The NumPy array: a structure for efficient numerical computation

Abstract

In the Python world, NumPy arrays are the standard representation for numerical data. Here, we show how these arrays enable efficient implementation of numerical computations in a high-level language. Overall, three techniques are applied to improve performance: vectorizing calculations, avoiding copying data in memory, and minimizing operation counts. We first present the NumPy array structure, then show how to use it for efficient computation, and finally how to share array data with other libraries.

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• Self-consistent Stellar Radial Velocities from LAMOST Medium-Resolution Survey (MRS) DR7
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: I. Kinematics of the stellar body
• A New Window into Planet Formation and Migration: Refractory-to-Volatile Elemental Ratios in Ultra-hot Jupiters
• Impact of non-parabolic electronic band structure on the optical and transport properties of photovoltaic materials
• Expanding associations in the Vela-Puppis region: 3D structure and kinematics of the young population
• The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
• The Formation of Isolated Ultra-Diffuse Galaxies in Romulus25
• Survival and mass growth of cold gas in a turbulent, multiphase medium
• Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band
• 3-D selection of 167 sub-stellar companions to nearby stars
• The PHLEK Survey: A New Determination of the Primordial Helium Abundance
• A New Generation of Cool White Dwarf Atmosphere Models. I. Theoretical Framework and Applications to DZ Stars
• Machine-Learning-Based Multiple Abnormality Prediction with Large-Scale Chest Computed Tomography Volumes
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• The Faint End of the z=5 Quasar Luminosity Function from the CFHTLS
• Exploiting plume structure to decode gas source distance using metal-oxide gas sensors
• pyJac: analytical Jacobian generator for chemical kinetics
• Characterization and Photometric Performance of the Hyper Suprime-Cam Software Pipeline
• A survey of C2H, HCN, and C18O in protoplanetary disks
• Searching for Light Relics with Large-Scale Structure
• How galaxies form stars: the connection between local and global star formation in galaxy simulations
• A physically motivated definition for the size of galaxies in an era of ultra-deep imaging
• The Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios
• The GTC exoplanet transit spectroscopy survey IX. Detection of Haze, Na, K, and Li in the super-Neptune WASP-127b
• A dusty veil shading Betelgeuse during its Great Dimming
• TESS full orbital phase curve of the WASP-18b system
• Double Trouble: Two Transits of the Super-Earth GJ 1132 b Observed with JWST NIRSpec G395H
• Negative cosmological constant in the dark sector?
• A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg${}^2$ of SPTpol Temperature and Polarization Data
• Detecting and Characterizing Young Quasars I: Systemic Redshifts and Proximity Zones Measurements
• Extended stellar systems in the solar neighborhood - II. Discovery of a nearby 120° stellar stream in Gaia DR2
• The population of long-period transiting exoplanets
• High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta
• Final Targeting Strategy for the SDSS-IV APOGEE-2S Survey
• Characterizing the variable dust permeability of planet-induced gaps
• Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data
• A survey of high-$z$ galaxies: SERRA simulations
• Final Targeting Strategy for the SDSS-IV APOGEE-2N Survey
• Architectures of Exoplanetary Systems. III: Eccentricity and Mutual Inclination Distributions of AMD-stable Planetary Systems
• The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at $z<1$
• The GALAH survey and Gaia DR2: Linking ridges, arches and vertical waves in the kinematics of the Milky Way
• qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients
• galstreams: A Library of Milky Way Stellar Stream Footprints and Tracks
• The CALYMHA survey: Ly$\alpha$ escape fraction and its dependence on galaxy properties at $z=2.23$
• Detection of the LMC-induced sloshing of the Galactic halo
• Orbital evolution of binary black holes in active galactic nucleus disks: a disk channel for binary black hole mergers?
• Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way
• A census of symbiotic stars in the 2MASS, WISE and Gaia surveys
• The X-shooter GRB afterglow legacy sample (XS-GRB)
• The Distribution and Excitation of CH${}_3$CN in a Solar Nebula Analog
• The star formation history of the Sco-Cen association. Coherent star formation patterns in space and time
• Electronic Structure Trends Across the Rare-Earth Series in Superconducting Infinite Layer Nickelates
• Observationally driven Galactic double white dwarf population for LISA
• Connecting Young Star Clusters to CO Molecular Gas in NGC 7793 with ALMA-LEGUS
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• pyspeckit: A spectroscopic analysis and plotting package
• Julia: A Fresh Approach to Numerical Computing
• On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
• Follow-up of the Neutron Star Bearing Gravitational Wave Candidate Events S190425z and S190426c with MMT and SOAR
• Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Kinematics of Antlia 2 and Crater 2 from The Southern Stellar Stream Spectroscopic Survey (S5)
• WASP-107b's density is even lower: a case study for the physics of planetary gas envelope accretion and orbital migration
• Using Gaia DR2 to Constrain Local Dark Matter Density and Thin Dark Disk
• The Spatial Relation between Young Star Clusters and Molecular Clouds in M 51 with LEGUS
• The information content in cold stellar streams
• Image-based deep learning for classification of noise transients in gravitational wave detectors
• Inferring Explosion Properties from Type II-Plateau Supernova Light Curves
• Modeling non-thermal emission from the jet-launching region of M 87 with adaptive mesh refinement
• A Physical Model-based Correction for Charge Traps in the Hubble Space Telescope's Wide Field Camera 3 Near-IR Detector and Applications to Transiting Exoplanets and Brown Dwarfs
• Streaming Instability for Particle-Size Distributions
• Gaia EDR3 Reveals the Substructure and Complicated Star Formation History of the Greater Taurus-Auriga Star Forming Complex
• Morpheus: A Deep Learning Framework For Pixel-Level Analysis of Astronomical Image Data
• $S^5$: The Orbital and Chemical Properties of One Dozen Stellar Streams
• High star cluster formation efficiency in the strongly lensed Sunburst Lyman-continuum galaxy at z=2.37
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• Beacons into the Cosmic Dark Ages: Boosted transmission of Ly$\alpha$ from UV bright galaxies at $z\gtrsim 7$
• A Deeper Look at the New Milky Way Satellites: Sagittarius II, Reticulum II, Phoenix II, and Tucana III
• Two Ultra-Faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey
• The R-Process Alliance: A Comprehensive Abundance Analysis of HD 222925, a Metal-Poor Star with an Extreme R-Process Enhancement of [Eu/H] = -0.14
• A comparison of Alpha Particle and Proton Beam Differential flow in Collisionally Young Solar Wind
• Benzonitrile as a proxy for benzene in the cold ISM: low temperature rate coefficients for CN + C${}_6$H${}_6$
• PRECESSION: Dynamics of spinning black-hole binaries with python
• JWST Noise Floor I: Random Error Sources in JWST NIRCam Time Series
• Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs
• Radiative Mixing Layers: Insights from Turbulent Combustion
• The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and $Gaia$ eDR3
• LACEwING: A New Moving Group Analysis Code
• Frankenstein: Protoplanetary disc brightness profile reconstruction at sub-beam resolution with a rapid Gaussian process
• Optical turbulence profiling with Stereo-SCIDAR for VLT and ELT
• PyAutoLens: Open-Source Strong Gravitational Lensing
• Long Dark Gaps in the Ly$\beta$ Forest at $z<6$: Evidence of Ultra Late Reionization from XQR-30 Spectra
• The nature of luminous Lyman-alpha emitters at z~2-3: maximal dust-poor starbursts and highly ionising AGN
• The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds
• Early light curves for Type Ia supernova explosion models
• The population of M dwarfs observed at low radio frequencies
• Multicolour photometry for exoplanet candidate validation
• Reconstructing the Disrupted Dwarf Galaxy $Gaia$-Sausage/Enceladus Using its Stars and Globular Clusters
• Inferring the properties of a population of compact binaries in presence of selection effects
• Confirmation of WASP-107b's extended Helium atmosphere with Keck II/NIRSPEC
• Natural Language Generation for Electronic Health Records
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• The Southern Stellar Stream Spectroscopic Survey (S5): Chemical Abundances of Seven Stellar Streams
• An Introduction to Programming for Bioscientists: A Python-based Primer
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data
• Kronos & Krios: Evidence for accretion of a massive, rocky planetary system in a comoving pair of solar-type stars
• Dual constraints with ALMA: new [O III] 88 $\mu$m and dust-continuum observations reveal the ISM conditions of luminous LBGs at $z\sim 7$
• The CARMA-NRO Orion Survey
• Proper motions of Milky Way Ultra-Faint satellites with $Gaia$ DR2 $\times$ DES DR1
• Using dust, gas and stellar mass selected samples to probe dust sources and sinks in low metallicity galaxies
• Virtual orbital many-body expansions: A possible route towards the full configuration interaction limit
• Non-detection of TiO and VO in the atmosphere of WASP-121b using high-resolution spectroscopy
• MMT Spectroscopy of Lyman-alpha at z$\simeq$7: Evidence for Accelerated Reionization Around Massive Galaxies
• A New Generation of Cool White Dwarf Atmosphere Models. IV. Revisiting the Spectral Evolution of Cool White Dwarfs
• Orbital Clustering Identifies the Origins of Galactic Stellar Streams
• Tidal interactions between binary stars drives lithium production in low-mass red giants
• Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
• Autonomous Gaussian Decomposition
• The Warm Neptune GJ 3470b has a Polar Orbit
• Kinematics of Highly R-Process-Enhanced Field Stars: Evidence for an Accretion Origin and Detection of Several Groups from Disrupted Satellites
• A NICER View of PSR J1231$-$1411: A Complex Case
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess
• Tidal disruptions by rotating black holes: effects of spin and impact parameter
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• preCICE v2: A Sustainable and User-Friendly Coupling Library
• The environmental dependence of the X_CO conversion factor
• Reionization after JWST: a photon budget crisis?
• GaussPy+: A fully automated Gaussian decomposition package for emission line spectra
• Measuring the properties of reionised bubbles with resolved Lyman alpha spectra
• Probing Massive Black Hole Binary Populations with LISA
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• Molecules with ALMA at Planet-forming Scales (MAPS). VII. Sub-stellar O/H and C/H and super-stellar C/O in planet feeding gas
• A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era
• Full Transport General Relativistic Radiation Magnetohydrodynamics for Nucleosynthesis in Collapsars
• Massive BH Binaries as Periodically-Variable AGN
• The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
• DarkHistory: A code package for calculating modified cosmic ionization and thermal histories with dark matter and other exotic energy injections
• Rayleigh scattering in the transmission spectrum of HAT-P-18b
• Long Term Photometric Variability in Kepler Full Frame Images: Magnetic Cycles of Sun-Like Stars
• High-redshift radio galaxies: a potential new source of 21-cm fluctuations
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region
• Evidence for He I 10830 Å~ absorption during the transit of a warm Neptune around the M-dwarf GJ 3470 with the Habitable-zone Planet Finder
• Characterisation of the ionosphere above the Murchison Radio Observatory using the Murchison Widefield Array
• Merger-Induced Metallicity Dilution in Cosmological Galaxy Formation Simulations
• Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
• The Neutrino Fast Flavor Instability in Three Dimensions
• Supernova Model Discrimination with Hyper-Kamiokande
• Large-Scale Mixing in a Violent Oxygen-Neon Shell Merger Prior to a Core-Collapse Supernova
• Bilby-MCMC: An MCMC sampler for gravitational-wave inference
• High-Performance Tensor Contraction without Transposition
• Hot gas around SN 1998bw: Inferring the progenitor from its environment
• Prevalence of Complex Organic Molecules in Starless and Prestellar Cores within the Taurus Molecular Cloud
• Detection of a Westward Hotspot Offset in the Atmosphere of a Hot Gas Giant CoRoT-2b
• The spatially resolved star formation history of CALIFA galaxies: Cosmic time scales
• The Sparkler: Evolved High-Redshift Globular Clusters Captured by JWST
• Unsupervised machine learning of topological phase transitions from experimental data
• SWIGLAL: Python and Octave interfaces to the LALSuite gravitational-wave data analysis libraries
• Discriminating Accretion States via Rotational Symmetry in Simulated Polarimetric Images of M87
• 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
• Optical phase curve of the ultra-hot Jupiter WASP-121b
• A unique hot Jupiter spectral sequence with evidence for compositional diversity
• A Flare-Type IV Burst Event from Proxima Centauri and Implications for Space Weather
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• No Such Thing as a Simple Flare: Substructure and QPPs Observed in a Statistical Sample of 20 Second Cadence TESS Flares
• Reflex motion in the Milky Way stellar halo resulting from the Large Magellanic Cloud infall
• EvryFlare III: Temperature Evolution and Habitability Impacts of Dozens of Superflares Observed Simultaneously by Evryscope and TESS
• The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization
• Predicting Quasar Continua Near Lyman-$\alpha$ with Principal Component Analysis
• Source Selection for Cluster Weak Lensing Measurements in the Hyper Suprime-Cam Survey
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• The Evolution of the Lyman-Alpha Luminosity Function During Reionization
• The Three Causes of Low-Mass Assembly Bias
• Origins of Hot Jupiters from the Stellar Obliquity Distribution
• All the PAHs: an AKARI-Spitzer Cross Archival Spectroscopic Survey of Aromatic Emission in Galaxies
• Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science
• Testing the radius scaling relation with $Gaia$ DR2 in the $Kepler$ field
• Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
• The X-SHOOTER Lyman-$\alpha$ survey at z=2 (XLS-z2) I: What makes a galaxy a Lyman-$\alpha$ emitter?
• PiNN: A Python Library for Building Atomic Neural Networks of Molecules and Materials
• The fast radio burst population evolves, consistent with the star-formation rate
• A novel DOI Positioning Algorithm for Monolithic Scintillator Crystals in PET based on Gradient Tree Boosting
• Particle-in-cell Simulation of the Neutrino Fast Flavor Instability
• The Local Group as a time machine: studying the high-redshift Universe with nearby galaxies
• First Constraint on the Neutrino-Induced Phase Shift in the BAO Spectrum
• Evidence of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters
• Warm dust in high-z galaxies: origin and implications
• Model-independent constraints on the hydrogen-ionizing emissivity at z>6
• The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416
• The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift
• zeus: A Python implementation of Ensemble Slice Sampling for efficient Bayesian parameter inference
• Multi-messenger tests of gravity with weakly lensed gravitational waves
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• The properties of "dark" ΛCDM halos in the Local Group
• Scaling Relations for Dark Matter Annihilation and Decay Profiles in Dwarf Spheroidal Galaxies
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Evidence For A Vertical Dependence on the Pressure Structure in AS 209
• Continuum Reverberation Mapping of the Accretion Disks in Two Seyfert 1 Galaxies
• A comparison of Galactic electron density models using PyGEDM
• Computing vibrational eigenstates with tree tensor network states (TTNS)
• Exploring the age dependent properties of M and L dwarfs using Gaia and SDSS
• Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
• Analysis of a JWST NIRSpec Lab Time Series: Characterizing Systematics, Recovering Exoplanet Transit Spectroscopy, and Constraining a Noise Floor
• Atmospheric mass loss due to giant impacts: the importance of the thermal component for hydrogen-helium envelopes
• Unlocking Galactic Wolf-Rayet stars with $\text{Gaia}$ DR2 I: Distances and absolute magnitudes
• Performance Verification of the EXtreme PREcision Spectrograph
• Transiting exocomets detected in broadband light by TESS in the $\beta$ Pictoris system
• The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) I. Ultraviolet to Infrared Photometry of 22 Million Stars in M33
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Solar wind prediction using deep learning
• The First Tidally Disrupted Ultra-Faint Dwarf Galaxy? - Spectroscopic Analysis of the Tucana III Stream
• Flares in Open Clusters with K2. II. Pleiades, Hyades, Praesepe, Ruprecht 147, and M67
• Star formation history of the Galactic bulge from deep HST imaging of low reddening windows
• rPICARD: A CASA-based Calibration Pipeline for VLBI Data
• 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
• Confirmation of Asymmetric Iron Absorption in WASP-76b with HARPS
• Robustness of dark energy phenomenology across different parameterizations
• Formation histories of stars, clusters and globular clusters in the E-MOSAICS simulations
• Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi
• The Gaia DR3 view of dynamical substructure in the stellar halo near the Sun
• A new technique for finding galaxies leaking Lyman-continuum radiation: [SII]-deficiency
• The Globular Cluster - Dark Matter Halo Connection
• Chemical Abundances of Main-Sequence, Turn-off, Subgiant and red giant Stars from APOGEE spectra I: Signatures of Diffusion in the Open Cluster M67
• An extremely metal poor star complex in the reionization era: Approaching Population III stars with JWST
• Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3
• Photometric redshifts for the Kilo-Degree Survey. Machine-learning analysis with artificial neural networks
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• The Hubble Space Telescope Survey of M31 Satellite Galaxies I. RR Lyrae-based Distances and Refined 3D Geometric Structure
• The Habitable-zone Planet Finder Reveals A High Mass and a Low Obliquity for the Young Neptune K2-25b
• Towards Building an Intelligent Anti-Malware System: A Deep Learning Approach using Support Vector Machine (SVM) for Malware Classification
• First gas-phase metallicity gradients of $0.1\lesssim z\lesssim 0.8$ galaxies with MUSE
• Detection of Atmospheric Escape from Four Young Mini Neptunes
• TESS spots a hot Jupiter with an inner transiting Neptune
• ACCESS & LRG-BEASTS: a precise new optical transmission spectrum of the ultrahot Jupiter WASP-103b
• "Garbage In, Garbage Out" Revisited: What Do Machine Learning Application Papers Report About Human-Labeled Training Data?
• A sub-Neptune sized planet transiting the M2.5-dwarf G 9-40: Validation with the Habitable-zone Planet Finder
• Molecules with ALMA at Planet-forming Scales (MAPS) VI: Distribution of the small organics HCN, C2H, and H2CO
• PHANGS-JWST First Results: A statistical view on bubble evolution in NGC628
• Physics of Eclipsing Binaries. IV. The impact of interstellar extinction on the light curves of eclipsing binaries
• Submillimeter-wave emission of three Galactic red novae: cool molecular outflows produced by stellar mergers
• Variable Outer Disk Shadowing Around the Dipper Star RX J1604.3-2130
• The Sloan Digital Sky Survey extended point spread functions
• TESS-Gaia Light Curve: a PSF-based TESS FFI light curve product
• Missing Red Supergiants and Carbon Burning
• Rapid Variability of Sgr A* across the Electromagnetic Spectrum
• adcc: A versatile toolkit for rapid development of algebraic-diagrammatic construction methods
• GOALS-JWST: Tracing AGN Feedback on the Star-Forming ISM in NGC 7469
• Inferring the IGM Neutral Fraction at z ~ 6-8 with Low-Luminosity Lyman Break Galaxies
• Galactic Archeology with the AEGIS Survey: The Evolution of Carbon and Iron in the Galactic Halo
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• A Hard X-ray Test of HCN Enhancements as a Tracer of Embedded Black Hole Growth
• A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data
• Diffuser-Assisted Infrared Transit Photometry for Four Dynamically Interacting \textit{Kepler} Systems
• Type II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling
• QED at NNLO with McMule
• Coping with loss: Stability of mass transfer from post-main sequence donor stars
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• 21cm foregrounds and polarization leakage: a user's guide on cleaning and mitigation strategies
• Radio observations of the tidal disruption event XMMSL1 J0740$-$85
• Discovery of a Gamma-ray Black Widow Pulsar by GPU-accelerated Einstein@Home
• The Effects of Population III X-ray and Radio Backgrounds on the Cosmological 21-cm Signal
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Think Global, Act Local: The Influence of Environment Age and Host Mass on Type Ia Supernova Light Curves
• Detailed Abundances in the Ultra-faint Magellanic Satellites Carina II and III
• Equilibrium models of the Milky Way mass are biased high by the LMC
• The Persistence of Population III Star Formation
• Metallicity Structure in the Milky Way Disk Revealed by Galactic HII Regions
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• Accelerating astronomical and cosmological inference with Preconditioned Monte Carlo
• ML-MOC: Machine Learning (kNN and GMM) based Membership Determination for Open Clusters
• The EDGE-CALIFA Survey: Evidence for Pervasive Extraplanar Diffuse Ionized Gas in Nearby Edge-On Galaxies
• The path to instability in compact multi-planetary systems
• Evolution of collisional neutrino flavor instabilities in spherically symmetric supernova models
• Systematically Measuring Ultra-Diffuse Galaxies (SMUDGes). V. The Complete SMUDGes Catalog and the Nature of Ultra-Diffuse Galaxies
• GOALS-JWST: Mid-Infrared Spectroscopy of the Nucleus of NGC 7469
• Making AI Forget You: Data Deletion in Machine Learning
• A massive mess: When a large dwarf and a Milky Way-like galaxy merge
• Progressive Analytics: A Computation Paradigm for Exploratory Data Analysis
• Using Recurrent Neural Networks to Optimize Dynamical Decoupling for Quantum Memory
• Predicting Stellar Angular Diameters from $V$, $I_C$, $H$, $K$ Photometry
• MusE GAs FLOw and Wind (MEGAFLOW) VIII. Discovery of a MgII emission halo probed by a quasar sightline
• Broken into Pieces: ATLAS and Aliqa Uma as One Single Stream
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• Towards Consistent Modeling of Atmospheric Chemistry and Dynamics in Exoplanets: Validation and Generalization of Chemical Relaxation Method
• Inhomogeneous phases in the Gross-Neveu model in 1+1 dimensions at finite number of flavors
• Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run
• CMB Polarization B-mode Delensing with SPTpol and Herschel
• Precise Dynamical Masses and Orbital Fits for $\beta$ Pic b and $\beta$ Pic c
• Hydrodynamical Simulations of Black-Hole Binary Formation in AGN Disks
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• Neural networks and kernel ridge regression for excited states dynamics of CH${}_2$NH${}_2^{+}$: From single-state to multi-state representations and multi-property machine learning models
• Temperatures and Metallicities of M dwarfs in the APOGEE Survey
• Far-infrared to millimeter data of protoplanetary disks: dust growth in the Taurus, Ophiuchus, and Chamaeleon I star-forming regions
• Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc
• GA-NIFS: Black hole and host galaxy properties of two z$\simeq$6.8 quasars from the NIRSpec IFU
• Diffprivlib: The IBM Differential Privacy Library
• Detection of Ongoing Mass Loss from HD 63433c, a Young Mini Neptune
• LSDCat: Detection and cataloguing of emission-line sources in integral-field spectroscopy datacubes
• Does the magnetic field suppress fragmentation in massive dense cores?
