Astrophysical Journal

Papers
(The median citation count of Astrophysical Journal is 4. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2022-05-01 to 2026-05-01.)
ArticleCitations
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H i Disk of Galaxies4351
Double Shells of the Planetary Nebula NGC 7009 Minor Axis1082
The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity–Spectral Type Dependence in Taurus–Auriga YSOs742
Searching for Axion Dark Matter Gegenschein of the Vela Supernova Remnant with FAST464
H I Absorption Line and Anomalous Dispersion in the Radio Pulses of PSR B1937+21451
Detecting Atmospheric CO2 Trends as Population-level Signatures for Long-term Stable Water Oceans and Biotic Activity on Temperate Terrestrial Exoplanets369
Parsec-scale SiO Emission in the Galactic Center274
Helium-deficient ER UMa-type Dwarf Nova below the Period Minimum with a Hot Secondary267
Modeling the UV to Radio Spectral Energy Distribution of NGC 6946: Star Formation Rates and Dust Attenuation Properties256
Zonal Flow and Self-regulating Mechanism in a Hydrodynamic Disk223
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei203
Evaluating Non-LTE Spectral Inversions with ALMA and IBIS197
Effect of Dust in Circumgalactic Halos on the Cosmic Shear Power Spectrum191
Evidence of the Alfvén Transition Layer and Particle Precipitation in the Cusp Region: 3D Global PIC Simulation of the Solar Wind–Earth Magnetosphere Interaction191
DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos182
Active Galactic Nucleus Variability in the Age of Rubin180
Weighing the Darkness. III. How Gaia Could, but Probably Will Not, Astrometrically Detect Free-floating Black Holes178
Criss-cross Nebula: A Case Study of Shock Regions with Resolved Microstructures at Scales of ∼1000 au173
Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure172
On the Width of a Collisionless Shock and the Index of the Cosmic Rays It Accelerates167
Dark Off-limb Gap: Manifestation of a Temperature Minimum and the Dynamic Nature of the Chromosphere164
Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?163
Single-pulse Gamma-Ray Bursts Have Prevalent Hard-to-soft Spectral Evolution162
Multiple Rebrightenings in the Optical Afterglow of GRB 210731A: Evidence for an Asymmetric Jet161
The Orion OB Association as a Generator for the Hot Circumgalactic Medium160
Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding160
Evaluating the Limits of Rotation Period Recovery Through Gyrochronology Criteria156
Interaction of Inner Heliosheath Ions with Electromagnetic Ion Cyclotron Waves155
Multiline Stokes Synthesis of Ellerman Bombs: Obtaining Seamless Information from Photosphere to Chromosphere150
Mitigating Polarization Leakage in Gas Pixel Detectors through Hybrid Machine Learning and Analytic Event Reconstruction150
The Splashback Mass Function in the Presence of Massive Neutrinos148
The Propagation of Fast Radio Bursts in the Magnetosphere Shapes Their Waiting-time and Flux Distributions146
Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus145
Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey144
A Monte Carlo Simulation on the Scattering Coefficients of Solar Radio Wave Propagation143
Planetary Nebulae in the eROSITA eRASS1 Catalog143
Observations of Magnetospheric Solar Wind Charge Exchange141
Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph138
Searching for Propionamide (C2H5CONH2) toward Sagittarius B2 at Centimeter Wavelengths136
First Measurement of 87Rb(αxn) Cross Sections at Weak r-process Energies in Supernova ν-driven Ejecta to Investigate Elemental Abundances in Low-metallicity St136
When is a Bulge Not a Bulge? Revealing the Satellite Nature of NGC 5474’s Bulge136
Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts135
Photometric and Spectroscopic Observations of GRB 210104A: Bright Reverse-shock Emission and Dense Circumburst Environment133
