8-1613 has the Largest Resolved Continuous Jet Ever Seen in an X-ray Binary
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• A Seven-Day Multi-Wavelength Flare Campaign on AU Mic I: High-Time Resolution Light Curves and the Thermal Empirical Neupert Effect
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• Accurate characterization of the stochastic gravitational-wave background with pulsar timing arrays by likelihood reweighting
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• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• ALMA-IMF II -- investigating the origin of stellar masses: Continuum Images and Data Processing
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• Unveiling the merger structure of black hole binaries in generic planar orbits
• Revisiting steady viscous flow of a generalized Newtonian fluid through a slender elastic tube using shell theory
• The star formation history of Eridanus II: on the role of SNe feedback in the quenching of ultra-faint dwarf galaxies
• Predictions of the LSST Solar System Yield: Near-Earth Objects, Main Belt Asteroids, Jupiter Trojans, and Trans-Neptunian Objects
• Constraining the AGN duty cycle in the cool-core cluster MS 0735.6+7421 with LOFAR data
• TOI-1278 B: SPIRou unveils a rare Brown Dwarf Companion in Close-In Orbit around an M dwarf
• Hybrid and Automated Machine Learning Approaches for Oil Fields Development: the Case Study of Volve Field, North Sea
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• The impact of spurious collisional heating on the morphological evolution of simulated galactic discs
• RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales
• Calibrations of the Compton Spectrometer and Imager
• The Cosmic Ultraviolet Baryon Survey (CUBS) V: On the Thermodynamic Properties of the Cool Circumgalactic Medium at $z<1$
• Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
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• Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties
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• The ALPINE-ALMA [C II] Survey: [C II]158micron Emission Line Luminosity Functions at $z\sim 4-6$
• Measuring the properties of active galactic nuclei disks with gravitational waves
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• Quantifying the effect of gate errors on variational quantum eigensolvers for quantum chemistry
• The Simons Observatory: gain, bandpass and polarization-angle calibration requirements for B-mode searches
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
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• Detection of Complex Organic Molecules in Young Starless Core L1521E
• A Comparative Analysis of the Chemical Compositions of Gaia-Enceladus/Sausage and Milky Way Satellites using APOGEE
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets
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• Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
• The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z~2.9-4.4
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• The Gaia EDR3 view of Johnson-Kron-Cousins standard stars: the curated Landolt and Stetson collections
• A Synoptic VLBI Technique for Localizing Non-Repeating Fast Radio Bursts with CHIME/FRB
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• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• Multi-phase outflows in high redshift quasar host galaxies
• The star cluster age function in the Galactic disc with Gaia DR2: Fewer old clusters and a low cluster formation efficiency
• Metallicity Distribution Functions of 13 Ultra-Faint Dwarf Galaxy Candidates from Hubble Space Telescope Narrowband Imaging
• Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts
• Deep Synoptic Array science: A massive elliptical host among two galaxy-cluster fast radio bursts
• Quantum approximate optimization algorithm for qudit systems
• Theory-agnostic Reconstruction of Potential and Couplings from Quasi-Normal Modes
• 97 Eclipsing Quadruple Star Candidates Discovered in TESS Full Frame Images
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
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• On the Correlation between Hot Jupiters and Stellar Clustering: High-eccentricity Migration Induced by Stellar Flybys
• Resolving the Complex Evolution of a Supermassive Black Hole Triplet in a Cosmological Simulation
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• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Photometric Redshifts from SDSS Images with an Interpretable Deep Capsule Network
• Still Brighter than Pre-Explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart
• Disorder-Induced Quantum Phase Transitions in Three-Dimensional Second-Order Topological Insulators
• Identifying RR Lyrae Variable Stars in Six Years of the Dark Energy Survey
• Can a Single Population Account for the Discriminant Properties in Fast Radio Bursts?
• Discovery of the Magellanic Stellar Stream Out to 100 Kiloparsecs
• Constraining early dark energy with gravitational waves before recombination
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map
• Galaxy and Mass Assembly (GAMA): Demonstrating the power of WISE in the study of Galaxy Groups to $z<0.1$
• Solving optimization problems with Rydberg analog quantum computers: Realistic requirements for quantum advantage using noisy simulation and classical benchmarks
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• Self-Consistent Spin, Tidal and Dynamical Equations of Motion in the REBOUNDx Framework
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• Constraining galaxy overdensities around three z~6.5 quasars with ALMA and MUSE
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• Statistical Study of the Star Formation Efficiency in Bars: Is Star Formation Suppressed in Gas-Rich Bars?
• Clinical Melanoma Diagnosis with Artificial Intelligence: Insights from a Prospective Multicenter Study
• LoTSS Jellyfish Galaxies IV: Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949
• Stellar Obliquities in Long-period Exoplanet Systems (SOLES) I: The Spin-Orbit Alignment of K2-140 b
• Impact of extreme spins and mass ratios on the post-merger observables of high-mass binary neutron stars
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• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
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• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
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• The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
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• The Astrophysical Distance Scale III: Distance to the Local Group Galaxy WLM using Multi-Wavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars
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• The photometric variability of massive stars due to gravity waves excited by core convection
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• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
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• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
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• Hyper Suprime-Cam Low Surface Brightness Galaxies II: A Hubble Space Telescope Study of the Globular Cluster Systems of Ultra-Diffuse Galaxies in Groups
• oMEGACat I: MUSE spectroscopy of 300,000 stars within the half-light radius of $\omega$ Centauri
• The K2 Galactic Archaeology Program Data Release 2: Asteroseismic results from campaigns 4, 6, & 7
• Detection of Intracluster Globular Clusters in the First JWST Images of the Gravitational Lens Cluster SMACS J0723.3-7327 at z = 0.39
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• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• A comprehensive search for the radio counterpart of GW190814 with the Australian Square Kilometre Array Pathfinder
• Hybrid physics-informed metabolic cybergenetics: process rates augmented with machine-learning surrogates informed by flux balance analysis
• Finding flares in Kepler and TESS data with recurrent deep neural networks
• High-Resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b
• Radio$-\gamma -$ray response in blazars as a signature of adiabatic blob expansion
• The State of Fortran
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• A Catalog of Interplanetary Coronal Mass Ejections Observed by Juno between 1 and 5.4 AU
• Multiband Detection of Repeating FRB 20180916B
• Estimating gate-set properties from random sequences
• Deep Learning the Functional Renormalization Group
• Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy
• Neutron-Induced, Single-Event Effects on Neuromorphic Event-based Vision Sensor: A First Step Towards Space Applications
• SplitStrains, a tool to identify and separate mixed Mycobacterium tuberculosis infections from WGS data
• Stochastic optimal well control in subsurface reservoirs using reinforcement learning
• Glitch systematics on the observation of massive black-hole binaries with LISA
• Machine learning detects multiplicity of the first stars in stellar archaeology data
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Polarization-Resolved Extreme Ultraviolet Second Harmonic Generation from LiNbO${}_3$
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• Follow-up of astrophysical transients in real time with the IceCube Neutrino Observatory
• Spectral Variability of Radio Sources at Low Frequencies
• Stellar Spins in the Open Cluster NGC 2516
• Ionized Outflows in Nearby Quasars are Poorly Coupled to their Host Galaxies
• Measuring black hole masses from tidal disruption events and testing the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ relation
• Predicting fluid-structure interaction with graph neural networks
• A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gas
• Are pulsar halos rare ?
• Modeling electronic response properties with an explicit-electron machine learning potential
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• Model exploration in gravitational-wave astronomy with the maximum population likelihood
• Instantaneous physics-based ground motion maps using reduced-order modeling
• The Kiloparsec-scale Neutral Atomic Carbon Outflow in the Nearby Type-2 Seyfert Galaxy NGC 1068: Evidence for Negative AGN Feedback
• A quantitative assessment of the VO line list: Inaccuracies hamper high-resolution VO detections in exoplanet atmospheres
• The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds
• Global 21-cm signal extraction from foreground and instrumental effects IV: Accounting for realistic instrument uncertainties and their overlap with foreground and signal models
• Magnetic Field Prediction Using Generative Adversarial Networks
• $\text{TESS}$ Giants Transiting Giants I: A Non-inflated Hot Jupiter Orbiting a Massive Subgiant
• Neutral vs Ion Linewidths in Barnard 5: Evidence for Penetration by MHD Waves
• Disturbed, diffuse, or just missing? A global study of the HI content of Hickson Compact Groups
• A topological perspective on weather regimes
• Mapping Local Green Hydrogen Cost-Potentials by a Multidisciplinary Approach
• Bayesian Solar Wind Modeling with Pulsar Timing Arrays
• Probing neutrino interactions and dark radiation with gravitational waves
• Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor ($[Fe/H]\lesssim -3$) Regime
• Strong [OIII]λ5007 emission line compact galaxies in LAMOST DR9: Blueberries, Green Peas and Purple Grapes
• Decoupling the rotation of stars and gas -- II: the link between black hole activity and MaNGA kinematics in TNG
• Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
• Error Bounds for Variational Quantum Time Evolution
• Local Integrals of Motion in Quasiperiodic Many-Body Localized Systems
• Cool circumgalactic gas in galaxy clusters: connecting the DESI legacy imaging survey and SDSS DR16 MgII absorbers
• Constraining spontaneous black hole scalarization in scalar-tensor-Gauss-Bonnet theories with current gravitational-wave data
• The Cosmic Ultraviolet Baryon Survey (CUBS) VI: Connecting Physical Properties of the Cool Circumgalactic Medium to Galaxies at $z\approx 1$
• Ordered magnetic fields around the 3C 84 central black hole
• Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS
• Dark photon dark matter from an oscillating dilaton
• A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
• Towards a population synthesis of discs and planets. II. Confronting disc models and observations at the population level
• Detection of Spectral Variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
• Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
• TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems
• FlashSyn: Flash Loan Attack Synthesis via Counter Example Driven Approximation
• Bayesian Hierarchical Probabilistic Forecasting of Intraday Electricity Prices
• Quantum Circuits for partial differential equations via Schrödingerisation
• Structure, Kinematics, and Observability of the Large Magellanic Cloud's Dynamical Friction Wake in Cold vs. Fuzzy Dark Matter
• The Dark Energy Survey Supernova Program: Cosmological biases from supernova photometric classification
• Weighing the Galactic disk using phase-space spirals I. Tests on one-dimensional simulations
• Inference of the neutron star equation of state from cosmological distances
• Revisit the periodicity of SGR J1935+2154 bursts with updated sample
• Inception Neural Network for Complete Intersection Calabi-Yau 3-folds
• Machine learning-based sampling of virtual experiments within the full stress state
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• $\text{Hi-COLA}$: Fast, approximate simulations of structure formation in Horndeski gravity
• Atomic forces by quantum Monte Carlo: application to phonon dispersion calculation
• Ultimate fate of apparent horizons during a binary black hole merger II: Horizons weaving back and forth in time
• Limit on Supernova Emission in the Brightest Gamma-ray Burst, GRB 221009A
• The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
• Hidden Worlds: Dynamical Architecture Predictions of Undetected Planets in Multi-planet Systems and Applications to TESS Systems
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• The stable climate of KELT-9b
• Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
• Mira variables in the Milky Way's nuclear stellar disc: discovery and classification
• Interior dynamics of super-Earth 55 Cancri e
• Constraining ultralight bosonic dark matter with Keck observations of S2's orbit and kinematics
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• A Coupled Analysis of Atmospheric Mass Loss and Tidal Evolution in XUV Irradiated Exoplanets: the TRAPPIST-1 Case Study
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Electromagnetic Properties of Indium Isotopes Elucidate the Doubly Magic Character of ${}^{100}$Sn
• Exploring Gender and Race Biases in the NFT Market
• AT 2021loi: A Bowen Fluorescence Flare with a Rebrightening Episode, Occurring in a Previously-Known AGN
• Matching Globular Cluster Models to Observations
• Estimation of the electric field in atom probe tomography experiments using charge state ratios
• Exploring Differential Geometry in Neural Implicits
• Substructures in Compact Disks of the Taurus Star-forming Region
• Fraction of Clumpy Star-Forming Galaxies at $0.5\le z\le 3$ in UVCANDELS: Dependence on Stellar Mass and Environment
• candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood
• Application of a hierarchical MCMC follow-up to Advanced LIGO continuous gravitational-wave candidates
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Predicting molecular vibronic spectra using time-domain analog quantum simulation
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• HST strong-lensing model for the first JWST galaxy cluster SMACS J0723.3-7327
• A lack of constraints on the cold opaque HI mass: HI spectra in M31 and M33 prefer multi-component models over a single cold opaque component
• Causality indices for bivariate time series data: a comparative review of performance
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• How Analytic Choices Can Affect the Extraction of Electromagnetic Form Factors from Elastic Electron Scattering Cross Section Data
• Modeling HI at the field level
• More Evidence for Variable Helium Absorption from HD 189733b
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• Improved Mixed Dark Matter Halo Model for Ultralight Axions
• Modeling the kinematics of globular cluster systems
• Inferring the properties of the sources of reionization using the morphological spectra of the ionized regions
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• Fitting infrared ice spectra with genetic modelling algorithms. Presenting the ENIIGMA fitting tool
• A multiband study and exploration of the radio wave - $\gamma$-ray connection in 3C 84
• TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M dwarf host
• Studies of RR Lyrae Variables in Binary Systems. I.: Evidence of a Trimodal Companion Mass Distribution
• Your: Your Unified Reader
• NOEMA High Fidelity Imaging of the Molecular Gas in and around M82
• Precise Dynamical Masses of Epsilon Indi Ba and Bb: Evidence of Slowed Cooling at the L/T Transition
• A ZTF Look at Optical Variability of Young Stellar Objects in the North America and Pelican Nebulae Complex
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Enhanced Star Formation Efficiency in the Central Regions of Nearby Quasars Hosts
• The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets
• On the evolution of the Anisotropic Scaling of Magnetohydrodynamic Turbulence in the Inner Heliosphere
• Relativistic Digital Twin: Bringing the IoT to the Future
• Comparing Three Generations of D-Wave Quantum Annealers for Minor Embedded Combinatorial Optimization Problems
• Gaussian Process Modeling Blazar Multiwavelength Variability: Indirectly Resolving Jet Structure
• Blazhko effect in the Galactic bulge fundamental mode RR Lyrae stars II: Modulation shapes, amplitudes and periods
• The HETDEX Survey: Emission Line Exploration and Source Classification
• Limits on the flux of nuclearites and other heavy compact objects from the "Pi of the Sky" project
• SUPPNet: Neural network for stellar spectrum normalisation
• Red Supergiants in M31: The Humphreys-Davidson limit at high metallicity
• Population synthesis of pulsar wind nebulae and pulsar halos in the Milky Way -- Predicted contributions to the very-high-energy sky
• Higher-Curvature Corrections and Tensor Modes
• Continuity Equation for the Flow of Fisher Information in Wave Scattering
• Sodium Brightening of (3200) Phaethon Near Perihelion
• CO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
• Examining the Decline in the C IV Content of the Universe over 4.3 < z < 6.3 using the E-XQR-30 Sample
• TimeSOAP: Tracking high-dimensional fluctuations in complex molecular systems via time-variations of SOAP spectra
• Hunting for C-rich long-period variable stars in the Milky Way's bar-bulge using unsupervised classification of Gaia BP/RP spectra
• The stellar halo in Local Group Hestia simulations II. The accreted component
• Weighing the Galactic disk using phase-space spirals III. Probing distant regions of the disk using the Gaia EDR3 proper motion sample
• MWC 656 is unlikely to contain a black hole
• The Power of Halometry
• Source Confusion from Neutron Star Binaries in Ground-Based Gravitational Wave Detectors is Minimal
• Variability and Spectral Characteristics of Three Flaring Gamma-ray Quasars Observed by VERITAS and Fermi-LAT
• The JWST/NIRISS Deep Spectroscopic Survey for Young Brown Dwarfs and Free-Floating Planets
• Prior-Informed AGN-Host Spectral Decomposition Using PyQSOFit
• Robust Low-Cost Drone Detection and Classification in Low SNR Environments
• No evidence for a significant evolution of $M_{\bullet }$-$M_{\ast }$ relation in massive galaxies up to z$\sim$4
• TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host
• Griffiths-McCoy singularity on the diluted Chimera graph: Monte Carlo simulations and experiments on the quantum hardware
• Imprint of planet formation in the deep interior of the Sun
• Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c
• Beam model of Doppler backscattering
• Nested sampling cross-checks using order statistics
• Prospects for distinguishing galaxy evolution models with surveys at redshifts $z\gtrsim 4$
• Photometric Classification of 2315 Pan-STARRS1 Supernovae with Superphot
• Symplectic integration of learned Hamiltonian systems
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• Whistler instability driven by the sunward electron deficit in the solar wind
• Non-LTE inversions of a confined X2.2 flare: I. Vector magnetic field in the photosphere and chromosphere
• Dispu$\tau$able: the high cost of a low optical depth
• WASP-117 b: an eccentric hot-Saturn as a future complex chemistry laboratory
• Earths in Other Solar Systems N-body simulations: the Role of Orbital Damping in Reproducing the Kepler Planetary Systems
• Simulating the infrared sky with a Spritz
• New Evidence for Extended HeII Reionization at z>3.5 from HeII Lyman Alpha and Beta Transmission Spikes
• Common envelope binary interaction simulations between a thermally-pulsating AGB star and a low mass companion
• Characterizing the Multi-Phase Origin of [CII] Emission in M101 and NGC 6946 with Velocity Resolved Spectroscopy