• Direct Imaging Discovery and Dynamical Mass of a Substellar Companion Orbiting an Accelerating Hyades Sun-like Star with SCExAO/CHARIS
• Accretion mode versus radio morphology in the LOFAR Deep Fields
• Probing the Protosolar Disk Using Dust Filtering at Gaps in the Early Solar System
• Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution
• The Galaxy Clustering Crisis in Abundance Matching
• From actinides to zinc: Using the full abundance pattern of the brightest star in Reticulum II to distinguish between different r-process sites
• A Tendency Toward Alignment in Single-Star Warm Jupiter Systems
• Constraining the physical properties of the first lensed $z\sim 10-16$ galaxy candidates with JWST
• Spectral Variability of VHS J1256-1257 b from 1 to 5 $\mu$m
• Identifying Type II Strongly Lensed Gravitational-Wave Images in Third-Generation Gravitational-Wave Detectors
• Significance Mode Analysis (SigMA) for hierarchical structures. An application to the Sco-Cen OB association
• Variations in the width, density, and direction of the Palomar 5 tidal tails
• PyCFTBoot: A flexible interface for the conformal bootstrap
• Revealing the tidal scars of the Small Magellanic Cloud
• GPI spectra of HR 8799 c, d, and e from 1.5 to 2.4$\mu$m with KLIP Forward Modeling
• Triggering optical AGN: the need for cold gas, and the indirect roles of galaxy environment and interactions
• Magnetic outflows from turbulent accretion disks: I. Vertical structure & secular evolution
• The Suppression of Star Formation on the Smallest Scales: What Role Does Environment Play?
• On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6
• 3D dynamics of the Orion cloud complex -- Discovery of coherent radial gas motions at the 100-pc scale
• The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
• Cosmological Forecast for non-Gaussian Statistics in large-scale weak Lensing Surveys
• Flares in Open Clusters with K2. I. M45 (Pleiades), M44 (Praesepe) and M67
• BAT AGN Spectroscopic Survey XXI: The Data Release 2 Overview
• Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution
• Dispersal of protoplanetary disks by the combination of magnetically driven and photoevaporative winds
• Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis
• The age of the Milky Way inner stellar spheroid from RR Lyrae population synthesis
• GA-NIFS: The core of an extremely massive proto-cluster at the Epoch of Reionization probed with JWST/NIRSpec
• Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys
• Unintended electromagnetic radiation from Starlink satellites detected with LOFAR between 110 and 188 MHz
• Multi-Gigayear White Dwarf Cooling Delays from Clustering-Enhanced Gravitational Sedimentation
• Gas infall and radial transport in cosmological simulations of Milky Way-mass disks
• Supernova Photometric Classification Pipelines Trained on Spectroscopically Classified Supernovae from the Pan-STARRS1 Medium-Deep Survey
• High performance Python for direct numerical simulations of turbulent flows
• Dynamics of skyrmionic states in confined helimagnetic nanostructures
• The Epoch of IGM heating by early sources of X-rays
• Detection of Hundreds of New Planet Candidates and Eclipsing Binaries in K2 Campaigns 0-8
• Molecules with ALMA at Planet-forming Scales (MAPS). A Circumplanetary Disk Candidate in Molecular Line Emission in the AS 209 Disk
• The chemical inventory of the planet-hosting disk PDS 70
• ABD-Net: Attentive but Diverse Person Re-Identification
• Reignition of Star Formation in Dwarf Galaxies
• Implications for Galaxy Formation Models from Observations of Globular Clusters around Ultra-Diffuse Galaxies
• Aperture-free star formation rate of SDSS star-forming galaxies
• The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
• Probing the Extent of Vertical Mixing in Brown Dwarf Atmospheres with Disequilibrium Chemistry
• The Visible Spectro-Polarimeter of the Daniel K. Inouye Solar Telescope
• Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
• Requirements for gravitational collapse in planetesimal formation --- the impact of scales set by Kelvin-Helmholtz and nonlinear streaming instability
• GJ 367b is a dark, hot, airless sub-Earth
• Slow many-body delocalization beyond one dimension
• The Pyrat Bay Framework for Exoplanet Atmospheric Modeling: A Population Study of Hubble/WFC3 Transmission Spectra
• Wave propagation characteristics of Parareal
• Modeling the Impact of Baryons on Subhalo Populations with Machine Learning
• JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146
• Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
• Astromers: Nuclear Isomers in Astrophysics
• Quenching timescales of dwarf satellites around Milky Way-mass hosts
• Black-hole kicks from numerical-relativity surrogate models
• The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
• Preferential Accretion and Circumbinary Disk Precession in Eccentric Binary Systems
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Many-Body Expanded Full Configuration Interaction. I. Weakly Correlated Regime
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Halogen Bonding in Nucleic Acid Complexes
• Unscrambling the lensed galaxies in JWST images behind SMACS0723
• Exploring the origin of low-metallicity stars in Milky Way-like galaxies with the NIHAO-UHD simulations
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• RASSINE: Interactive tool for normalising stellar spectra I. Description and performance of the code
• Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae
• Anisotropy of the Milky Way's stellar halo using K giants from LAMOST and $Gaia$
• A Galaxy-Targeted Search for the Optical Counterpart of the Candidate NS-BH Merger S190814bv with Magellan
• Six More Ultra-Faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
• Multiple Chemodynamic Stellar Populations of the Ursa Minor Dwarf Spheroidal Galaxy
• Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
• Witnessing the onset of reionisation via Lyman-$\alpha$ emission at redshift 13
• Weighing the Darkness: Astrometric Mass Measurement of Hidden Stellar Companions using Gaia
• pyUPMASK: an improved unsupervised clustering algorithm
• Turbulence-Level Dependence of Cosmic-Ray Parallel Diffusion
• An Extreme Precision Radial Velocity Pipeline: First Radial Velocities from EXPRES
• The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities
• The Little Engines That Could? Globular Clusters Contribute Significantly to Reionization-era Star Formation
• How deep is deep enough? -- Quantifying class separability in the hidden layers of deep neural networks
• Breaking degeneracies in the first galaxies with clustering
• Cosmic shear power spectra in practice
• Escaping Helium from TOI 560.01, a Young Mini Neptune
• Outflows and extended [CII] halos in high redshift galaxies
• Constraints on Metastable Helium in the Atmospheres of WASP-69b and WASP-52b with Ultra-Narrowband Photometry
• Many-Body Expanded Full Configuration Interaction. II. Strongly Correlated Regime
• On the nature and physical conditions of the luminous Lya emitter CR7 and its rest-frame UV components
• Accretion onto Stars in the Disks of Active Galactic Nuclei
• GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane $345^{\circ }<l<67^{\circ }$, $180^{\circ }<l<240^{\circ }$
• Lighting the Dark: The Evolution of the Post-Inflationary Universe
• Interrogating Seyferts with NebulaBayes: Spatially probing the narrow-line region radiation fields and chemical abundances
• The lanthanide fraction distribution in metal-poor stars: a test of neutron star mergers as the dominant r-process site
• Dynamical characterization of galaxies up to $z\sim 7$
• Planck Sunyaev-Zel'dovich Cluster Mass Calibration using Hyper Suprime-Cam Weak Lensing
• The Grism Lens-Amplified Survey from Space (GLASS). XI. Detection of CIV in Multiple Images of $z=6.11$ Ly$\alpha$ Emitter Behind RXCJ2248.7-4431
• The eROSITA Final Equatorial-Depth Survey (eFEDS): Galaxy Clusters and Groups in Disguise
• Triage of the Gaia DR3 astrometric orbits. I. A sample of binaries with probable compact companions
• Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602
• Credit spread approximation and improvement using random forest regression
• Lyman-alpha emitters gone missing: the different evolution of the bright and faint populations
• On the kinematics of a runaway Be star population
• Velocity dispersion in the interstellar medium of early galaxies
• GPU-accelerated massive black hole binary parameter estimation with LISA
• Analyzing Atmospheric Temperature Profiles and Spectra of M dwarf Rocky Planets
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• An 8.8 minute orbital period eclipsing detached double white dwarf binary
• Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• ALMA observations of the narrow HR 4796A debris ring
• Enabling rootless Linux Containers in multi-user environments: the udocker tool
• The Mass of Stirring Bodies in the AU Mic Debris Disk Inferred from Resolved Vertical Structure
• Gas Kinematics in FIRE Simulated Galaxies Compared to Spatially Unresolved HI Observations
• Possible Bright Starspots on TRAPPIST-1
• MuSCAT2 multicolour validation of TESS candidates: an ultra-short-period substellar object around an M dwarf
• Sub-Chandrasekhar progenitors favoured for type Ia supernovae: Evidence from late-time spectroscopy
• Robust and model-independent cosmological constraints from distance measurements
• Local Simulations of Spiral Galaxies with the TIGRESS Framework: I. Star Formation and Arm Spurs/Feathers
• Rotation Period Evolution in Low-Mass Binary Stars: The Impact of Tidal Torques and Magnetic Braking
• Sparsity through evolutionary pruning prevents neuronal networks from overfitting
• Comparing Foreground Removal Techniques for Recovery of the LOFAR-EoR 21cm Power Spectrum
• Velocity-coherent Filaments in NGC 1333: Evidence for Accretion Flow?
• Detecting and Characterizing Young Quasars II: Four Quasars at $z\sim 6$ with Lifetimes $<10^4$ years
• The recent LMC-SMC collision: Timing and impact parameter constraints from comparison of Gaia LMC disk kinematics and N-body simulations
• Calibration of the Halpha Age-Activity relation for M dwarfs
• Strong lens systems search in the Dark Energy Survey using Convolutional Neural Networks
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• Anomaly detection in the Zwicky Transient Facility DR3
• Detection of PAH Absorption and Determination of the Mid-Infrared Diffuse Interstellar Extinction Curve from the Sightline Toward Cyg OB2-12
• SDSS-IV MaNGA: Radial Gradients in Stellar Population Properties of Early-Type and Late-Type Galaxies
• Modelling the observed luminosity function and clustering evolution of Lyman-$\alpha$ emitters: growing evidence for late reionization
• Stellar Mass Black Hole Formation and Multi-messenger Signals from Three Dimensional Rotating Core-Collapse Supernova Simulations
• You Can't Always Get What You Want: The Impact of Prior Assumptions on Interpreting GW190412
• The Frequency of Dwarf Galaxy Multiples at Low Redshift in SDSS vs. Cosmological Expectations
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• Torques Induced by Scattered Pebble-flow in Protoplanetary Disks
• Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
• A circular polarisation survey for radio stars with the Australian SKA Pathfinder
• Peter Pan Disks: Long-lived Accretion Disks Around Young M Stars
• Evaluating approximate asymptotic distributions for fast neutrino flavor conversions in a periodic 1D box
• Constraining the Milky Way Mass Profile with Phase-Space Distribution of Satellite Galaxies
• Dense gas kinematics and a narrow filament in the Orion A OMC1 region using NH3
• AOtools -- a Python package for adaptive optics modelling and analysis
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• LRG-BEASTS: transmission spectroscopy and retrieval analysis of the highly-inflated Saturn-mass planet WASP-39b
• Reinforcement Learning Produces Dominant Strategies for the Iterated Prisoner's Dilemma
• Claimed detection of PH${}_3$ in the clouds of Venus is consistent with mesospheric SO${}_2$
• Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
• Modeling UV Radiation Feedback from Massive Stars: I. Implementation of Adaptive Ray Tracing Method and Tests
• Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
• The Carnegie-Chicago Hubble Program. IX. Calibration of the Tip of the Red Giant Branch Method in the Mega-Maser Host Galaxy, NGC4258 (M106)
• Dust Evolution in Galaxy Cluster Simulations
• A ring in a shell: the large-scale 6D structure of the Vela OB2 complex
• Resolving the extended atmosphere and the inner wind of Mira ($o$ Ceti) with long ALMA baselines
• Construction of Wave Dark Matter Halos: Numerical Algorithm and Analytical Constraints
• Ultra-High-Energy Cosmic Rays from Radio Galaxies
• Large Interferometer For Exoplanets (LIFE): II. Signal simulation, signal extraction and fundamental exoplanet parameters from single epoch observations
• Evolution of the Exoplanet Size Distribution: Forming Large Super-Earths Over Billions of Years
• ASKAP Detection of Periodic and Elliptically Polarized Radio Pulses from UV Ceti
• Two Views of the Radius Gap and the Role of Light Curve Fitting
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• Chemical Abundance Signature of J0023+0307 -- A Second-Generation Main-Sequence Star with [Fe/H]<-6
• Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors
• DASH: Deep Learning for the Automated Spectral Classification of Supernovae and their Hosts
• High-resolution spectroscopy of the GD-1 stellar stream localizes the perturber near the orbital plane of Sagittarius
• PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
• Stellar Wind Confinement of Evaporating Exoplanet Atmospheres and its Signatures in 1083 nm Observations
• Hot Circumsingle Disks Drive Binary Black Hole Mergers in Active Galactic Nucleus Disks
• Stars behind bars I: The Milky Way's central stellar populations
• Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
• Mapping deuterated methanol toward L1544: I. Deuterium fraction and comparison with modeling
• Rapid Rotation in the Kepler Field: Not a Single Star Phenomenon
• The discovery of WASP-151b, WASP-153b, WASP-156b: Insights on giant planet migration and the upper boundary of the Neptunian desert
• Atmospheric turbulence forecasting with a General Circulation Model for Cerro Paranal
• An evolutionary study of volatile chemistry in protoplanetary disks
• Inelastic electron-vortex-beam scattering
• Models of Tidally Induced Gas Filaments in the Magellanic Stream
• Quenching low-mass satellite galaxies: evidence for a threshold ICM density
• Old, Metal-Poor Extreme Velocity Stars in the Solar Neighborhood
• Gaia May Detect Hundreds of Well-characterised Stellar Black Holes
• Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars
• Preventing Anomalous Torques in Circumbinary Accretion Simulations
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• No escaping helium from 55 Cnc e
• Stellar Characterization of M-dwarfs from the APOGEE Survey: A Calibrator Sample for the M-dwarf Metallicities
• Early Time Light Curves of Type Ia Supernovae Observed with TESS
• The post-transit tail of WASP-107b observed at 10830A
• DimReader: Axis lines that explain non-linear projections
• The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
• BACCHUS Analysis of Weak Lines in APOGEE Spectra (BAWLAS)
• A Relationship Between Stellar Metallicity Gradients and Galaxy Age in Dwarf Galaxies
• Blasts from the Past: Supernova Shock Breakouts among X-Ray Transients in the XMM-Newton Archive
• The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at $z=5.4$ with JWST/NIRCam in GOODS-S
• Complex Rotational Modulation of Rapidly Rotating M-Stars Observed with TESS
• Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
• BASS XXVI: DR2 Host Galaxy Stellar Velocity Dispersions
• Pre-Common-Envelope Mass Loss from Coalescing Binary Systems
• The First Maps of ${\kappa }_d$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
• Characterizing the Nature of the Unresolved Point Sources in the Galactic Center
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329
• Large-scale Maps of the Cosmic Infrared Background from Planck
• $B_c\to J/\psi$ Form Factors for the full $q^2$ range from Lattice QCD
• Actinide-rich and Actinide-poor $r$-Process Enhanced Metal-Poor Stars do not Require Separate $r$-Process Progenitors
• The ALMA-PILS survey: First detection of the unsaturated 3-carbon molecules Propenal (C${}_2$H${}_3$CHO) and Propylene (C${}_3$H${}_6$) towards IRAS 16293$-$2422 B
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• Wobble: A Data-driven Analysis Technique for Time-series Stellar Spectra
• Cataloging the radio-sky with unsupervised machine learning: a new approach for the SKA era
• Quasinormal modes and their overtones at the common horizon in a binary black hole merger
• Machine Learning at Microsoft with ML .NET
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search
• Predicting the observational signature of migrating Neptune-sized planets in low-viscosity disks
• 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
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Radiative transfer modelling of W33A MM1: 3-D structure and dynamics of a complex massive star forming region
• Molecules with ALMA at Planet-forming Scales (MAPS) XI: CN and HCN as Tracers of Photochemistry in Disks
• Loo.py: transformation-based code generation for GPUs and CPUs
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• Jet collimation and acceleration in the giant radio galaxy NGC 315
• A comparison of quasar emission reconstruction techniques for $z\ge 5.0$ Lyman-$\alpha$ and Lyman-$\beta$ transmission
• Damping Wing-Like Features in the Stacked Ly$\alpha$ Forest: Potential Neutral Hydrogen Islands at $z<6$
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments
• Joint CMB and BBN Constraints on Light Dark Sectors with Dark Radiation
• Variability of Red Supergiants in M31 from the Palomar Transient Factory
• i-Process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-Peak Neutron-Capture Elements
• The effects of disk self-gravity and radiative cooling on the formation of gaps and spirals by young planets
• Galaxy Zoo: Unwinding the Winding Problem - Observations of Spiral Bulge Prominence and Arm Pitch Angles Suggest Local Spiral Galaxies are Winding
• The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models
• A Relationship Between Stellar Age and Spot Coverage
• TheHaloMod: An online calculator for the halo model
• Dynamically cold disks in the early Universe: myth or reality?