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification133
Spectral Evolution of Ultraluminous X-Ray Pulsar NGC 300 ULX-1132
The “Canonical” White Dwarf Cooling Sequence of M5130
Global Distribution of the Key Species on the Surface of Europa130
Nucleosynthesis Conditions in Outflows of White Dwarfs Collapsing to Neutron Stars129
Photochemical Hazes Dramatically Alter Temperature Structure and Atmospheric Circulation in 3D Simulations of Hot Jupiters129
RRAT J2325–0530: A Rotating Radio Transient with an Atypical Waiting-time Distribution125
The z ≳ 9 Galaxy UV Luminosity Function from the JWST Advanced Deep Extragalactic Survey: Insights into Early Galaxy Evolution and Reionization119
A Census of Star Formation Histories of Massive Galaxies at 0.6 < z < 1 from Spectrophotometric Modeling Using Bagpipes and Prospector119
Improving Photometric Redshift Estimation for Cosmology with LSST Using Bayesian Neural Networks118
Quantifying the High Early Solar Cosmic-Ray Flux with Cosmogenic Neon Isotopes in Refractory Minerals118
Self-consistent Spin, Tidal, and Dynamical Equations of Motion in the REBOUNDx Framework117
Star Formation in the Lopsided Galaxy Arp 291117
The Role of Magnetic and Rotation Axis Alignment in Driving Fast Radio Burst Phenomenology115
Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae115
The Density Distribution of Compressively Forced, Supersonic Turbulence Depends on the Driving Correlation Time115
Impact of Current Uncertainties in the 12C+12C Nuclear Reaction Rate on Intermediate-mass Stars and Massive White Dwarfs114
How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-dust Geometry Model in Spectral Energy Distribution Fitting114
Azimuthal Size Scales of Solar Wind Periodic Density Structures114
The Local Group L-band Survey: The First Measurements of Localized Cold Neutral Medium Properties in the Low-metallicity Dwarf Galaxy NGC 6822113
A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity112
GASP. XLV. Stellar Bars in Jellyfish Galaxies: Analysis of Ionized Gas and Stellar Populations111
Physical Properties of 5000 Cool Large Magellanic Cloud Supergiants with Gaia XP Spectra: A Detailed Portrait of the Upper H-R Diagram Hints at Missing Supernova Progenitors110
Radiative Signatures of Magnetic Reconnection: An Approach to Remote Probing of Reconnection Dynamics108
Possibility of Using 3.3 μm Polycyclic Aromatic Hydrocarbon Luminosity as a Molecular Gas Mass Estimator108
When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multiband Imaging Data108
A Novel Blast Wave Solution for the Propagation of Coronal And Interplanetary Shocks107
The Internal Proper Motion Kinematics of NGC 346: Past Formation and Future Evolution104
The Origin and Evolution of the Normal Type Ia SN 2018aoz with Infant-phase Reddening and Excess Emission104
Identifying Signatures of Inflow onto Face-on Galaxies Using the Balmer Decrement104
The Diffusion Tensor of Protons at 1 au: Comparing Simulation, Observation, and Theory103
Repeating Nuclear Transients from Repeating Partial Tidal Disruption Events: Reproducing ASASSN-14ko and AT2020vdq101
The Effects of Turbulent Electrical Resistivity on the Response of the Solar Atmosphere to Flare Energy Input. I. Results of Radiative Hydrodynamic Simulations100
Dust Properties of 870 μm-selected Galaxies in GOODS-S100
Mode Mixing and Rotational Splittings. II. Reconciling Different Approaches to Mode Coupling 100
Coherent Imaging with Photonic Lanterns99
Interplanetary Type III Radio Emission Locations Deduced from the Underlying Electron Exciter Beam Kinematics99
Statistical Study of the Timing of the Appearance of H α Postflare Loops: Simple Scaling Law Based on Radiative Cooling99
Testing the Physical Parameter Constraining Power of HCN and HNC with Neural Networks97