• Bekenstein-Hod Universal Bound on Information Emission Rate Is Obeyed by LIGO-Virgo Binary Black Hole Remnants
• 3D mapping of the Crab Nebula with SITELLE. I. Deconvolution and kinematic reconstruction
• The relationship between age, metallicity, and abundances for disk stars in a simulated Milky Way galaxy
• Theory of rheology and aging of protein condensates
• Bioverse: The Habitable Zone Inner Edge Discontinuity as an Imprint of Runaway Greenhouse Climates on Exoplanet Demographics
• Panspermia in a Milky Way-like Galaxy
• First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud
• StarcNet: Machine Learning for Star Cluster Identification
• Fortifying gravitational-wave tests of general relativity against astrophysical assumptions
• Deep learning with photosensor timing information as a background rejection method for the Cherenkov Telescope Array
• Perfect density models cannot guarantee anomaly detection
• A sub-solar metallicity on the ultra-short period planet HIP 65Ab
• An improved Compton parameter map of thermal Sunyaev-Zeldovich effect from Planck PR4 data
• Beamed emission from a neutron-star ULX in a GRRMHD simulation
• The Ionizing Spectra of Extremely Metal-Poor O Stars: Constraints from the Only HII Region in Leo P
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• Variable star classification across the Galactic bulge and disc with the VISTA Variables in the Vía Láctea survey
• A Deep Chandra X-ray Observatory Study of the Millisecond Pulsar Population in the Globular Cluster Terzan 5
• SN 2022acko: the First Early Far-Ultraviolet Spectra of a Type IIP Supernova
• Manifold learning with arbitrary norms
• Modelling Continuum Reverberation in AGN: A Spectral-Timing Analysis of the UV Variability Through X-ray Reverberation in Fairall 9
• Approaches to Constrained Quantum Approximate Optimization
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Polydisperse Streaming Instability II. Methods for solving the linear stability problem
• Distributional Modeling and Forecasting of Natural Gas Prices
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Lithologic Controls on Silicate Weathering Regimes of Temperate Planets
• Investigating the asymmetric chemistry in the disk around the young star HD 142527
• Empirically estimating the distribution of the loudest candidate from a gravitational-wave search
• Magnetised Winds in Transition Discs I: 2.5D Global Simulations
• TESS Data for Asteroseismology: Light Curve Systematics Correction
• Two decades of optical timing of the shortest-period binary star system HM Cancri
• Floquet Engineering Ultracold Polar Molecules to Simulate Topological Insulators
• Convective Mixing in Gas Giant Planets with Primordial Composition Gradients
• A statistical inference approach to time-delay interferometry for gravitational-wave detection
• Modelling the cosmological Lyman-Werner background radiation field in the Early Universe
• Separatrix Divergence of Stellar Streams in Galactic Potentials
• HMCLab: a framework for solving diverse geophysical inverse problems using the Hamiltonian Monte Carlo method
• J0107a: A Barred Spiral Dusty Star-forming Galaxy at $z=2.467$
• High-resolution emission spectroscopy retrievals of MASCARA-1b with CRIRES+: Strong detections of CO, H${}_2$O and Fe emission lines and a C$/$O consistent with solar
• Addressing the challenges of detecting time-overlapping compact binary coalescences
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• Planets larger than Neptune have elevated eccentricities
• Single-shot MHz velocity-map-imaging using two Timepix3 cameras
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• Primordial Black Holes from Axion Domain Wall Collapse
• SLITronomy: towards a fully wavelet-based strong lensing inversion technique
• Search for lithium-rich giants in 32 open clusters with high-resolution spectroscopy
• The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way
• GASTON: Galactic Star Formation with NIKA2. Evidence for the mass growth of star-forming clumps
• Synthetic RGB photometry of bright stars: definition of the standard photometric system and UCM library of spectrophotometric spectra
• Secular chaos in white-dwarf planetary systems: origins of metal pollution and short-period planetary companions
• Noncollinear electric dipoles in a polar, chiral phase of CsSnBr${}_3$ perovskite
• Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
• The interaction of Type Iax supernova ejecta with a helium companion star
• A Practical Probabilistic Benchmark for AI Weather Models
• Directly imaged exoplanets in reflected starlight. The importance of knowing the planet radius
• Quantum-Selected Configuration Interaction: classical diagonalization of Hamiltonians in subspaces selected by quantum computers
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• Localizing FRBs through VLBI with the Algonquin Radio Observatory 10-m Telescope
• Observed polarized scattered light phase functions of planet-forming disks
• IGM Transmission Bias for $z$ $\ge$ 2.9 Lyman Continuum Detected Galaxies
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Accurate Identification of Galaxy Mergers with Stellar Kinematics
• Constructing high-fidelity halo merger trees in AbacusSummit
• Matter ejections behind the highs and lows of the transitional millisecond pulsar PSR J1023+0038
• Investigating Gravitational Collapse of a Pebble Cloud to form Transneptunian Binaries
• The Stars Kepler Missed: Investigating the Kepler Target Selection Function Using Gaia DR2
• VERTICO IV: Environmental Effects on the Gas Distribution and Star Formation Efficiency of Virgo Cluster Spirals
• Tracing Accretion onto Herbig Ae/Be Stars Using the Brγ Line
• The ALMA-CRISTAL Survey: Spatial extent of [CII] line emission in star-forming galaxies at $z=4-6$
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• Mapping the merging zone of late infall in the AB Aur planet-forming system
• The Giant Metrewave Radio Telescope Cold-HI AT $z\approx 1$ Survey
• An Updated Formalism For Line-Driven Radiative Acceleration and Implications for Stellar Mass Loss
• Empirical constraints on the turbulence in QSO host nebulae from velocity structure function measurements
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• The impact of cosmic-ray attenuation on the carbon cycle emission in molecular clouds
• Dark and luminous mass components of Omega Centauri with stellar kinematics
• Role of magma oceans in controlling carbon and oxygen of sub-Neptune atmospheres
• Flexible mapping of ringdown amplitudes for nonprecessing binary black holes
• The NANOGrav 12.5-Year Data Set: Monitoring Interstellar Scattering Delays
• Observable gravitational waves from tidal disruption events and their electromagnetic counterpart
• Contrasting random and learned features in deep Bayesian linear regression
• Compressing the cosmological information in one-dimensional correlations of the Lyman-$\alpha$ forest
• Dynamical phase transitions in the nonreciprocal Ising model
• Discovery and modelling of broad-scale plasma lensing in black-widow pulsar J2051$-$0827
• Pair correlation of dilute Active Brownian Particles: from low activity dipolar correction to high activity algebraic depletion wings
• Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• A Quick Look at the 3GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey
• A CO isotopologue Line Atlas within the Whirlpool galaxy Survey (CLAWS)
• Correcting Stellar Flare Frequency Distributions Detected by TESS and Kepler
• Physics-informed neural networks for understanding shear migration of particles in viscous flow
• WorkflowHub: Community Framework for Enabling Scientific Workflow Research and Development -- Technical Report
• Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium
• A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Where are the magnetar binary companions? Candidates from a comparison with binary population synthesis predictions
• Wigner negativity in the steady-state output of a Kerr parametric oscillator
• Light Fields during Inflation from BOSS and Future Galaxy Surveys
• Rapid search for massive black hole binary coalescences using deep learning
• Automatic Differentiation for the Direct Minimization Approach to the Hartree-Fock Method
• Exploring the differences of integrated and spatially resolved analysis using integral field unit data: The case of Abell 14
• Multimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M${}_{\odot }$
• Radio Measurements of the Depth of Air-Shower Maximum at the Pierre Auger Observatory
• Redshift evolution of the dark matter haloes shapes
• Local Wind Regime Induced by Giant Linear Dunes: Comparison of ERA5-Land Reanalysis with Surface Measurements
• Modeling overcontact binaries, I. The effect of tidal deformation
• Cooling driven coagulation
• The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z=7.31$
• Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
• Swing Amplification and the Gaia Phase Spirals
• Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
• Suppressed heat conductivity in the intracluster medium: implications for the magneto-thermal instability
• Johari-Goldstein $\beta$ relaxation in glassy dynamics originates from two-scale energy landscape
• VETTAM: A scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method
• Hot Rocks Survey II: The thermal emission of TOI-1468 b reveals a hot bare rock
• The ESO SupJup Survey II: The 12C/13C ratios of three young brown dwarfs with CRIRES${}^{+}$
• Hot corino chemistry in the Class I binary source Ser-emb 11
• Constraining interacting dark energy models with the halo concentration-mass relation
• CHILES VERDES: Radio variability at an unprecedented depth and cadence in the COSMOS field
• Extreme Variability Quasars in Their Various States. I: The sample selection and composite SDSS spectra
• Maximum diffusion reinforcement learning
• Framework for analysis of next generation, polarised CMB data sets in the presence of galactic foregrounds and systematic effects
• Open Hardware Solutions in Quantum Technology
• Hidden in the Haystack: Low-luminosity globular clusters towards the Milky Way bulge
• Hot Jupiters, cold kinematics: High phase space densities of host stars reflect an age bias
• Simple and statistically sound recommendations for analysing physical theories
• The GALAH survey: Chemical homogeneity of the Orion complex
• Spectrum of kinetic plasma turbulence at 0.3-0.9 astronomical units from the Sun
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• The oblateness of the Milky Way dark matter halo from the stellar streams of NGC 3201, M68, and Palomar 5
• Simultaneous evidence of edge collapse and hub-filament configurations: A rare case study of a Giant Molecular Filament G45.3+0.1
• Milky Way archaeology using RR Lyrae and type II Cepheids II. High velocity RR Lyrae stars, and mass of the Milky Way
• GPCAL: a generalized calibration pipeline for instrumental polarization in VLBI data
• Euclid: Early Release Observations -- Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field
• BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
• The period-age relation of long-period variables
• Describe, Transform, Machine Learning: Feature Engineering for Grain Boundaries and Other Variable-Sized Atom Clusters
• The TESS View of LOFAR Radio-Emitting Stars
• Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
• Elemental abundances in M31: [Fe/H] and [α/Fe] in M31 Dwarf Galaxies Using Coadded Spectra
• Through the eyes of a descriptor: Constructing complete, invertible descriptions of atomic environments
• Galactic chemical evolution of exoplanet host stars: Are high-mass planetary systems young?
• A Mesoscale Perspective on the Tolman Length
• The KOBE experiment: K-dwarfs Orbited By habitable Exoplanets. Project goals, target selection and stellar characterization
• Direct Formation of Planetary Embryos in Self-Gravitating Disks
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• Probing the angular and polarization reconstruction of the ARIANNA detector at the South Pole
• The expected kinematic matter dipole is robust against source evolution
• Redshift requirements for cosmic shear with intrinsic alignment
• Performance of teleportation-based error correction circuits for bosonic codes with noisy measurements
• Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis
• How Close are Compact Multi-Planet Systems to the Stability Limit?
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• Active region chromospheric magnetic fields
• The post-Herschel view of intrinsic AGN emission: constructing templates for galaxy and AGN emission at IR wavelengths
• A Machine-Learning-Based Direction-of-Origin Filter for the Identification of Radio Frequency Interference in the Search for Technosignatures
• The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?
• Investigating the visible phase-curve variability of 55 Cnc e
• Transportability without positivity: a synthesis of statistical and simulation modeling
• An eccentric Brown Dwarf eclipsing an M dwarf
• Capturing the physics of MaNGA galaxies with self-supervised Machine Learning
• The HST large programme on $\omega$ Centauri -- V. Exploring the Ultracool Dwarf Population with Stellar Atmosphere and Evolutionary Modelling
• From ridges to manifolds: 3D characterization of the moving groups in the Milky Way disc
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• A radio-jet driven outflow in the Seyfert 2 galaxy NGC 2110?
• The Orbital Architecture of Qatar-6: A Fully Aligned 3-Body System?
• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• GASTLI: An open-source coupled interior-atmosphere model to unveil gas giant composition
• DUSTiER (DUST in the Epoch of Reionization): dusty galaxies in cosmological radiation-hydrodynamical simulations of the Epoch of Reionization with RAMSES-CUDATON
• Magnetic Misalignment of Interstellar Dust Filaments
• A Generalized Boltzmann Kinetic Theory for Strongly Magnetized Plasmas with Application to Friction
• Water UV-shielding in the terrestrial planet-forming zone: Implications for carbon dioxide emission
• NEID Rossiter-McLaughlin Measurement of TOI-1268b: A Young Warm Saturn Aligned with Its Cool Host Star
• Weighing the Galactic disk in sub-regions of the solar neighbourhood using Gaia DR2
• ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA
• High-dimensional and Permutation Invariant Anomaly Detection
• TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by TTVs
• Machine-Guided Discovery of a Real-World Rogue Wave Model
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• The Kick Velocity Distribution of Isolated Neutron Stars
• HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
• The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters
• Broad-emission-line dominated hydrogen-rich luminous supernovae
• Solar prominence diagnostics from non-LTE modelling of Mgii h&k line profiles
• Statistical recovery of 21cm visibilities and their power spectra with Gaussian constrained realisations and Gibbs sampling
• On spectroscopic phase-curve retrievals: H2 dissociation and thermal inversion in the atmosphere of the ultra-hot Jupiter WASP-103 b
• PHANGS-JWST First Results: Stellar Feedback-Driven Excitation and Dissociation of Molecular Gas in the Starburst Ring of NGC 1365?
• The extinction law in the inner $3\times 3$ deg${}^2$ of the Milky Way and the red clump absolute magnitude in the inner bar-bulge
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• Dynamical Masses and Stellar Evolutionary Model Predictions of M-Stars
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• TDCOSMO. XVI. Measurement of the Hubble Constant from the Lensed Quasar WGD2038$-$4008
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• The size--mass and other structural parameter ($n,{\mu }_z,R_z$) relations for local bulges/spheroids from multicomponent decompositions
• Electronic noise of warm electrons in semiconductors from first-principles
• Shaping the Milky Way: The interplay of mergers and cosmic filaments
• Growth or Decay -- I: universality of the turbulent dynamo saturation
• On convergence rates of adaptive ensemble Kalman inversion for linear ill-posed problems
• Visual Vibration Tomography: Estimating Interior Material Properties from Monocular Video
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Searching for Anomalies in the ZTF Catalog of Periodic Variable Stars
• Extremely precise age and metallicity of the open cluster NGC 2506 using detached eclipsing binaries
• Relativistic force-free models of the thermal X-ray emission in millisecond pulsars observed by NICER
• Supercell-core software: a useful tool to generate an optimal supercell for vertically stacked nanomaterials
• A tale of two tails: insights from simulations into the formation of the peculiar dwarf galaxy NGC 1427A
• Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey
• Reimagining the water snowline
• Conversions between gas-phase metallicities in MaNGA
• Compensating for non-linear distortions in controlled quantum systems
• Implicit biases in transit models using stellar pseudo-density
• Variability of massive stars in M31 from the Palomar Transient Factory
• Total Energy in Supernova Neutrinos and the Tidal Deformability and Binding Energy of Neutron Stars
• A semi-linear wave model for critical collapse
• The SOPHIE search for northern extrasolar planets. XVIII: Six new cold Jupiters, including one of the most eccentric exoplanet orbits
• Linear matter density perturbations in the ${\Lambda }_{\mathrm{s}}$CDM model: Examining growth dynamics and addressing the $S_8$ tension
• Ultrafast critical ground state preparation via bang-bang protocols
• Ring Formation in Protoplanetary Disks Driven by an Eccentric Instability
• OptiMic: A tool to generate optimized polycrystalline microstructures for materials simulations
• Quantifying Bore-bore Capture on Natural Beaches
• Application of Contour Minkowski Tensor and $\mathcal{D}$ Statistic to the Planck $E$-mode data
• Drivers of asymmetry in synthetic H I emission-line profiles of galaxies in the EAGLE simulation
• Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
• Constraining the Milky Way's Ultraviolet to Infrared SED with Gaussian Process Regression
• The Local Group Symbiotic Star Population and its Tenuous Link with Type Ia Supernovae
• oMEGACat. VI. Analysis of the overall kinematics of Omega Centauri in 3D: velocity dispersion, kinematic distance, anisotropy, and energy equipartition
• Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?
• Towards an understanding of YSO variability: A multi-wavelength analysis of bursting, dipping, and symmetrically varying light curves of disc-bearing YSOs
• Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• A broadband spectral-timing study of QPOs in the bright black hole X-ray binary Swift J1727.8-1613
• Adaptive variational preparation of the Fermi-Hubbard eigenstates
• A novel convergence enhancement method based on Online Dimension Reduction Optimization
• Can the Fe K-alpha Line Reliably Predict Supernova Remnant Progenitors?
• Molecular gas and dust properties in $z>7$ quasar hosts
• New candidates for magnetar counterparts from a deep search with the Hubble Space Telescope
• Precise Measurements of the LMC Bar's Geometry With Gaia DR3 and a Novel Solution to Crowding Induced Incompleteness in Star Counting
• Weighing the Galactic disk using phase-space spirals IV. Tests on a three-dimensional galaxy simulation
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• Cuspy dark matter density profiles in massive dwarf galaxies
• The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS)
• CHANCES, the Chilean Cluster Galaxy Evolution Survey: Selection and initial characterisation of clusters and superclusters
• The GRBSN webtool: An open-source repository for gamma-ray burst-supernova associations
• MAXI and NuSTAR observations of the faint X-ray transient MAXI J1848-015 in the GLIMPSE-C01 Cluster
• Extra-tidal star candidates in globular clusters of the Sagittarius dwarf spheroidal galaxy
• IBIS-A: The IBIS data Archive. High resolution observations of the solar photosphere and chromosphere with contextual data
• Hypercubes of AGN Tori (HYPERCAT) -- II. Resolving the Torus with Extremely Large Telescopes
• A Combined Radio Multi-Survey Catalog of Fermi Unassociated Sources
• ALMA High-resolution Multiband Analysis for the Protoplanetary Disk around TW Hya
• Interpretable Multimodal Machine Learning Analysis of X-ray Absorption Near-Edge Spectra and Pair Distribution Functions
• Optical Rebrightening of Extragalactic Transients from the Zwicky Transient Facility
• The effects of rotation on massive star spectroscopic observables
• CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC
• MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate and metallicity of galaxies
• Carbon-enhanced stars with short orbital and spin periods
• Tri-Resonant Leptogenesis in a Seesaw Extension of the Standard Model
• The fine-scale structure of polar coronal holes
• Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems using Recurrent Inference Machines
• Revisiting the multi-planetary system of the nearby star HD 20794: Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarf
• Is the molecular KS relationship universal down to low metallicities?