• Regimes of cosmic-ray diffusion in Galactic turbulence
• Fast Point Spread Function Modeling with Deep Learning
• Resolving The Peak Of The Black Hole Mass Spectrum
• Photoevaporative Dispersal of Protoplanetary Disks around Evolving Intermediate-mass Stars
• Asteroid: the PyTorch-based audio source separation toolkit for researchers
• In-situ extreme mass ratio inspirals via sub-parsec formation and migration of stars in thin, gravitationally unstable AGN discs
• Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour
• 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
• The ALMA REBELS Survey: Efficient Ly$\alpha$ Transmission of UV-Bright z$\simeq$7 Galaxies from Large Velocity Offsets and Broad Line Widths
• Assessing the data-analysis impact of LISA orbit approximations using a GPU-accelerated response model
• Layer formation in horizontally forced stratified turbulence: connecting exact coherent structures to linear instabilities
• The SLUGGS Survey: Measuring globular cluster ages using both photometry and spectroscopy
• Introducing CGOLS: The Cholla Galactic OutfLow Simulation Suite
• Delayed Circumstellar Interaction for Type Ia SN 2015cp Revealed by an HST Ultraviolet Imaging Survey
• An Effective Model for the Cosmic-Dawn 21-cm Signal
• Finite-Difference Time-Domain simulations of transmission microscopy enable a better interpretation of 3D nerve fiber architectures in the brain
• Long-term Evolution of Tightly-Packed Stellar Black Holes in AGN Disks: Formation of Merging Black-Hole Binaries via Close Encounters
• Two temperate Earth-mass planets orbiting the nearby star GJ1002
• The Dragonfly Wide Field Survey. I. Telescope, Survey Design and Data Characterization
• CRPropa 3.1 -- A low energy extension based on stochastic differential equations
• tax2vec: Constructing Interpretable Features from Taxonomies for Short Text Classification
• Modelling unresolved binaries of open clusters in color-magnitude diagram. I. method and application of NGC3532
• Formation of an extended stellar halo around an ultra-faint dwarf galaxy following one of the earliest mergers from galactic building blocks
• Near-ultraviolet Transmission Spectroscopy of HD 209458b: Evidence of Ionized Iron Beyond the Planetary Roche Lobe
• Gamma-ray Urgent Archiver for Novel Opportunities (GUANO): Swift/BAT event data dumps on demand to enable sensitive sub-threshold GRB searches
• Towards Robust Constraints on Axion Dark Matter using PSR J1745-2900
• Polluted White Dwarfs: Mixing Regions and Diffusion Timescales
• One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field
• A Precessing Numerical Relativity Waveform Surrogate Model for Binary Black Holes: A Gaussian Process Regression Approach
• Discovery of post-mass-transfer helium-burning red giants using asteroseismology
• An empirical study of dust properties at the earliest epochs
• Observations of the Crab Nebula and Pulsar with the Large-Sized Telescope Prototype of the Cherenkov Telescope Array
• Automated galaxy-galaxy strong lens modelling: no lens left behind
• A helium-flash-induced mixing event can explain the lithium abundances of red clump stars
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the $TESS$ Continuous Viewing Zones and beyond
• Dynamical evolution of stars and gas of young embedded stellar sub-clusters
• Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks
• Transverse kinematics of the Galactic bar-bulge from VVV and Gaia
• Distance-Weighted Graph Neural Networks on FPGAs for Real-Time Particle Reconstruction in High Energy Physics
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• 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
• Constraints on sterile neutrino models from strong gravitational lensing, Milky Way satellites, and Lyman-$\alpha$ forest
• Low-frequency monitoring of flare star binary CR Draconis: Long-term electron-cyclotron maser emission
• NuRadioMC: Simulating the radio emission of neutrinos from interaction to detector
• The JCMT Gould Belt Survey: Evidence for Dust Grain Evolution in Perseus Star-forming Clumps
• PRODIGE -- Envelope to Disk with NOEMA II. Small-scale temperature structure and a streamer feeding the SVS13A protobinary using CH3CN and DCN
• Topological Information Data Analysis
• Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
• Practical adaptive quantum tomography
• The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• Impact of astrophysical binary coalescence timescales on the rate of lensed gravitational wave events
• WASP-4 is Accelerating Toward the Earth
• Widespread Molecular Outflows in the Infrared Dark Cloud G28.37+0.07: Indications of Orthogonal Outflow-Filament Alignment
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Metallicity, ionization parameter, and pressure variations of HII regions in the TYPHOON spiral galaxies
• Atomic Clock Ensemble in Space (ACES) data analysis
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• Prediction of galaxy halo masses in SDSS DR7 via a machine learning approach
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The ultra-steep diffuse radio emission observed in the cool-core cluster RX J1720.1+2638 with LOFAR at 54 MHz
• Spatially resolved mass-to-light from the CALIFA survey. Mass-to-light ratio vs. color relations
• The Exoplanet Population Observation Simulator. II -- Population Synthesis in the Era of Kepler
• Interpreting High-Resolution Spectroscopy of Exoplanets Using Cross-Correlations and Supervised Machine Learning
• Second Data Release of the All-sky NOIRLab Source Catalog
• Planet Hunters TESS II: Findings from the first two years of TESS
• The Astrochemical Impact of Cosmic Rays in Protoclusters I: Molecular Cloud Chemistry
• Radio Afterglows of Very High Energy Gamma-Ray Bursts 190829A and 180720B
• A Machine Learning Based Source Property Inference for Compact Binary Mergers
• ALMA resolves CI emission from the $\beta$ Pictoris debris disk
• SDSS-IV MaNGA: local and global chemical abundance patterns in early-type galaxies
• Full-sky Cosmic Microwave Background Foreground Cleaning Using Machine Learning
• The structural and size evolution of star-forming galaxies over the last 11 Gyrs
• Many bioinformatics programming tasks can be automated with ChatGPT
• AutoEmbedder: A semi-supervised DNN embedding system for clustering
• Pre-collapse Properties of Superluminous Supernovae and Long Gamma-Ray Burst Progenitor Models
• Systematically Measuring Ultra-Diffuse Galaxies (SMUDGes). III. The Southern SMUDGes Catalog
• The K2 Galactic Archaeology Program Data Release 3: Age-abundance patterns in C1-C8 and C10-C18
• Gamma-rays from kilonova: a potential probe of r-process nucleosynthesis
• Fidimag -- a finite difference atomistic and micromagnetic simulation package
• LRG-BEASTS III: Ground-based transmission spectrum of the gas giant orbiting the cool dwarf WASP-80
• The far-infrared polarization spectrum of Rho Ophiuchi A from HAWC+/SOFIA observations
• Alkaline Exospheres of Exoplanet Systems: Evaporative Transmission Spectra
• On the origin of star-gas counterrotation in low-mass galaxies
• Radiative age mapping of the remnant radio galaxy B2 0924+30: the LOFAR perspective
• The First Dynamical Mass Measurement in the HR 8799 System
• EHT-HOPS pipeline for millimeter VLBI data reduction
• Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II
• Keck/NIRSPEC studies of He I in the atmospheres of two inflated hot gas giants orbiting K dwarfs: WASP-52b and WASP-177b
• UGC 4211: A Confirmed Dual Active Galactic Nucleus in the Local Universe at 230 pc Nuclear Separation
• Structure of Axion Miniclusters
• Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
• The Formation of a Stellar Association in the NGC 7000/IC 5070 Complex: Results from Kinematic Analysis of Stars and Gas
• Neural-Network Heuristics for Adaptive Bayesian Quantum Estimation
• On the Effects of Self-Obscuration in the (Sub-)Millimeter Spectral Indices and Appearance of Protostellar Disks
• The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
• Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars
• Gamma rays as probes of cosmic-ray propagation and interactions in galaxies
• Characterization of Ring Substructures in the Protoplanetary Disk of HD 169142 from Multi-Wavelength ALMA Observations
• Searching for changing-state AGNs in massive datasets -- I: applying deep learning and anomaly detection techniques to find AGNs with anomalous variability behaviours
• Presupernova neutrinos: directional sensitivity and prospects for progenitor identification
• Identifying Stellar Streams in Gaia DR2 with Data Mining Techniques
• Enhanced Lidov-Kozai migration and the formation of the transiting giant planet WD1856+534b
• Galactic Chemical Evolution of Radioactive Isotopes
• Polarized point sources in the LOFAR Two-meter Sky Survey: A preliminary catalog
• How dark the sky: the JWST backgrounds
• GHOST: Using Only Host Galaxy Information to Accurately Associate and Distinguish Supernovae
• Is the expansion of the universe accelerating? All signs still point to yes a local dipole anisotropy cannot explain dark energy
• Discovery of an Ultra-Faint Stellar System near the Magellanic Clouds with the DECam Local Volume Exploration (DELVE) Survey
• Importance nested sampling with normalising flows
• A Study of Two Diffuse Dwarf Galaxies in the Field
• A trend in the effective spin distribution of LIGO binary black holes with mass
• WASP-128b: a transiting brown dwarf in the dynamical-tide regime
• Luminous Supernovae: Unveiling a Population Between Superluminous and Normal Core-collapse Supernovae
• FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) 2: Possible evidence for formation of NGC~6618 cluster in M17 by cloud-cloud collision
• 2D Retrieval Frameworks for Hot Jupiter Phase Curves
• Detailed Chemical Abundances for a Benchmark Sample of M Dwarfs from the APOGEE Survey
• A Search for Axionic Dark Matter Using the Magnetar PSR J1745-2900
• The primordial deuterium abundance at z = 2.504 from a high signal-to-noise spectrum of Q1009+2956
• Hot subdwarfs formed from the merger of two He white dwarfs
• A Complex Luminosity Function for the Anomalous Globular Clusters in NGC1052-DF2 and NGC1052-DF4
• Kink instability: evolution and energy dissipation in Relativistic Force-Free Non-Rotating Jets
• The Gravitational Wave Treasure Map: A Tool to Coordinate, Visualize, and Assess the Electromagnetic Follow-Up of Gravitational Wave Events
• Large scale simulations of H and He reionization and heating driven by stars and more energetic sources
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• Binarity and beyond in A stars I. Survey description and first results of VLTI/GRAVITY observations of VAST targets with high Gaia-Hipparcos accelerations
• Rotation and Lithium Confirmation of a 500 Parsec Halo for the Open Cluster NGC 2516
• SMASHing THE LMC: Mapping a Ring-like Stellar Overdensity in the LMC Disk
• Active Anomaly Detection for time-domain discoveries
• TESS observations of the WASP-121 b phase curve
• The origin of the 'blue tilt' of globular cluster populations in the E-MOSAICS simulations
• ULYSSES: Universal LeptogeneSiS Equation Solver
• Eridanus II: A Fossil from Reionization with an Off-Center Star Cluster
• The Zwicky Transient Facility Type Ia supernova survey: first data release and results
• Molecules with ALMA at Planet-forming Scales (MAPS) XIII: HCO${}^{+}$ and disk ionization structure
• The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of $z\sim 2.3$ Star-forming Galaxies
• Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
• JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results
• 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
• Model-based Iterative Reconstruction for Flat-Panel Cone-Beam CT with Focal Spot Blur, Detector Blur, and Correlated Noise
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies
• The impact of stripped Nuclei on the Super-Massive Black Hole number density in the local Universe
• The Spatially Resolved Dust-to-Metals Ratio in M101
• On Neural Architectures for Astronomical Time-series Classification with Application to Variable Stars
• Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
• Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation
• TESS observations of Cepheid stars: first light results
• Observational Inference on the Delay Time Distribution of Short Gamma-ray Bursts
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Rejuvenated accretors have less bound envelopes: Impact of Roche lobe overflow on subsequent common envelope events
• Observing Carbon & Oxygen Carriers in Protoplanetary Disks at Mid-infrared Wavelengths
• SDSS-IV MaNGA: Spatially resolved star-formation histories and the connection to galaxy physical properties
• Chemo-kinematics of the Milky Way spiral arms and bar resonances: connection to ridges and moving groups in the Solar vicinity
• Dynamics and Formation of the Near-Resonant K2-24 System: Insights from Transit-Timing Variations and Radial Velocities
• The Sandwich Mode for Vertical Shear Instability in Protoplanetary Disks
• TangoSIDM: Tantalizing models of Self-Interacting Dark Matter
• The CO(3-2)/CO(1-0) luminosity line ratio in nearby star-forming galaxies and AGN from xCOLD GASS, BASS and SLUGS
• A large H$\alpha$ survey of star formation in relaxed and merging galaxy cluster environments at $z\sim 0.15-0.3$
• The Detectability of Rocky Planet Surface and Atmosphere Composition with JWST: The Case of LHS 3844b
• A New Sedimentation Model for Greater Cloud Diversity in Giant Exoplanets and Brown Dwarfs
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• The Galaxy Progenitors of Stellar Streams around Milky Way-mass Galaxies in the FIRE Cosmological Simulations
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• The 30-Year Search for the Compact Object in SN 1987A
• A universal spin-mass relation for brown dwarfs and planets
• Setting the stage for the search for life with the Habitable Worlds Observatory: Properties of 164 promising planet survey targets
• Physics of ULIRGs with MUSE and ALMA: PUMA IV. No tight relation between cold molecular outflow rates and AGN luminosities
• Measuring distances to low-luminosity galaxies using surface brightness fluctuations
• Multi-path Summation for Decoding 2D Topological Codes
• Helium Variation Across Two Solar Cycles Reveals A Speed-Dependent Phase Lag
• General purpose ray-tracing and polarized radiative transfer in General Relativity
• Particle acceleration in kink-unstable jets
• AU Microscopii in the FUV: Observations in Quiescence, During Flares, and Implications for AU Mic b and c
• Adorym: A multi-platform generic x-ray image reconstruction framework based on automatic differentiation
• STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
• Equivalent widths of Lyman $\alpha$ emitters in MUSE-Wide and MUSE-Deep
• UV Exoplanet Transmission Spectral Features as Probes of Metals and Rainout
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• A Search for a Surviving White Dwarf Companion in SN 1006
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• Exomoons in the habitable zones of M dwarfs
• Modeling Dark Photon Oscillations in Our Inhomogeneous Universe
• Anisotropic winds in Wolf-Rayet binary identify potential gamma-ray burst progenitor
• Linear stability of athermal regularized lattice Boltzmann methods
• RUBIES: A Spectroscopic Census of Little Red Dots; All V-Shaped Point Sources Have Broad Lines
• TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on $H_0$
• An Excess of Globular Clusters in UDGs Formed Through Tidal Heating
• The WAGGS project - I. The WiFeS Atlas of Galactic Globular cluster Spectra
• Self-lensing flares from black hole binaries I: general-relativistic ray tracing of black hole binaries
• Photoevaporation of Jeans-unstable molecular clumps
• Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• Disk structure around the Class I protostar L1489 IRS revealed by ALMA: a warped disk system
• Euclid preparation: XVI. Exploring the ultra low-surface brightness Universe with Euclid/VIS
• Assessing the sources of reionisation: a spectroscopic case study of a 30$\times$ lensed galaxy at $z\sim 5$ with Lyα, CIV, MgII, and [NeIII]
• $\text{simsurvey}$: Estimating Transient Discovery Rates for the Zwicky Transient Facility
• VERITAS observations of the BL Lac object TXS 0506+056
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• Warm Jupiters in TESS Full-Frame Images: A Catalog and Observed Eccentricity Distribution for Year 1
• An Ultra-deep Multi-band VLA Survey of the Faint Radio Sky (COSMOS-XS): Source Catalog and Number Counts
• The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at $2<z<6$ with two bright clump
• Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds
• A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation
• On the treatment of boundary conditions for bond-based peridynamic models
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• Anomaly Detection in the Open Supernova Catalog
• First SETI Observations with China's Five-hundred-meter Aperture Spherical radio Telescope (FAST)
• The host galaxy of the short GRB111117A at $z=2.211$: impact on the short GRB redshift distribution and progenitor channels
• Classification of Magnetohydrodynamic Simulations using Wavelet Scattering Transforms
• After The Fall: Resolving the Molecular Gas in Post-Starburst Galaxies
• Accelerating Non-Cartesian MRI Reconstruction Convergence using k-space Preconditioning
• Deep Subaru Hyper Suprime-Cam observations of Milky Way satellites Columba I and Triangulum II
• Accretion Flows or Outflow Cavities? Uncovering the Gas Dynamics around Lupus 3-MMS
• Nucleosynthesis of binary-stripped stars
• Systematically Measuring Ultra-Diffuse Galaxies (SMUDGes). II. Expanded Survey Description and the Stripe 82 Catalog
• Persistent starspot signals on M dwarfs: multi-wavelength Doppler observations with the Habitable-zone Planet Finder and Keck/HIRES
• Observing the Sun as a star: Design and early results from the NEID solar feed
• Unveiling the Intrinsic Alignment of Galaxies with Self-Calibration and DECaLS DR3 data
• The Richness-to-Mass Relation of CAMIRA Galaxy Clusters from Weak-lensing Magnification in the Subaru Hyper Suprime-Cam Survey
• EvryFlare II: Rotation Periods of the Cool Flare Stars in TESS Across Half the Southern Sky
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• A Thousand Earths: A Very Large Aperture, Ultralight Space Telescope Array for Atmospheric Biosignature Surveys
• Correlations between Triaxial Shapes and Formation History of Dark Matter Haloes
• Pre-merger localization of compact-binary mergers with third generation observatories
• Deep Learning on the 2-Dimensional Ising Model to Extract the Crossover Region with a Variational Autoencoder
• Slow Star Formation in the Milky Way: Theory Meets Observations
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
• Kinematics of the Palomar 5 stellar stream from RR Lyrae stars
• Optically thick HI does not dominate dark gas in the local ISM
• The role of C/O in nitrile astrochemistry in PDRs and planet-forming disks
• Evolutionary models for R Coronae Borealis stars
• Winds Can "Blow Up" AGN Accretion Disk Sizes
• The stellar population and initial mass function of NGC 1399 with MUSE
• The Pan-STARRS1 Proper-motion Survey for Young Brown Dwarfs in Nearby Star-forming Regions. I. Taurus Discoveries and a Reddening-free Classification Method for Ultracool Dwarfs
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Four-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: On-sky Receiver Performance at 40, 90, 150, and 220 GHz Frequency Bands
• HST/WFC3 H$\alpha$ Direct-Imaging Detection of a Point-like Source in the Disk Cavity of AB Aur
• Multiwavelength observations of the blazar BL Lacertae: a new fast TeV gamma-ray flare
• Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae
• Extended stellar systems in the solar neighborhood - III. Like ships in the night: the Coma Berenices neighbor moving group
• Diffuse polarized emission in the LOFAR Two-meter Sky Survey
• Radial abundance gradients in the outer Galactic disk as traced by main-sequence OB stars
• Parametrized tests of post-Newtonian theory using principal component analysis
• Variability in the Atmosphere of the Hot Jupiter Kepler-76b
• Chemical Cartography with LAMOST and Gaia Reveal Azimuthal and Spiral Structure in the Galactic Disk
• Color gradients and half-mass radii of galaxies out to $z=2$ in the CANDELS/3D-HST fields: further evidence for important differences in the evolution of mass-weighted and light-weighted sizes
• Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator
• A random version of principal component analysis in data clustering
• QInfer: Statistical inference software for quantum applications
• Asymmetric, Closed-Form, Finite-Parameter Models of Multinomial Choice
• A Search for FeH in Hot-Jupiter Atmospheres with High-Dispersion Spectroscopy
• TOI-3714 b and TOI-3629 b: Two gas giants transiting M dwarfs confirmed with HPF and NEID
• The velocity anisotropy of the Milky Way satellite system
• User interfaces for computational science: a domain specific language for OOMMF embedded in Python
• The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population
• Orbital misalignment of the super-Earth $\pi$ Men c with the spin of its star
• A minimal power-spectrum-based moment expansion for CMB B-mode searches
• Introducing a New Spitzer Master BLISS Map to Remove the Instrument-Systematic -- Phase-Curve-Parameter Degeneracy, as Demonstrated by a Reanalysis of the 4.5$\mu m$ WASP-43b Phase Curve
• Resolving the kinematics of the disks around Galactic B[e] supergiants
• The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis
• Mass-Metallicity and Star Formation Rate in Galaxies: a complex relation tuned to stellar age
• Oxygen atom reactions with C2H6, C2H4, and C2H2 in ices
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• Increases to Inferred Rates of Planetesimal Accretion Due to Thermohaline Mixing in Metal Accreting White Dwarfs
• Inferring the lensing rate of LIGO-Virgo sources from the stochastic gravitational wave background
• Bias-tailored quantum LDPC codes
• No Redshift Evolution of Dust Temperatures from $0<z<2$
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• deepCR: Cosmic Ray Rejection with Deep Learning
• A Variational Perspective on Diffusion-Based Generative Models and Score Matching
• JWST Noise Floor II: Systematic Error Sources in JWST NIRCam Time Series
• A Detection of the Environmental Dependence of the Sizes and Stellar Haloes of Massive Central Galaxies
• The R-Process Alliance: Discovery of the first metal-poor star with a combined r- and s-process element signature
• Diffuse Ionized Gas in Simulations of Multiphase, Star-Forming Galactic Disks
• The Most Metal-poor Stars in the Magellanic Clouds are $r$-process Enhanced
• The Pan-STARRS1 $\mathbf{z}>5.6$ Quasar Survey: III. The $\mathbf{z}\approx 6$ Quasar Luminosity Function
• Transmission spectroscopy for the warm sub-Neptune HD3167c: evidence for molecular absorption and a possible high metallicity atmosphere
• Evolutionary modelling of subdwarf B stars using MESA with the predictive mixing and convective premixing schemes
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• A tale of two transients: GW170104 and GRB170105A
• The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
• On the halo-mass and radial scale dependence of the lensing is low effect
• Black Mirror: The impact of rotational broadening on the search for reflected light from 51 Pegasi b with high resolution spectroscopy
• The Saga of M81: Global View of a Massive Stellar Halo in Formation
• A More Informative Map: Inverting Thermal Orbital Phase and Eclipse Lightcurves of Exoplanets
• A New Infrared Criterion for Selecting Active Galactic Nuclei to Lower Luminosities
• SO and SiS Emission Tracing an Embedded Planet and Compact ${}^{12}$CO and ${}^{13}$CO Counterparts in the HD 169142 Disk
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• The multiplicity fraction in 202 open clusters from Gaia
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• The MAVERIC Survey: Chandra/ACIS Catalog of Faint X-ray sources in 38 Galactic globular clusters
• RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales
• The X-ray reactivation of the radio bursting magnetar SGR 1935+2154
• Bar effect on gas-phase abundance gradients. I. Data sample and chemical abundances
• Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
• Pre-processing, group accretion and the orbital trajectories of associated subhaloes
• Forcer, a FORM program for the parametric reduction of four-loop massless propagator diagrams
• Tkwant: a software package for time-dependent quantum transport
• The edges of galaxies: Tracing the limits of star formation
• $\nu \text{bhlight}$: Radiation GRMHD for Neutrino-Driven Accretion Flows
• Resolving Linear Polarization due to Emission and Extinction of Aligned Dust Grains on NGC1333 IRAS4A with JVLA and ALMA
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• The Decoupling of Binaries from Their Circumbinary Disks
• Stellar classification from single-band imaging using machine learning
• Enhanced low-energy $\gamma$-decay strength of ${}^{70}$Ni and its robustness within the shell model
• Inference of Heating Properties from "Hot" Non-flaring Plasmas in Active Region Cores. II. Nanoflare Trains
• ALMA observations of NGC 6334S $-$ I: Forming massive stars and cluster in subsonic and transonic filamentary clouds
• Constraining the AGN duty cycle in the cool-core cluster MS 0735.6+7421 with LOFAR data
• Detection of Galactic and Extragalactic Millimeter-Wavelength Transient Sources with SPT-3G
• Inferring the Thermal History of the Intergalactic Medium from the Properties of the Hydrogen and Helium Lyman-alpha Forest
• V-LoTSS: The Circularly-Polarised LOFAR Two-metre Sky Survey
• Chasing Accreted Structures within Gaia DR2 using Deep Learning
• The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• Rotation periods for cool stars in the open cluster NGC 3532. The transition from fast to slow rotation
• Cohort-based T-SSIM Visual Computing for Radiation Therapy Prediction and Exploration
• Evidence for Radial Expansion at the Core of the Orion Complex with Gaia EDR3
• ALMA-IMF II -- investigating the origin of stellar masses: Continuum Images and Data Processing
• The GTC exoplanet transit spectroscopy survey II: An overly-large Rayleigh-like feature for exoplanet TrES-3b
• Cloudy with A Chance of Rain: Accretion Braking of Cold Clouds
• The Structure of Tidal Disruption Event Host Galaxies on Scales of Tens to Thousands of Parsecs
• The Sloan Digital Sky Survey Reverberation Mapping Project: the CIV Blueshift, Its Variability, and Its Dependence Upon Quasar Properties
• Galaxy pairs in the Sloan Digital Sky Survey -- XIV. Galaxy mergers do not lie on the Fundamental Metallicity Relation
• A New Generation of Cool White Dwarf Atmosphere Models. II. A DZ Star with Collision-Induced Absorption
• JADES: Primaeval Lyman-$\alpha$ emitting galaxies reveal early sites of reionisation out to redshift $z\sim 9$
• Carbon-Oxygen Phase Separation in MESA White Dwarf Models
• A prescription for the asteroseismic surface correction
• Imprints of Mass Accretion History on the Shape of the Intracluster Medium and the $T_X-M$ Relation
• Finite Versus Infinite Neural Networks: an Empirical Study
• Direct characterization of young giant exoplanets at high spectral resolution by coupling SPHERE and CRIRES+
• Constraints on the End of Reionization from the Density Fields Surrounding Two Highly Opaque Quasar Sightlines
• Lyα emission from galaxies in the Epoch of Reionization
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• The HI content of dark matter halos at $z\approx 0$ from ALFALFA
• Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST
• Origin of the CEMP-no Group Morphology in the Milky Way
• The rotation period distribution of the rich Pleiades-age Southern open cluster NGC 2516. Existence of a representative zero-age main sequence distribution
• The Highest Energy HAWC Sources are Likely Leptonic and Powered by Pulsars
• Action-based distribution function modelling for constraining the shape of the Galactic dark matter halo
• A Critical Assessment of Solutions to the Galaxy Diversity Problem
• Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Further Evidence of Modified Spin-down in Sun-like Stars: Pileups in the Temperature-Period Distribution
• A warm Jupiter transiting an M dwarf: A TESS single transit event confirmed with the Habitable-zone Planet Finder
• Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties
• Open Cluster Chemical Homogeneity Throughout the Milky Way
• Radio fossils, relics, and haloes in Abell 3266: cluster archaeology with ASKAP-EMU and the ATCA
• The correlation between photometric variability and radial velocity jitter, based on TESS and HARPS observations
• The Milky Way's stellar streams and globular clusters do not align in a Vast Polar Structure
• PyXtal FF: a Python Library for Automated Force Field Generation
• The Radial Acceleration Relation in Disk Galaxies in the MassiveBlack-II Simulation
• Global fits of axion-like particles to XENON1T and astrophysical data
• Giant Planet Scatterings and Collisions: Hydrodynamics, Merger-Ejection Branching Ratio, and Properties of the Remnants
• Detection and timing of gamma-ray pulsations from the $707$ Hz pulsar J0952$-$0607
• A Tidal Disruption Event Candidate Discovered in the Active Galactic Nucleus SDSS J022700.77-042020.6
• The Survey of Centaurus A's Baryonic Structures (SCABS). II. The Extended Globular Cluster System of NGC5128 and its Nearby Environment
• Architectures of Exoplanetary Systems. II: An Increase in Inner Planetary System Occurrence Toward Later Spectral Types for Kepler's FGK Dwarfs
• Towards Robust Expert Finding in Community Question Answering Platforms
• Synthesizing the repeating FRB population using frbpoppy
• Efficient first principles simulation of electron scattering factors for transmission electron microscopy
• Which bright fast radio bursts repeat?