The Impact of Cosmic Filaments on the Abundance of Satellite Galaxies96
The Radial Distribution of Ion-scale Waves in the Inner Heliosphere95
The Expanding 3 kpc Arms Are Neither Expanding nor Spiral Arms but X1 Orbits Driven by the Galactic Bar95
Quantitative Sensitivity Assessment of Martian Geodetic Parameters to Interior Model: Implications for Joint Inversion94
Scattering of Stellar Mass Black Holes and Gravitational-wave Bremsstrahlung Radiation in Active Galactic Nucleus Disks93
ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field93
Numerical Simulation of Hot Accretion Flow around Bondi Radius93
Spectropolarimetry of GRB 180427A: Evidence for Distinct Emission Sites with Varying Polarization92
Igneous Rim Accretion on Chondrules in Low-velocity Shock Waves91
Electrostatic Transport Characteristics of Olivine Particles under Electron Irradiation in Vacuum90
Geminga: A Window into the Role Played by the Local Halo in the Cosmic-Ray Propagation Process90
Ultraviolet and Gravitational Wave Signatures of Magnetar Formation90
Including Neutrino-driven Convection in the Force Explosion Condition to Predict Explodability of Multidimensional Core-collapse Supernovae (FEC+)89
Investigating the Impact of Atomic Data Uncertainties on the Measured Physical Parameters of the Perseus Galaxy Cluster89
A Holistic Exploration of the Potentially Recoverable Redshift Information of Stage IV Galaxy Surveys89
Small-scale Inhomogeneity Effects on Coherent Solar Radio Emission89
FAST Drift-scan Survey for H i Intensity Mapping: Simulation on Hunting H i Filament with Pairwise Stacking88
The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method88
Gravitational Influence from Planets on the Measured Rates of Period Change of Pulsating White Dwarfs88
Extreme Solar Flare-driven Short-wave Fadeout Observed by SuperDARN ZHO Radar87
XMM-Newton and NuSTAR Observations of the Compact Millisecond Pulsar Binary PSR J1653–015887
Binding Energies of Interstellar Complex Organic Molecules on Water Ice Surfaces: A Quantum Chemical Investigation87
The Velocity Map Asymmetry of Ionized Gas in MaNGA. II. Correlation between Velocity Map Morphology, Star Formation, and Metallicity in Regular Disk Galaxies86
Exploring the Evolution of a Dwarf Spheroidal Galaxy with Smoothed-particle Hydrodynamics Simulations. I. Stellar Feedback86
A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes. IV. Ultraviolet Spectroscopy* †85
Erratum: “The Longest Delay: A 14.5 yr Campaign to Determine the Third Time Delay in the Lensing Cluster SDSS J1004+4112” (2022, ApJ, 937, 34)84
A Data-driven Approach for Star Formation Parameterization Using Symbolic Regression84
Erratum: “Wave Generation by Flare-accelerated Ions and Implications for 3 He Acceleration” (2024, ApJ, 964, 97)83
Erratum: “Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm” (2023, ApJ, 942, 4 )83
Asymptotic Normalization Coefficient Investigation of the 17 O( d , p 83
Erratum: “Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains” (2021, ApJ, 919, 65)83
Erratum: “Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration” (2022, ApJ, 940, 74)83
Magnetic Field of the Quasar 1604+159 from Parsec to Kiloparsec Scale82
AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 81782
Discovering High- z BL Lacs Using Swift/UVOT and SARA Observations with the Dropout Technique82
Modeling of Condensations in Coronal Loops Produced by Impulsive Heating with Variable Frequencies and Locations81
Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation80
Spatiotemporal Evolution of the 2022 March Interplanetary Coronal Mass Ejection Revealed by Multipoint Observations of Forbush Decreases80
Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 with Radiant Energies of 1042.5±1.6 erg79
The Massive and Distant Clusters of WISE Survey. XI. Stellar Mass Fractions and Luminosity Functions of MaDCoWS Clusters at z ∼ 179