• Automated Extended Aperture Photometry of K2 variable stars
• Beyond MP2 initialization for unitary coupled cluster quantum circuits
• GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
• Characterisation of local halo building blocks: Thamnos and Sequoia
• Fast multi-qubit global-entangling gates without individual addressing of trapped ions
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Precision Ephemerides for Gravitational-wave Searches -- IV: Corrected and refined ephemeris for Scorpius X-1
• The Non-Axisymmetric Influence: Radius and Angle-Dependent Trends in a Barred Galaxy
• Metallicity profiles of Ultra Diffuse Galaxies in NIHAO simulations
• HyperSLICE: HyperBand optimized Spiral for Low-latency Interactive Cardiac Examination
• A Quantum Computing Implementation of Nuclear-Electronic Orbital (NEO) Theory: Towards an Exact pre-Born-Oppenheimer Formulation of Molecular Quantum Systems
• Mode Mixing and Rotational Splittings: I. Near-Degeneracy Effects Revisited
• Symmetry-informed transferability of optimal parameters in the Quantum Approximate Optimization Algorithm
• Role of Filamentary Structures in the Formation of Two Dense Cores, L1544 and L694-2
• The origin of star-gas misalignments in simulated galaxies
• Analytical determination of orbital elements using Fourier analysis. II. Gaia astrometry and its combination with radial velocities
• Quenching star formation with low-luminosity AGN winds
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• Kinematic constraints on the ages and kick velocities of Galactic neutron star binaries
• Optimizing performance of quantum operations with non-Markovian decoherence: the tortoise or the hare?
• Biochars at the molecular level. Part 2 -- Development of realistic molecular models of biochars
• The binary system of the spinning-top Be star Achernar
• Resonant Ultrasound Spectroscopy for Irregularly-Shaped Samples and its Application to Uranium Ditelluride
• Modeling X-ray Photoelectron Spectroscopy of Macromolecules Using GW
• A Cross-correlation Study between IceCube Neutrino Events and the Fermi Unresolved Gamma-ray Sky
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• Detector signal characterization with a Bayesian network in XENONnT
• The formation of CO${}_2$ through consumption of gas-phase CO on vacuum-UV irradiated water ice
• Low-Frequency Vibrational States in Ideal Glasses with Random Pinning
• Impact of Surface Adsorbates and Dimensionality on Templating of Halide Perovskites
• QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
• TIC 114936199: A Quadruple Star System with a 12-day Outer Orbit Eclipse
• Effectiveness of quantum annealing for continuous-variable optimization
• Hundreds of TESS exoplanets might be larger than we thought
• Euclid preparation. LIII. LensMC, weak lensing cosmic shear measurement with forward modelling and Markov Chain Monte Carlo sampling
• Towards efficient structure prediction and pre-compensation in multi-photon lithography
• Fingerprints of a Non-Inflationary Universe from Massive Fields
• Chemical abundance of LINER galaxies -- Metallicity calibrations based on SDSS-IV MaNGA
• Satellite group infall into the Milky Way: exploring the Crater-Leo case with new HST proper motions
• Astrocyte control bursting mode of spiking neuron network with memristor-implemented plasticity
• Wavefront tolerances of space-based segmented telescopes at very high contrast: Experimental validation
• Interaction of large- and small-scale dynamos in isotropic turbulent flows from GPU-accelerated simulations
• Polarimetric and radiative transfer modelling of HD 172555
• Likelihood-Based Jump Detection and Cosmic Ray Rejection for Detectors Read Out Up-the-Ramp
• Gas dynamics and star formation in NGC 6822
• Radio Emission from Binary Ultracool Dwarf Systems
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers
• Estimating Atmospheric Parameters from LAMOST Low-Resolution Spectra with Low SNR
• Photometry and Polarimetry of 2010 XC${}_{15}$: Observational Confirmation of E-type Near-Earth Asteroid Pair
• Physically motivated improvements of Variational Quantum Eigensolvers
• GLANCE -- Gravitational Lensing Authenticator using Non-Modelled Cross-Correlation Exploration of Gravitational Wave Signals
• Chemical Cartography with APOGEE: Two-process Parameters and Residual Abundances for 288,789 Stars from Data Release 17
• A Flat-Spectrum Radio Transient at 122 Mpc consistent with an Emerging Pulsar Wind Nebula
• Alignment of dense molecular core morphology and velocity gradients with ambient magnetic fields
• Analyzing the Galactic pulsar distribution with machine learning
• Constraining density and metallicity of the Milky Way's hot gas halo from O VII spectra and ram-pressure stripping
• A multi-layer network approach to modelling authorship influence on citation dynamics in physics journals
• Infrared view of the multiphase ISM in NGC 253 I. Observations and fundamental parameters of the ionised gas
• Our Galaxy's youngest disc
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• Filamentary Dust Polarization and the Morphology of Neutral Hydrogen Structures
• Real-time Dynamics of the Schwinger Model as an Open Quantum System with Neural Density Operators
• Radio Variable and Transient Sources on Minute Timescales in the ASKAP Pilot Surveys
• Temperature-chemistry coupling in the evolution of gas giant atmospheres driven by stellar flares
• TwinBooster: Synergising Large Language Models with Barlow Twins and Gradient Boosting for Enhanced Molecular Property Prediction
• Filling in the Gaps: Can Gravitationally Unstable Discs Form the Seeds of Gas Giant Planets?
• Flaring Stars in a Non-targeted mm-wave Survey with SPT-3G
• Variations of the HCO${}^{+}$, HCN, HNC, N${}_2$H${}^{+}$ and NH${}_3$ deuterium fractionation in high-mass star-forming regions
• Quantum Electrometer for Time-Resolved Material Science at the Atomic Lattice Scale
• Gradient and Uncertainty Enhanced Sequential Sampling for Global Fit
• The Occurrence Rate of Quiescent Radio Emission for Ultracool Dwarfs using a Generalized Semi-Analytical Bayesian Framework
• Resource analysis of quantum algorithms for coarse-grained protein folding models
• The influence of globular cluster evolution on the specific frequency in dwarf galaxies
• Evidence for C and Mg variations in the GD-1 stellar stream
• An Intent-based Framework for Vehicular Edge Computing
• Inference of Probabilistic Programs with Moment-Matching Gaussian Mixtures
• Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
• HDO ice detected toward an isolated low-mass protostar with JWST
• Photometric Signature of Ultra-Harmonic Resonances in Barred Galaxies
• Analytic Light Curve for Mutual Transits of Two Bodies Across a Limb-darkened Star
• Enhanced Astronomical Source Classification with Integration of Attention Mechanisms and Vision Transformers
• A spectroscopically confirmed Gaia-selected sample of 318 new young stars within $\sim$200 pc
• Photometric Classifications of Evolved Massive Stars: Preparing for the Era of Webb and Roman with Machine Learning
• Free-Streaming Neutrinos and Their Phase Shift in Current and Future CMB Power Spectra
• Gravitational Microlensing Time Delays at High Optical Depth: Image Parities and the Temporal Properties of Fast Radio Bursts
• LINX: A Fast, Differentiable, and Extensible Big Bang Nucleosynthesis Package
• Direction Dependent Corrections in Polarimetric Radio Imaging III: A-to-Z Solver -- Modeling the full Jones antenna aperture illumination pattern
• A Search for L4 Earth Trojan Asteroids Using a Novel Track-Before-Detect Multi-Epoch Pipeline
• Driven-dissipative Rydberg blockade in optical lattices
• The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at $\approx$2 AU
• Fast entangling gates for Rydberg atoms via resonant dipole-dipole interaction
• Quasinormal Modes in Modified Gravity using Physics-Informed Neural Networks
• How to find a unicorn: a novel model-free, unsupervised anomaly detection method for time series
• Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite
• The pattern speeds of vertical breathing waves
• AutoPV: Automated photovoltaic forecasts with limited information using an ensemble of pre-trained models
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Near subsonic solar wind outflow from an active region
• Mapping the Thermal Condensation of Diffuse H I in the North Celestial Pole Loop
• Probing the efficiency of tidal synchronization in outspiralling double white dwarf binaries with LISA
• ACCESS: An optical transmission spectrum of the high-gravity, hot Jupiter HAT-P-23b
• Bayesian Optimization of the Beam Injection Process into a Storage Ring
• What's in a binary black hole's mass parameter?
• LISA Constraints on an Intermediate-Mass Black Hole in the Galactic Centre
• Binary fraction of O and B-type stars from LAMOST data
• Detecting gravitational-wave bursts from black hole binaries in the Galactic Center with LISA
• Non-parametric learning critical behavior in Ising partition functions: PCA entropy and intrinsic dimension
• Constraints on dark matter self-interaction from galactic core size
• Inferring Type II-P Supernova Progenitor Masses from Plateau Luminosities
• Cold dark matter protohalo structure around collapse: Lagrangian cosmological perturbation theory versus Vlasov simulations
• Simulation-based inference of black hole ringdowns in the time domain
• Isochronic evolution and the radioactive decay of r-process nuclei
• Emission Line Variability during a Nonthermal Outburst in the Gamma-Ray Bright Quasar 1156+295
• QAOA-MC: Markov chain Monte Carlo enhanced by Quantum Alternating Operator Ansatz
• Metal content of the circumgalactic medium around star-forming galaxies at z $\sim$ 2.6 as revealed by the VIMOS Ultra-Deep Survey
• Interpreting Ultrafast Electron Transfer on Surfaces with a Converged First-Principles Newns-Anderson Chemisorption Function
• Living with Neighbors. III. The Origin of the Spin$-$Orbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
• Distributed YSOs in the Perseus Molecular Cloud from the Gaia and LAMOST Surveys
• Introducing the Texas Euclid Survey for Lyman Alpha (TESLA) Survey: Initial Study Correlating Galaxy Properties to Lyman-Alpha Emission
• De-noising of galaxy optical spectra with autoencoders
• Star formation in IC1396: Kinematics and subcluster structure revealed by Gaia
• Outer Solar System Perihelion Gap Formation Through Interactions with a Hypothetical Distant Giant Planet
• Quantum yield and charge diffusion in the Nancy Grace Roman Space Telescope infrared detectors
• Crystal structure identification with 3D convolutional neural networks with application to high-pressure phase transitions in SiO${}_2$
• Radio-loud fraction of z>6 quasars
• Precision-medicine-toolbox: An open-source python package for facilitation of quantitative medical imaging and radiomics analysis
• The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies
• Time series analysis of bright TESS RRc stars: Additional modes, phase variations and more
• On the origin of the split main sequences of the young massive cluster NGC 1856
• SDSS-IV MaNGA: the chemical co-evolution of gas and stars in spiral galaxies
• Statistical Equivalence of Metrics for Meteor Dynamical Association
• Emulators for Scarce and Noisy Data: Application to Auxiliary-Field Diffusion Monte Carlo for Neutron Matter
• Detections of 21-cm absorption with a blind FAST survey at z $⩽$ 0.09
• Quantum spin liquids of Rydberg excitations in a honeycomb lattice induced by density-dependent Peierls phases
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• The AstraLux-TESS high-spatial resolution imaging survey. Search for stellar companions of 215 planet candidates from TESS
• Variational Quantum Multi-Objective Optimization
• A simple method to measure numax for asteroseismology: application to 16,000 oscillating Kepler red giants
• Mode matching error signals using radio-frequency beam shape modulation
• The Swan: Data-Driven Inference of Stellar Surface Gravities for Cool Stars from Photometric Light Curves
• Survey2Survey: A deep learning generative model approach for cross-survey image mapping
• A multi-wavelength search for intrinsic linear polarization in Wolf-Rayet winds
• Deep learning polarization distributions in ferroelectrics from STEM data: with and without atom finding
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• XLuminA: An Auto-differentiating Discovery Framework for Super-Resolution Microscopy
• LMC-driven anisotropic boosts in stream--subhalo interactions
• Cyclostationary signals in LISA: a practical application to Milky Way satellites
• radioactivedecay: A Python package for radioactive decay calculations
• Gravitational Wave Statistics for Pulsar Timing Arrays: Examining Bias from Using a Finite Number of Pulsars
• Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Plasma lensing near the eclipses of the Black Widow pulsar B1957+20
• Diving into the planetary system of Proxima with NIRPS -- Breaking the metre per second barrier in the infrared
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Detecting high-dimensional entanglement in cold-atom quantum simulators
• 1/f Noise Analysis for FAST HI Intensity Mapping Drift-Scan Experiment
• The variational quantum eigensolver self-consistent field method within a polarizable embedded framework
• Survey for Distant Solar Twins (SDST) -- I. EPIC method for stellar parameter measurement
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Brought to Light I: Quantification of Disk Substructure in Dwarf Early-Type Galaxies
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• A matched-filter approach to radio variability and transients: searching for orphan afterglows in the VAST Pilot Survey
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• Hiding in plain sight: observing planet-starspot crossings with the James Webb Space Telescope
• Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
• Tilted discs in six poorly studied cataclysmic variables
• Significant mutual inclinations between the stellar spin and the orbits of both planets in the HAT-P-11 system
• A Radio Study of Persistent Radio Sources in Nearby Dwarf Galaxies: Implications for Fast Radio Bursts
• Neutron-capture elements in dwarf galaxies III: A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies
• Leveraging Analog Quantum Computing with Neutral Atoms for Solvent Configuration Prediction in Drug Discovery
• The GALAH Survey: No chemical evidence of an extragalactic origin for the Nyx stream
• Efficient Numerical Schemes for Multidimensional Population Balance Models
• Synthetic CO emission and the $X_{\mathrm{CO}}$ factor of young molecular clouds: a convergence study
• JWST Observations of Starbursts: Relations between PAH features and CO clouds in the starburst galaxy M 82
• A hot Mars-sized exoplanet transiting an M dwarf
• Efficient and precise transit light curves for rapidly-rotating, oblate stars
• Post-Newtonian-accurate pulsar timing array signals induced by inspiralling eccentric binaries: accuracy, computational cost, and single-pulsar search
• Molecular simulations matching denaturation experiments for N6-Methyladenosine
• SKYSURF-4: Panchromatic HST All-Sky Surface-Brightness Measurement Methods and Results
• Capturing research literature attitude towards Sustainable Development Goals: an LLM-based topic modeling approach
• Explaining ultra-massive quiescent galaxies at $3<z<5$ in the context of their environments
• Templated Anisotropic Analyses of the LISA Galactic Foreground
• Impact of bar resonances in the velocity-space distribution of the solar neighbourhood stars in a self-consistent $N$-body Galactic disc simulation
• The Chemical Composition of Extreme-Velocity Stars
• A Machine Learning approach to enhance the SUPG stabilization method for advection-dominated differential problems
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Mesoscopic transport signatures of disorder-induced non-Hermitian phases
• WIYN Open Cluster Study. XC. Radial-velocity Measurements and Spectroscopic Binary Orbits in the Open Cluster NGC 2506
• Primordial acoustic turbulence: three-dimensional simulations and gravitational wave predictions
• New technique for determining a pulsar period: Waterfall principal component analysis
• Faint Stars in a Faint Galaxy: II. The Low Mass Stellar Initial Mass Function of the Boötes I Ultrafaint Dwarf Spheroidal Galaxy
• A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images
• Spin-filtered measurements of Andreev bound states
• Measured Spin-Orbit Alignment of Ultra-Short Period Super-Earth 55 Cancri e
• Bayesian fitting of multi-Gaussian expansion models to galaxy images
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Integer Quantum Hall Effect: Disorder, temperature, floating, and plateau width
• M Subdwarf Research. II. Atmospheric Parameters and Kinematics
• Initial analysis of the impact of the Ukrainian power grid synchronization with Continental Europe
• Wide binaries from the H3 survey: the thick disk and halo have similar wide binary fractions
• On effects of surface bipolar magnetic regions on the convection zone dynamo
• The Simons Observatory: Characterizing the Large Aperture Telescope Receiver with Radio Holography
• Towards a complete picture of the Sco-Cen outflow
• IGRINS observations of WASP-127 b: H${}_2$O, CO, and super-Solar atmospheric metallicity in the inflated sub-Saturn
• A compartmental model for Xylella fastidiosa diseases with explicit vector seasonal dynamics
• Evolution of solar wind sources and coronal rotation driven by the cyclic variation of the Sun's large-scale magnetic field
• SUREL+: Moving from Walks to Sets for Scalable Subgraph-based Graph Representation Learning
• Confirmation and characterisation of three giant planets detected by TESS from the FIES/NOT and Tull/McDonald spectrographs
• The imprint of X-ray photoevaporation of planet-forming discs on the orbital distribution of giant planets -- II. Theoretical predictions
• Astrometry in crowded fields towards the Galactic Bulge
• Exploring the Observability of Surviving Companions of Stripped-Envelope Supernovae: A Case Study of Type Ic SN 2020oi
• The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
• Getting More Out of Black Hole Superradiance: a Statistically Rigorous Approach to Ultralight Boson Constraints from Black Hole Spin Measurements
• Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
• A dichotomy in group II Herbig disks: ALMA gas disk height measurements show both shadowed large vertically extended disks and compact flat disks
• The cooler past of the intracluster medium in TNG-Cluster
• 183 GHz water megamasers in active galactic nuclei: a new accretion disk tracer
• Towards chemical accuracy with shallow quantum circuits: A Clifford-based Hamiltonian engineering approach
• Estimating uncertainties in the back-mapping of the fast solar wind
• A Dynamical Systems Approach to the Theory of Circumbinary Orbits in the Circular Restricted Problem
• Wide binaries demonstrate the consistency of rotational evolution between open cluster and field stars
• A Reputation Game Simulation: Emergent Social Phenomena from Information Theory
• Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches
• Determining star formation rates of active galactic nuclei host galaxies based on SED fitting with sub-mm data
• Rapid binary mass transfer: Circumbinary outflows and angular momentum losses
• The stochastic nature of power-grid frequency in South Africa
• RV-exoplanet eccentricities: Good, Beta, and Best
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Feeding plankton to whales: high-redshift supermassive black holes from tiny black hole explosions
• Kinematics and Metallicity of Red Giant Branch Stars in the Northeast Shelf of M31
• The Solar System Notification Alert Processing System (SNAPS): Design, Architecture, and First Data Release (SNAPShot1)
• Benchmarking Noisy Intermediate Scale Quantum Error Mitigation Strategies for Ground State Preparation of the HCl Molecule
• Excited-state molecular dynamics simulation based on variational quantum algorithms
• Light bending by the cosmological constant
• Star Formation Variability as a Probe for the Baryon Cycle within Galaxies
• AGEL: Is the Conflict Real? Investigating Galaxy Evolution Models using Strong Lensing at 0.3 < z < 0.9
• The unusual M-dwarf Warm Jupiter TOI-1899~b: Refinement of orbital and planetary parameters
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Period-Luminosity Relations for Galactic classical Cepheids in the Sloan bands
• The Massive and Distant Clusters of WISE Survey IX: High Radio Activity in a Merging Cluster
• Measurement of Magnetic Susceptibility of Diamagnetic Liquids Exploiting the Moses Effect
• Fast neutrino cooling in the accreting neutron star MXB 1659-29
• Unsupervised KPIs-Based Clustering of Jobs in HPC Data Centers
• JWST-TST DREAMS: Non-Uniform Dayside Emission for WASP-17b from MIRI/LRS
• Wertheim's thermodynamic perturbation theory with double-bond association and its application to colloid-linker mixtures
• Transfer of 0-order coherence matrix along spin-1/2 chain
• Abundance and properties of dark radiation from the cosmic microwave background
• X-ray burst ignition location on the surface of accreting X-ray pulsars: Can bursts preferentially ignite at the hotspot?