• New analytic solution for the heat flow through a general harmonic network
• Closed-formed ab initio solutions of geometric albedos and reflected light phase curves of exoplanets
• The POlarised GLEAM Survey (POGS) I: First Results from a Low-Frequency Radio Linear Polarisation Survey of the Southern Sky
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• Chromospheric Activity of HAT-P-11: an Unusually Active Planet-Hosting K Star
• The Quest for the Missing Dust: II -- Two Orders of Magnitude of Evolution in the Dust-to-Gas Ratio Resolved Within Local Group Galaxies
• Multi-epoch X-ray burst modelling: MCMC with large grids of 1D simulations
• SN 2016iet: The Pulsational or Pair Instability Explosion of a Low Metallicity Massive CO Core Embedded in a Dense Hydrogen-Poor Circumstellar Medium
• Statistical Test of Distance--Duality Relation with Type Ia Supernovae and Baryon Acoustic Oscillations
• An Algorithm to Compress Line-transition Data for Radiative-transfer Calculations
• An extended Pal 5 stream in Gaia DR2
• An Aligned Orbit for the Young Planet V1298 Tau b
• Structural and photometric properties of barred galaxies from the Auriga cosmological simulations
• Evidence for Cosmic Acceleration is Robust to Observed Correlations Between Type Ia Supernova Luminosity and Stellar Age
• The Demographics of Kepler's Earths and super-Earths into the Habitable Zone
• Fundamental Properties of Co-Moving Stars observed by $Gaia$
• The volumetric rate of calcium-rich transients in the local universe
• Superplot: a graphical interface for plotting and analysing MultiNest output
• A quantitative in-depth analysis of the prototype sdB+BD system SDSS J08205+0008 revisited in the Gaia era
• The CubeSpec space mission. I. Asteroseismology of massive stars from time series optical spectroscopy: science requirements and target list prioritisation
• Neutral ISM, Lyman-Alpha and Lyman-continuum in the nearby starburst Haro 11
• Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity
• A New Analysis of 8 Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• FLEET: A Redshift-Agnostic Machine Learning Pipeline to Rapidly Identify Hydrogen-Poor Superluminous Supernovae
• Centroid vetting of transiting planet candidates from the Next Generation Transit Survey
• Gravitational Self-Lensing in Populations of Massive Black Hole Binaries
• Dynamic alignment and plasmoid formation in relativistic magnetohydrodynamic turbulence
• Type II supernovae from the Carnegie Supernova Project-I. I. Bolometric light curves of 74 SNe II using uBgVriYJH photometry
• Direct measurement of the [CI] luminosity to molecular gas mass conversion factor in high-redshift star-forming galaxies
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• SDSS-IV MaNGA: global and local stellar population properties of elliptical galaxies
• SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy
• Mapping Protoplanetary Disk Vertical Structure with CO Isotopologue Line Emission
• Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?
• SYGMA: Stellar Yields for Galactic Modeling Applications
• A Comparison of Machine Learning Algorithms for the Surveillance of Autism Spectrum Disorder
• Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
• Phases of Mass Transfer from Hot Subdwarfs to White Dwarf Companions and Their Photometric Properties
• A Gaia-based catalog of candidate stripped nuclei and luminous globular clusters in the halo of Centaurus A
• Gaia Gaps and the Physics of Low-Mass Stars. I. The Fully Convective Boundary
• A kinematically detected planet candidate in a transition disk
• Extremely late photometry of SN~2011fe
• Extracting the cold neutral medium from HI emission with deep learning: Implications for Galactic foregrounds at high latitude
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• Discovery and Physical Characterization of a Large Scattered Disk Object at 92 AU
• First detection of 13CH in the interstellar medium
• The GTC exoplanet transit spectroscopy survey XI. Possible detection of Rayleigh scattering in the atmosphere of the Saturn-mass planet WASP-69b
• Constraining coherent low frequency radio flares from compact binary mergers
• JWST Transit Spectra I: Exploring Potential Biases and Opportunities in Retrievals of Tidally-locked Hot Jupiters with Clouds and Hazes
• The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
• Axion Miniclusters Made Easy
• Mapping the Tidal Disruption of the Hercules Dwarf: A Wide-Field DECam Imaging Search for RR Lyrae Stars
• Collimation of the relativistic jet in the quasar 3C 273
• Expansion and Brightness Changes in the Pulsar-Wind Nebula in the Composite Supernova Remnant Kes 75
• DisCoPy: Monoidal Categories in Python
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Cloud Atlas: Rotational Modulations in the L/T Transition Brown Dwarf Companion HN Peg B
• Detection of phosphorus-bearing molecules towards a Solar-type protostar
• Abell 1201: Detection of an Ultramassive Black Hole in a Strong Gravitational Lens
• The GLASS-JWST Early Release Science Program. II. Stage I release of NIRCam imaging and catalogs in the Abell 2744 region
• Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies
• Temperature and Distance Dependence of Tidal Circularization in Close Binaries: A Catalog of Eclipsing Binaries in the Southern Hemisphere Observed by the TESS Satellite
• The supermassive black hole coincident with the luminous transient ASASSN-15lh
• The VMC survey -- XLI. Stellar proper motions within the Small Magellanic Cloud
• Photometric detection at $7.7\mu \mathrm{m}$ of a galaxy beyond redshift $14$ with JWST/MIRI
• HAZMAT. V. The Ultraviolet and X-ray Evolution of K Stars
• A New Test of Copper and Zinc Abundances in Late-Type Stars Using Ultraviolet Cu II and Zn II Lines
• An Early-Time Optical and Ultraviolet Excess in the type-Ic SN 2020oi
• The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b
• The Swift Bulge Survey: Motivation, Strategy, and First X-ray Results
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• Super-resolution trends in the ALMA Taurus survey: Structured inner discs and compact discs
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Col-OSSOS: Color and Inclination are Correlated Throughout the Kuiper Belt
• Stellar Characterization of Keck HIRES Spectra with The Cannon
• Prospects for Backtracing 1I/`Oumuamua and Future Interstellar Objects
• Candidate radio supernova remnants observed by the GLEAM survey over $345^{\circ }<l<60^{\circ }$ and $180^{\circ }<l<240^{\circ }$
• Kinematic modelling of clusters with Gaia: the Death Throes of the Hyades
• The Preservation of Super Earths and the Emergence of Gas Giants after Their Progenitor Cores have Entered the Pebble Isolation Phase
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• Thermal and turbulent properties of the Warm Neutral Medium in the solar neighborhood
• Simulating intergalactic gas for DESI-like small scale Lymanα forest observations
• On the Detection of Exomoons Transiting Isolated Planetary-Mass Objects
• Evidence for sub-Chandrasekhar Type Ia supernovae from the last major merger
• Self-lensing flares from black hole binaries II: observing black hole shadows via light-curve tomography
• The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
• Monitoring the large-scale magnetic field of AD~Leo with SPIRou, ESPaDOnS and Narval. Toward a magnetic polarity reversal?
• Constraining the Stochastic Gravitational Wave Background with Photometric Surveys
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• LieTransformer: Equivariant self-attention for Lie Groups
• Gravitational Wave Detection with Photometric Surveys
• A Featureless Infrared Transmission Spectrum for the Super-Puff Planet Kepler-79d
• Spinney: post-processing of first-principles calculations of point defects in semiconductors with Python
• The star cluster age function in the Galactic disc with Gaia DR2: Fewer old clusters and a low cluster formation efficiency
• Lyman-alpha transmission properties of the intergalactic medium in the CoDaII simulation
• Elemental Abundances in M31: First Alpha and Iron Abundance Measurements in M31's Giant Stellar Stream
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Constraining Mass Transfer Histories of Blue Straggler Stars with COS Spectroscopy of White Dwarf Companions
• On The Lack of Circumbinary Planets Orbiting Isolated Binary Stars
• CameraTransform: a Scientific Python Package for Perspective Camera Corrections
• Cloud Atlas: High-Contrast Time-Resolved Observations of Planetary-Mass Companions
• Stellar Obliquities in Long-period Exoplanet Systems (SOLES) I: The Spin-Orbit Alignment of K2-140 b
• A Second Earth-Sized Planet in the Habitable Zone of the M Dwarf, TOI-700
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• A Gravitational Redshift Measurement of the White Dwarf Mass-Radius Relation
• Turbulence in Milky Way Star-Forming Regions Traced by Young Stars and Gas
• The Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump Stars
• The SPIRou wavelength calibration for precise radial velocities in the near infrared
• Galaxy and Mass Assembly (GAMA): Demonstrating the power of WISE in the study of Galaxy Groups to $z<0.1$
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• Decimetre-scaled spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from OSIRIS observations
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Tensor Renormalization Group with Randomized Singular Value Decomposition
• Unidentified Gamma-ray Sources as Targets for Indirect Dark Matter Detection with the Fermi-Large Area Telescope
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map
• K2-146: Discovery of Planet c, Precise Masses from Transit Timing, and Observed Precession
• wdwarfdate: A Python Package to Derive Bayesian Ages of White Dwarfs
• Stellar Properties of Active G and K Stars: Exploring the Connection Between Starspots and Chromospheric Activity
• Probing the Milky Way's Dark Matter Halo for the 3.5 keV Line
• The Universe is at Most 88% Neutral at z=10.6
• Exploring the brighter fatter effect with the Hyper Suprime-Cam
• The spatial extension of extended narrow line regions in MaNGA AGN
• The surprisingly low carbon mass in the debris disk around HD 32297
• Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
• The POlarised GLEAM Survey (POGS) II: Results from an All-Sky Rotation Measure Synthesis Survey at Long Wavelengths
• Bootes III is a disrupting dwarf galaxy associated with the Styx stellar stream
• Detection and parameter estimation challenges of Type-II lensed binary black hole signals
• The cosmic carbon footprint of massive stars stripped in binary systems
• Can a negative-mass cosmology explain dark matter and dark energy?
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts
• The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at $7<z<8$
• The $\rho$ Oph region revisited with Gaia EDR3
• Millimeter-sized Dust Grains Appear Surviving the Water-sublimating Temperature in the Inner 10 au of the FU Ori Disk
• Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
• Methane in Analogs of Young Directly Imaged Exoplanets
• Automatic microscopic image analysis by moving window local Fourier Transform and Machine Learning
• Statistical Analysis of Semiclassical Dispersion Corrections
• Stars made in outflows may populate the stellar halo of the Milky Way
• High-redshift Extreme Variability Quasars from Sloan Digital Sky Survey Multi-Epoch Spectroscopy
• Opacities of Singly and Doubly Ionised Neodymium and Uranium for Kilonova Emission Modeling
• A Systematic Search for Short-period Close White Dwarf Binary Candidates Based on Gaia EDR3 Catalog and Zwicky Transient Facility Data
• Star Formation at z=2.481 in the Lensed Galaxy SDSS J1110+6459, II: What is missed at the normal resolution of the Hubble Space Telescope?
• Efficient Monte Carlo Integration Using Boosted Decision Trees and Generative Deep Neural Networks
• SDSS-IV MaNGA: spatially resolved dust attenuation in spiral galaxies
• The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
• Classifying Single Stars and Spectroscopic Binaries Using Optical Stellar Templates
• Gaia view of a stellar sub-structure in front of the Small Magellanic Cloud
• Extended stellar systems in the solar neighborhood. IV. Meingast 1: the most massive stellar stream in the solar neighborhood
• ELFI: Engine for Likelihood-Free Inference
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Unlocking Galactic Wolf-Rayet stars with $\text{Gaia}$ DR2 II: Cluster and Association membership
• Water Ice Cloud Variability & Multi-Epoch Transmission Spectra of TRAPPIST-1e
• No Time for Dead Time: Use the Fourier Amplitude Differences to Normalize Dead-time-affected Periodograms
• EXP: N-body integration using basis function expansions
• Corona and XUV emission modelling of the Sun and Sun-like stars
• Tidal Disruptions of Main Sequence Stars of Varying Mass and Age: Inferences from the Composition of the Fallback Material
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• Optical and mid-infrared line emission in nearby Seyfert galaxies
• A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment's Sample-Variance Limited E-Mode Measurement
• The Luminous and Double-Peaked Type Ic Supernova 2019stc: Evidence for Multiple Energy Sources
• FEASTS: IGM cooling triggered by tidal interactions through the diffuse HI phase around NGC 4631
• Unsupervised Classification of Variable Stars
• Determination of the escape velocity of the Milky Way using a proper motion selected halo sample
• MWA and ASKAP observations of atypical radio-halo-hosting galaxy clusters: Abell 141 and Abell 3404
• A MeerKAT-meets-LOFAR Study of MS 1455.0+2232: A 590 kiloparsec 'Mini'-Halo in a Sloshing Cool-Core Cluster
• Precision and consistency of astrocombs
• The ZTF Source Classification Project: I. Methods and Infrastructure
• The radial acceleration relation in a $\Lambda$CDM universe
• A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 AU New Horizons-LORRI Data
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• Fast neutrino flavor conversions in a supernova: Emergence, evolution, and effects
• unyt: Handle, manipulate, and convert data with units in Python
• Investigating fragmentation of gas structures in OB cluster-forming molecular clump G33.92+0.11 with 1000 AU resolution observations of ALMA
• $\text{PyTranSpot}$ - A tool for multiband light curve modeling of planetary transits and stellar spots
• Beyond the bulge-halo conspiracy? Density profiles of Early-type galaxies from extended-source strong lensing
• PUSHing core-collapse supernovae to explosions in spherical symmetry V: Equation of state dependency of explosion properties, nucleosynthesis yields, and compact remnants
• Gravitational Potential and Surface Density Drive Stellar Populations -- II. Star-Forming Galaxies
• Calibration and 21-cm Power Spectrum Estimation in the Presence of Antenna Beam Variations
• Reaching for the Edge I: Probing the Outskirts of Massive Galaxies with HSC, DECaLS, SDSS, and Dragonfly
• Satellites of Satellites: The Case for Carina and Fornax
• The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas
• 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
• The PEPSI Exoplanet Transit Survey (PETS). II. A Deep Search for Thermal Inversion Agents in KELT-20 b/MASCARA-2 b with Emission and Transmission Spectroscopy
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Carnegie Supernova Project: Classification of Type Ia Supernovae
• Unraveling Twisty Linear Polarization Morphologies in Black Hole Images
• Holomorphic Hartree-Fock Theory: The Nature of Two-Electron Problems
• Color Classification of Extrasolar Giant Planets: Prospects and Cautions
• Binary companions of evolved stars in APOGEE DR14: Orbital circularization
• An observational test for star formation prescriptions in cosmological hydrodynamical simulations
• Effects of stellar density on the photoevaporation of circumstellar discs
• On The Statistical Properties of the Lower Main Sequence
• An HST Survey of Protostellar Outflow Cavities: Does Feedback Clear Envelopes?