Characterizing Stellar and Gas Properties in NGC 628: Spatial Distributions, Radial Gradients, and Resolved Scaling Relations79
How Does the Critical Torus Instability Height Vary with the Solar Cycle?78
Determining the Spectral Content of MOSES Images77
Inferring Line-of-sight Velocities and Doppler Widths from Stokes Profiles of GST/NIRIS Using Stacked Deep Neural Networks77
Effects of Alpha Particle Fraction on Kinetic Plasma Turbulence77
The Complex Multiwavelength Morphology of the Peculiar Compact Galaxy Group IC 243175
Internal 1000 au Scale Structures of the R CrA Cluster-forming Cloud. I. Filamentary Structures75
Search for Fast Radio Bursts and Radio Pulsars from Pulsing Ultraluminous X-Ray Sources75
Spectro-polarimetric Properties of Sunquake Sources in X1.5 Flare and Evidence for Electron and Proton Beam Impacts75
Reconstruction of Coronal Magnetic Fields Using a Poloidal–Toroidal Representation74
What if the Universe Expands Linearly? A Local General Relativity to Solve the “Zero Active Mass” Problem74
Constraints on Evolutions of Fundamental Constants from Clustering of Fast Radio Burst Dispersion Measure73
A Heating Mechanism via Magnetic Pumping in the Intracluster Medium73
The Kinematic Signature of the Warp and Waves in the Milky Way Disk73
Observations of the X-Ray Millihertz Quasiperiodic Oscillations in Hercules X-173
Simultaneous Evidence of Edge Collapse and Hub-filament Configurations: A Rare Case Study of a Giant Molecular Filament, G45.3+0.172
The Timescales of Embedded Star Formation as Observed in STARFORGE72
XRISM Constrains Atmospheric Motion and Turbulent Dissipation in the Archetypal Radio-mode Feedback System Hydra-A72
MOSEL Survey: Spatially Offset Lyman-continuum Emission in a New Emitter at z = 3.088 Can Explain the Low Number Density of Observed LyC Leakers72
Exploring the Signature of Assembly Bias and Modified Gravity Using Small-scale Clusterings of Galaxies71
Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension71
Methyl Isocyanate Formation from Oxygen Insertion in Methyl Cyanide Ices71
On the Deepest Search for Galactic Center Pulsars and an Examination of an Intriguing Millisecond Pulsar Candidate70
Convolutional Neural Networks for Searching Superflares from Pixel-level Data of the Transiting Exoplanet Survey Satellite70
Massive Debris Disks May Hinder Secular Stirring by Planetary Companions: An Analytic Proof of Concept70
Searching for Broadband Pulsed Beacons from 1883 Stars Using Neural Networks70
Solution to the Conflict between the Estimations of Resolved and Unresolved Galaxy Stellar Mass from the Perspective of JWST70
A Unified Photometric Redshift Calibration for Weak Lensing Surveys Using the Dark Energy Spectroscopic Instrument70
Discovery of Evolution of the Temporal Features of X-Ray Bursts from SGR J1935+215469
The Merging Galaxy Cluster Environment Affects the Morphology of Radio Active Galactic Nuclei69
The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes69
Revealing the CME Impact on the Martian Nightside Ionosphere Based on MAVEN and Tianwen-1 Observations69
The Search for Thermonuclear Transients from the Tidal Disruption of a White Dwarf by an Intermediate-mass Black Hole69
An SMA Survey of Chemistry in Disks Around Herbig AeBe Stars69
Stellar Mergers or Truly Young? Intermediate-age Stars on Highly Radial Orbits in the Milky Way’s Stellar Halo68
Total Power and Low-energy Cutoff Time Evolution of Solar Flare Accelerated Electrons Using X-Ray Observations and Warm-target Model68
LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results68
Is the Radio Source Dipole from NVSS Consistent with the Cosmic Microwave Background and ΛCDM?68
DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy68
Differential Rotation of CoRoT Stars and a Kepler Binary Star from Starspot Transit Mapping68