• Diagnostic diagrams for ram-pressure stripped candidates
• Sky marginalization in black hole spectroscopy and tests of the area theorem
• Revealing the Nature of a Lyman-$\alpha$ Halo in a Strongly Lensed Interacting System at $z=2.92$
• Coordinated JWST Imaging of Three Distance Indicators in a SN Host Galaxy and an Estimate of the TRGB Color Dependence
• A unified Green's function approach for spectral and thermodynamic properties from algorithmic inversion of dynamical potentials
• Spatially resolved Lyman-$\alpha$ emission around radio bright quasars
• Fast Correlation Function Calculator -- A high-performance pair counting toolkit
• Model-Independent Mass Reconstruction of the Hubble Frontier Field Clusters with MARS Based on Self-Consistent Strong Lensing Data
• Terahertz Magneto-optical investigation of quadrupolar spin-lattice effects in magnetically frustrated Tb2Ti2O7
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Constraints on the X-ray Luminosity Function of AGN at z=5.7-6.4 with the Extragalactic Serendipitous Swift Survey
• Distinguishing Time Clustering of Astrophysical Bursts
• A Gaussian process approach for rapid evaluation of skin tension
• Dust in High-Redshift Galaxies: Reconciling UV Attenuation and IR Emission
• An Optical Spectrum of the Diffuse Galactic Light from BOSS and IRIS
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• The X-ray spectral-timing contribution of the stellar wind in the hard state of Cyg X-1
• Inferring the progenitor mass-kinetic energy relation of stripped-envelope core-collapse supernovae from nebular spectroscopy
• TIC 219006972: A Compact, Coplanar Quadruple Star System Consisting of Two Eclipsing Binaries with an Outer Period of 168 days
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• RHINO: A large horn antenna for detecting the 21cm global signal
• Identifying 850 delta Scuti pulsators in a narrow Gaia colour range with TESS 10-minute full-frame images
• ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Nested Morphological and Kinematic Structures of Outflows Revealed in SiO and CO Emission
• Influence of neutrino-electron scattering and neutrino-pair annihilation on hypermassive neutron star
• Estimating the Feasibility of 21cm-Ly$\alpha$ Synergies using the Hydrogen Epoch of Reionization Array
• Testing velocity kinks as a planet-detection method: Do velocity kinks in surface gas emission trace planetary spiral wakes in the midplane continuum?
• Morphologies of galaxies within voids
• A segmented period-luminosity relation for nearby extragalactic $\delta$ Scuti stars
• The unusual 3D distribution of NaCl around the AGB star IK Tau
• Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim 9-17$
• Extremely Buried Nucleus of IRAS 17208$-$0014 Observed at Sub-Millimeter and Near-Infrared Wavelengths
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM
• Weak-lensing Mass Reconstruction of Galaxy Clusters with Convolutional Neural Network
• Force Fields for Deep Eutectic Mixtures: Application to Structure and 2D-Infrared Spectroscopy
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• Apocalypse When? No Certainty of a Milky Way -- Andromeda Collision
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• Science Using Single-Pulse Exploration with Combined Telescopes. I. The mode switching, flaring, and single-pulse morphology of PSR B1822-09
• Improving Binary Millisecond Pulsar Distances with Gaia
• Leptogenesis and low-energy CP violation in a type-II-dominated left-right seesaw model
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• exoALMA. VIII. Probabilistic Moment Maps and Data Products using Non-parametric Linear Models
• Ab initio electron-lattice downfolding: potential energy landscapes, anharmonicity, and molecular dynamics in charge density wave materials
• Interlacing in atomic resolution scanning transmission electron microscopy
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• Zwicky Transient Facility and Globular Clusters: the Period-Luminosity and Period-Luminosity-Color Relations for Late-Type Contact Binaries
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• A Generative Model for Quasar Spectra
• Time-Frequency Phase Retrieval for Audio -- The Effect of Transform Parameters
• Revising Properties of Planet-host Binary Systems I.: Methods and Pilot Study
• Spectral and angular differential imaging with SPHERE/IFS. Assessing the performance of various PCA-based approaches to PSF subtraction
• MOJAVE XXI. Decade-long linear polarization variability in AGN jets at parsec scales
• Angle-dependent in-situ fast flavor transformations in post-neutron star merger disks
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• Analytical formulation of the second-order derivative of energy for orbital-optimized variational quantum eigensolver: application to polarizability
• Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample
• Barium stars as tracers of s-process nucleosynthesis in AGB stars III. Systematic deviations from the AGB models
• SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1$-$1148 at $z\sim 0.5$
• High-Order harmonics of Thermal Tides observed in the atmosphere of Mars by the Pressure Sensor on the Insight lander
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• Mapping circumstellar magnetic fields of late-type evolved stars with the Goldreich-Kylafis effect: CARMA observations at $\lambda 1.3$ mm of R Crt and R Leo
• Four new PLanetesimals Around TYpical and Pre-main seqUence Stars (PLATYPUS) Debris Discs at 8.8mm
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• The relation between globular cluster systems and supermassive black holes in spiral galaxies III. The link to the $M_{\bullet }-M_{\ast }$ correlation
• Measuring the Cosmic X-ray Background in 3-20keV with Straylight from NuSTAR
• RJ-plots: An improved method to classify structures objectively
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• Limitations and biases in the retrieval of the polar magnetic field I: the role of the magnetic filling factor in Milne-Eddington inversions of simulated Hinode/SP data
• Measurement of proton light yield of water-based liquid scintillator
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• A multishock scenario for the formation of radio relics
• The BlueTides Mock Image Catalogue: Simulated observations of high-redshift galaxies and predictions for JWST imaging surveys
• Resolving the Vicinity of Supermassive Black Holes with Gravitational Microlensing
• $4-8\mathrm{GHz}$ Spectro-temporal Emission from the Galactic Center Magnetar $\mathrm{PSR}J1745-2900$
• Measurements of multijet event isotropies using optimal transport with the ATLAS detector
• Improving Distances to Binary Millisecond Pulsars with Gaia
• Additional JWST/NIRSpec Transits of the Rocky M Dwarf Exoplanet GJ 1132 b Reveal a Featureless Spectrum
• The Extremely Metal-Poor SN 2023ufx: A Local Analog to High-Redshift Type II Supernovae
• End-to-End Reinforcement Learning of Koopman Models for Economic Nonlinear Model Predictive Control
• A Complete Classification of Sub-Shocks in the Shock Structure of a Binary Mixture of Eulerian Gases with Different Degrees of Freedom
• Hermitian chiral boundary states in non-Hermitian topological insulators
• Modeling Intense-Electron-Beam Generated Plasmas Using a Rigid-Beam Approximation
• Testing Lyman alpha emission line reconstruction routines at multiple velocities in one system
• Understanding the Star Formation Efficiency in Dense Gas: Initial Results from the CAFFEINE Survey with ArTéMiS
• Efficient decoupling of a non-linear qubit mode from its environment
• Prospects for Detecting Gaps in Globular Cluster Stellar Streams in External Galaxies with the Nancy Grace Roman Space Telescope
• Quick recipes for gravitational-wave selection effects
• Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
• Gravitational lensing of gravitational waves: prospects for probing intermediate-mass black holes in galaxy lenses with global minima image
• Exploring Lottery Ticket Hypothesis in Media Recommender Systems
• Stochastic waveform estimation at the fundamental quantum limit
• Feature-weighted Stacking for Nonseasonal Time Series Forecasts: A Case Study of the COVID-19 Epidemic Curves
• Superflares on solar-like stars: A new method for identifying the true flare sources in photometric surveys
• Lensed CMB power spectrum biases from masking extragalactic sources
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• Evolutionary and Observational Consequences of Dyson Sphere Feedback
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• Quenching in the Right Place at the Right Time: Tracing the Shared History of Starbursts, AGNs, and Post-starburst Galaxies Using Their Structures and Multiscale Environments
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models
• SCoRe: A New Framework to Study Unmodeled Physics from Gravitational Wave Data
• Parallel Quantum Chemistry on Noisy Intermediate-Scale Quantum Computers
• Relative energies without electronic perturbations via Alchemical Integral Transform
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• Tackling the Unique Challenges of Low-frequency Solar Polarimetry with the Square Kilometre Array Low Precursor: Pipeline Implementation
• Ram pressure stripping in clusters: Gravity can bind the ISM but not the CGM
• A Performance Analysis of Basin Hopping Compared to Established Metaheuristics for Global Optimization
• Size and Quality of Quantum Mechanical Data Sets for Training Neural Network Force Fields for Liquid Water
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• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Spectrally accurate solutions to inhomogeneous elliptic PDE in smooth geometries using function intension
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Interpreting the Si II and C II line spectra from the COS Legacy Spectroscopic SurveY using a virtual galaxy from a high-resolution radiation-hydrodynamic simulation
• Optical Observations of the Nearby Type Ia Supernova 2021hpr
• Long period modulation of the classical T Tauri star CI Tau: evidence for an eccentric close-in massive planet at 0.17 au
• Revealing the Low Temperature Phase of FAPbI${}_3$ using A Machine-Learned Potential
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• ALMA 300 pc resolution imaging of a z=6.79 quasar: no evidence for supermassive black hole influence on the [C II] kinematics
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• New Solutions for Rotating Boson Stars
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• Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
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• Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
• Impact of anti-symmetric contributions to signal multipoles in the measurement of black-hole spins
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• Black and Gray Box Learning of Amplitude Equations: Application to Phase Field Systems
• Perihelion Asymmetry in the Water Production Rate of the Interstellar Object 3I/ATLAS
• The SunPy Project: An Interoperable Ecosystem for Solar Data Analysis
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• 21cmFirstCLASS II. Early linear fluctuations of the 21cm signal
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• New Periodograms Separating Orbital Radial Velocities and Spectral Shape Variation
• Discovery of a Planar Black Hole Mass Scaling Relation for Spiral Galaxies
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• What's Behind the Elephant's Trunk? Identifying Young Stellar Objects on the Outskirts of IC1396
• On the differences in the periodic behaviour of magnetic helicity flux in flaring active regions with and without X-class events
• Globally Optimal Multi-Scale Monocular Hand-Eye Calibration Using Dual Quaternions
• Gaussian Process Model for the Local Stellar Velocity Field from Gaia Data Release 2
• Dissecting the active galactic nucleus in Circinus IV. MUSE NFM observations unveil a tuning-fork ionised gas morphology
• Probing quasar lifetimes with proximate $21$-centimetre absorption in the diffuse intergalactic medium at redshifts $z\ge 6$
• Comparing the Locations of Supernovae to CO (2-1) Emission in their Host Galaxies
• Accurate modeling of grazing transits using umbrella sampling
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• On the gamma-ray emission from the core of the Sagittarius dwarf galaxy
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• One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors
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• The Carousel Lens: A Well-Modeled Strong Lens with Multiple Lensed Sources
• Connecting the X-ray/UV variability of Fairall 9 with NICER: A Possible Warm Corona
• $Herschel$/PACS OH Spectroscopy of Seyfert, LINER, and Starburst Galaxies
• Influence of chirp and carrier-envelope phase on non-integer high-harmonic generation
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• Inverse-Compton Scattering of the Cosmic Infrared Background
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
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• Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• Evidence for Centrifugal Breakout around the Young M Dwarf TIC 234284556
• Machine learning for accuracy in density functional approximations
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• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Testing the robustness of simulation-based gravitational-wave population inference
• Theory and Implementation of a Novel Stochastic Approach to Coupled Cluster
• Polluting White Dwarfs with Oort Cloud Comets
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• Simulation of neutral beam current drive on EAST tokamak
• A morphological analysis of the substructures in radio relics
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Computation of Green's function by local variational quantum compilation
• Generative Models of Multi-channel Data from a Single Example -- Application to Dust Emission
• An Integrative Analysis of the Rich Planetary System of the Nearby Star e Eridani: Ideal Targets For Exoplanet Imaging and Biosignature Searches
• A fixed point for black hole distributions
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• The Luminosity Phase Space of Galactic and Extragalactic X-ray Transients Out to Intermediate Redshifts
• The nuclear charge radius of ${}^{13}\mathrm{C}$
• Toward source region tomography with inter-source interferometry: Shear wave velocity from 2018 West Bohemia swarm earthquakes
• Flavor Equilibration of Supernova Neutrinos: Exploring the Dynamics of Slow Modes
• UVIT Study of the MAgellanic Clouds (U-SMAC) II. A Far-UV catalog of the Small Magellanic Cloud: Morphology and Kinematics of young stellar population
• Testing tidal theory using Gaia binaries: the red giant branch
• The prototype X-ray binary GX 339-4: using TeV gamma-rays to assess LMXBs as Galactic cosmic ray accelerators
• Investigating the Origin of Observed Central Dips in Radial Metallicity Profiles
• A Sensitive Test of Non-Gaussianity in Gravitational-wave Detector Data
• The BoRG-$JWST$ Survey: Abundance and Mass-to-light Ratio of Luminous $z=7-9$ Galaxies from Independent Sight Lines with NIRSpec
• Inclination Dynamics of Resonant Planets under the Influence of an Inclined External Companion
• Strong nebular HeII emission induced by He${}^{+}$ ionizing photons escaping through the clumpy winds of massive stars
• Can galaxy evolution mimic cosmic reionization?