• The spatially resolved star formation history of mergers: A comparative study of the LIRGs IC1623, NGC6090, NGC2623, and Mice
• Testing strong lensing subhalo detection with a cosmological simulation
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
• QmeQ 1.0: An open-source Python package for calculations of transport through quantum dot devices
• Organic complexity in protostellar disk candidates
• The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
• Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system
• Spectral and spatial analysis of the dark matter subhalo candidates among Fermi Large Area Telescope unidentified sources
• The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
• Atom Interferometer Tests of Dark Matter
• Imaging Extended Emission-Line Regions of Obscured AGN with the Subaru Hyper Suprime-Cam Survey
• Millimeter Transient Point Sources in the SPTpol 100 Square Degree Survey
• A bottom-heavy initial mass function for the likely-accreted blue-halo stars of the Milky Way
• Search for helium in the upper atmosphere of the hot Jupiter WASP-127 b using Gemini/Phoenix
• KIC5950759: a high-amplitude $\delta$ Sct star with amplitude and frequency modulation near the terminal age main sequence
• Destruction of refractory carbon grains drives the final stage of proto-planetary disk chemistry
• Predictably Missing Satellites: Subhalo Abundance in Milky Way-like Halos
• A First Look at Spatially Resolved Balmer Decrements at $1.0<z<2.4$ from JWST NIRISS Slitless Spectroscopy
• Thermal Instability in the CGM of $L_{\star }$ Galaxies: Testing "Precipitation" Models with the FIRE Simulations
• Where are All the Gas-Bearing Local Dwarf Galaxies? Quantifying Possible Impacts of Reionization
• MusE GAs FLOw and Wind (MEGAFLOW) V. The dust/metallicity-anisotropy of the Circum-Galactic Medium
• Unlocking CO Depletion in Protoplanetary Disks II. Primordial C/H Predictions Inside the CO Snowline
• An Atlas of Convection in Main-Sequence Stars
• What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
• On the Amplitude and Stokes Parameters of a Stochastic Gravitational-Wave Background
• Estimating the Ultraviolet Emission of M dwarfs with Exoplanets from Ca II and H$\alpha$
• Accretion of Gas Giants Constrained by the Tidal Barrier
• Spatially Resolved Stellar Spectroscopy of the Ultra-diffuse Galaxy Dragonfly 44. III. Evidence for an Unexpected Star-Formation History
• BASS XXVIII: Near-infrared Data Release 2, High-Ionization and Broad Lines in Active Galactic Nuclei
• On the Properties of Spectroscopically-Confirmed Ultra-Diffuse Galaxies Across Environment
• New Constraints on Protoplanetary Disk Gas Masses in Lupus
• Auto-Differentiable Spectrum Model for High-Dispersion Characterization of Exoplanets and Brown Dwarfs
• Resolving the Dust-to-Metals Ratio and CO-to-H${}_2$ Conversion Factor in the Nearby Universe
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• The Three Hundred Project: the stellar and gas profiles
• Radial measurements of IMF-sensitive absorption features in two massive ETGs
• The R-Process Alliance: J1521-3538, a very metal-poor, extremely r-process-enhanced star with [Eu/Fe]=+2.2, and the class of r-III stars
• Effect of local and large-scale environments on nuclear activity and star formation
• Synthesizing the intrinsic FRB population using frbpoppy
• Atomium: A high-resolution view on the highly asymmetric wind of the AGB star Pi1 Gruis. I. First detection of a new companion and its effect on the inner wind
• Deep Horizon; a machine learning network that recovers accreting black hole parameters
• Mean motion resonance capture in the context of type-I migration
• Stellar graveyards: Clustering of compact objects in globular clusters NGC 3201 and NGC 6397
• Identifying Tidal Disruption Events with an Expansion of the FLEET Machine Learning Algorithm
• Tidally perturbed pulsations in the pre-main sequence $\delta$ Scuti binary RS Cha
• A hybrid classical-quantum workflow for natural language processing
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Chaos and Lévy Flights in the Three-Body Problem
• A self-consistent semi-analytic model for Population III star formation in minihalos
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The deepest $Chandra$ view of RBS 797: evidence for two pairs of equidistant X-ray cavities
• Intrinsic Lyman alpha Profiles of High-Velocity G, K, and M Dwarfs
• Stellar disc streams as probes of the Galactic potential and satellite impacts
• Remnant Radio Galaxies Discovered in a Multi-frequency Survey
• Anomaly in the Opacity of the Post-Reionization Intergalactic Medium in the Ly$\alpha$ and Ly$\beta$ Forest
• Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
• Circuitscape in Julia: High Performance Connectivity Modelling to Support Conservation Decisions
• The R-Process Alliance: Chemical Abundances for a Trio of R-Process-Enhanced Stars -- One Strong, One Moderate, One Mild
• CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
• The TROY project: II. Multi-technique constraints on exotrojans in nine planetary systems
• Stars behind bars II: A cosmological formation scenario for the Milky Way's central stellar structure
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• MaNGA DynPop -- III. Stellar dynamics versus stellar population relations in 6000 early-type and spiral galaxies: Fundamental Plane, mass-to-light ratios, total density slopes, and dark matter fractions
• Angular momentum regulates HI gas content and HI central hole size in the discs of spirals
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• Objective estimation of sensory thresholds based on neurophysiological parameters
• Detecting the gravitational wave memory effect with TianQin
• Three-Dimensional Kinematic Reconstruction of the Optically-Emitting, High-Velocity, Oxygen-Rich Ejecta of Supernova Remnant N132D
• Black hole parameter estimation with synthetic Very Long Baseline Interferometry data from the ground and from space
• An optimal method for scheduling observations of large sky error regions for finding optical counterparts to transients
• A Flexible Analytic Model of Cosmic Variance in the First Billion Years
• Spectral Methods in the Presence of Discontinuities
• Magnetically regulated disk-formation in the inner 100 au region of the Class 0 young stellar object OMC-3/MMS~6 resolved by JVLA and ALMA
• The Graph Curvature Calculator and the curvatures of cubic graphs
• The Flattening Metallicity Gradient in the Milky Way's Thin Disk
• Bar effect on gas-phase abundance gradients. II. Luminosity-dependent flattening
• Kiloparsec-scale Variations in the Star Formation Efficiency of Dense Gas: the Antennae Galaxies (NGC 4038/39)
• Beryllium detection in the very fast nova ASASSN-16kt (V407 Lupi)
• Possible Photometric Signatures of Moderately Advanced Civilizations: The Clarke Exobelt
• Diagnosing 0.1-10 au scale morphology of the FU\,Ori disk using ALMA and VLTI/GRAVITY
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• SUPER V. ALMA continuum observations of z~2 AGN and the elusive evidence of outflows influencing star formation
• The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center
• Polycyclic Aromatic Hydrocarbons, the Anomalous Microwave Emission, and Their Connection to the Cold Neutral Medium
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• Biases in Planet Occurrence Caused by Unresolved Binaries in Transit Surveys
• The Simons Observatory: Galactic Science Goals and Forecasts
• Relativistic fluid modelling of gamma-ray binaries. I. The model
• ACCESS: A Visual to Near-infrared Spectrum of the Hot Jupiter WASP-43b with Evidence of ${\mathrm{H}}_2\mathrm{O}$, but no evidence of Na or K
• $\Lambda$CDM Predictions for the Satellite Population of M33
• EDEN: Sensitivity Analysis and Transiting Planet Detection Limits for Nearby Late Red Dwarfs
• Three dynamically distinct stellar populations in the halo of M49
• Quantifying the effects of spatial resolution and noise on galaxy metallicity gradients
• The NANOGrav 12.5-Year Data Set: Polarimetry and Faraday Rotation Measures from Observations of Millisecond Pulsars with the Green Bank Telescope
• Transiting Planets near the Snow Line from Kepler. I. Catalog
• Modeling Synchrotron Self-Compton and Klein-Nishina Effects in Gamma-Ray Burst Afterglows
• Day-timescale variability in the radio light curve of the Tidal Disruption Event AT2022cmc: confirmation of a highly relativistic outflow
• Variational Integrators for Nonvariational Partial Differential Equations
• The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies
• Real-Time Likelihood-Free Inference of Roman Binary Microlensing Events with Amortized Neural Posterior Estimation
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Maps of Magnetic Field Strength in the OMC-1 using HAWC+ FIR Polarimetric data
• A preserved high-z compact progenitor in the heart of NGC3311 revealed with MUSE 2D stellar population analysis
• Where are Milky Way's Hadronic PeVatrons?
• MusE GAs Flow and Wind (MEGAFLOW) VI. A study of CIV and MgII absorbing gas surrounding [OII] emitting galaxies
• The Local Group: The Ultimate Deep Field
• The dependency of Type Ia Supernova parameters on host galaxy morphology for the Pantheon cosmological sample
• V1298 Tau with TESS: Updated Ephemerides, Radii, and Period Constraints from a Second Transit of V1298 Tau e
• Radiative turbulent mixing layers at high Mach numbers
• KS-pies: Kohn-Sham Inversion Toolkit
• Gas Accretion Can Drive Turbulence in Galaxies
• R-process-rich stellar streams in the Milky Way
• Virial shocks are suppressed in cosmic ray-dominated galaxy halos
• A Mathematical Theory for Clustering in Metric Spaces
• Velocity Dispersion of the GD-1 Stellar Stream
• Bayesian estimation of our local motion from the Planck-2018 CMB temperature map
• Probing Early Universe Supercooled Phase Transitions with Gravitational Wave Data
• The dependence of protostar formation on the geometry and strength of the initial magnetic field
• Exploiting Orbital Constraints from Optical Data to Detect Binary Gamma-ray Pulsars
• J-PLUS: 2-D analysis of the stellar population in NGC 5473 and NGC 5485
• Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by $\text{ASteCA}$
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Towards constraining warm dark matter with stellar streams through neural simulation-based inference
• Multicolor Optical Monitoring of the Blazar S5 0716+714 from 2017 to 2019
• MusE GAs FLOw and Wind (MEGAFLOW) IV: A two sightline tomography of a galactic wind
• GraKeL: A Graph Kernel Library in Python
• Extension of HOPS Out to 500 ParSecs (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds
• A mirage of the cosmic shoreline: Venus-like clouds as a statistical false positive for exoplanet atmospheric erosion
• Wavelet-Based Characterization of Small-Scale Solar Emission Features at Low Radio Frequencies
• VFPred: A Fusion of Signal Processing and Machine Learning techniques in Detecting Ventricular Fibrillation from ECG Signals
• Halo assembly bias from Separate Universe simulations
• Probing the Southern Fermi Bubble in Ultraviolet Absorption using Distant AGNs
• Evaluating Black Hole Detectability with LISA
• A New Approach to the Internal Calibration of Reverberation Mapping Spectra
• Search for globular clusters associated with the Milky Way dwarf galaxies using Gaia DR2
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• Testing the intrinsic scatter of the asteroseismic scaling relations with Kepler red giants
• Evryscope and K2 Constraints on TRAPPIST-1 Superflare Occurrence and Planetary Habitability
• A Pulsar Wind Nebula Embedded in the Kilonova AT2017gfo Associated with GW 170817/GRB 170817A
• Self-intersecting marginally outer trapped surfaces
• The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access
• Statistical Models for the Number of Successful Cyber Intrusions
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Searching for axion-like time-dependent cosmic birefringence with data from SPT-3G
• Compact planetary nebulae: Improved IR diagnostic criteria based on classification tree modelling
• VIS3COS: II. Nature and nurture in galaxy structure and morphology
• Random Forests as a viable method to select and discover high redshift quasars
• Using Commensurabilities and Orbit Structure to Understand Barred Galaxy Evolution
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• PHIBSS: Exploring the Dependence of the CO-H${}_2$ Conversion Factor on Total Mass Surface Density at $z<1.5$
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Systematic challenges for future gravitational wave measurements of precessing binary black holes
• Searching for parity violation with the LIGO-Virgo-KAGRA network
• Current Challenges in Cepheid Distance Calibrations Using Gaia EDR3
• TOI-519 b: a short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis
• ChemKED: a human- and machine-readable data standard for chemical kinetics experiments
• Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS
• Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9979b
• Gravitational Waves from the Inspiral of Supermassive Black Holes in Galactic-scale Simulations
• X-Ray Spectral Variability of Ultraluminous X-Ray Sources in Extragalactic Globular Clusters
• The importance of galaxy formation histories in models of reionization
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum
• r-Process Radioisotopes from Near-Earth Supernovae and Kilonovae
• Validation of TESS exoplanet candidates orbiting solar analogues in the all-sky PLATO input catalogue
• ORIGIN: Blind detection of faint emission line galaxies in MUSE datacubes
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Competing endogenous RNA crosstalk at system level
• Parker Solar Probe Observations of a Dust Trail in the Orbit of (3200) Phaethon
• An Iwasawa-Taniguchi Effect for Compton-thick Active Galactic Nuclei
• The Event Horizon Telescope Image of the Quasar NRAO 530
• Mapping Spatial Variations of HI Turbulent Properties in the Small and Large Magellanic Cloud
• Consistent Iron Abundances Derived from Neutral and Singly-Ionized Iron Lines in Ultraviolet and Optical Spectra of Six Warm Metal-Poor Stars
• Approximating photo-$z$ PDFs for large surveys
• Supernova Siblings: Assessing the Consistency of Properties of Type Ia Supernovae that Share the Same Parent Galaxies
• The K2 Galactic Archaeology Program Data Release 2: Asteroseismic results from campaigns 4, 6, & 7
• Hyper Suprime-Cam Low Surface Brightness Galaxies II: A Hubble Space Telescope Study of the Globular Cluster Systems of Ultra-Diffuse Galaxies in Groups
• Optical Analysis and Modeling of HD96670, a new Black Hole X-ray Binary Candidate
• Molecules with ALMA at Planet-forming Scales (MAPS). X. Studying deuteration at high angular resolution toward protoplanetary disks
• Prospects of gravitational-waves detections from common-envelope evolution with LISA
• The Goldilocks problem of the quasar contribution to reionization
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• Retention of Long-Period Gas Giant Planets: Type II Migration Revisited
• The WAGGS project - II. The reliability of the calcium triplet as a metallicity indicator in integrated stellar light
• On the population III binary black hole mergers beyond the pair-instability mass gap
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• Spatially Resolved Modeling of Optical Albedos for a Sample of Six Hot Jupiters
• As a matter of dynamical range -- scale dependent energy dynamics in MHD turbulence
• A NICER look at thermonuclear X-ray bursts from Aql X-1
• Measuring the EoR Power Spectrum Without Measuring the EoR Power Spectrum
• Propositionalization and Embeddings: Two Sides of the Same Coin
• Positron Effects on Polarized Images and Spectra from Jet and Accretion Flow Models of M87* and Sgr A*
• Thermal Emission and Radioactive Lines, but No Pulsar, in the Broadband X-Ray Spectrum of Supernova 1987A
• FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN). VI. Dense gas and mini-starbursts in the W43 giant molecular cloud complex
• New candidate radio supernova remnants detected in the GLEAM survey over $345^{\circ }<l<60^{\circ }$, $180^{\circ }<l<240^{\circ }$
• Modeling the γ-ray Pulsar Wind Nebulae population in our Galaxy
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• An automated search for transiting exocomets
• Discovery of Extended Tidal Tails around the Globular Cluster Palomar 13
• Numerical simulation of InGaN Schottky solar cell
• Spectroscopic Confirmation of the Sixth Globular Cluster in the Fornax Dwarf Spheroidal Galaxy
• Spectral Learning on Matrices and Tensors
• The Python-based Simulations of Chemistry Framework (PySCF)
• Boosting galactic outflows with enhanced resolution
• Identification of a Group III CEMP-no Star in the Dwarf Spheroidal Galaxy Canes Venatici I
• What Sets the Slope of the Molecular Kennicutt-Schmidt Relation?
• Pressure Distortion of the H${}_2$-He Collision-Induced Absorption at the Photosphere of Cool White Dwarf Stars
• FabricNet: A Fiber Recognition Architecture Using Ensemble ConvNets
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• Detecting Thin Stellar Streams in External Galaxies: Resolved Stars & Integrated Light
• A faint halo star cluster discovered in the Blanco Imaging of the Southern Sky Survey
• Multi-wavelength Stellar Polarimetry of the Filamentary Cloud IC5146: I. Dust Properties
• Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at $1.5<z<6.4$
• MCR-TRGB: A Multiwavelength-Covariant, Robust Tip of the Red Giant Branch Measurement Method
• Inviscid instabilities in rotating ellipsoids on eccentric Kepler orbits
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• The 33 M${}_{\odot }$ black hole Gaia BH3 is part of the disrupted ED-2 star cluster
• Transient glitch mitigation in Advanced LIGO data with $\text{glitschen}$
• Spectroscopic membership for the populous 300 Myr-old open cluster NGC 3532
• Multimessenger pulsar timing array constraints on supermassive black hole binaries traced by periodic light curves
• CMZoom II: Catalog of Compact Submillimeter Dust Continuum Sources in the Milky Way's Central Molecular Zone
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• The spin-orbit alignment of visual binaries
• Diffuser-assisted Photometric Follow-up Observations of the Neptune-sized Planets K2-28b and K2-100b
• Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants
• Two-Moment Neutrino Flavor Transformation with applications to the Fast Flavor Instability in Neutron Star Mergers
• The Galactic Chemical Evolution of phosphorus observed with IGRINS
• On the stellar clustering and architecture of planetary systems
• JINGLE V: Dust properties of nearby galaxies derived from hierarchical Bayesian SED fitting
• Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum
• Anisotropic halo assembly bias and redshift-space distortions
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• Finding flares in Kepler and TESS data with recurrent deep neural networks
• $B_s\to D_s^{\ast }$ Form Factors for the full $q^2$ range from Lattice QCD
• A Differentiable Model of the Assembly of Individual and Populations of Dark Matter Halos
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• The N5K Challenge: Non-Limber Integration for LSST Cosmology
• Extended Tidal Tails of IC 4756 detected by {\it Gaia} EDR3
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Searches for Shapiro delay in seven binary pulsars using the MeerKAT telescope
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• $\text{TESS}$ Giants Transiting Giants I: A Non-inflated Hot Jupiter Orbiting a Massive Subgiant
• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• Probing the initial mass function of the first stars with transients
• Ultimate fate of apparent horizons during a binary black hole merger II: Horizons weaving back and forth in time
• Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection
• A new method for deriving composition of S-type asteroids from noisy and incomplete near-infrared spectra
• Cygrid: A fast Cython-powered convolution-based gridding module for Python
• Stellar Spins in the Open Cluster NGC 2516
• Follow-up of astrophysical transients in real time with the IceCube Neutrino Observatory
• Exploring the origin of multiwavelength activities of high-redshift FSRQ PKS 1502+106 during 2014-2018
• Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor ($[Fe/H]\lesssim -3$) Regime
• Diffuse galaxy cluster emission at 168 MHz within the Murchison Widefield Array Epoch of Reionization 0-hour field
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: 40 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
• A bound on the 12C/13C ratio in near-pristine gas with ESPRESSO
• Spectral Variability of Radio Sources at Low Frequencies
• Exponential Decay Of Concentration Variance During Magma Mixing: Robustness Of A Volcanic Chronometer And Implications For The Homogenization Of Chemical Heterogeneities In Magmatic Systems
• Simulation study of a new InGaN p-layer free Schottky based solar cell
• Improving \textsl{Gaia} parallax precision with a data-driven model of stars
• Are pulsar halos rare ?
• Scrutinizing FR 0 Radio Galaxies as Ultra-High-Energy Cosmic Ray Source Candidates
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Electron Captures on ${}^{14}\mathrm{N}$ as a Trigger for Helium Shell Detonations
• Two Wolf-Rayet stars at the heart of colliding-wind binary Apep
• A New Generation of Cool White Dwarf Atmosphere Models. III. WD J2356$-$209: Accretion of a Planetesimal with an Unusual Composition
• Runaway Coalescence of Pre-Common-Envelope Stellar Binaries
• On the streaming model for redshift-space distortions
• A quantitative assessment of the VO line list: Inaccuracies hamper high-resolution VO detections in exoplanet atmospheres
• candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood
• Hidden Worlds: Dynamical Architecture Predictions of Undetected Planets in Multi-planet Systems and Applications to TESS Systems
• Multiwavelength Absolute Magnitudes and Colours of Red Clump Stars in {\it Gaia} Era
• The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
• TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Global 21-cm signal extraction from foreground and instrumental effects IV: Accounting for realistic instrument uncertainties and their overlap with foreground and signal models
• Disturbed, diffuse, or just missing? A global study of the HI content of Hickson Compact Groups
• Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium
• Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
• A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae
• Open(G)PIAS: An open source solution for the construction of a high-precision Acoustic-Startle-Response (ASR) setup for tinnitus screening and threshold estimation in rodents
• Precise optical timing of PSR J1023+0038, the first millisecond pulsar detected with Aqueye+ in Asiago
• Magnetic activity evolution of solar-like stars: I. S_ph-Age relation derived from Kepler observations
• HST strong-lensing model for the first JWST galaxy cluster SMACS J0723.3-7327
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• WISDOM project -- XIV. SMBH mass in the early-type galaxies NGC0612, NGC1574, and NGC4261 from CO dynamical modelling
• Mira variables in the Milky Way's nuclear stellar disc: discovery and classification
• Persistent Non-Gaussian Structure in the Image of Sagittarius A* at 86 GHz
• Modeling HI at the field level
• As a matter of tension -- kinetic energy spectra in MHD turbulence
• Multi-wavelength Emission from Galactic Jets: the Case of the Microquasar SS433
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• Modeling Quasar UV/Optical Variability with the Corona-heated Accretion-disk Reprocessing (CHAR) Model
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• Hunting for C-rich long-period variable stars in the Milky Way's bar-bulge using unsupervised classification of Gaia BP/RP spectra
• PyPanda: a Python Package for Gene Regulatory Network Reconstruction
• Dynamical modelling of globular clusters: challenges for the robust determination of IMBH candidates
• Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z=1
• exoALMA. VI. Rotating under Pressure: Rotation curves, azimuthal velocity substructures, and pressure variations
• Multimessenger Constraints on Intergalactic Magnetic Fields from the Flare of TXS 0506+056
• The stellar populations of high-redshift dwarf galaxies
• From Blue Cloud to Red Sequence: Evidence of Morphological Transition Prior to Star Formation Quenching
• Entropy-stable, high-order summation-by-parts discretizations without interface penalties
• The Effect of Solar Wind Expansion and Non-Equilibrium Ionization on the Broadening of Coronal Emission Lines
• The imprint of X-ray photoevaporation of planet-forming discs on the orbital distribution of giant planets
• CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between $0.5\lesssim z\lesssim 1.7$ using H$\alpha$ Emission Line Maps
• The Power of Halometry
• What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest
• The Photometric LSST Astronomical Time-series Classification Challenge (PLAsTiCC): Selection of a performance metric for classification probabilities balancing diverse science goals
• Earths in Other Solar Systems N-body simulations: the Role of Orbital Damping in Reproducing the Kepler Planetary Systems
• Meso-scale Instability Triggered by Dust Feedback in Dusty Rings: Origin and Observational Implications
• Structure and kinematics of shocked gas in Sgr B2: further evidence of a cloud-cloud collision from SiO emission maps
• The TREX Survey: Kinematical Complexity Throughout M33's Stellar Disk and Evidence for a Stellar Halo
• Imprint of planet formation in the deep interior of the Sun
• The Gravitational Afterglow of Boson Stars
• Can Helium-detonation Model Explain the Observed Diversity of Type Ia Supernovae?
• Prospects for distinguishing galaxy evolution models with surveys at redshifts $z\gtrsim 4$
• Constraining Compact Object Formation with 2M0521
• Exoplanet Transmission Spectroscopy using KMOS
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz
• The Quintuplet Cluster: Extended Structure and Tidal Radius
• Methane formation in cold regions from carbon atoms and molecular hydrogen
• Exoplanet Interior Retrievals: core masses and metallicities from atmospheric abundances
• Red Supergiants in M31: The Humphreys-Davidson limit at high metallicity
• Turbulent magnetic fields in the merging galaxy cluster MACS J0717.5+3745: polarization analysis
• Dynamical Mass of the Exoplanet Host Star HR 8799
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo
• Spatially Resolved Metal Loss from M31
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
• Variations of Observed Lyman-α Spectra Shapes due to the Intergalactic Absorption
• TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host
• Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c
• A Survey for High-redshift Gravitationally Lensed Quasars and Close Quasars Pairs. I. the Discoveries of an Intermediately-lensed Quasar and a Kpc-scale Quasar Pair at $z\sim 5$
• More Evidence for Variable Helium Absorption from HD 189733b
• CO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
• Clustrophile: A Tool for Visual Clustering Analysis
• The stellar halo in Local Group Hestia simulations II. The accreted component
• Estimating Extinction using Unsupervised Machine Learning
• Sodium Brightening of (3200) Phaethon Near Perihelion
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• Alternative model for the administration and analysis of research-based assessments
• Constraints to neutron-star kicks in High-Mass X-ray Binaries with Gaia EDR3
• Detecting the power spectrum turnover with HI intensity mapping
• Population synthesis of pulsar wind nebulae and pulsar halos in the Milky Way -- Predicted contributions to the very-high-energy sky
• Cataloging Accreted Stars within Gaia DR2 using Deep Learning
• New Evidence for Extended HeII Reionization at z>3.5 from HeII Lyman Alpha and Beta Transmission Spikes
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• The impact of dynamic pressure bumps on the observational properties of protoplanetary disks
• Modelling Cosmic Radiation Events in the Tree-ring Radiocarbon Record
• An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission
• The Origin of the Heaviest Metals in Most Ultra-Faint Dwarf Galaxies
• Resolving Structure in the Debris Disk around HD 206893 with ALMA
• SLITronomy: towards a fully wavelet-based strong lensing inversion technique
• Testing the Flux-based statistical prediction of the Three-Body Problem
• MiMO: Mixture Model for Open Clusters in Color-Magnitude Diagrams
• RadioAstron reveals a spine-sheath jet structure in 3C 273
• MARXS: A modular software to ray-trace X-ray instrumention
• Separatrix Divergence of Stellar Streams in Galactic Potentials
• Learning Neural Event Functions for Ordinary Differential Equations
• Sumo Puff: Tidal Debris or Disturbed Ultra-Diffuse Galaxy?
