Astrophysical Journal

Papers
(The H4-Index of Astrophysical Journal is 91. 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
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
Searching for Propionamide (C2H5CONH2) toward Sagittarius B2 at Centimeter Wavelengths136
Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts135
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification133
Photometric and Spectroscopic Observations of GRB 210104A: Bright Reverse-shock Emission and Dense Circumburst Environment133
Spectral Evolution of Ultraluminous X-Ray Pulsar NGC 300 ULX-1132
Global Distribution of the Key Species on the Surface of Europa130
The “Canonical” White Dwarf Cooling Sequence of M5130
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 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 Internal Proper Motion Kinematics of NGC 346: Past Formation and Future Evolution104
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
Dust Properties of 870 μm-selected Galaxies in GOODS-S100
Mode Mixing and Rotational Splittings. II. Reconciling Different Approaches to Mode Coupling 100
The Effects of Turbulent Electrical Resistivity on the Response of the Solar Atmosphere to Flare Energy Input. I. Results of Radiative Hydrodynamic Simulations100
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
Coherent Imaging with Photonic Lanterns99
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
ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field93
Numerical Simulation of Hot Accretion Flow around Bondi Radius93
Scattering of Stellar Mass Black Holes and Gravitational-wave Bremsstrahlung Radiation in Active Galactic Nucleus Disks93
Spectropolarimetry of GRB 180427A: Evidence for Distinct Emission Sites with Varying Polarization92
Igneous Rim Accretion on Chondrules in Low-velocity Shock Waves91
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