• Extreme giant molecular clouds in the luminous infrared galaxy NGC 3256
• The Dragonfly Wide Field Survey. II. Accurate Total Luminosities and Colors of Nearby Massive Galaxies and Implications for the Galaxy Stellar Mass Function
• Evaluating Named Entity Recognition: A comparative analysis of mono- and multilingual transformer models on a novel Brazilian corporate earnings call transcripts dataset
• Unravelling sub-stellar magnetospheres
• Near-field imaging of local interference in radio interferometric data: Impact on the redshifted 21 cm power spectrum
• REVEL Framework to measure Local Linear Explanations for black-box models: Deep Learning Image Classification case of study
• Searching for QCD Instantons at Hadron Colliders
• Planning ride-pooling services with detour restrictions for spatially heterogeneous demand: A multi-zone queuing network approach
• Optical and Near-Infrared Excesses are Correlated in T Tauri Stars
• A Framework for Simultaneously Measuring Field Densities and the High-z Luminosity Function
• Evolution and Kinematics of Protostellar Envelopes in the Perseus Molecular Cloud
• Prospects of Gravitational Wave Follow-up Through a Wide-field Ultra-violet Satellite: a Dorado Case Study
• Electroweak Nuclear Properties from Single Molecular Ions in a Penning Trap
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Estimating the Convective Turnover Time
• Marginal Bayesian Statistics Using Masked Autoregressive Flows and Kernel Density Estimators with Examples in Cosmology
• MusE GAs FLOw and Wind (MEGAFLOW) XIII. Cool gas traced by MgII around isolated galaxies
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• Measuring Cosmological Distances Using Cluster Edges as a Standard Ruler
• Reliable stellar abundances of individual stars with the MUSE integral-field spectrograph
• Searching for solar-like oscillations in pre-main sequence stars using APOLLO
• Band structure of n- and p-doped core-shell nanowires
• The Fitness Value of Information with Delayed Phenotype Switching: Optimal Performance with Imperfect Sensing
• Systematic Reanalysis of KMTNet Microlensing Events, Paper II: Two New Planets in Giant-Source Events
• Comparing extragalactic megahertz-peaked spectrum and gigahertz-peaked spectrum sources
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• Multiwavelength analysis and the C IV λ1549 Å emission line behavior from 2008 to 2020 of the FSRQ B2 1633+382
• NQontrol: An open-source platform for digital control-loops in quantum-optical experiments
• Machine-learning enabled optimization of atomic structures using atoms with fractional existence
• Toward hybrid quantum simulations with qubits and qumodes on trapped-ion platforms
• Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
• Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
• Quantum transport and mobility spectrum of topological carriers in (001) SnTe/PbTe heterojunctions
• The phenomenology of the external field effect in cold dark matter models
• ASymba: HI global profile asymmetries in the Simba simulation
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• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• Constructing `full-frequency' spectra via moment constraints for coupled cluster Green's functions
• An Integrative Analysis of the HD 219134 Planetary System and the Inner Solar System: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria
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• The Northern Cross Fast Radio Burst project - II. Monitoring of repeating FRB 20180916B, 20181030A, 20200120E and 20201124A
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• The closest extremely low-mass white dwarf to the Sun
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• Cosmological Parameter Estimate from Persistent Radio Sources of Fast Radio Bursts
• Mass-stream trajectories with non-synchronously rotating donors
• Structural and Dynamical Analysis of the Quiescent Molecular Ridge in the Large Magellanic Cloud
• Numerically assisted determination of local models in network scenarios
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• Fast generation of mock galaxy catalogues with COLA
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• QSO MUSEUM II: Search for extended Ly$\alpha$ emission around eight $z\sim 3$ quasar pairs
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• Black hole virial masses from single-epoch photometry: the miniJPAS test case
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• An inner warp discovered in the disk around HD 110058 using VLT/SPHERE and HST/STIS
• Delayed Development of Cool Plasmas in X-ray Flares from kappa1 Ceti
• Crystal Structure Generation Based on Polyhedra using Dual Periodic Graphs
• 3D Detection and Characterisation of ALMA Sources through Deep Learning
• fBLS -- a fast-folding BLS algorithm
• The evolution of phase space densities in star-forming regions
• The fastest generation of multipartite entanglement with natural interactions
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• ApSense: Data-driven Algorithm in PPG-based Sleep Apnea Sensing
• Multiple components in the molecular outflow of the red supergiant NML Cyg
• McFACTS II: Mass Ratio--Effective Spin Relationship of Black Hole Mergers in the AGN Channel
• Late-time Hubble Space Telescope Observations of AT 2018cow. I. Further Constraints on the Fading Prompt Emission and Thermal Properties 50--60 Days Post-discovery
• Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum
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• Uniform Modelling of the Stellar Density of Thirteen Tidal Streams within the Galactic Halo
• Dominance of 2-Minute Oscillations near the Alfvén Surface
• A search for transients in the Reionization Lensing Cluster Survey (RELICS): Three new supernovae
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• HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
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• The active centaur 2020 MK4
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• Variational Quantum Eigensolver Ansatz for the $J_1$-$J_2$-model
• Improved model of the Supernova Refsdal cluster MACS J1149.5+2223 thanks to VLT/MUSE
• Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of $\alpha$ Cen A. I. Observations, Orbital and Physical Properties, and Exozodi Upper Limits
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• No swan song for Sun-as-a-star helioseismology: performances of the Solar-SONG prototype for individual mode characterisation
• Quantifying Quantum Computational Advantage on a Processor of Ultracold Atoms
• SAGUARO: Time-domain Infrastructure for the Fourth Gravitational-wave Observing Run and Beyond
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• Template bank to search for exotic gravitational wave signals from astrophysical compact binaries
• The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-${\chi }_{\mathrm{eff}}$ correlation
• Warm Jupiters Beyond the Tidal Synchronization Limit May Exhibit a Wide Range of Secondary Eclipse Depths
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• Flaires: A Comprehensive Catalog of Dust-Echo-like Infrared Flares
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• Unravelling cosmic velocity flows: a Helmholtz-Hodge decomposition algorithm for cosmological simulations
• Revisit of open clusters UPK 39, UPK 41 and PHOC 39 : a new binary open cluster found
• Propagation and reconstruction of re-entry uncertainties using continuity equation and simplicial interpolation
• Non-Halo Structures and their Effects on Gravitational Lensing
• Understanding Heating in Active Region Cores through Machine Learning II. Classifying Observations
• A GALAH View of the Chemical Homogeneity and Ages of Stellar Strings Identified in Gaia
• FUMES III: Ultraviolet and Optical Variability of M Dwarf Chromospheres
• Peeking beneath the precision floor -- II. Probing the chemo-dynamical histories of the potential globular cluster siblings, NGC 288 and NGC 362
• The Solar Neighborhood LI: A Variability Survey of Nearby M Dwarfs with Planets from Months to Decades with TESS and the CTIO/SMARTS 0.9 m Telescope
• On measuring divergence for magnetic field modeling
• Early-Type Galaxies: Elliptical and S0 Galaxies, or Fast and Slow Rotators
• Prevalence of non-stationarity in quasi-periodic pulsations (QPPs) associated with M- and X-class solar flares
• Deterministic entangling gates with nonlinear quantum photonic interferometers
• GPT-4.1 Sets the Standard in Automated Experiment Design Using Novel Python Libraries
• On the anti-correlation between pericentric distance and inner dark matter density of Milky Way's dwarf spheroidal galaxies
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• Dynamical Complex Network Models of the Turbulent Cascade
• Pymablock: an algorithm and a package for quasi-degenerate perturbation theory
• Dynamic stability of electric power grids: Tracking the interplay of the network structure, transmission losses and voltage dynamics
• Earth mover's distance as a measure of CP violation
• Global Stochastic Optimization of Stellarator Coil Configurations
• Using angular momentum maps to detect kinematically distinct galactic components
• Validation of strategies for coupling exoplanet PSFs into single-mode fibres for high-dispersion coronagraphy
• Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D): I. Overview, Magnetohydrodynamic Modeling, and Stokes Profile Synthesis
• Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experiment
• Dynamically Forming Extremely Low-Mass White Dwarf Binaries in Wide Orbits
• A spectroscopic map of the Galactic centre -- Observations and resolved stars
• Taming numerical errors in simulations of continuous variable non-Gaussian state preparation
• Estimates of the dynamic structure factor for the finite temperature electron liquid via analytic continuation of path integral Monte Carlo data
• A neural network emulator of the Advanced LIGO and Advanced Virgo selection function
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Probing the Circumstellar Environment of highly luminous type IIn SN ASASSN-14il
• High-Resolution Spectral Discriminants of Ocean Loss for M Dwarf Terrestrial Exoplanets
• Limitations of Hartree-Fock with quantum resources
• Hubbard physics with Rydberg atoms: using a quantum spin simulator to simulate strong fermionic correlations
• Yet Another Sunshine Mystery: Unexpected Asymmetry in GeV Emission from the Solar Disk
• Constraining the cosmic-ray pressure in the inner Virgo Cluster using H.E.S.S. observations of M 87
• A numerical method for suspensions of articulated bodies in viscous flows
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• Are NH${}_3$ and CO${}_2$ ice present on Miranda?
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Inner Habitable Zone Boundary for Eccentric Exoplanets
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• Solar Polar Flux Redistribution based on Observed Coronal Holes
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Identifying supermassive black hole recoil in elliptical galaxies
• Effect of dilute impurities on short graphene Josephson junctions
• Modern Microscopy with the Web of Things: The OpenFlexure Microscope Software Stack
• Mergers all the way down: stellar collisions and kinematics of a dense hierarchically forming massive star cluster in a dwarf starburst
• The halo bias for number counts on the light cone from relativistic N-body simulations
• Searching for dark energy in the matter-dominated era
• The physical and chemical structure of Sagittarius B2, VIII. Full molecular line survey of hot cores
• Improving cosmological reach of a gravitational wave observatory using Deep Loop Shaping
• Pareto Front-Diverse Batch Multi-Objective Bayesian Optimization
• Diurnal and Seasonal Mapping of Martian Ices With EMIRS
• Electromagnetic moments of the odd-mass nickel isotopes ${}^{59-67}$Ni
• Fast generation of entanglement between coupled spins using optimization and deep learning methods
• Rational social distancing policy during epidemics with limited healthcare capacity
• Galactic disc heating by density granulation in fuzzy dark matter simulations
• Impact of Galactic dust non-Gaussianity on searches for B-modes from inflation
• Main-belt and Trojan Asteroid Phase Curves from the ATLAS Survey
• The Perkins INfrared Exosatellite Survey (PINES) II. Transit Candidates and Implications for Planet Occurrence around L and T Dwarfs
• Surveys of Clumps, Cores, and Condensations in the Cygnus X: II. Radio Properties of the Massive Dense Cores
• VELOcities of CEpheids (VELOCE) II. Systematic Search for Spectroscopic Binary Cepheids
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
• Solving the PTA Data Analysis Problem with a Global Gibbs Scheme
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• A study of Dipolar Signal in distant Quasars with various observables
• PHANGS-HST: Globular Cluster Systems in 17 Nearby Spiral Galaxies
• A Homogeneous Catalog of Oscillating Solar-Type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity
• Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams II: Applications to Nearby Elliptical Galaxies
• A Harsh Test of Far-Field Scrambling with the Habitable Zone Planet Finder and the Hobby Eberly Telescope
• HST survey of the Orion Nebula Cluster in the H${}_2$O 1.4 $\mu$m absorption band: III. The population of sub-stellar binary companions
• BASS. XLIX. Characterization of highly luminous and obscured AGNs: local X-ray and [NeV]$\lambda$3426 emission in comparison with the high-redshift Universe
• Statistical Approach to Quantum Phase Estimation
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Ansatz-Independent Variational Quantum Classifier
• Hunting for QCD Instantons at the LHC in Events with Large Rapidity Gaps
• The ESO SupJup Survey VIII. Chemical fingerprints of young L dwarf twins
• Towards fast machine-learning-assisted Bayesian posterior inference of microseismic event location and source mechanism
• Multiple giant eruptions and X-ray emission in the recoiling AGN/LBV candidate SDSS1133
• The Volatile Inventory of 3I/ATLAS as seen with JWST/MIRI
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• One-Pixel Attack Deceives Computer-Assisted Diagnosis of Cancer
• Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation
• Searching for Dwarf Galaxies in $Gaia$ DR2 Phase-Space Data Using Wavelet Transforms
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks
• Gaussianization of peculiar velocities and bulk flow measurement
• The impact of magnetic fields on momentum transport and saturation of shear-flow instability by stable modes
• Physical and chemical properties of Wolf-Rayet planetary nebulae
• Water ice in the debris disk around HD 181327
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• Predicting the outcome of collisional neutrino flavor conversion
• Galactic Geology: Probing Time-Varying Dark Matter Signals with Paleo-Detectors
• How many suns are in the sky? A SPHERE multiplicity survey of exoplanet host stars I -- Four new close stellar companions including a white dwarf
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• SN 2017hpa: A carbon-rich type Ia supernova
• Analysis of Seismic Inversion with Optimal Transportation and Softplus Encoding
• PICASO 4.0: Clouds and Photochemistry in Climate Models of Brown Dwarfs and Exoplanets
• Probing patchy reionisation with JWST: IGM opacity constraints from the Lyman-$\alpha$ forest of galaxies in legacy extragalactic fields
• Spatially resolved [CII]-gas conversion factor in early galaxies
• Greedy Emulators for Nuclear Two-Body Scattering
• An accreting dwarf star orbiting the S-type giant star pi1 Gru
• Chondrules from high-velocity collisions: thermal histories and the agglomeration problem
• Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
• 10 Years of Archival High-Resolution NIR Spectra: The Raw and Reduced IGRINS Spectral Archive (RRISA)
• Diversity in the haziness and chemistry of temperate sub-Neptunes
• Detecting dark matter subhalos with the Nancy Grace Roman Space Telescope
• Extreme winds on the emerging dayside of an ultrahot Jupiter
• Controlled Latent Diffusion Models for 3D Porous Media Reconstruction
• Simple Improved Reference Subtraction for H4RG, H2RG, and H1RG Near-infrared Array Detectors
• Physical and kinematic conditions of the local merging galaxy NGC 1487
• Systematic biases from ignoring environmental tidal effects in gravitational wave observations
• Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of $\alpha$ Cen A. II. Binary Star Modeling, Planet and Exozodi Search, and Sensitivity Analysis
• JWST + ALMA ubiquitously discover companion systems within $\lesssim 18$kpc around four $z$$\approx$3.5 luminous radio-loud AGN
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• New perspectives on MASCARA-1b: A combined analysis of pre- and post-eclipse emission data using CRIRES+
• The defocused observations of bright sources with Athena/X-IFU
• Periods and classifications of RR Lyrae stars in the globular cluster M15
• Unveiling a 36 Billion Solar Mass Black Hole at the Centre of the Cosmic Horseshoe Gravitational Lens
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• Intrinsic galaxy alignments in the KiDS-1000 bright sample: dependence on colour, luminosity, morphology, and galaxy scale
• Scalable evaluation of quantum-circuit error loss using Clifford sampling
• FEASTS Combined with Interferometry. III. The Low Column Density HI Around M51 and Possibility of Turbulent-mixing Gas Accretion
• Direct Spectroscopy of 51 Eridani b with JWST NIRSpec
• The Galactic Bulge exploration IV.: RR~Lyrae stars as traces of the Galactic bar -- 3D and 5D analysis, extinction variation
• Towards automated extraction and characterization of scaling regions in dynamical systems
• Multiresolution angular momentum measurements of z~1.5-2 star-forming galaxies
• TDCOSMO XVII. New time delays in 22 lensed quasars from optical monitoring with the ESO-VST 2.6m and MPG 2.2m telescopes
• Joint inference of the Milky Way star formation history and IMF from Gaia all-sky $G<13$ data
• The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra
• CosTuuM: polarized thermal dust emission by magnetically oriented spheroidal grains
• Retrieving day- and nightside atmospheric properties of the ultra-hot Jupiter TOI-2109b. Detection of Fe and CO emission lines and evidence for inefficient heat transport
• Classical Pre-optimization Approach for ADAPT-VQE: Maximizing the Potential of High-Performance Computing Resources to Improve Quantum Simulation of Chemical Applications
• Using Cosmic Rays detected by HST as Geophysical Markers I: Detection and Characterization of Cosmic Rays
• Reuse-Aware Compilation for Zoned Quantum Architectures Based on Neutral Atoms
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• The contribution by luminous blue variable stars to the dust content of the Magellanic Clouds
• Photometric Data-driven Classification of Type Ia Supernovae in the Open Supernova Catalog
• A non-axisymmetric potential for the Milky Way disk
• Dynamics of metastable Standard Model particles from long-lived particle decays in the MeV primordial plasma
• The completeness of the open cluster census towards the Galactic anticentre
• $\text{Xsec}$: the cross-section evaluation code
• Flow Matching for Atmospheric Retrieval of Exoplanets: Where Reliability meets Adaptive Noise Levels
• Emerging chirality and moiré dynamics in twisted layered material heterostructures
• Boyajian's Star B: The co-moving stellar companion to KIC 8462852
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Quantum Closures for Neutrino Moment Transport
• NGDEEP: The Star Formation and Ionization Properties of Galaxies at $1.7<z<3.4$
• Advanced Classification of Hot Subdwarf Binaries Using Artificial Intelligence Techniques and Gaia DR3 data
• Uncertainty Analysis of Limit Cycle Oscillations in Nonlinear Dynamical Systems with the Fourier Generalized Polynomial Chaos Expansion
• Hitting the mark: Optimising Marked Power Spectra for Cosmology
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• PDS 70b Shows Stellar-like Carbon-to-oxygen Ratio
• Low-overhead magic state distillation with color codes
• A Nuclear Equation of State Inferred from Stellar r-process Abundances
• A Deep Learning Earth System Model for Efficient Simulation of the Observed Climate
• MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars
• Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations
• A novel analytic atmospheric $T(\tau )$ relation for stellar models
• Binding of the three-hadron $D{D}^{\ast }K$ system from the lattice effective field theory
• Testing the wavelength dependence of oscillations and granulation in red giants using Kepler and TESS
• Europa's H${}_2$O${}_2$: Temperature Insensitivity and a Correlation with CO${}_2$
• Precise Photometric Measurements from a 1903 Photographic Plate Using a Commercial Scanner
• Why fixing alpha in the NRTL model might be a bad idea -- Identifiability analysis of a binary Vapor-Liquid equilibrium
• Disentangling the dust and gas contributions of the JWST/MIRI spectrum of Sz28
• Eddington Ratios of Dust-obscured Quasars at $z\lesssim 1$: Evidence Supporting Dust-obscured Quasars as Young Quasars
• Many-body localization crossover is sharper in quasiperiodic spin chains
• The Curious Case of Twin Fast Radio Bursts: Evidence for Neutron Star Origin?