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• pulsar_spectra: A pulsar flux density catalogue and spectrum fitting repository
• Constraining the Tail-End of Reionization Using Lyman-$\alpha$ Transmission Spikes
• A statistical inference approach to time-delay interferometry for gravitational-wave detection
• Spotting Stellar Activity Cycles in Gaia Astrometry
• Perfect density models cannot guarantee anomaly detection
• Predicting Lyman-alpha escape fractions with a simple observable: Lyman-alpha in emission as an empirically calibrated star formation rate indicator
• Planet Hunters TESS IV: A massive, compact hierarchical triple star system TIC 470710327
• Unlocking the Full Potential of Extragalactic Ly$\alpha$ through Its Polarization Properties
• Two new outbursts and transient hard X-rays from 1E 1048.1$-$5937
• A metallicity study of F, G, K and M dwarfs in the Coma Berenices open cluster from the APOGEE survey
• The MUSE view of the planetary nebula NGC 3132
• Confirmation of Water Absorption in the Thermal Emission Spectrum of the Hot Jupiter WASP-77Ab with HST/WFC3
• GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity
• A Deep Chandra X-ray Observatory Study of the Millisecond Pulsar Population in the Globular Cluster Terzan 5
• Montblanc: GPU accelerated Radio Interferometer Measurement Equations in support of Bayesian Inference for Radio Observations
• Independent Vector Analysis via Log-Quadratically Penalized Quadratic Minimization
• Lithologic Controls on Silicate Weathering Regimes of Temperate Planets
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Follow-up Imaging of Disk Candidates from the Disk Detective Citizen Science Project: New Discoveries and False-Positives in WISE Circumstellar Disk Surveys
• Investigating Gravitational Collapse of a Pebble Cloud to form Transneptunian Binaries
• The interaction of Type Iax supernova ejecta with a helium companion star
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• Planetary Spin and Obliquity from Mergers
• A first estimate of the Milky Way dark matter halo spin
• Supervised Ensemble Classification of Kepler Variable Stars
• Beamed emission from a neutron-star ULX in a GRRMHD simulation
• Dust Settling Instability in Protoplanetary Discs
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Accurate Identification of Galaxy Mergers with Stellar Kinematics
• TAPAS IV. TYC 3667-1280-1 b - the most massive red giant star hosting a warm Jupiter
• Consistent radial velocities of classical Cepheids from the cross-correlation technique
• An Updated Formalism For Line-Driven Radiative Acceleration and Implications for Stellar Mass Loss
• Bridging the Planet Radius Valley: Stellar Clustering as a Key Driver for Turning Sub-Neptunes into Super-Earths
• SuperBoRG: Search for The Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
• Polydisperse Streaming Instability II. Methods for solving the linear stability problem
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• Dissecting the super-critical filaments embedded in the 0.5 pc subsonic region of Barnard 5
• A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• A Mesoscale Perspective on the Tolman Length
• Implications of the Gaia Sausage for Dark Matter Nuclear Interactions
• MOPSS I: Flat Optical Spectra for the Hot Jupiters WASP-4 b and WASP-52b
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• The Southern HII Region Discovery Survey I: The Bright Catalog
• Exploring the differences of integrated and spatially resolved analysis using integral field unit data: The case of Abell 14
• Dating individual quasars with the HeII proximity effect
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• Generating Synthetic Cosmological Data with GalSampler
• Elemental abundances in M31: [Fe/H] and [α/Fe] in M31 Dwarf Galaxies Using Coadded Spectra
• Statistical Analysis on E-Commerce Reviews, with Sentiment Classification using Bidirectional Recurrent Neural Network (RNN)
• Low-Cost Energy Meter Calibration Method for Measurement and Verification
• Cooling driven coagulation
• CHILES VERDES: Radio variability at an unprecedented depth and cadence in the COSMOS field
• Interpolation of turbulent magnetic fields and its consequences on diffusive cosmic ray propagation
• Long-term trends of light pollution assessed from SQM measurements and an empirical atmospheric model
• Near-Chandrasekhar-Mass Type Ia Supernovae from the Double-Degenerate Channel
• Euclid: Early Release Observations -- Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field
• Direct Formation of Planetary Embryos in Self-Gravitating Disks
• The Orbital Architecture of Qatar-6: A Fully Aligned 3-Body System?
• Convolutional Neural Networks for Histopathology Image Classification: Training vs. Using Pre-Trained Networks
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Relativistic fluid modelling of gamma-ray binaries. II. Application to LS 5039
• DUSTiER (DUST in the Epoch of Reionization): dusty galaxies in cosmological radiation-hydrodynamical simulations of the Epoch of Reionization with RAMSES-CUDATON
• Image-based Classification of Variable Stars: First Results from Optical Gravitational Lensing Experiment Data
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Suppressed heat conductivity in the intracluster medium: implications for the magneto-thermal instability
• The TESS View of LOFAR Radio-Emitting Stars
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionised bubble at z = 6.53
• The REASONS Survey: Resolved Millimeter Observations of a Large Debris Disk Around the Nearby F Star HD 170773
• Optically-pumped dynamic nuclear hyperpolarization in ${}^{13}$C enriched diamond
• Correcting Sky Quality Meter measurements for aging effects using twilight as calibrator
• Redshift requirements for cosmic shear with intrinsic alignment
• GPCAL: a generalized calibration pipeline for instrumental polarization in VLBI data
• Identifying Tidal Disruption Events via Prior Photometric Selection of Their Preferred Hosts
• A chemo-dynamical link between the Gjöll stream and NGC 3201
• High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare
• Stellar Evolution in Real Time: Models Consistent with Direct Observation of Thermal Pulse in T Ursae Minoris
• Hot corino chemistry in the Class I binary source Ser-emb 11
• An eccentric Brown Dwarf eclipsing an M dwarf
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
• On-sky verification of Fast and Furious focal-plane wavefront sensing: Moving forward toward controlling the island effect at Subaru/SCExAO
• Absorption and emission features of ${}^7$Be{\sc II} in the outburst spectra of V838 Her (Nova Her 1991)
• On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram
• Coffee-stain growth dynamics on dry and wet surfaces
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
• Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
• Minor Mergers are not enough: The importance of Major Mergers during Brightest Cluster Galaxy assembly
• The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?
• Rank-3 Moment Closures in General Relativistic Neutrino Transport
• Globular Clusters in High-Redshift Dwarf Galaxies: A Case Study from the Local Group
• PySE: Software for Extracting Sources from Radio Images
• NEID Rossiter-McLaughlin Measurement of TOI-1268b: A Young Warm Saturn Aligned with Its Cool Host Star
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• A synthetic sample of short-cadence solar-like oscillators for TESS
• Focal-plane wavefront sensing with the vector Apodizing Phase Plate
• The HIX galaxy survey I: Study of the most gas rich galaxies from HIPASS
• A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries
• The HI intensity mapping bispectrum including observational effects
• Extreme Variability Quasars in Their Various States. I: The sample selection and composite SDSS spectra
• Water UV-shielding in the terrestrial planet-forming zone: Implications for carbon dioxide emission
• TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by TTVs
• Probing Transit Timing Variation and its Possible Origin with Twelve New Transits of TrES-3b
• Variational Integrators for Reduced Magnetohydrodynamics
• HST Grism-derived Forecasts for Future Galaxy Redshift Surveys
• The Most Metal-poor Stars in the Inner Bulge
• The SPHERE view of three interacting twin disc systems in polarised light
• A two-step gravitational cascade for the fragmentation of self-gravitating discs
• Reaction Rate Sensitivity of the Production of $\gamma$-ray Emitting Isotopes in Core-Collapse Supernova
• 21cmfish: Fisher-matrix framework for fast parameter forecasts from the cosmic 21-cm signal
• MCSED: A flexible spectral energy distribution fitting code and its application to $z\sim 2$ emission-line galaxies
• JWST NIRCam Defocused Imaging: Photometric Stability Performance and How it Can Sense Mirror Tilts
• The Ages and Metallicities of the Globular Clusters in the Sparkler
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Statistical recovery of 21cm visibilities and their power spectra with Gaussian constrained realisations and Gibbs sampling
• 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
• Simultaneous spectral energy distribution and near-infrared interferometry modeling of HD 142666
• On Trapped Modes In Variable White Dwarfs As Probes Of The ${}^{12}$C($\alpha ,\gamma$)${}^{16}$O Reaction Rate
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Kinetic Tomography. II. A second method for mapping the velocity field of the Milky Way Interstellar Medium and a comparison with spiral structure models
• Coffea -- Columnar Object Framework For Effective Analysis
• Robust integration of fast flavor conversions in classical neutrino transport
• The Detection of Intergalactic Halpha Emission from the Slug Nebula at z~2.3
• Expanding CO Shells in the Orion A Molecular Cloud
• The mass and environmental dependence on the secular processes of AGN in terms of morphology, colour, and specific star-formation rate
• High Resolution Optical Spectroscopy of Stars in the Sylgr Stellar Stream
• Gliese 12 b: A temperate Earth-sized planet at 12 pc ideal for atmospheric transmission spectroscopy
• Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations
• The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star
• The Pristine survey -- XVII. The C-19 stream is dynamically hot and more extended than previously thought
• Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetised molecular cloud cores
• The Young Planet DS Tuc Ab has a Low Obliquity
• Improved Coupling of Hydrodynamics and Nuclear Reactions via Spectral Deferred Corrections
• Stochastic Modelling of Star Formation Histories III. Constraints from Physically-Motivated Gaussian Processes
• Tidal Dissipation in Dual-Body, Highly Eccentric, and Non-synchronously Rotating Systems: Applications to Pluto-Charon and the Exoplanet TRAPPIST-1e
• Ephemeris Errors and the Gravitational Wave Signal: Harmonic Mode Coupling in Pulsar Timing Array Searches
• Ultra-compact dwarfs beyond the centre of the Fornax galaxy cluster: Hints of UCD formation in low-density environments
• A Mock Catalog of Gravitationally Lensed Quasars for the LSST Survey
• New Constraints on Early-Type Galaxy Assembly from Spectroscopic Metallicities of Globular Clusters in M87
• Galactic googly: the rotation-metallicity bias in the inner stellar halo of the Milky Way
• The jet collimation profile at high resolution in BL Lacertae
• Gas inflow and outflow in an interacting high-redshift galaxy: The remarkable host environment of GRB 080810 at $z=3.35$
• A New Approach to Convective Core Overshooting: Probabilistic Constraints from Color-Magnitude Diagrams of LMC Clusters
• Physical and chemical structure of the Serpens filament -- fast formation and gravity-driven accretion
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• Ancient Very Metal-Poor Stars Associated With the Galactic Disk in the H3 Survey
• Automatic Survey-Invariant Variable Star Classification
• HST Imaging of the Local Volume Dwarf Galaxies Pisces A&B: Prototypes for Local Group Dwarfs
• Anisotropic magnetized white dwarfs: Unifying under- and over-luminous peculiar and standard type Ia supernovae
• DuctApe: a suite for the analysis and correlation of genomic and OmnilogTM Phenotype Microarray data
• Considerations for the Observability of Kinematically Offset Binary AGN
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• Classical Novae Masquerading as Dwarf Novae? Outburst Properties of Cataclysmic Variables with ASAS-SN
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments I: Mapping Star Formation in HI-Rich UDGs
• PyTorch Metric Learning
• Investigation of coronal properties of X-ray bright G-dwarf stars based on the solar surface magnetic field -- corona relation
• OH Megamasers in HI Surveys: Forecasts and a Machine Learning Approach to Separating Disks from Mergers
• The origin of X-ray coronae around simulated disc galaxies
• Bolometric treatment of irradiation effects: general discussion and application to binary stars
• Measuring the Largest Angular Scale CMB B-mode Polarization with Galactic Foregrounds on a Cut Sky
• Constraints on the antistar fraction in the Solar system neighborhood from the 10-years Fermi Large Area Telescope gamma-ray source catalog
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• Tracking Advanced Planetary Systems (TAPAS) with HARPS-N. VI. HD 238914 and TYC 3318-01333-1 - two more Li-rich giants with planets
• C3, A Command-line Catalogue Cross-match tool for large astrophysical catalogues
• 2004 EW95: A phyllosilicate bearing carbonaceous asteroid in the Kuiper Belt
• A Highly Magnified Gravitationally Lensed Red QSO at z = 2.5 with a Significant Flux Ratio Anomaly
• Residual Carbon in Oxygen-Neon White Dwarfs and its Implications for Accretion-Induced Collapse
• An ALMA Gas-dynamical Mass Measurement of the Supermassive Black Hole in the Local Compact Galaxy UGC 2698
• The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
• Extended Aperture Photometry of K2 RR Lyrae stars
• Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
• On the radial acceleration relation of $\Lambda$CDM satellite galaxies
• Effects of Ringed Structures and Dust Size Growth on Millimeter Observations of Protoplanetary Disks
• Searching for intergalactic star forming regions in Stephan's Quintet with SITELLE. I. Ionised gas structures and kinematics
• Anisotropic cosmic-ray diffusion in isotropic Kolmogorov turbulence
• LINNA: Likelihood Inference Neural Network Accelerator
• Circumstellar ammonia in oxygen-rich evolved stars
• ExoTiC-ISM: A Python package for marginalised exoplanet transit parameters across a grid of systematic instrument models
• The space weather around the exoplanet GJ 436b
• Extending the FIP bias sample to magnetically active stars. Challenging the FIP bias paradigm?
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Sixteen overlooked open clusters in the fourth Galactic quadrant. A combined analysis of UBVI photometry and Gaia DR2 with ASteCA
• Integration of Leaky-Integrate-and-Fire-Neurons in Deep Learning Architectures
• Pycobra: A Python Toolbox for Ensemble Learning and Visualisation
• An Improved Statistical Point-Source Foreground Model for the Epoch of Reionization
• Main-belt asteroids in the K2 Uranus field
• ArtPop: A Stellar Population and Image Simulation Python Package
• Losing Oceans: The Effects of Composition on the Thermal Component of Impact-driven Atmospheric Loss
• An Operator-Based Local Discontinuous Galerkin Method Compatible With the BSSN Formulation of the Einstein Equations
• Host Galaxy Mass Combined with Local Stellar Age Improve Type Ia Supernovae Distances
• The winds of young Solar-type stars in the Hyades
• Stellar Population Diagnostics of the Massive Star Binary Fraction
• Multi-resolution filtering: an empirical method for isolating faint, extended emission in Dragonfly data and other low resolution images
• ULYSSES, Universal LeptogeneSiS Equation Solver: version 2
• Radiation-driven acceleration in the expanding WR140 dust shell
• Two Year Cosmology Large Angular Scale Surveyor (CLASS) Observations: Long Timescale Stability Achieved with a Front-End Variable-delay Polarization Modulator at 40 GHz
• Resonance-based Detection of Magnetic Nanoparticles and Microbeads Using Nanopatterned Ferromagnets
• TOI-1859b: A 64-Day Warm Jupiter on an Eccentric and Misaligned Orbit
• Highly turbulent gas on GMC-scales in NGC 3256, the nearest luminous infrared galaxy
• Tidally stripped halo stars from the Large Magellanic Cloud in the Galactic North
• Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
• Effects of Photoionization and Photoheating on Lyman-alpha Forest Properties from Cholla Cosmological Simulations
• Spectroscopy of the Young Stellar Association Price-Whelan 1: Origin in the Magellanic Leading Arm and Constraints on the Milky Way Hot Halo
• HAZMAT. VIII. A Spectroscopic Analysis of the Ultraviolet Evolution of K Stars: Additional Evidence for K Dwarf Rotational Stalling in the First Gigayear
• Optical high-resolution spectroscopy of 14 young $\alpha$-rich stars
• Mitigating stellar activity jitter with different line lists for least-squares deconvolution: analysis of a parametric and a randomised line selection
• Accretion History of AGN II: Constraints on AGN Spectral Parameters using the Cosmic X-ray Background
• Tracking Dust Grains During Transport and Growth in Protoplanetary Disks
• The viscous evolution of circumstellar discs in young star clusters
• Shaping the structure of a GMC with radiation and winds
• Evidence for Primordial Alignment: Insights from Stellar Obliquity Measurements for Compact Sub-Saturn Systems
• The edge-on protoplanetary disk HH 48 NE I. Modeling the geometry and stellar parameters
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Connecting optical and X-ray tracers of galaxy cluster relaxation
• The XXL Survey XXVIII. Galaxy luminosity functions of the XXL-N clusters
• Radio Spectra of Luminous, Heavily Obscured WISE-NVSS Selected Quasars
• A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing Runs
• Complex Modulation of Rapidly Rotating Young M Dwarfs: Adding Pieces to the Puzzle
• Entropy evaluation sheds light on ecosystem complexity
• The effect of interior heat flux on the atmospheric circulation of hot and ultra-hot Jupiters
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Super-Keplerian Equatorial Outflows in SS 433. Centrifugal Ejection of the Circumbinary Disk
• Characterisation of the Particle-Induced Background of XMM-Newton EPIC-pn: Short and Long Term Variability
• Boundary Layer Circumplanetary Accretion: How Fast Could an Unmagnetized Planet Spin Up Through Its Disk?
• Evolution of circumstellar discs in young star-forming regions
• The GTC exoplanet transit spectroscopy survey VIII. Flat transmission spectrum for the warm gas giant WASP-80
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Angular clustering of point sources at 150 MHz in the TGSS survey
• Aldebaran b's temperate past uncovered in planet search data
• Circalunar variations of the night sky brightness -- an FFT perspective on the impact of light pollution
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• Phosphorus Abundances in the Hyades and Galactic Disk
• Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave vs. Particle Dark Matter Predictions
• Alchemical Grid Dock (AlGDock): Binding Free Energy Calculations between Flexible Ligands and Rigid Receptors
• The turbulent gas structure in the centers of NGC253 and the Milky Way
• Constraints on parity and Lorentz violations in gravity from GWTC-3 through a parametrization of modified gravitational wave propagations
• Searching for new solar twins: The Inti survey for the Northern Sky
• On the origin of the North Celestial Pole Loop
• Analytical tolerancing of segmented telescope co-phasing for exo-Earth high-contrast imaging
• The substructure of the Perseus star forming region: A survey with Gaia DR2
• Photometric detection of internal gravity waves in upper main-sequence stars. III. Comparison of amplitude spectrum fitting and Gaussian process regression using celerite2
• Comparative Analysis of TRGBs (CATs) from Unsupervised, Multi-Halo-Field Measurements: Contrast is Key
• BALRoGO: Bayesian Astrometric Likelihood Recovery of Galactic Objects -- Global properties of over one hundred globular clusters with Gaia EDR3
• Particle Dynamics in 3D Self-gravitating Disks II: Strong Gas Accretion and Thin Dust Disks
• Particle Dynamics in 3D Self-gravitating Disks I: Spirals
• The X-ray and radio activity of typical and luminous Lya emitters from z~2 to z~6: evidence for a diverse, evolving population
• Pterodactyls: A Tool to Uniformly Search and Vet for Young Transiting Planets In TESS Primary Mission Photometry
• The Three Hundred Project: The gas disruption of infalling objects in cluster environments
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
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• The accretion flow geometry of MAXI J1820+070 through broadband noise research with Insight-HXMT
• SoK: Privacy Preserving Machine Learning using Functional Encryption: Opportunities and Challenges
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• Cloud Atlas: High-precision HST/WFC3/IR Time-Resolved Observations of Directly-Imaged Exoplanet HD106906b
• Machine Learning for Exploring Small Polaron Configurational Space
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• SN 2020sck: deflagration in a carbon-oxygen white dwarf
• Evidence of a Decreased Binary Fraction for Massive Stars Within 20 Milliparsecs of the Supermassive Black Hole at the Galactic Center
• Classification of OGLE eclipsing binary stars based on their morphology type with Locally Linear Embedding
• HeAT -- a Distributed and GPU-accelerated Tensor Framework for Data Analytics
• The Galactic Nova Rate: Estimates from the ASAS-SN and Gaia Surveys
• Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant
• J-PAS: Measuring emission lines with artificial neural networks
• The In-situ Origins of Dwarf Stellar Outskirts in FIRE-2
• Burst-Disk Interaction in 4U 1636-536 as observed by NICER
• Stellar Spins in the Pleiades, Praesepe, and M35 Open Clusters
• Physical Parameters of the Multi-Planet Systems HD 106315 and GJ 9827
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Rotational modulation of spectroscopic Zeeman signatures in low-mass stars
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Oxygen-enhanced extremely metal-poor DLAs: A signpost of the first stars?