Assessing the Observability of Deep Meridional Flow Cells in the Solar Interior67
Delayed Thermal Relaxation of Rapid Cooling Neutron Stars: Nucleon Superfluidity and Nonnucleon Particles67
Discovery of a 21 cm Absorption System at z = 2.327 with CHIME67
Impact of Multimessenger Spectral Modeling on Blazar–Neutrino Associations67
Spectral Energy Distribution Variability of the Blazar OJ 287 During 2009–202167
The Study of Jet Formation Mechanism in Fermi Blazars67
Searching for Anisotropic Stochastic Gravitational-wave Backgrounds with Constellations of Space-based Interferometers66
Investigation of Phase Shift and Travel Time of Acoustic Waves in the Lower Solar Atmosphere Using Multiheight Velocities66
The Cooling of the Central Compact Object in Cas A from 2006 to 202066
Quiet Sun Center to Limb Variation of the Linear Polarization Observed by CLASP2 Across the Mg ii h and k Lines66
Discovery of a ∼208 day Quasiperiodic Oscillation in the X-Ray Emission of the TeV Blazar 1ES 1959+65065
Do Hα Stokes V Profiles Probe the Chromospheric Magnetic Field? An Observational Perspective*65
UVIT Observations of the Small Magellanic Cloud: Point-source Catalog65
The 230 GHz Variability of Numerical Models of Sagittarius A*. II. The Physical Origins of the Variability65
Deep Two-phase, Hemispherical Magma Oceans on Lava Planets65
Mode Composition Shapes Magnetic Anisotropy in Solar Wind Turbulence64
Galactic Magnetic Fields. II. Applying the Model to Nearby Galaxies64
Spin and Obliquity Evolution of Hot Jupiter Hosts from Resonance Locks64
Disentangling Magnetic Fields in NGC 6946 with Wide-band Polarimetry64
Photon Ring Polarimetry with Next-generation Black Hole Imaging. I. M87*63
Neutral Gas Phase Distribution from H I Morphology: Phase Separation with Scattering Spectra and Variational Autoencoders63
Multiple Measurements of Gravitational Waves Acting as Standard Probes: Model-independent Constraints on the Cosmic Curvature with DECIGO63
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters63
S-type Stars: Line List for the A2Π–X2Σ+ Band System of LaO63
Ambipolar Heating of Magnetars63
Investigating the Time Evolution of the Thermal Emission from the Putative Neutron Star in SN 1987A for 50+ Years63
Wave Emission of Nonthermal Electron Beams Generated by Magnetic Reconnection63
Dark Matter in Fractional Gravity. I. Astrophysical Tests on Galactic Scales62
Evolution of Magnetic Fields and Energy Release Processes during Homologous Eruptive Flares62
Rotation of Polarization Angle in Gamma-Ray Burst Prompt Phase. III. The Influence of the Magnetic Field Orientation61
Recovering Cosmic Microwave Background Polarization Signals with Machine Learning61
The Dependence of Joy’s Law and Mean Tilt as a Function of Flux Emergence Phase61
Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter61
Black Hole Dragging: A New Mechanism for Forming Nuclear Star Clusters in Giant Elliptical Galaxies61
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow60
Coronal Heating and Solar Wind Generation by Flux Cancellation Reconnection60
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets60
Suprathermal Population Associated with Stream Interaction Regions Observed by STEREO-A: New Insights60
Improving the Low-energy Transient Sensitivity of AMEGO-X using Single-site Events59
Line List for the A2Π−X2Σ+ and the B2Σ+−X2Σ+ Band Systems of CaF58
Search for Kink Events in Variable Fermi-LAT Blazars58
Turbulent Magnetic Field Amplification by the Interaction of a Shock Wave and Inhomogeneous Medium58
Uncertainty-aware Neural Networks for Fuzzy Dark Matter Model Selection from x H I 58
Steep Balmer Decrement in Weak AGNs May Not Be Caused by Dust Extinction: Clues from Low-luminosity AGNs and Changing-look AGNs58
The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGL⃗E Sample58
The Imprint of Dark Matter on the Galactic Acceleration Field58