• Microphysical Prescriptions for Parameterized Water Cloud Formation on Ultra-cool Substellar Objects
• False positives for gravitational lensing: the gravitational-wave perspective
• Ba Enrichment in Gaia MS+WD Binaries: Tracing $s$-Process Element Production
• Toward a test of Gaussianity of a gravitational wave background
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• Limitations and rotation of the two-armed phase spiral in the Milky Way stellar disc
• Euclid preparation. LI. Forecasting the recovery of galaxy physical properties and their relations with template-fitting and machine-learning methods
• DESI Massive Post-Starburst Galaxies at $\mathbf{z}\sim 1.2$ have compact structures and dense cores
• ViPErLEED package I: Calculation of $I(V)$ curves and structural optimization
• The Discovery and Evolution of a Possible New Epoch of Cometary Activity by the Centaur (2060) Chiron
• A comprehensive approach to incorporating intermolecular dispersion into the openCOSMO-RS model. Part 1: Halocarbons
• The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure
• Baryonification extended to thermal Sunyaev Zeldovich
• Analyzing JWST/NIRSpec Hydrogen Line Detections at TWA 27B: Constraining Accretion Properties and Geometry
• The Milky Way as Seen by Classical Cepheids I: Distances Based on Mid-infrared Photometry
• Measuring the matter fluctuations in the Local Universe with the ALFALFA catalog
• Very High Energy Afterglow of Structured Jets: GW 170817 and Prospects for Future Detections
• Period Ratio Sculpting Near Second-Order Mean-Motion Resonances
• Strength in numbers: A multiphase wind model with multiple cloud populations
• Identification of new nearby white dwarfs using Gaia DR3
• Rank-DistiLLM: Closing the Effectiveness Gap Between Cross-Encoders and LLMs for Passage Re-Ranking
• Variational Quantum Algorithms for Differential Equations on a Noisy Quantum Computer
• Spatio-temporal map of star clusters in the Magellanic Clouds using Gaia: Synchronized peaks and radial shrinkage of cluster formation
• A Cohesive Deep Drilling Field Strategy for LSST Cosmology
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Multiwavelength Observations of the Blazar VER J0521+211 During an Elevated TeV Gamma-Ray State
• 60 Microlensing Events from the Three Years of Zwicky Transient Facility Phase One
• Composite Bayesian Optimization In Function Spaces Using NEON -- Neural Epistemic Operator Networks
• Polariton response in the presence of Brownian dissipation from molecular vibrations
• Globular Cluster Intrinsic Iron Abundance Spreads: II. Protocluster Metallicities and the Age-Metallicity Relations of Milky Way Progenitors
• Non-equilibrium microbial dynamics unveil a new macroecological pattern beyond Taylor's law
• Comparing the hardness of MAX 2-SAT problem instances for quantum and classical algorithms
• Uncovering Tidal Treasures: Automated Classification of Faint Tidal Features in DECaLS Data
• TMM$-$Sim: A Versatile Tool for Optical Simulation of Thin$-$Film Solar Cells
• A Simple Molecular Model for Hydrated Silicate Ionic Liquids, a Realistic Zeolite Precursor
• Stabilizer ground states for simulating quantum many-body physics: theory, algorithms, and applications
• Disk-Integrated Thermal Properties of Ceres Measured at Millimeter Wavelengths
• A comprehensive kinematic model of the LMC disk from star clusters and field stars using Gaia DR3: Tracing the disk characteristics, rotation, bar, and the outliers
• Spectral Analysis of ionospheric density variations measured with the large radio telescope in the Low-Latitude region
• Spatially oscillating correlation functions in $\left(2+1\right)$-dimensional four-fermion models: The mixing of scalar and vector modes at finite density
• OpenDust: A fast GPU-accelerated code for calculation forces, acting on microparticles in a plasma flow
• Recovered SN Ia rate from simulated LSST images
• Signal Synchronization Strategies and Time Domain SETI with Gaia DR3
• Assessment of a new sub-grid model for magnetohydrodynamical turbulence. II. Kelvin-Helmholtz instability
• High-performance multiqubit system with double-transmon couplers: Toward scalable superconducting quantum computers
• High angular momentum hot differentially rotating equilibrium star evolutions in conformally flat spacetime
• On the linear stability of nonrelativistic selfinteracting boson stars
• RUMBoost: Gradient Boosted Random Utility Models
• Polarization-dependent beam shifts upon metallic reflection in high-contrast imagers and telescopes
• Identifying thermal effects in neutron star merger remnants with model-agnostic waveform reconstructions and third-generation detectors
• Where to Drill Next? A Dual-Weighted Approach to Adaptive Optimal Design of Groundwater Surveys
• Improved motif-scaffolding with SE(3) flow matching
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Locality Error Free Effective Core Potentials for 3d Transition Metal Elements Developed for the Diffusion Monte Carlo Method
• Contributing Components of Metabolic Energy Models to Metabolic Cost Estimations in Gait
• Measuring distances to galaxies with globular cluster velocity dispersions
• Physical properties of the eclipsing binary KIC 9851944 and analysis of its tidally-perturbed p- and g-mode pulsations
• Properties of the Hot Ambient Medium of Early-type Galaxies Hosting Powerful Radio Sources
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Magnetic Fields, Star Formation Rates and Gas Densities at Sub-kpc Scales in a Pilot Sample of Nearby Galaxies
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
• Massive pre-main-sequence stars in M17 -- Modelling hydrogen and dust in MYSO disks
• Resolved galactic superwinds reconstructed around their host galaxies at z>3
• Mgii h&k fine structure prominence modelling and the consequences for observations
• Stabilizing the calculation of the self-energy in dynamical mean-field theory using constrained residual minimization
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Are nonrelativistic ground state $\ell$-boson stars only stable for $\ell =0$ and $\ell =1$?
• Characterising SMSS J2157--3602, the most luminous known quasar, with accretion disc models
• Magnetic flux eruptions at the root of time-lags in low-luminosity AGN
• Multi-wavelength observations of multiple eruptions of the recurrent nova M31N 2008-12a
• On the instability of the magnetohydrodynamic pipe flow subject to a transverse magnetic field
• A variable active galactic nucleus at $z=2.06$ triply-imaged by the galaxy cluster MACS J0035.4-2015
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• NOEMA reveals the true nature of luminous red JWST z>10 galaxy candidates
• Hotter Than Expected: HST/WFC3 Phase-resolved Spectroscopy of a Rare Irradiated Brown Dwarf with Strong Internal Heat Flux
• Cosmological constraints from low redshift 21 cm intensity mapping with machine learning
• Parameterizing pressure-temperature profiles of exoplanet atmospheres with neural networks
• Recovering complete positivity of non-Markovian quantum dynamics with Choi-proximity regularization
• SPT-CL J2215-3537: A Massive Starburst at the Center of the Most Distant Relaxed Galaxy Cluster
• On the Benefit of Optimal Transport for Curriculum Reinforcement Learning
• Post-processing variationally scheduled quantum algorithm for constrained combinatorial optimization problems
• Do Type Ia Supernovae Explode Inside Planetary Nebulae?
• Universal imaginary-time critical dynamics on a quantum computer
• Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
• The BINGO Project IX: Search for Fast Radio Bursts -- A Forecast for the BINGO Interferometry System
• Fragmented superconductivity in the Hubbard model as solitons in Ginzburg-Landau theory
• Improving image quality of sparse-view lung tumor CT images with U-Net
• Astrosat: Forecasting satellite transits for optical astronomical observations
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• Removing Aliases in Time-Series Photometry
• Testing the Cosmological Principle: On the Time Dilation of Distant Sources
• Simulating single-coil MRI from the responses of multiple coils
• Total light bending in non-asymptotically flat black hole spacetimes
• Effect of Spherical Polarization on the Magnetic Spectrum of the Solar Wind
• Exploring the Link between the X-ray Power Spectra and Energy Spectra of Active Galactic Nuclei
• Solar Cycle Variation of 0.3-1.29 MeV/nucleon Heavy Ion Composition during Quiet Times near 1 AU in Solar Cycles 23 and 24
• Variability of Young Stellar Objects in the Perseus Molecular Cloud
• Massive pre-main-sequence stars in M17: $1^{\mathrm{st}}$ and $2^{\mathrm{nd}}$ overtone CO bandhead emission and the thermal infrared
• Performance Assessment of the KASI-Deep Rolling Imaging Fast-optics Telescope pathfinder
• Large-scale Hydrodynamical Shocks as the Smoking Gun Evidence for a Bar in M31
• Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
• Tailoring galaxies: size-luminosity-surface brightness relations of bulges and disks along the morphological sequence
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Revising Properties of Planet-host Binary Systems II: Apparent Near-Earth Analog Planets in Binaries Are Often Sub-Neptunes
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Exploring the stellar surface phenomena of WASP-52 and HAT-P-30 with ESPRESSO
• SOFIA/HAWC+ observations of the Crab Nebula: dust properties from polarised emission
• Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA
• Cluster aggregates surrounding Pismis 5 in the Vela Molecular Ridge
• Smoke on the wind: dust nucleation in archetype colliding wind pinwheel WR104
• Amplitude amplification-inspired QAOA: Improving the success probability for solving 3SAT
• An archival search for type Ia supernova siblings
• Rippling of two-dimensional materials by line defects
• Magnetic interactions in orbital dynamics
• Synthetic radio images of structured GRB and kilonova afterglows
• Nanoflare Heating of the Solar Corona Observed in X-rays
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• Multiphase condensation in cluster halos: interplay of cooling, buoyancy and mixing
• Accurate first-principle bandgap predictions in strain-engineered ternary III-V semiconductors
• OpTaS: An Optimization-based Task Specification Library for Trajectory Optimization and Model Predictive Control
• Multiwavelength Mitigation of Stellar Activity in Astrometric Planet Detection
• The $\text{Gaia}$ view of the Cepheus OB2 association
• Symbolic Implementation of Extensions of the $\text{PyCosmo}$ Boltzmann Solver
• Validation Solutions to the Full-Sky Radio Interferometry Measurement Equation for Diffuse Emission
• Deciphering Faint Gyrosynchrotron Emission from Coronal Mass Ejection using Spectro-polarimetric Radio Imaging
• Dynamics of a buffer-gas-loaded, deep optical trap for molecules
• Network topology of interlocked chiral particles
• Growth of disc-like pseudo-bulges in SDSS DR7 since z = 0.1
• Fastcc: fast colour corrections for broadband radio telescope data
• Comparison of dynamical and kinematic reference frames via pulsar positions from timing, Gaia, and interferometric astrometry
• Development of a Cooperative Localization System using a UWB Network and BLE Technology
• Forward and Back: Kinematics of the Palomar 5 Tidal Tails
• Observing Circumplanetary Disks with METIS
• An Eddington ratio-driven origin for the ${\mathrm{L}}_{\mathrm{X}}-{\mathrm{M}}_{\ast }$ relation in quiescent and star forming active galaxies
• Magnetic Moments of Astrophysical Neutrinos
• Statistical mechanical model for crack growth
• Improved detection statistics for non Gaussian gravitational wave stochastic backgrounds
• Reliable computational prediction of supramolecular ordering of complex molecules under electrochemical conditions
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• Comparing Lensing and Stellar Orbital Models of a Nearby Massive Strong-Lens Galaxy
• SImMER: A Pipeline for Reducing and Analyzing Images of Stars
• A Dynamic Trajectory Fit to Multi-Sensor Fireball Observations
• The Fornax3D project: Intrinsic Correlations between Orbital Properties and the Stellar Initial Mass Function
• Temporal patterns in insulin needs for Type 1 diabetes
• Skyrmion automotion in confined counter-sensor device geometries
• Detection of a 20 minute time lag observed from Sgr A* between 8 and 10 GHz with the VLA
• Revisiting the Spectral-Energy Correlations of GRBs with {\it Fermi} Data I: Model-wise Properties
• Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
• Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content
• The Impact of Stellar Clustering on the Observed Multiplicity of Super-Earth systems: Outside-in Cascade of Orbital Misalignments Initiated by Stellar Flybys
• A data-scientific noise-removal method for efficient submillimeter spectroscopy with single-dish telescopes
• The Host Galaxies of Hybrid Morphology Radio Sources
• LatticeOPT: A heuristic topology optimization framework for thin-walled, 2D extruded lattices
• High-Resolution Chemical Abundances of the Nyx Stream
• JexoSim 2.0: End-to-End JWST Simulator for Exoplanet Spectroscopy -- Implementation and Case Studies
• Spectral properties of near-Earth objects with low-Jovian Tisserand invariant
• Nanoflare Diagnostics from Magnetohydrodynamic Heating Profiles
• Near-Gaussian distributions for modelling discrete stellar velocity data with heteroskedastic uncertainties
• Cluster-based multidimensional scaling embedding tool for data visualization
• Speciesist Language and Nonhuman Animal Bias in English Masked Language Models
• Numerical Simulations of Tidal Deformation and Resulting Light Curves of Small Bodies: Material Constraints of 99942 Apophis and 1I/`Oumuamua
• Interlopers speak out: studying the dark universe using small-scale lensing anisotropies
• Confinement of Bose-Einstein magnon condensates in adjustable complex magnetization landscapes
• Weighing the Local Interstellar Medium using Gamma Rays and Dust
• PyfastSPM: A Python package to convert 1D FastSPM data streams into publication quality movies
• Photometrically-Classified Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey: A Case Study for Science with Machine Learning-Based Classification
• The Role of Magnetic Fields in the Formation of the Filamentary Infrared Dark Cloud G11.11-0.12
• Mitigating Mismatch Compression in Differential Local Field Potentials
• HyDe: The First Open-Source, Python-Based, GPU-Accelerated Hyperspectral Denoising Package
• TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with HPF
• HORuS transmission spectroscopy and revised planetary parameters of KELT-7b
• Accretion History of AGN: Estimating the Host Galaxy Properties in X-ray Luminous AGN from z=0-3
• Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
• Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267
• Fitting Splines to Axonal Arbors Quantifies Relationship between Branch Order and Geometry
• The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS
• Three-dimensional Reconstruction of Coronal Plasma Properties from a Single Perspective
• Rapid Brightening of 3I/ATLAS Ahead of Perihelion
• Root-finding Approaches for Computing Conformal Prediction Set
• Efficient time stepping for numerical integration using reinforcement learning
• Apparent nonlinear damping triggered by quantum fluctuations
• Direct driving of simulated planetary jets by upscale energy transfer
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• The infrared counterpart and proper motion of magnetar SGR0501+4516
• Regularizing the Pulsar Timing Array likelihood: A path towards Fourier Space
• Surgeons vs. Computer Vision: A comparative analysis on surgical phase recognition capabilities
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• A Survey of Computational Tools in Solar Physics
• Integral field spectroscopy with the solar gravitational lens
• Interplay between Young Stars and Molecular Clouds in the Ophiuchus Star-forming Complex
• Topology of Pulsar Profiles (ToPP). I. Graph theory method and classification of the EPN
• A Machine Learning Approach to Correct for Mass Resolution Effects in Simulated Halo Clustering Statistics
• Preparing for Solar and Heliospheric Science with the SKAO: An Indian Perspective
• Galactic Winds across the Gas-Rich Merger Sequence II. Lyman Alpha Emission and Highly Ionized O VI and N V Outflows in Ultraluminous Infrared Galaxies
• Accelerating reactive-flow simulations using vectorized chemistry integration
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve
• Size-consistency and orbital-invariance issues revealed by VQE-UCCSD calculations with the FMO scheme
• The S stars' zone of avoidance in the Galactic center
• A Modularized Design Approach for GelSight Family of Vision-based Tactile Sensors
• Characterising the Apertif primary beam response
• Sensitivity of Bayesian 21 cm power spectrum estimation to foreground model errors
• The Low-Mass Stellar Initial Mass Function in Nearby Ultrafaint Dwarf Galaxies
• Emission Line Predictions for Mock Galaxy Catalogues: a New Differentiable and Empirical Mapping from DESI
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Faster Bayesian inference with neural network bundles and new results for $f(R)$ models
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Cait: analysis toolkit for cryogenic particle detectors in Python
• Ionized gas metallicity of the strong [OIII]λ emission-line compact galaxies in the LAMOST survey
• Unraveling stochastic fundamental diagrams considering empirical knowledge: modeling, limitation and further discussion
• Neural Network Training as an Optimal Control Problem: An Augmented Lagrangian Approach
• Variability of Known Exoplanet Host Stars Observed by TESS
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• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Serendipitous discovery of a dusty disc around WDJ181417.84-735459.83
• A Joint Ranking Statistic for Multi-messenger Astronomical Searches with Gravitational Waves
• The Rotation Period Distribution in the Young Open Cluster NGC 6709
• Set-Encoder: Permutation-Invariant Inter-Passage Attention for Listwise Passage Re-Ranking with Cross-Encoders
• Sensitivity study of chemistry in AGB outflows using chemical kinetics
• Detection of quantum phase transition in spin-1 chain through multipartite high-order correlations
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• CIRCUS: an autonomous control system for antimatter, atomic and quantum physics experiments
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• $\tau$SPECT: A spin-flip loaded magnetic ultracold neutron trap for a determination of the neutron lifetime
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• QArray: a GPU-accelerated constant capacitance model simulator for large quantum dot arrays
• Rotational evolution of young-to-old stars with data-driven three-dimensional wind models
• Active galactic nuclei catalog from the AKARI NEP Wide field
• Time evolution as an optimization problem: The hydrogen atom in strong laser fields in a basis of time-dependent Gaussian wave packets
• Relative baryon-dark matter velocities in cosmological zoom simulations
• MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at $z>0.25$
• Grover Speedup from Many Forms of the Zeno Effect
• The GALAH Survey: Improving our understanding of confirmed and candidate planetary systems with large stellar surveys
• Multi-wavelength aperture polarimetry of debris disc host stars
• Fresh Insights on the Kinematics of M49's Globular Cluster System with MMT/Hectospec Spectroscopy
• Chandra Observations of Six Peter Pan Disks: Diversity of X-ray-driven Internal Photoevaporation Rates Doesn't Explain Their Rare Longevity
• Giant molecular clouds and their Type classification in M74: Toward understanding star formation and cloud evolution
• The largest bright ULX population in a galaxy: X-ray variability and Luminosity Function in the Cartwheel ring Galaxy
• J-PLUS: Bayesian object classification with a strum of BANNJOS
• Wavelet-based tools to analyze, filter, and reconstruct transient gravitational-wave signals
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• ALMA resolves molecular clouds in the metal poor Magellanic Bridge A
• Instabilities at recollimation shocks in MHD jets
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Testing planet formation from the ultraviolet to the millimeter
• Major Mergers Mean Major Offset: Drivers of Intrinsic Scatter in The $M_{GCS}-M_h$ Scaling Relation for Massive Elliptical Galaxies
• Damping of three-dimensional waves on coating films dragged by moving substrates
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• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• CHANG-ES: XXXVI. The thin and thick radio discs
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• On the contributions of extragalactic CO emission lines to ground-based CMB observations
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• Tempo vs. Pitch: understanding self-supervised tempo estimation
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• Particle-in-Cell Simulations of Relativistic Magnetic Reconnection with Advanced Maxwell Solver Algorithms
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• The Ages of Optically Bright Sub-Clusters in the Serpens Star-Forming Region
• The HI Structure of the Local Volume Dwarf Galaxy Pisces A
• Possible evidence of hydrogen emission in the first-overtone and multi-mode RR Lyrae variables
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae II: Rotation and Turbulence
• The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies
• Inferring the Distribution of the Ionising Photon Escape Fraction
• Towards a fully consistent Milky Way disk model V. The disk model for 4 $-$ 14 kpc
• Exploration of the parameter space of quasisymmetric stellarator vacuum fields through adjoint optimisation
• WALOP-South: A Four-Camera One-Shot Imaging Polarimeter for PASIPHAE Survey. Paper II -- Polarimetric Modelling and Calibration
• The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
• Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
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• ACCESS: Tentative detection of H${}_2$O in the ground-based optical transmission spectrum of the low-density hot Saturn HATS-5b
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• The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
• First observations with a GNSS antenna to radio telescope interferometer
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• The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
• Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scale
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• HIP 15429: A newborn Be star on an eccentric binary orbit
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• Filamentary Hierarchies and Superbubbles I: Characterizing filament properties across a simulated spiral galaxy
• The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
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• Compilation of Entangling Gates for High-Dimensional Quantum Systems
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• The Galactic population of magnetars : a simulation-based inference study
• Dipolar dark matter simulations on galaxy scales with the RAMSES code
• Inelastic neutron scattering study of the anisotropic $S=1$ spin chain [Ni(HF${}_2$)(3-Clpyridine)${}_4$]BF${}_4$
• Characterizing and mitigating coherent errors in a trapped ion quantum processor using hidden inverses
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• A Refined Model of Convectively-Driven Flicker in Kepler Light Curves
• Pulse Timing Discovery of a Three-Day Companion to the Hot Subdwarf BPM 36430
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• Constraints on the gas-phase C/O ratio of DR Tau's outer disk from CS, SO, and C${}_2$H observations
• 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
• Two-Dimensional Radiation-Hydrodynamic Simulations of Luminous Red Novae
• A Novel Machine Learning Approach to Disentangle Multi-Temperature Regions in Galaxy Clusters
• The effect of spectroscopic binning on atmospheric retrievals
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• Toward Reliability in the NISQ Era: Robust Interval Guarantee for Quantum Measurements on Approximate States
• A Time-Resolved High-Resolution Spectroscopic Analysis of Ionized Calcium and Dynamical Processes in the Ultra-Hot Jupiter HAT-P-70 b
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• Distributed Out-of-Memory NMF on CPU/GPU Architectures
• Explosive dismantling of two-dimensional random lattices under betweenness centrality attacks
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• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• Characterising X-ray variability in light curves with complex sampling patterns: application to the eROSITA south ecliptic pole survey
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• Machine Learning the Fates of Dark Matter Subhalos: A Fuzzy Crystal Ball
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• The SRG/eROSITA all-sky survey: View of the Fornax galaxy cluster
• First measurement of the triaxiality of the inner dark matter halo of the Milky Way
• CO${}_2$ collision-induced line parameters for the ${\nu }_3$ band of ${}^{12}$CH${}_4$ measured using a hard-collision speed-dependent line shape and the relaxation matrix formalism
• Evaluation of the Radius of Maximum Wind over the North Indian Basin with the help of Tropical Cyclone characteristics
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• Deep Node Ranking for Neuro-symbolic Structural Node Embedding and Classification
• AI for Scientific Discovery is a Social Problem
• UVIT Study of the MAgellanic Clouds (U-SMAC) I. Recent star formation history and kinematics of the Shell region in the North-Eastern Small Magellanic Cloud
• Apertif 1.4 GHz continuum observations of the Boötes field and their combined view with LOFAR
• JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD
• Universal Density and Velocity Distributions of Dark Matter around Massive Black Holes
• The Spatial Distribution of the Unidentified 2.07 \textmu m Absorption Feature on Europa and Implications for its Origin
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• The First Model-Independent Chromatic Microlensing Search: No Evidence in the Gravitational Wave Catalog of LIGO-Virgo-KAGRA
• HALO7D III: Chemical Abundances of Milky Way Halo Stars from Medium Resolution Spectra
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Peptide Classification from Statistical Analysis of Nanopore Translocation Experiments
• H-FISTA: A hierarchical algorithm for phase retrieval with application to pulsar dynamic spectra
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Reconciling the Results of the z~2 MOSDEF and KBSS-MOSFIRE Surveys
• New Globular Cluster Candidates in the M81 group
• Tumbling Dice: Radio Constraints on the Presence of Circumstellar Shells around Type Ia Supernovae with Impact Near Maximum Light
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• Quantum gates between distant atoms mediated by a Rydberg excitation antiferromagnet
• Multiplexed Pseudo-Deterministic Photon Source with Asymmetric Switching Elements
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• High-Resolution M-band Spectroscopy of CO towards the Massive Young Stellar Binary W3 IRS5
• Impact of the finite life-time of UHECR sources
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Social Network Heterogeneity Promotes Depolarization of Multidimensional Correlated Opinions
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• KOBE-1: The first planetary system from the KOBE survey. Two planets likely residing in the sub-Neptune mass regime around a late K-dwarf
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• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
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• LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with HST Template Observations
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• Searching for Hot Water World Candidates with CHEOPS: Refining the radii and analysing the internal structures and atmospheric lifetimes of TOI-238 b and TOI-1685 b
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• Solar Wind Structures from the Gaussianity of Magnetic Magnitude
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• A single-layer based numerical method for the slender body boundary value problem
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• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• In search of gravity mode signatures in main sequence solar-type stars observed by Kepler
• High-Resolution Simulations of LS 5039
• Sensitivity Analysis in the Presence of Intrinsic Stochasticity for Discrete Fracture Network Simulations
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• Forming short period sub-stellar companions in 47 Tucanae -- II. Analytic expressions for the orbital evolution of planets in dense environments
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• Multivariate Functional Linear Discriminant Analysis for the Classification of Short Time Series with Missing Data
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• HOLISMOKES XVI: Lens search in HSC-PDR3 with a neural network committee and post-processing for false-positive removal
• Accelerating LISA inference with Gaussian processes
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Andromeda XXXV: The Faintest Dwarf Satellite of the Andromeda Galaxy
• Detectability of Solar Rotation Period Across Various Wavelengths
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Fundamental relation in isolated galaxies, pairs, and triplets in the local universe
• Weakly supervised anomaly detection for resonant new physics in the dijet final state using proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• The Type Ia Supernova and Asymptotic Giant Branch Stellar Ejecta-regulated Interstellar Medium of Massive Galaxies
• Insights on the Scale of Leptogenesis from Neutrino Masses and Neutrinoless Double-Beta Decay
• SOFIA/HAWC+ Far-Infrared Polarimetric Large Area CMZ Exploration Survey. V. The Magnetic Field Strength and Morphology in the Sagittarius C Complex
• The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Linear scaling causal discovery from high-dimensional time series by dynamical community detection
• Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun
• Scaling analysis and renormalization group on the mobility edge in the quantum random energy model
• A Multi-fidelity Estimator of the Expected Information Gain for Bayesian Optimal Experimental Design
• Distributed quantum error correction based on hyperbolic Floquet codes
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Exploring membership and variability in NGC 7419: An open cluster rich in super giants and Be type stars
• TP-AGB stars and stellar population properties of a post-starburst galaxy at $z\sim 2$ through optical and NIR spectroscopy with JWST
• Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
• Shear-gravity transition determines the steep velocity dispersion-size relation in molecular clouds: confronting analytical formula with observations
• Tracking X-ray Variability in Next Generation EHT LLAGN Targets
• Foundations of the Theory of Performance-Based Ranking
• Fundamental thresholds for computational and erasure errors via the coherent information
• Anomalous Dynamics of Superparamagnetic Colloidal Microrobots with Tailored Statistics
• UFig v1: The ultra-fast image generator
• Enhancing the detection of low-energy M dwarf flares: Wavelet-based denoising of CHEOPS data
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• Distortions in Charged-Particle Images of Laser Direct-Drive Inertial Confinement Fusion Implosions
• The Exoplanet Edge: Planets Don't Induce Observable TTVs with a Dominant TTV Period Faster than Half their Orbital Period
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• On the origin of the Hercules group: I. chemical signatures indicating the outer bar origin
• Hybrid approach to reconstruct nanoscale grating dimensions using scattering and fluorescence with soft X-rays
• The Correlation Between Dust and Gas Contents in Molecular Clouds
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• PSF Calibration of DAMPE for gamma-ray Observations
• Inequality constraints in variational quantum circuits with qudits
• Dust Drift Timescales in Protoplanetary Disks at the Cusp of Gravitational Instability
• Hypothesis tests and model parameter estimation on data sets with missing correlation information
• Capturing Turbulence with Numerical Dissipation: a Simple Dynamical Model for Unresolved Turbulence in Hydrodynamic Simulations
• A First-look at Spatially-resolved Infrared Supernova Remnants in M33 with JWST
• Improved quantum algorithm for calculating eigenvalues of differential operators and its application to estimating the decay rate of the perturbation distribution tail in stochastic inflation
• Stellar halos tracing the assembly of ultra-faint dwarf galaxies
• Partial disruption of a planet around a white dwarf: the effect of perturbation from the remnant planet on the accretion
• A solution for co-locating 2D histology images in 3D for histology-to-CT and MR image registration: closing the loop for bone sarcoma treatment planning
• B4: Towards Optimal Assessment of Plausible Code Solutions with Plausible Tests
• The qspec Python package: A physics toolbox for laser spectroscopy
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Reionization relics in the cross-correlation between the Ly$\alpha$ forest and 21 cm intensity mapping in the post-reionization era
• Probing populations of dark stellar remnants in the globular clusters 47 Tuc and Terzan 5 using pulsar timing
• High Strain Rate Compressive Deformation Behavior of Nickel Microparticles
• M giants with IGRINS IV. Identification and characterization of a near-IR line of the s-element Barium
• VIRIS: Simulating indoor airborne transmission combining architectural design and people movement
• From 100 MHz to 10 GHz: Unveiling the spectral evolution of the X-shaped radio galaxy in Abell 3670
• HOLISMOKES -- XIV. Time-delay and differential dust extinction determination with lensed type II supernova color curves
• A candidate giant planet companion to the massive, young white dwarf GALEX J071816.4+373139 informs the occurrence of giant planets orbiting B stars
• Combination of searches for singly produced vector-like top quarks in pp collisions at $\sqrt{s}=13$ TeV with the ATLAS detector
• Westward hotspot offset explained by subcritical dynamo action in an ultra-hot Jupiter atmosphere
• Hierarchical Bayesian estimation of motor-evoked potential recruitment curves yields accurate and robust estimates
• Theory for the Anomalous Phase Behavior of Inertial Active Brownian Particles
• The disc origin of the Milky Way bulge: On the high velocity dispersion of metal-rich stars at low latitude
• Rates and beaming angles of GRBs associated with compact binary coalescences
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• General Guide Concepts for Compact, High-Brilliance Neutron Moderators
• Adapting coherent-state superpositions in noisy channels
• Constrained or Unconstrained? Neural-Network-Based Equation Discovery from Data
• Accelerating Graph-based Tracking Tasks with Symbolic Regression
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• A library of meteoroid environments encountered by spacecraft in the inner solar system
• On the Flux-Intensity Relation of Molecular Clouds
• Gravitational-wave model for neutron star merger remnants with supervised learning
• The Pulsar Science Collaboratory: Multi-Epoch Scintillation Studies of Pulsars
• Sensing force gradients with cavity optomechanics while evading backaction
• CMB-PAInT: An inpainting tool for the cosmic microwave background
• First Search for High-Energy Neutrino Emission from Galaxy Mergers
• Simulating electronic structure on bosonic quantum computers
• Density Classification with Non-Unitary Quantum Cellular Automata
• [CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation
• A common framework for fermion mass hierarchy, leptogenesis and dark matter
• Spectral Operator Representations
• Adaptive time step selection for Spectral Deferred Correction
• Indirect measurement of atomic magneto-optical rotation via Hilbert transform
• A link between the size and composition of comets
• Experimental study of dynamic wetting behavior through curved microchannels with automated image analysis
• Minimal cellular automaton model with heterogeneous cell sizes predicts epithelial colony growth
• A new analytical model of the cosmic-ray energy flux for Galactic diffuse radio emission
• On the development of a practical Bayesian optimisation algorithm for expensive experiments and simulations with changing environmental conditions
• Exponentiation of Parametric Hamiltonians via Unitary interpolation
• Pump-efficient Josephson parametric amplifiers with high saturation power
• Resonance Cascades and Number Theory
• Evidence for axion miniclusters with an increased central density
• Discrete Time Crystal Phase of Higher Dimensional Integrable Models
• Reducing measurement costs by recycling the Hessian in adaptive variational quantum algorithms
• Resource-Efficient Quantum Circuits for Molecular Simulations: A Case Study of Umbrella Inversion in Ammonia
• Leveraging commuting groups for an efficient variational Hamiltonian ansatz
• A catalogue of observed geo-effective CME/ICME characteristics
• Active smectics on a sphere
• Evaluating the Practicality of Quantum Optimization Algorithms for Prototypical Industrial Applications
• Controlling Nonequilibrium Bose-Einstein Condensation with Engineered Environments
• Photonic implementation of the quantum Morra game
• One- and two-argument equation of state parametrizations with continuous sound speed for neutron star simulations
• Kernel-, mean- and noise-marginalised Gaussian processes for exoplanet transits and $H_0$ inference
• Discovery of a Proto-White Dwarf with a Massive Unseen Companion
• Bayesian inference for near-field interferometric tests of collapse models
• On Q-balls in Anti de Sitter Space
• Differencing and Coadding JWST Images with Matched Point Spread Function
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• Optical and X-ray variations during 5 outbursts of Aql X-1 in 3.6 years from 2016
• Switching Time Optimization for Binary Quantum Optimal Control
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• FLORAH: A generative model for halo assembly histories
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• Viscous tweezers: controlling particle orientation with viscosity
• Empirical sandwich variance estimator for iterated conditional expectation g-computation
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• On Stellar Migration from Andromeda to the Milky Way
• Minimizing the negativity of quantum circuits in overcomplete quasiprobability representations
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• An irradiated-Jupiter analogue hotter than the Sun
• Accelerated Bayesian inference of plasma profiles with self-consistent MHD equilibria at W7-X via neural networks
• Analytical and Numerical Analysis of Circumbinary Disk Dynamics -- I: Coplanar Systems
• Using Giant Pulses to Measure the Impulse Response of the Interstellar Medium
• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• Hamiltonian Switching Control of Noisy Bipartite Qubit Systems
• GUTS: Generalized Uncertainty-Aware Thompson Sampling for Multi-Agent Active Search
• VQE-generated quantum circuit dataset for machine learning
• Desynchronizing two oscillators while stimulating and observing only one
• Tree-based solvers for adaptive mesh refinement code FLASH -- IV: An X-ray radiation scheme to couple discrete and diffuse X-ray emission sources to the thermochemistry of the interstellar medium
• Combined mechanistic and machine learning method for construction of oil reservoir permeability map consistent with well test measurements
• Computation of entanglement entropy in inhomogeneous free fermions chains by algebraic Bethe ansatz
• Searching for Supernovae in HETDEX Data Release 3
• Analytic auto-differentiable $\Lambda$CDM cosmography
• Accurate computation of chemical contrast in field ion microscopy
• COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3<z<4$
• Diabatic quantum and classical annealing of the Sherrington-Kirkpatrick model
• Photometry of the Four Anti-Galactocentric Old Open Clusters: Czernik 30, Berkeley 34, Berkeley 75, and Berkeley 76
• A Close-in Planet Orbiting Giant Star HD 167768
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• PATHFINDER: Designing Stimuli for Neuromodulation through data-driven inverse estimation of non-linear functions
• Stability of the manifold boundary approximation method for reductions of nuclear structure models
• Elemental Abundances of Kepler Objects of Interest in APOGEE DR17
• Mapping State Transition Susceptibility in Quantum Annealing
• Interplay of gross and fine structures in strongly-curved sheets
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• Enhanced Small-Scale Structure in the Cosmic Dark Ages
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• Cosmological perturbation theory using generalized Einstein de Sitter cosmologies
• Trigonal warping effects on optical properties of anomalous Hall materials
• Probing Disorder in 2CzPN using Core and Valence States
• Weighing the Darkness III: How Gaia Could, but Probably Won't, Astrometrically Detect Free-Floating Black Holes
• Instabilities in a current sheet with plasma jet
• The complex dynamical past and future of double eclipsing binary CzeV343: misaligned orbits and period resonance
• Unexpected solar-cycle variation of acoustic mode power in Sun-as-a-star observations
• A Novel Solution for Resonant Scattering Using Self-Consistent Boundary Conditions
• Inflation from a chaotic potential with a step
• Correlated metallic two-particle bound states in Wannier--Stark flatbands
• Multiplicity Statistics of Stars in the Sagittarius Dwarf Spheroidal Galaxy: Comparison to the Milky Way
• Transverse Vector Decomposition Method for Analytical Inversion of Exoplanet Transit Spectra
• Constructing Local Bases for a Deep Variational Quantum Eigensolver for Molecular Systems
• Energetic neutron identification with pulse shape discrimination in pure CsI crystals
• Toolkit for Scalar Fields in Universes with finite-dimensional Hilbert Space
• Two parameter scaling in the crossover from symmetry class BDI to AI
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Forming short period sub-stellar companions in 47 Tuc: I. Dynamical model and brown dwarf tidal capture rates
• 3D Kinematics of Stellar SiO Masers in the Galactic Center
• K2 Discovery of a Circumsecondary Disk Transiting EPIC 220208795
• Spatial variation in temperature and density in the IC 63 PDR from ${\mathrm{H}}_2$ Spectroscopy
• New applications for the Boris Spectral Deferred Correction algorithm for plasma simulations
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• Estimating Total Lung Volume from Pixel-level Thickness Maps of Chest Radiographs Using Deep Learning
• Molecules with ALMA at Planet-forming Scales (MAPS XVIII): Kinematic Substructures in the Disks of HD 163296 and MWC 480
• Molecules with ALMA at Planet-forming Scales (MAPS) XIX. Spiral Arms, a Tail, and Diffuse Structures Traced by CO around the GM Aur Disk
• Out-of-focus holography at the Effelsberg telescope
• Molecules with ALMA at Planet-forming Scales (MAPS) III: Characteristics of Radial Chemical Substructures
• Wavelet Selection and Employment for Side-Channel Disassembly
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
• Approach for modeling single branches of meadow orchard trees with 3D point clouds
• Axion-Photon Conversion in Neutron Star Magnetospheres: The Role of the Plasma in the Goldreich-Julian Model
• Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-7219