• DELVE-ing into the Jet: a thin stellar stream on a retrograde orbit at 30 kpc
• The Southern HII Region Discovery Survey. II. The Full Catalog
• Evidence of Core Growth in the Dragon Infrared Dark Cloud: A Path for Massive Star Formation
• The Cosmic Dispersion Measure in the EAGLE Simulations
• A LAMOST BHB Catalog and Kinematics Therein I: Catalog and Halo Properties
• Cloud Parameterizations and their Effect on Retrievals of Exoplanet Reflection Spectroscopy
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• The LOFAR Two Metre Sky Survey: Deep Fields. II. The ELAIS-N1 LOFAR deep field
• The extreme colliding-wind system Apep: resolved imagery of the central binary and dust plume in the infrared
• Ecole: A Gym-like Library for Machine Learning in Combinatorial Optimization Solvers
• Identifying structural changes with unsupervised machine learning methods
• Reconstructing Masses of Merging Neutron Stars from Stellar $R$-Process Abundance Signatures
• MALT-45: A 7mm survey of the southern Galaxy - II. ATCA follow-up observations of 44GHz class I methanol masers
• An absolute calibration of the near-infrared Period-Luminosity Relations of Type II Cepheids in the Milky Way and in the Large Magellanic Cloud
• 3D Hydrodynamical Simulations of Helium-Ignited Double-degenerate White Dwarf Mergers
• Microphysics of Water Clouds in the Atmospheres of Y Dwarfs and Temperate Giant Planets
• BAT AGN Spectroscopic Survey-XXIII. A New Mid-Infrared Diagnostic for Absorption in Active Galactic Nuclei
• FUMES. II. Ly$\alpha$ Reconstructions of Young, Active M Dwarfs
• Photometric identification of compact galaxies, stars and quasars using multiple neural networks
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• Stellar Chromospheric Activity Database of Solar-like Stars Based on the LAMOST Low-Resolution Spectroscopic Survey
• Understanding binary neutron star collisions with hypermodels
• Fornax 3D project: automated detection of planetary nebulae in the centres of early-type galaxies and first results
• Star Formation Efficiencies at Giant Molecular Cloud Scales in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)
• Fast and robust method for flow analysis using GPU assisted diffractive optical element based background oriented schlieren (BOS)
• Halo models of HI selected galaxies
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Synthetic Large-Scale Galactic Filaments -- on their Formation, Physical Properties, and Resemblance to Observations
• The Spin-Orbit Misalignment of TOI-1842b: The First Measurement of the Rossiter-McLaughlin Effect for a Warm Sub-Saturn around a Massive Star
• The remnant radio galaxy associated with NGC 1534
• The First Mid-Infrared Detection of HNC in the Interstellar Medium: Probing the Extreme Environment Towards the Orion Hot Core
• Size and Temperature Transferability of Direct and Local Deep Neural Networks for Atomic Forces
• Salt-bearing disk candidates around high-mass young stellar objects
• Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
• Three-Dimensional Structure and Dust Extinction in the Small Magellanic Cloud
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• A MeerKAT-meets-LOFAR study of Abell 1413: a moderately disturbed non-cool-core cluster hosting a $\sim 500$ kpc 'mini'-halo
• X-PSI Parameter Recovery for Temperature Map Configurations Inspired by PSR J0030+0451
• Neutrino Interactions in the Late Universe
• Investigating the Projected Phase Space of Gaussian and Non-Gaussian Clusters
• A global view on star formation: The GLOSTAR Galactic plane survey VIII. Formaldehyde absorption in Cygnus~X
• An Extension of the Athena++ Framework for General Equations of State
• The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
• Spatially-resolved chemodynamics of the starburst dwarf galaxy CGCG 007-025: Evidence for recent accretion of metal-poor gas
• Periodic repeating fast radio bursts: interaction between a magnetized neutron star and its planet in an eccentric orbit
• Signatures of magnetic activity: On the relation between stellar properties and p-mode frequency variations
• X-Ray Spectroscopy of Newly Identified ULXs Associated With M87's Globular Cluster Population
• Galactic synchrotron distribution derived from 152 HII region absorption features in the full GLEAM survey
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• The Nonstandard Properties of a "Standard" PWN: Unveiling the Mysteries of PWN G21.5-0.9 Using its IR and X-ray emission
• Behavior of the maximum likelihood in quantum state tomography
• On the Dust Signatures Induced by Eccentric Super-Earths in Protoplanetary Disks
• Discovery of Magellanic Stellar Debris in the H3 Survey
• A Young, Low-Density Stellar Stream in the Milky Way Disk: Theia 456
• A Faraday Rotation Study of the Stellar Bubble and HII Region Associated with the W4 Complex
• Orbital distribution of infalling satellite halos across cosmic time
• Molecular gas and Star Formation Properties in Early Stage Mergers: SMA CO(2-1) Observations of the LIRGs NGC 3110 and NGC 232
• The Metallicity Gradient and Complex Formation History of the Outermost Halo of the Milky Way
• Hydrodynamic Winds From Twin-Star Binaries
• The GTC exoplanet transit spectroscopy survey X. Stellar spots versus Rayleigh scattering: the case of HAT-P-11b
• Systematic uncertainties in models of the cosmic dawn
• Forecasting Chemical Abundance Precision for Extragalactic Stellar Archaeology
• XAutoML: A Visual Analytics Tool for Understanding and Validating Automated Machine Learning
• The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
• The galaxy-galaxy strong lensing cross-sections of simulated LCDM galaxy clusters
• The halo of M105 and its group environment as traced by planetary nebula populations: I. Wide-field photometric survey of planetary nebulae in the Leo I group
• The Effects of Asymmetric Dark Matter on Stellar Evolution I: Spin-Dependent Scattering
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q Band
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• Lyman continuum leakage in faint star-forming galaxies at redshift z=3-3.5 probed by gamma-ray bursts
• A Population of Dipper Stars from the Transiting Exoplanet Survey Satellite Mission
• The inner disk of RY Tau: evidence of stellar occultation by the disk atmosphere at the sublimation rim from K-band continuum interferometry
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• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• The globular cluster system of the Auriga simulations
• Exoplanet Transits with Next-Generation Radio Telescopes
• Early Planet Formation in Embedded Disks (eDisk) V: Possible Annular Substructure in a Circumstellar Disk in the Ced110 IRS4 System
• TauRunner: A Public Python Program to Propagate Neutral and Charged Leptons
• MINOT: Modeling the intracluster medium (non-)thermal content and observable prediction tools
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• The nature of CR7 revealed with MUSE: a young starburst powering extended Lyman-$\alpha$ emission at z=6.6
• Establishing significance of gravitational-wave signals from a single observatory in the PyCBC offline search
• Benchmarking Dust Emission Models in M101
• The MAVERIC Survey: Radio catalogs and source counts from deep Very Large Array imaging of 25 Galactic globular clusters
• The Epoch of Giant Planet Migration Planet Search Program. I. Near-Infrared Radial Velocity Jitter of Young Sun-like Stars
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Physics of Thermonuclear Explosions: Magnetic Field Effects on Deflagration Fronts and Observable Consequences
• Comment on "An excess of massive stars in the local 30 Doradus starburst"
• Towards a full $w$CDM map-based analysis for weak lensing surveys
• Training Agents using Upside-Down Reinforcement Learning
• Identifying Flux Rope Signatures Using a Deep Neural Network
• Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics
• Mass-to-Light Ratios of Spatially Resolved Stellar Populations in M31
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Phase-Apodized-Pupil Lyot Coronagraphs for Arbitrary Telescope Pupils
• On the possible triple central star system of PN SuWt 2: No ménage à trois at the heart of the Wedding Ring
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• Magnetohydrodynamic Simulations of the Tayler Instability in Rotating Stellar Interiors
• KLLR: A scale-dependent, multivariate model class for regression analysis
• The Impact of Stellar Clustering on the Observed Multiplicity and Orbital Periods of Planetary Systems
• Exploring Parameter Spaces with Artificial Intelligence and Machine Learning Black-Box Optimisation Algorithms
• The Unusual Apparition of Comet 252P/2000 G1 (LINEAR) and Comparison with Comet P/2016 BA14 (PanSTARRS)
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• On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres
• TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS
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• Detection of Al II in the Ultraviolet Spectra of Metal-Poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
• HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco
• Limits on the Auroral Generation of H${}_3^{+}$ in Brown Dwarf and Extrasolar Giant Planet Atmospheres with Keck/NIRSPEC
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• A Black Hole Kicked At Birth: MAXI J1305-704
• The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) II. The radial structure of debris discs
• KSP-SN-2016kf: a long-rising H-rich Type II Supernova with unusually high ${}^{56}$Ni mass discovered in the KMTNet Supernova Program
• The mid-infrared molecular inventory towards Orion IRc2
• Galaxy morphologies at cosmic noon with JWST: A foundation for exploring gas transport with bars and spiral arms
• Detecting Globular Cluster Tidal Extensions with Bayesian Inference: I. Analysis of $\omega$ Centauri with Gaia EDR3
• Estimating fast transient detection pipeline efficiencies at UTMOST via real-time injection of mock FRBs
• Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System
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• The unseen host galaxy and high dispersion measure of a precisely-localised Fast Radio Burst suggests a high-redshift origin
• Optical photometry of two transitional millisecond pulsars in the radio pulsar state
• Universal non-Debye low-frequency vibrations in sheared amorphous solids
• Radio Counterpart Candidates to 4FGL-DR2 Unassociated Sources
• The SLUGGS Survey: The Inner Dark Matter Density Slope of the Massive Elliptical Galaxy NGC 1407
• Multiple shock fronts in RBS 797: the Chandra window on shock heating in galaxy clusters
• TESS discovery of a super-Earth and three sub-Neptunes hosted by the bright, Sun-like star HD 108236
• Connecting optical morphology, environment, and HI mass fraction for low-redshift galaxies using deep learning
• The merging galaxy cluster Abell 3266 at low radio frequencies
• USID and Pycroscopy -- Open frameworks for storing and analyzing spectroscopic and imaging data
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• Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Millisecond Pulsars Modify the Radio-SFR Correlation in Quiescent Galaxies
• Interplay between $k$-core and community structure in complex networks
• $S^5$: The destruction of a bright dwarf galaxy as revealed by the chemistry of the Indus stellar stream
• Evolution of Helium Star - White Dwarf Binaries Leading up to Thermonuclear Supernovae
• A RAD approach to deep mixture models
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• RE-EDS Using GAFF Topologies: Application to Relative Hydration Free-Energy Calculations for Large Sets of Molecules
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• Diffuse interstellar bands λ5780 and λ5797 in the Antennae Galaxy as seen by MUSE
• SystemDS: A Declarative Machine Learning System for the End-to-End Data Science Lifecycle
• Rave: A non-parametric method for recovering the surface brightness and height profiles of edge-on debris disks
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• Day-night transport induced chemistry and clouds on WASP-39b I: Gas-phase composition
• The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution and the Nyquist-Shannon theorem
• An Adaptive Feature Extraction Algorithm for Classification of Seismocardiographic Signals
• Molecules with ALMA at Planet-forming Scales (MAPS). Complex Kinematics in the AS 209 Disk Induced by a Forming Planet and Disk Winds
• The trajectories of galaxies in groups: mass loss and preprocessing
• The Three Hundred Project: the evolution of physical baryon profiles
• Accretion History of AGN III: Radiative Efficiency and AGN Contribution to Reionization
• An elusive dark central mass in the globular cluster M4
• MR. Estimator, a toolbox to determine intrinsic timescales from subsampled spiking activity
• 174P/Echeclus and its Blue Coma Observed Post-outburst
• Quantum chemistry with Coulomb Sturmians: Construction and convergence of Coulomb Sturmian basis sets at Hartree-Fock level
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• New member candidates of Upper Scorpius from Gaia DR1
• Extreme Ionizing Properties of Metal-Poor, Muv ~ -12 Star Complex in the first Gyr
• The winds of young Solar-type stars in the Pleiades, AB Doradus, Columba and $\beta$ Pictoris
• Invisible Higgs search through Vector Boson Fusion: A deep learning approach
• Aluminum-26 Enrichment in the Surface of Protostellar Disks Due to Protostellar Cosmic Rays
• Free-Floating Planets, Survivor Planets, Captured Planets and Binary Planets from Stellar Flybys
• Ram pressure stripping of the multiphase ISM: a detailed view from TIGRESS simulations
• Recombination Lines and Molecular Gas from Hypercompact HII regions in W51 A
• R Coronae Borealis Star Evolution: Simulating 3D Merger Events to 1D Stellar Evolution Including Large Scale Nucleosynthesis
• Radial migration of gap-opening planets in protoplanetary disks. II. The case of a planet pair
• A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain
• Sacrificing information for the greater good: how to select photometric bands for optimal accuracy
• X-Ray and Gamma-Ray Emission From Core-collapse Supernovae: Comparison of Three-dimensional Neutrino-driven Explosions With SN 1987A
• A revisited study of Cepheids in open clusters in the Gaia era
• Murchison Widefield Array rapid-response observations of the short GRB 180805A
• A full-fledged micromagnetic code in less than 70 lines of NumPy
• Molecular Flows in Contemporary Active Galaxies and the Efficacy of Radio-Mechanical Feedback
• A Phantom Menace: On the Morphology of the Galactic Center Excess
• Common Envelope Wind Tunnel: Range of Applicability and Self-Similarity in Realistic Stellar Envelopes
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments II: Star Formation and Pressure Balance in HI-Rich UDGs
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• Probing the Star Formation Main Sequence down to $10^8$ M${}_{\odot }$ at $1.0<z<3.0$
• A candidate relativistic tidal disruption event at 340 Mpc
• Multi-Channel Auto-Calibration for the Atmospheric Imaging Assembly using Machine Learning
• JeLLyFysh-Version1.0 -- a Python application for all-atom event-chain Monte Carlo
• Analytical marginalisation over photometric redshift uncertainties in cosmic shear analyses
• The secular growth of bars revealed by flat (peak + shoulders) density profiles
• Predicting Acute Kidney Injury at Hospital Re-entry Using High-dimensional Electronic Health Record Data
• Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectors
• Learning Optimal Control of Synchronization in Networks of Coupled Oscillators using Genetic Programming-based Symbolic Regression
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Bayesian Characterisation of Circumbinary Exoplanets with LISA
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• M giants with IGRINS I. Stellar parameters and $\alpha$-abundance trends of the solar neighborhood population
• Thunder and Lightning: Using Neutron-Star Mergers as Simultaneous Standard Candles and Sirens to Measure Cosmological Parameters
• Expectations on the mass determination using astrometric microlensing by Gaia
• Bayesian Dynamic Mapping of an Exo-Earth from Photometric Variability
• A 3mm chemical exploration of small organics in Class I YSOs
• A Star-sized Impact-Produced Dust Clump in the Terrestrial Zone of the HD 166191 System
• The prototypical major cluster merger Abell 754. I. Calibration of MeerKAT data and radio/X-ray spectral mapping of the cluster
• Anomalous dynamics of interstitial dopants in soft crystals
• Probing an X-ray flare pattern in Mrk 421 induced by multiple stationary shocks: a solution to the bulk Lorentz factor crisis
• Fusion of Array Operations at Runtime
• Dusty, Self-obscured Transients from Stellar Coalescence
• Constraining the orbit of the planet-hosting binary $\tau$ Boötis: Clues about planetary formation and migration
• Linking nearby stellar streams to more distant halo overdensities
• The Impact of Initial-Final Mass Relations on Black Hole Microlensing
• Measurements of the Hyperfine Structure of Atomic Energy Levels in Co II
• Presence of red giant population in the foreground stellar sub-structure of the Small Magellanic Cloud
• Substructures, Resonances and debris streams
• The GALAH+ Survey: A New Library of Observed Stellar Spectra Improves Radial Velocities and Hints at Motions within M67
• The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS) I: A Pilot Study of the stellar populations in NGC 2298 and NGC 3201
• Fast optimization of parametrized quantum optical circuits
• MAXI J1848-015: The First Detection of Relativistically Moving Outflows from a Globular Cluster X-ray Binary
• An ultra-deep multi-band VLA survey of the faint radio sky (COSMOS-XS): New constraints on the cosmic star formation history
• Three Ultraluminous X-ray Sources Hosted by Globular Clusters in NGC 1316
• Tracer particles for core-collapse supernova nucleosynthesis: The advantages of moving backward
• Heavy Positive Ion Groups in Titan's Ionosphere from Cassini Plasma Spectrometer IBS Observations
• Galactic Conformity in both Star-formation and Morphological Properties
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• ED-2: a cold but not so narrow stellar stream crossing the Solar neighbourhood
• Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
• Plane-wave approach to the exact van der Waals interaction between colloid particles
• Constraints On Short, Hard Gamma-Ray Burst Beaming Angles From Gravitational Wave Observations
• T CrB: Radio Observations During the 2016--2017 "Super-Active" State
• Atomium: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae. I. Morpho-kinematical interpretation of CO and SiO emission
• Stellar intensity interferometry of Vega in photon counting mode
• Evolution Reinforces Cooperation with the Emergence of Self-Recognition Mechanisms: an empirical study of the Moran process for the iterated Prisoner's dilemma
• Long-term study of extreme giant pulses from PSR B0950+08 with AARTFAAC
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?
• KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
• A Comparison of Rotating and Binary Stellar Evolution Models: Effects on Massive Star Populations
• Spirals and clumps in V960 Mon: signs of planet formation via gravitational instability around an FU Ori star?
• The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
• A double-peaked Lyman-$\alpha$ emitter with a strong blue peak multiply imaged by the galaxy cluster RXC J0018.5+1626
• Microlensing and the type Ia supernova iPTF16geu
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• The Age-Metallicity-Specific Orbital Energy Relation for the Milky Way's Globular Cluster System Confirms the Importance of Accretion for Its Formation
• The ALHAMBRA survey: 2-D analysis of the stellar populations in massive early-type galaxies at z < 0.3
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
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• The VLT/SPHERE view of the ATOMIUM cool evolved star sample. I. Overview: Sample characterization through polarization analysis
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• TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by \textit{TESS}
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• Pulsational instability of pre-main-sequence models from accreting protostars II. Modelling echelle diagrams of $\delta$ Scuti stars without rotational splitting
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• The Development of Non-coherent Passive Radar Techniques for Space Situational Awareness with the Murchison Widefield Array
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• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
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• Modeling JWST MIRI-MRS Observations of T Cha: Mid-IR Noble Gas Emission Tracing a Dense Disk Wind
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• One-third of Sun-like stars are born with misaligned planet-forming disks
• Can primordial black holes explain the overabundance of bright super-early galaxies?
• Search for Blazar Flux-Correlated TeV Neutrinos in IceCube 40-String Data
• SN 2012ij: A low-luminosity type Ia supernova and evidence for continuous distribution from 91bg-like explosion to normal ones
• The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries
• Reducing ground-based astrometric errors with Gaia and Gaussian processes
• The First Data Release from SweetSpot: 74 Supernovae in 36 Nights on WIYN+WHIRC
• $Chempy$: A flexible chemical evolution model for abundance fitting - Do the Sun's abundances alone constrain chemical evolution models?