Photospheric Horizontal Magnetic Field Decrease Preceding a Major Solar Eruption58
Discovery of a Rapidly Evolving Global Magnetic Field in the M Dwarf YZ Cet and Constraints on the Magnetic Field of Its Planet YZ Cet b57
Magnetization Factors of Gamma-Ray Burst Jets Revealed by a Systematic Analysis of the Fermi Sample57
Investigating Mass Segregation of the Binary Stars in the Open Cluster NGC 681957
Spatially Resolved Modeling of Galactic Hα Emission for Galaxy Clustering57
Photometric and Spectroscopic Studies of Two Early-type Eclipsing Binaries57
Tidally Driven Inertial Waves Enhance Eccentricity Damping and Spin Evolution in Planets and Stars57
Are Radio Minihalos Confined by Cold Fronts in Galaxy Clusters? Minihalos and Large-scale Sloshing in A3444 and MS 1455.0+223257
An Elemental Abundance Diagnostic for Coordinated Solar Orbiter/SPICE and Hinode/EIS Observations56
On the Parameters of the Spherically Symmetric Parameterized Rezzolla–Zhidenko Spacetime through Solar System Tests, the Orbit of the S2 Star about Sgr A*, and Quasiperiodic Oscillations56
Nodal Precession and Tidal Evolution of Two Hot Jupiters: WASP-33 b and KELT-9 b56
Diffuse Emission of Galactic High-energy Neutrinos from a Global Fit of Cosmic Rays56
How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster Simulation56
MINDS: Detection of an Inner Gas Disk Caused by Evaporating Bodies around HD 17255556
Accretion from a Shock-inflated Companion: Spinning Down Neutron Stars to Hour-long Periods56
The Active Optics System on the Vera C. Rubin Observatory: Optimal Control of Degeneracy among the Large Number of Degrees of Freedom56
The Late Afterglow of GW170817/GRB 170817A: A Large Viewing Angle and the Shift of the Hubble Constant to a Value More Consistent with the Local Measurements56
Bell Instability and Cosmic-Ray Acceleration in Active Galactic Nuclei Ultrafast Outflow Shocks56
Detection of the Extended γ-Ray Emission around TeV Source 1LHAASO J0249+6022 with Fermi-LAT56
Radio Emission From a z = 10.1 Black Hole in UHZ156
Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content56
Gone with the Wind: JWST-MIRI Unveils a Strong Outflow from the Quiescent Stellar-mass Black Hole A0620-0055
Solar Eruptive Phenomena Associated with Solar Energetic Electron Spectral Types55
The Formation of Filaments and Dense Cores in the Cocoon Nebula (IC 5146)55
Clustercentric Distance or Local Density? It Depends on Galaxy Morphology55
Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-353755
Rotational Fingerprints of Vinylketene for Astronomical Observations55
COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey55
The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud55
Updated Low-temperature Gas Opacities with ÆSOPUS 2.055
Void Lensing in Cubic Galileon Gravity55
Implications of NICER for Neutron Star Matter: The QHC21 Equation of State55
Stratified Evolution of Ryugu’s Regolith Revealed by Spectroscopic Analyses of Two Hayabusa2 Collected Particles54
Investigating the Impact of Vertically Extended Coronae on X-Ray Reverberation Mapping54
Dense Molecular Gas Properties of the Central Kiloparsec of Nearby Ultraluminous Infrared Galaxies Constrained by ALMA Three Transition-line Observations54
Similar Signatures of Coplanar Gas Inflow and Disk Warps in Galactic Gas Kinematic Maps54
Tilted Disk Precession and Negative Superhumps in HS 2325+8205: A Multiwindow Analysis54
Evidence for YORP-induced Spin Deceleration in Asteroid (433) Eros54
The Use of Binary Black Holes Merging in Active Galactic Nuclei Disks for Hubble Constant Measurements54
Statistical Plasma Properties of the Planar and Nonplanar ICME Magnetic Clouds during Solar Cycles 23 and 2454
Plausible Constraints on the Range of Bulk Terrestrial Exoplanet Compositions in the Solar Neighborhood54
The Carbon Isotopic Ratio and Planet Formation54
0.19783997535706