• Adsorption from Binary Liquid Solutions into Mesoporous Silica: A Capacitance Isotherm on 5CB Nematogen/Methanol Mixtures
• A Bayesian method for point source polarization estimation
• Generalized asymptotic formulae for estimating statistical significance in high energy physics analyses
• Inferring Time-Dependent Distribution Functions from Kinematic Snapshots
• A Bayesian neural network predicts the dissolution of compact planetary systems
• Q4EDA: A Novel Strategy for Textual Information Retrieval Based on User Interactions with Visual Representations of Time Series
• A variational discrete element method for the computation of Cosserat elasticity
• On the best choice of Lasso program given data parameters
• Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below $z=1.0$
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Cerman: Software for simulating streamer propagation in dielectric liquids based on the Townsend-Meek criterion
• The Possible Equation Of State Of Dark Matter in Low Surface Brightness Galaxies
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Positivity-Preserving Adaptive Runge-Kutta Methods
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• On the Deepest Search for Galactic Center Pulsars and an Examination of an Intriguing Millisecond Pulsar Candidate
• Warps survive beyond fly-by encounters in protoplanetary disks. RW Aur A as a case study
• VEGA: Voids idEntification using Genetic Algorithm
• Non-Exchangeable Conformal Risk Control
• A coherent full microwave scattering formulation for random layered media
• MirrorCBO: A consensus-based optimization method in the spirit of mirror descent
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• CHANG-ES XXXVII. Effects of spectral aging on radio scale heights
• zELDA II: reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• A Comparison of Strategies to Embed Physics-Informed Neural Networks in Nonlinear Model Predictive Control Formulations Solved via Direct Transcription
• Photonic Interactions with Semiconducting Barrier Discharges
• SPLENDAQ: A Detector-Agnostic Data Acquisition System for Small-Scale Physics Experiments
• What to expect from scalar-tensor space geodesy
• Comparison of Herschel and ArTéMiS observations of massive filaments
• Efficient Shapley Performance Attribution for Least-Squares Regression
• Long-distance genuine multipartite Entanglement between Magnetic Defects in Spin Chains
• Estimating the contribution of foreground halos to the FRB 180924 dispersion measure
• Constants of motion in gravitational self-force theory
• Automatic Machine Learning Framework to Study Morphological Parameters of AGN Host Galaxies within $z<1.4$ in the Hyper Supreme-Cam Wide Survey
• Synthesis of pulses from particle detectors with a Generative Adversarial Network (GAN)
• New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
• MeerKAT discovery of GHz radio emission extending from Abell 3017 toward Abell 3016
• Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra I cluster. V. Integrated stellar population properties
• Learning atomic forces from uncertainty-calibrated adversarial attacks
• SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• The HI gas fraction scaling relation of the Green Pea galaxies
• A Constrained Optimisation Framework for Parameter Identification of the SIRD Model
• Signatures of cubic gravity in the strong regime
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• Galactic magnetic fields II. Applying the model to nearby galaxies
• Testing solar surface flux transport models in the first days after active region emergence
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• EISPY2D: An Open-Source Python Library for the Development and Comparison of Algorithms in Two-Dimensional Electromagnetic Inverse Scattering Problems
• Extending the definition of atomic basis sets to atoms with fractional nuclear charge
• Variance-Reduced Stochastic Optimization for Efficient Inference of Hidden Markov Models
• LASED: A Laser-Atom Interaction Simulator derived from Quantum Electrodynamics
• The Indian Pulsar Timing Array Data Release 2: II. Customised Single-Pulsar Noise Analysis and Noise Budget
• A search for photometric variability towards the globular cluster M3 with the TWenty Inch Survey Telescope
• From isolated polyelectrolytes to star-like assemblies: The role of sequence heterogeneity on the statistical structure of the intrinsically disordered Neurofilament-low tail domain
• Time delay interferometry with minimal null frequencies and shortened time span
• A CFL condition for the finite cell method
• Fast, accurate, and predictive method for atom detection in site-resolved images of microtrap arrays
• Thermal Models of Asteroids with Two-band Combinations of Wide-field Infrared Survey Explorer Cryogenic Data
• Spatial distribution and clustering properties of the young stellar populations in the Carina Nebula complex and Car OB1
• A search for transiting companions in the J1407 (V1400 Cen) system
• Hidden facts in Landau-Zener transitions revealed by the Riccati Equation
• Asymmetry at Low Surface Brightness as an Indicator of Environmental Processes in the Fornax Cluster
• Elucidating Many-Body Effects in Molecular Core Spectra through Real-Time Approaches: Efficient Classical Approximations and a Quantum Perspective
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Theory of Generalized Hertzian Hyperspheres
• Exploration of faint X-ray and radio sources in the massive globular cluster M14: A UV-bright counterpart to Nova Ophiuchus 1938
• Knobs and dials of retrieving JWST transmission spectra. II. Impacts of pipeline-level differences on retrieval posteriors
• Syndrome decoding by quantum approximate optimization
• Possible counterpart signal of the Fermi bubbles at the cosmic-ray positrons
• Software implemented fault diagnosis of natural gas pumping unit based on feedforward neural network
• KAgoshima Galactic Object survey with Nobeyama 45-metre telescope by Mapping in Ammonia lines (KAGONMA): Discovery of parsec-scale CO depletion in the Canis Major star-forming region
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Analysis of late-time tails in spin-aligned eccentric binary black hole mergers
• Photonuclear treatment for spent fuel radiotoxicity reduction: a case study investigation on minor actinides
• Machine Learning Unveils the Power Law of Finite-Volume Energy Shifts
• Consistencies and inconsistencies in redshift-independent distances
• Exploring the Magnetic Field Geometry in NGC 891 with SOFIA/HAWC+
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Optimal weights and priors in simultaneous fitting of multiple small-angle scattering datasets
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• Mitigation of correlated readout errors without randomized measurements
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods I: Spectral analysis
• Source REconstruction of Arcs behind Cluster Halos (SourceREACH): A New Source Reconstruction Algorithm Optimized for Giant Arcs and Galaxy Cluster Lenses
• CMB Constraints on Loop-Induced Decays of Leptophilic Dark Matter
• A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy
• The viewing angle in AGN SED models, a data-driven analysis
• Studies in Pulse Shape Discrimination for an Optimized ASIC Design
• Models of Vimentin Organization Under Actin-Driven Transport
• Simulated Rotation Measure Sky from Primordial Magnetic Fields
• Investigation of individual pulse emission behaviours from pulsar J1741$-$0840
• XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Climate Change in Hell: Long-Term Variation in Transits of the Evaporating Planet K2-22b
• Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization
• Local models and Bell inequalities for the minimal triangle network
• Testing general relativity with gravitational waves -- improving and extending Modified Dispersion Relation tests
• KerrGeoPy: A Python Package for Computing Timelike Geodesics in Kerr Spacetime
• Towards spinning $U(1)$ gauged non-topological solitons in the model with Chern-Simons term
• The role of entanglement in energy-restricted communication and randomness generation
• Pairwise accelerated failure time regression models for infectious disease transmission in close-contact groups with external sources of infection
• Positive energy density leads to no squeezing
• Exploring the physical properties of Type II Quasar candidates at intermediate redshifts with CIGALE
• An Agent-based Model of Citation Behavior
• The Origin of the Large Magellanic Cloud Globular Cluster NGC 2005
• Ab initio study of angle-resolved electron reflection spectroscopy of few-layer graphene
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIV. A Candidate Type-II Quasar at z=6.1292
• Exploring Scalarized Einstein-Gauss-Bonnet Theories Through the Lens of Parametrized Post-Newtonian Formalism
• Period-Luminosity Relations for Galactic Type II Cepheids in the Sloan bands
• A disk and no signatures of tidal distortion in the galaxy "lacking" dark matter NGC 1052-DF2
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• Implementation of the Emulator-based Component Analysis
• The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars
• Identifying substructure associations in the Milky Way halo using chemo-kinematic tagging
• Taking control of compressible modes: bulk viscosity and the turbulent dynamo
• Natural polynomials for Kerr quasi-normal modes
• DKIST resolves sub-arcsec photospheric scattering polarization
• The Gaia-ESO Survey: new spectroscopic binaries in the Milky Way
• Thermal Evolution of an Active Region through Quiet and Flaring Phases as Observed by NuSTAR XRT, and AIA
• Helioseismological determination of the subsurface spatial spectrum of solar convection: Demonstration using numerical simulations
• Higher-Order Mean-Motion Resonances Can Form in Type-I Disk Migration
• On-sky Demonstration of Subdiffraction-limited Astronomical Measurement Using a Photonic Lantern
• Structure formation in O-type stars and Wolf-Rayet stars
• Immersed Cantilever Apparatus for Mechanics and Microscopy
• Pulsed Magnetophononics in Gapped Quantum Magnets
• Approximation of sea surface velocity field by fitting surrogate two-dimensional flow to scattered measurements
• Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
• Two-body currents at finite momentum transfer and applications to M1 transitions
• COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS
• PhotoD with LSST: Stellar Photometric Distances Out to the Edge of the Galaxy
• Identification of stellar-mass black hole binaries and the validity of linear orbital motion approximation in microlensing
• Single and Multi-Objective Optimization of Distributed Acoustic Sensing Cable Layouts for Geophysical Applications
• Engineering the uncontrollable: Steering noisy spin-correlated radical-pairs with coherent and incoherent control
• Learning effective good variables from physical data
• Probing evolution of Long GRB properties through their cosmic formation history aided by Machine Learning predicted redshifts
• Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space
• Quantum Optimization Benchmarking Library - The Intractable Decathlon
• Exploring the quasar disc-wind-jet connection with LoTSS and SDSS
• A Broad Grid of 2D Kilonova Emission Models
• Considerations for optimizing photometric classification of supernovae from the Rubin Observatory
• Probabilistic plugging of airways by sliding mucus films
• Modulational instability in large-amplitude linear laser wakefields
• State Specific Measurement Protocols for the Variational Quantum Eigensolver
• Analysis of 42 years of Cosmic Ray Measurements by the Neutron Monitor at Lomnický stít Observatory
• Mass scaling relations for dark halos from an analytic universal outer density profile
• Considerations with stacking absorption spectra: cold HI gas in cirrus region of the Milky Way
• A comparison of shrinkage estimators of the cosmological precision matrix
• Interplay of large-scale drift and turbulence in the heliospheric propagation of solar energetic particles
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Stable and efficient FEM-BEM coupling with OSRC regularisation for acoustic wave transmission
• Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attention
• Shape-Driven Selection Effects for Aspherical Near-Earth Objects in Systematic Surveys
• Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
• Astrophysical uncertainties challenge 21-cm forecasts: A primordial black hole case study
• The Effect of Hydration and Dynamics on the Mass Density of Single Proteins
• Determination of Navier's slip parameter using data assimilation
• Intermodulation spectroscopy and the nonlinear response of two-level systems in superconducting coplanar waveguide resonators
• How Internal Structure Shapes the Metallicity of Giant Exoplanets
• Accelerating the time-domain LISA response model with central finite differences and hybridization techniques
• The Arp 240 Galaxy Merger: A Detailed Look at the Molecular Kennicutt-Schmidt Star Formation Law on Sub-kpc Scales
• SDSS J100711.74+193056.2: A Candidate Common Motion Substellar Companion to the Nearest B-Type Star Regulus
• A Parametrized Test of General Relativity for LISA Massive Black Hole Binary Inspirals
• Bright [CII]158$\mu$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at $z=4.3$
• Reconstructing the Sun's Alfvén surface and wind braking torque with Parker Solar Probe
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: II. Angular Power Spectra and Likelihood
• Bayesian approach to equipartition estimation of magnetic field strength
• NLO Oriented Event-Shape Distributions for Massive Quarks
• A Global Perspective with Updated Constraints on the Ultra-hot Jupiter WASP-19b: Atmospheric Properties and Stellar Activity
• Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
• Typical Machine Learning Datasets as Low-Depth Quantum Circuits
• Fast Generation of Feasible Trajectories in Direct Optimal Control
• The evolution of velocity dispersion in the Sco-Cen OB association
• The Statistic Analysis of GeV Spectral Breaks in Bright Gamma-Ray FSRQs
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• OGLE-2017-BLG-1038: A Possible Brown-dwarf Binary Revealed by Spitzer Microlensing Parallax
• A continuous calibration of the ATLAS flavour-tagging classifiers via optimal transportation maps
• Efficient tensor networks for control-enhanced quantum metrology
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
• Lindblad-like quantum tomography for non-Markovian quantum dynamical maps
• Testing the Impact of Planet-stirring, Self-stirring, and Mixed-stirring on Debris Disc Architecture: A Case Study of HD 16743
• The systemic recoil velocity distribution and the scale height of field millisecond pulsar systems: Implications on neutron star retention fractions in star clusters
• Large deviations of connected components in the stochastic block model
• Relating spatially resolved optical attenuation, dust and gas in nearby galaxies
• Seeds of imperfection rule the mesocrystalline disorder in natural anhydrite single crystals
• RIANN -- A Robust Neural Network Outperforms Attitude Estimation Filters
• Galaxy-scale lens search in the PEARLS NEP TDF and CEERS JWST fields
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• Amoeba: An AGN Model of Optical Emissions Beyond steady-state Accretion discs
• Detecting cosmic voids via maps of geometric-optics parameters
• Using Elliptical Galaxy Kinematics to Compare of the Strength of Gravity in Cosmological Regions of Differing Gravitational Potential -- A First Look
• NASIM: Revealing the low surface brightness Universe from legacy VISTA data
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• CECILIA: Ultra-Deep Rest-Optical Spectra of Faint Galaxies at Cosmic Noon
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• Studying the variability of the He triplet to understand the detection limits of evaporating exoplanet atmospheres
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• Measurement of the photosphere oblateness of $\gamma$ Cassiopeiae via Stellar Intensity Interferometry with the VERITAS Observatory
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• Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission
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• Study of the Inner Structure of the Molecular Torus in IRAS 08572+3915 NW with Velocity Decomposition of CO Rovibrational Absorption Lines
• Learning Post-Newtonian Corrections from Numerical Relativity
• Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Virtual Realities: Is there only one advanced image display that astronomers need?
• Optimized tandem catalyst patterning for CO${}_2$ reduction flow reactors
• Dynamical orbital evolution scenarios of the wide-orbit eccentric planet HR 5183b
• Efficient Search for Detection Candidates Using a Peak Finder Strategy for All-Sky-All-Frequency Gravitational Wave Radiometer
• The Atacama Cosmology Telescope: Machine Learning Driven Tools for Detecting Millimeter Sources in Timestream Pre-processing
• Numerical analysis of a non-clamped dynamic thermoviscoelastic contact problem
• Yano-Schrödinger Hyperfluid: Cosmological Implications
• Optimisation-Based Coupling of Finite Element Model and Reduced Order Model for Computational Fluid Dynamics
• Star Formation Histories and Stellar Dynamics in the Central Galaxies of RX J0820.9+0752, A1835, and PKS 0745-191
• Measuring Scaling Relationships: Fitting Technique Matters
• Thomson scattering above solar active regions and an ad-hoc polarization correction method for the emissive corona
• Quantitative and Optimal Device-Independent Lower Bounds on Detection Efficiency
• MOMOS: The Multi-Object MKID Optical Spectrometer Simulator and Data Reduction Package
• Causal inference in time series in terms of Rényi transfer entropy
• A Fully Three-Dimensional Kinetic Particle-In-Cell Framework for Modeling Laser-Dielectric Interactions: Few-Cycle Pulse Damage
• Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles
• Evolution of solar surface inflows around emerging active regions
• Probing accretion dynamics and spin evolution in the X-ray pulsar RX J0520.5-6932 during its 2024 Outburst
• On the Age Calibration of Open Clusters using Red Clump Stars
• A deep ALMA Band 3 survey of HDFS/MUSE3D: Survey description and initial results
• Incorporation of physics-based strengthening coefficients into phenomenological crystal plasticity models
• Interaction as Interference: A Quantum-Inspired Aggregation Approach
• Finite inflation in curved space
• Critical Motility-Induced Phase Separation in Three Dimensions is Consistent with Ising Universality
• The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder V. Rotational measurements of NGC 891
• Skykatana: a scalable framework to construct sky masks for the Vera Rubin Observatory and large astronomical surveys
• Unveiling SN 2022eyw: A Bright Member of the Type Iax Supernova Subclass
• Stellar Cores Live Long and Prosper in Cuspy Dark Matter Halos
• Aerosol deposition in mucus-lined ciliated airways
• EstrellaNueva: an open-source software to study the interactions and detection of neutrinos emitted by supernovae
• Picosecond laser test unit for photosensor characterization at ambient and low temperatures
• Static Charged Polytropic Spheres with a Cosmological Constant: Physical Acceptability and Trapped Orbits
• Multivariate Uncertainty Quantification with Tomographic Quantile Forests
• Transfer Learning Bayesian Optimization to Design Competitor DNA Molecules for Use in Diagnostic Assays
• Coronagraphic Data Post-processing Using Projections on Instrumental Modes
• QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon
• Readdressing the contribution of photonuclear reactions to the muon content of extensive air showers: a heuristic approach
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• cosmokdtree: a flexible OpenMP-parallelized k-d tree for computational astrophysics applications
• Time Delay Cosmography: Analysis of Quadruply Lensed QSO SDSSJ1433 from Wendelstein Observatory
• Rotational Light-curve Recovery and Predictions of the LSST Yield of Hildas
• Data-Driven Predictions for Dark Photon and Millicharged Particle Production
• Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
• MUSE Analysis of Gas around Galaxies (MAGG) -- VII. Emission line galaxies near strong blended Ly$\alpha$ absorption systems at $z\gtrsim 3$
• Measurements of quasar proximity zones with the Ly$\alpha$ forest of DESI Y1 quasars
• The Sesquinary Catastrophe on Deimos can reconcile its excited past with its dynamically cool present
• VLCs: Managing Parallelism with Virtualized Libraries
• Orbital alignment of HD 332231 b
• Projected sensitivity of CTAO to axion-like particles from blazars with a machine learning approach
• Design optimization of tendon-driven robots considering tendon wrapping and shortcut
• CWTHF: Subhalo Identification with Continuous Wavelet Transform
• Constraining the selection corrected luminosity function and total pulse count for radio transients
• (Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383
• Across the Universe: GW231123 as a magnified and diffracted black hole merger
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Cosmological perturbations on an averaged background
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• Testing MOND using the dynamics of nearby stellar streams
• Pulsars identified in the LOFAR Two-metre Sky Survey at 144 MHz
• Dynamical mass determination and partial eclipses of the heartbeat star HD 181793
• Nusselt number for steady periodically developed heat transfer in micro- and mini-channels with arrays of offset strip fins subject to a uniform heat flux
• Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• LibppRPA: An Open-Source Library for Particle-Particle Random Phase Approximation
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Near-degeneracy effects in Quadrupolar Mixed Modes. From an Asymptotic Description to Data Fitting
• A Near-Earth Object Model Calibrated to Earth Impactors