• Designing an Optimal LSST Deep Drilling Program for Cosmology with Type Ia Supernovae
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Prospects for Directly Imaging Young Giant Planets at Optical Wavelengths
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• A DECam Search for Explosive Optical Transients Associated with IceCube Neutrinos
• Evolution and the quasistationary state of collective fast neutrino flavor conversion in three dimensions without axisymmetry
• M Giants with IGRINS II. Chemical Evolution of Fluorine at High Metallicities
• Precise Ages of Field Stars From White Dwarf Companions in Gaia DR2
• Characterisation of the ground layer of turbulence at Paranal using a robotic SLODAR system
• The WAGGS project -- III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity
• Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
• Distance mapping applied to four well-known planetary nebulae and a nova shell
• Non-Local Thermodynamic Equilibrium Transmission Spectrum Modelling of HD209458b
• Probing fermionic asymmetric dark matter cores using global neutron star properties
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• 3D orbital architecture of a dwarf binary system and its planetary companion
• A Preliminary Calibration of the JAGB Method Using Gaia EDR3
• Static Energy in ($2+1+1$)-Flavor Lattice QCD: Scale Setting and Charm Effects
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Strong Near-Infrared Carbon Absorption in the Transitional Type Ia SN 2015bp
• The Lyman Alpha Spectral Database (LASD)
• Galaxy Tagging: photometric redshift refinement and group richness enhancement
• Cherenkov Telescope Array sensitivity to branon dark matter models
• Which Part of Dense Cores Feeds Material to Protostars?: The Case of L1489 IRS
• Non-Radial Pulsations in Post-Outburst Novae
• Stellar flare morphology with TESS across the main sequence
• DmpIRFs and DmpST: DAMPE Instrument Response Functions and Science Tools for Gamma-Ray Data Analysis
• Limits on a population of collisional-triples as progenitors of Type-Ia supernovae
• Harvesting BAT-GUANO with NITRATES (Non-Imaging Transient Reconstruction And TEmporal Search): Detecting and localizing the faintest GRBs with a likelihood framework
• Step Change Improvement in ADMET Prediction with PotentialNet Deep Featurization
• Dimensionalities and multiplicities determination of crystal nets
• Sensitivity of the Cherenkov Telescope Array to dark subhalos
• MBRL-Lib: A Modular Library for Model-based Reinforcement Learning
• BAT AGN Spectroscopic Survey -- XIII. The nature of the most luminous obscured AGN in the low-redshift universe
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• Probing the cold neutral medium through HI emission morphology with the scattering transform
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• NEID Reveals that The Young Warm Neptune TOI-2076 b Has a Low Obliquity
• On the Rotation of the Solar Chromosphere
• Recovering the origins of the lenticular galaxy NGC 3115 using multi-band imaging
• Atmospheric Characterization of Hot Jupiter CoRoT-1 b Using the Wide Field Camera 3 on the Hubble Space Telescope
• Bayesian hierarchical inference of asteroseismic inclination angles
• Characteristics of flares on giant stars
• Mass function of a young cluster in a low-metallicity environment. Sh 2-209
• Angular Momentum Evolution of Young Stars in the Nearby Scorpius-Centaurus OB Association
• GWSim: Python package for creating mock GW samples for different astrophysical populations and cosmological models of binary black holes
• X-Ray Luminous Supernovae: Threats to Terrestrial Biospheres
• Search for very-high-energy emission from Gamma-ray Bursts using the first 18 months of data from the HAWC Gamma-ray Observatory
• Asteroid (21) Lutetia: Disk-resolved Photometric Analysis of Baetica Region
• PHIDL: Python CAD layout and geometry creation for nanolithography
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Aerosol Constraints on the Atmosphere of the Hot Saturn-mass planet WASP-49b
• Performance and characterization of the SPT-3G digital frequency-domain multiplexed readout system using an improved noise and crosstalk model
• Deflation reveals dynamical structure in nondominant reaction coordinates
• Ultra-deep imaging of NGC1052-DF2 and NGC1052-DF4 to unravel their origins
• The universality of the rapid neutron-capture process revealed by a possible disrupted dwarf galaxy star
• LEO-Py: Estimating likelihoods for correlated, censored, and uncertain data with given marginal distributions
• Using the Properties of Broad Absorption Line Quasars to Illuminate Quasar Structure
• X-ray Absorption in Young Core-Collapse Supernova Remnants
• Neural networks: solving the chemistry of the interstellar medium
• A Versatile and Accurate Method for Halo Mass Determination from Phase-Space Distribution of Satellite Galaxies
• Assessing Spectroscopic-Binary Multiplicity Properties Using Robo-AO Imaging
• Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
• Spectroscopic Analysis Tool for intEgraL fieLd unIt daTacubEs (satellite): Case studies of NGC 7009 and NGC 6778 with MUSE
• Shape of the outer stellar warp in the Large Magellanic Cloud disk
• Internal magnetic field structures observed by PSP/WISPR in a filament related coronal mass ejection
• Multimessenger Gamma-Ray and Neutrino Coincidence Alerts using HAWC and IceCube sub-threshold Data
• Chlorine Isotope Ratios in M Giants
• Gaia's brightest very metal-poor (VMP) stars. Metallicity catalogue of a thousand VMP stars from Gaia's radial velocity spectrometer spectra
• Optimal Fitting and Debiasing for Detectors Read Out Up-the-Ramp
• The nebular spectra of SN 2023ixf: A lower mass, partially stripped progenitor may be the result of binary interaction
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• Water shielding in the terrestrial planet-forming zone: Implication for inner disk organics
• Constraining the Shape Distribution of Near Earth Objects from Partial Lightcurves
• Cross-Comparison of Sampling Algorithms for Pulse Profile Modeling of PSR J0740+6620
• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
• A 4-8 GHz Galactic Center Search for Periodic Technosignatures
• Search for Extremely Metal-Poor Stars with GEMINI-N/GRACES I. Chemical-Abundance Analysis
• A Transparent Window into Early-Type Stellar Variability
• The DEHVILS Survey Overview and Initial Data Release: High-Quality Near-Infrared Type Ia Supernova Light Curves at Low Redshift
• Targeted modeling of GW150914's binary black hole source with dart_board
• On the Galactic rotation curve inferred from the Jeans equations Assessing its robustness using Gaia DR3 and cosmological simulations
• An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models
• PRODIGE -- Envelope to Disk with NOEMA III. The origin of complex organic molecule emission in SVS13A
• Edges and Endpoints in 21-cm Observations from Resonant Photon Production
• Globular Clusters UVIT Legacy Survey (GlobULeS) I. FUV-optical Color-Magnitude Diagrams for Eight Globular Clusters
• Reconstructing Probability Distributions with Gaussian Processes
• Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-Dominated Shells
• Searching for NLTE effects in the high-resolution transmission spectrum of WASP-121 b with Cloudy for Exoplanets
• TDCOSMO VIII: A key test of systematics in the hierarchical method of time-delay cosmography
• The FluxCompensator: Making Radiative Transfer Models of hydrodynamical Simulations Directly Comparable to Real Observations
• Dust Survival in Galactic Winds
• The inner circumstellar dust of the red supergiant Antares as seen with VLT/SPHERE/ZIMPOL
• APOGEE/Kepler Overlap Yields Orbital Solutions for a Variety of Eclipsing Binaries
• A Multilevel Scheduling Framework for Distributed Time-domain Large-area Sky Survey Telescope Array
• Passive and active colloidal chemotaxis in a microfluidic channel: mesoscopic and stochastic models
• The origin of the soft X-ray excess in the narrow-line Seyfert 1 galaxy SBS 1353+564
• Tidal Wave Breaking in the Eccentric Lead-In to Mass Transfer and Common Envelope Phases
• Target of Opportunity Observations Detectability of Kilonovae with WFST
• Improved detection of farside solar active regions using deep learning
• Asteroid Photometry from the Transiting Exoplanet Survey Satellite: A Pilot Study
• Footprints of population III stars in the gravitational-wave background
• Dark Matter Substructure under the Electron Scattering Lamppost
• Kinematical Investigation of Possible Fast Collimated Outflows in Twelve Planetary Nebulae
• A Study of Stellar Spins in 15 Open Clusters
• Limitations imposed by optical turbulence profile structure and evolution on tomographic reconstruction for the ELT
• The VLT-MUSE and ALMA view of the MACS 1931.8-2635 brightest cluster galaxy
• Galactic Extinction: How Many Novae Does it Hide and How Does it Affect the Galactic Nova Rate?
• Gravitational Self-Force Regularization in the Regge-Wheeler and Easy Gauges
• Improved Sensitivity for Space Domain Awareness Observations with the Murchison Widefield Array
• Calculating the distance from an electronic wave function to the manifold of Slater determinants through the geometry of Grassmannians
• AVIATOR: Morphological object reconstruction in 3D. An application to dense cores
• Analysis of high-resolution FEROS spectroscopy for a sample of variable B-type stars assembled from TESS photometry
• Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
• Constraining properties of neutron star merger outflows with radio observations
• Debris Disks in Multi-Planet Systems: Are Our Inferences Compromised by Unseen Planets?
• A bias in VLBI measurements of the core shift effect in AGN jets
• Accelerating Hybrid Monte Carlo simulations of the Hubbard model on the hexagonal lattice
• Two Planets Straddling the Habitable Zone of The Nearby K Dwarf Gl 414A
• JWST Transit Spectra II: Constraining Aerosol Species, Particle-size Distributions, Temperature, and Metallicity for Cloudy Exoplanets
• An analysis of the most distant catalogued open clusters -- Re-assessing fundamental parameters with Gaia EDR3 and $\text{ASteCA}$
• Exploring the relation between dust mass and galaxy properties using Dusty SAGE
• Forecasting COVID-19 spreading trough an ensemble of classical and machine learning models: Spain's case study
• Radio light curves and imaging of the helium nova V445 Puppis reveal seven years of synchrotron emission
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• Detection of Pb II in the Ultraviolet Spectra of Three Metal-Poor Stars
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• A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
• Rotation of Kepler field dwarfs and sub giants: Spectroscopic $v\sin I$ from APOGEE
• Linking the primordial composition of planet building disks to the present-day composition of rocky exoplanets
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• The impact and response of minihalos and the inter-halo medium on cosmic reionization
• Self-consistent ring model in protoplanetary disks: temperature dips and substructure formation
• Stellar Population and Elemental Abundance Gradients of Early-type Galaxies
• Hiding Signatures of Gravitational Instability in Protoplanetary Discs with Planets
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• Chemo-Dynamical Clustering applied to APOGEE data: Re-Discovering Globular Clusters
• Planet formation in the PDS 70 system: Constraining the atmospheric chemistry of PDS 70b and c
• A pilot ASKAP survey for radio transients towards the Galactic Centre
• Characteristic mass in galaxy quenching: environmental versus internal effects
• A neural network model for solvency calculations in life insurance
• Towards a fully consistent Milky Way disk model -- IV. The impact of Gaia DR2 and APOGEE
• High-contrast observations of brown dwarf companion HR 2562 B with the vector Apodizing Phase Plate coronagraph
• The outermost edges of the Milky Way halo from galaxy kinematics
• Statistical Detection of IGM Structures during Cosmic Reionization using Absorption of the Redshifted 21 cm line by HI against Compact Background Radio Sources
• Stability and detectability of exomoons orbiting HIP 41378 f, a temperate Jovian planet with an anomalously low apparent density
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Share the Tensor Tea: How Databases can Leverage the Machine Learning Ecosystem
• On the nature of radio-wave radiation from particle cascades
• Wide-Band Spectral Variability of Peaked Spectrum Sources
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• The impact of mass map truncation on strong lensing simulations
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Radial and vertical constraints on the icy origin of H${}_2$CO in the HD 163296 Protoplanetary Disk
• A new software implementation of the Oslo method with rigorous statistical uncertainty propagation
• New Ionization Models and the Shocking Nitrogen Excess at z > 5
• 44 GHz methanol masers: Observations toward 95 GHz methanol masers
• A Larger Extent for the Ophiuchus Stream
• Extending the view of ArH+ chemistry in diffuse clouds
• Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopes
• Tasks, stability, architecture, and compute: Training more effective learned optimizers, and using them to train themselves
• Debris of asteroid disruptions close to the Sun
• Testing CMB Anomalies in E-mode Polarization with Current and Future Data
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Beyond the first galaxies primordial black holes shine
• The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging
• Cross Helicity and the Helium Abundance as an in situ Metric of Solar Wind Acceleration
• The PFS view of TOI-677 b: A spin-orbit aligned warm Jupiter in a dynamically hot system
• Exploring the low-mass regime of galaxy-scale strong lensing: Insights into the mass structure of cluster galaxies
• Fundamental MHD scales -- II: the kinematic phase of the supersonic small-scale dynamo
• Towards ultra metal-poor DLAs: linking the chemistry of the most metal-poor DLA to the first stars
• Clusters, Clouds, and Correlations: Relating Young Clusters to Giant Molecular Clouds in M33 and M31
• Shedding New Light on Weak Emission-Line Quasars in the C${}_{\mathrm{IV}}$-H$\beta$ Parameter Space
• A BCool survey of stellar magnetic cycles
• Hunting Down White Dwarf--Main Sequence Binaries Using Multi-Wavelength Observations
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• Elemental abundances in M31: Individual and Coadded Spectroscopic [Fe/H] and [α/Fe] throughout the M31 Halo with SPLASH
• A hybrid map-$C_{\ell }$ component separation method for primordial CMB $B$-mode searches
• Why weak lensing cluster shapes are insensitive to self-interacting dark matter
• The First Two Years of FLEET: an Active Search for Superluminous Supernovae
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• The death of Vulcan: NEID reveals the planet candidate orbiting HD 26965 is stellar activity
• Finding $r$-II sibling stars in the Milky Way with the Greedy Optimistic Clustering algorithm
• The star formation history in the last 10 billion years from CIB cross-correlations
• Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars. Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey: III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-Transit Jupiter Orbiting TOI-2010
• Stability Constrained Characterization of the 23 Myr-old V1298 Tau System: Do Young Planets Form in Mean Motion Resonance Chains?
• Magnetic catalysis in the (2+1)-dimensional Gross-Neveu model
• A galaxy-free phenomenological model for the 21-cm power spectrum during reionization
• Early-time Searches for Coherent Radio Emission from Short GRBs with the Murchison Widefield Array
• The bar rotation rate as a diagnostic of dark matter content in the centre of disc galaxies
• On the Reionization-Era Globular Cluster in Low-Mass Galaxy Eridanus II
• Modeling Polarization Signals from Cloudy Brown Dwarfs: Luhman 16 A and B in Three Dimensions
• Warping Away Gravitational Instabilities in Protoplanetary Discs
• Hunting intermediate-mass black holes with LISA binary radial velocity measurements
• The nascent milliquasar VT J154843.06+220812.6: tidal disruption event or extreme accretion-state change?
• Tracers of Dense Gas in the Outer Galaxy
• Constraining CMB temperature evolution with Sunyaev-Zel'dovich galaxy clusters from the Atacama Cosmology Telescope
• Exploring the Limits of Synthetic Creation of Solar EUV Images via Image-to-Image Translation
• TedNet: A Pytorch Toolkit for Tensor Decomposition Networks
• On the Impulsive Heating of Quiet Solar Corona
• A Nascent Tidal Dwarf Galaxy Forming within the Northern HI Streamer of M82
• Multi-dimensional population modelling using frbpoppy: magnetars can produce the observed Fast Radio Burst sky
• A Census of Thermally-Pulsing AGB stars in the Andromeda Galaxy and a First Estimate of their Contribution to the Global Dust Budget
• First images of phosphorus molecules towards a proto-Solar analog
• repro_eval: A Python Interface to Reproducibility Measures of System-oriented IR Experiments
• Distributional Generalization: A New Kind of Generalization
• Detection of 2$-$4 GHz Continuum Emission from $\epsilon$ Eridani
• Modeling optical roughness and first-order scattering processes from OSIRIS-REx color images of the rough surface of asteroid (101955) Bennu
• PySAD: A Streaming Anomaly Detection Framework in Python
• Structure and Isotropy of Lattice Pressure Tensors for Multi-range Potentials
• A misfired outburst in the neutron star X-ray binary Centaurus X-4
• USuRPER: Unit-Sphere Representation PERiodogram for full spectra
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• The AstroSat Mass Model: Imaging and Flux studies of off-axis sources with CZTI
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• Analytical halo models of cosmic tidal fields
• The Exomoon Corridor for Multiple Moon Systems
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• Galactic Magnetic Field Bias on Inferences from UHECR Data
• Interstellar anatomy of the TeV gamma-ray peak in the IC443 supernova remnant
• LOFAR observations of radio burst source sizes and scattering in the solar corona
• Dynamics of Laterally Propagating Flames in X-ray Bursts. I. Burning Front Structure
• Separating the Intrinsic Alignment Signal and the Lensing Signal using Self-Calibration in Photo-z Surveys with KiDS450 and KV450 Data
• Searching for energy-resolved quasi-periodic oscillations in AGN
• SDSS-IV MaNGA: the "G-dwarf problem" revisited
• A hyper-runaway white dwarf in Gaia DR2 as a Type Iax supernova primary remnant candidate
• Design and Performance Analysis of a Highly Efficient Polychromatic Full-Stokes Polarization Modulator for the CRISP Imaging Spectrometer
• Accurate mass estimates from the proper motions of dispersion-supported galaxies
• When the Peas Jump around the Pod: How Stellar Clustering Affects the Observed Correlations between Planet Properties in Multi-Planet Systems
• Enabling catalog simulations of transient and variable sources based on LSST cadence strategies
• Prospects for Observing the low-density Cosmic Web in Lyman-alpha Emission
• A systematic study of galactic outflows via fluorescence emission: implications for their size and structure
• Computational Prediction of Muon Stopping Sites: a Novel Take on the Unperturbed Electrostatic Potential Method
• Titanium and Iron in the Cassiopeia A Supernova Remnant
• Joint Bayesian analysis of large angular scale CMB temperature anomalies
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• Observations of the Kepler Field with TESS: Predictions for Planet Yield and Observable Features
• Spin-down rate of the transitional millisecond pulsar PSR J1023+0038 in the optical band with Aqueye+
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• Beyond optical depth: Future determination of ionization history from the CMB
• Estimating probabilistic context-free grammars for proteins using contact map constraints
• The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups
• Variational Integrators for Inertial Magnetohydrodynamics
• The Rotation-Disk Connection in Young Brown Dwarfs: Strong Evidence for Early Rotational Braking
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• Insights from snapshot spectroscopic radio observations of a weak Type I noise storm
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• On estimating angular momenta of infalling protostellar cores from observations
• Edge-on Low-surface-brightness Galaxy Candidates Detected from SDSS Images Using YOLO
• The Search for Fast Transients with CZTI
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• Three Dusty Star Forming Galaxies at $z\sim 1.5$: Mergers and Disks on the Main Sequence
• Flaring Stars in a Non-targeted mm-wave Survey with SPT-3G
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• A Flat-Spectrum Radio Transient at 122 Mpc consistent with an Emerging Pulsar Wind Nebula
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• Extremely precise age and metallicity of the open cluster NGC 2506 using detached eclipsing binaries
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• Testing the dark matter subhalo hypothesis of the gamma-ray source 3FGL J2212.5+0703
• Likelihood-Based Jump Detection and Cosmic Ray Rejection for Detectors Read Out Up-the-Ramp
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• Conversions between gas-phase metallicities in MaNGA
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• 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
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• A multispectral analysis of the northeastern shell of IC 443
• Three Dimensional Optimal Spectral Extraction (TDOSE) from Integral Field Spectroscopy
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• 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
• The $n$-point streaming model: how velocities shape correlation functions in redshift space
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• UOCS-IX. AstroSat/UVIT study of the open cluster NGC 2818: Blue Stragglers, Yellow Stragglers, Planetary Nebula, and their membership
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• The peculiar chemical abundance of the transitional millisecond pulsar PSR J1023+0038 -- Li enhancement
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• Local Analogs to High-Redshift Galaxies: I. Characterization of Dust Emission and Star Formation History
• Improved Atomic Transition Probabilities for UV and Optical Lines of Hf II and Determination of the Hf Abundance in Two Metal-Poor Stars
• Automated Extended Aperture Photometry of K2 variable stars
• EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope
• Variability of massive stars in M31 from the Palomar Transient Factory
• Group pre-processing versus cluster ram-pressure stripping: the case of ESO156-G029
• The cosmology dependence of the concentration-mass-redshift relation
• An Improved Method for Coupling Hydrodynamics with Astrophysical Reaction Networks
• Radio Emission from Binary Ultracool Dwarf Systems
• Long-term X-ray Variability of the Symbiotic System RT Cru based on Chandra Spectroscopy
• Quenching star formation with low-luminosity AGN winds
• OSSOS XII: Variability studies of 65 Trans-Neptunian Objects using the Hyper Suprime-Cam
• The influence of globular cluster evolution on the specific frequency in dwarf galaxies
• Probing delayed-end reionization histories with the 21cm-LAE cross-power spectrum
• Discovery of δ Scuti Pulsations in the Young Hybrid Debris Disk Star HD 156623
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• The spatially resolved stellar population and ionized gas properties in the merger LIRG NGC 2623
• As A Matter of State: The role of thermodynamics in magnetohydrodynamic turbulence
• A Python Extension for the Massively Parallel Multiphysics Simulation Framework waLBerla
• Python Open Source Waveform Extractor (POWER): An open source, Python package to monitor and post-process numerical relativity simulations
• GEOMAX: beyond linear compression for 3pt galaxy clustering statistics
• Dynamical Formation Scenarios for GW190521 and Prospects for Decihertz Gravitational-Wave Astronomy with GW190521-Like Binaries
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• ATLASGAL: 3-mm class I methanol masers in high-mass star formation regions
• 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
• Retrieving cosmological information from small-scale CMB foregrounds I. The thermal Sunyaev Zel'dovich effect
• The Stellar "Snake" I: Whole Structure and Properties
• The MAVERIC survey: A catalogue of radio sources in southern globular clusters from the Australia Telescope Compact Array
• SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations
• Large-scale turbulent driving regulates star formation in high-redshift gas-rich galaxies II: Influence of the magnetic field and the turbulent compressive fraction
• Can the Fe K-alpha Line Reliably Predict Supernova Remnant Progenitors?
• A census of dwarf galaxy satellites around LMC-mass galaxy NGC 2403
• Constraints on the extragalactic magnetic field strength from blazar spectra based on 145 months of Fermi-LAT observations
• The Occurrence Rate of Quiescent Radio Emission for Ultracool Dwarfs using a Generalized Semi-Analytical Bayesian Framework
• Universal gravity-driven isothermal turbulence cascade in disk galaxies
• A wide survey for circumstellar disks in the Lupus complex
• High Energy Cosmic Rays from Fanaroff-Riley Radio Galaxies
• Toward More Reliable Analytic Thermochemical-equilibrium Abundances
• A comparative analysis of the outer-belt primitive families
• Ring Formation in Protoplanetary Disks Driven by an Eccentric Instability
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
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• Precise Measurements of the LMC Bar's Geometry With Gaia DR3 and a Novel Solution to Crowding Induced Incompleteness in Star Counting
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• Constraining the Milky Way's Ultraviolet to Infrared SED with Gaussian Process Regression
• Analyzing the Galactic pulsar distribution with machine learning
• Filling in the Gaps: Can Gravitationally Unstable Discs Form the Seeds of Gas Giant Planets?
• Streaming Classification of Variable Stars
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• A detailed understanding of the rotation-activity relationship using the 300 Myr old open cluster NGC 3532
• A hot Mars-sized exoplanet transiting an M dwarf
• The Solar Benchmark: Rotational Modulation of the Sun Reconstructed from Archival Sunspot Records
• Measured Spin-Orbit Alignment of Ultra-Short Period Super-Earth 55 Cancri e
• Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite
• SDSS-IV MaNGA: the chemical co-evolution of gas and stars in spiral galaxies
• A Pristine Star-Forming Complex at z=4.19
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