Astrophysical Journal

Papers
(The H4-Index of Astrophysical Journal is 95. 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 2022-08-01 to 2026-08-01.)
ArticleCitations
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H i Disk of Galaxies4926
Double Shells of the Planetary Nebula NGC 7009 Minor Axis1239
The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity–Spectral Type Dependence in Taurus–Auriga YSOs867
Parsec-scale SiO Emission in the Galactic Center544
Modeling the UV to Radio Spectral Energy Distribution of NGC 6946: Star Formation Rates and Dust Attenuation Properties505
Zonal Flow and Self-regulating Mechanism in a Hydrodynamic Disk433
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei315
Evidence of the Alfvén Transition Layer and Particle Precipitation in the Cusp Region: 3D Global PIC Simulation of the Solar Wind–Earth Magnetosphere Interaction302
DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos271
Active Galactic Nucleus Variability in the Age of Rubin250
Criss-cross Nebula: A Case Study of Shock Regions with Resolved Microstructures at Scales of ∼1000 au228
Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure219
On the Width of a Collisionless Shock and the Index of the Cosmic Rays It Accelerates212
Dark Off-limb Gap: Manifestation of a Temperature Minimum and the Dynamic Nature of the Chromosphere210
Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?207
Single-pulse Gamma-Ray Bursts Have Prevalent Hard-to-soft Spectral Evolution202
Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding200
ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field195
The Orion OB Association as a Generator for the Hot Circumgalactic Medium195
Scattering of Stellar Mass Black Holes and Gravitational-wave Bremsstrahlung Radiation in Active Galactic Nucleus Disks194
Ultraviolet and Gravitational Wave Signatures of Magnetar Formation187
Geminga: A Window into the Role Played by the Local Halo in the Cosmic-Ray Propagation Process184
Electrostatic Transport Characteristics of Olivine Particles under Electron Irradiation in Vacuum175
A Holistic Exploration of the Potentially Recoverable Redshift Information of Stage IV Galaxy Surveys174
Including Neutrino-driven Convection in the Force Explosion Condition to Predict Explodability of Multidimensional Core-collapse Supernovae (FEC+)173
Small-scale Inhomogeneity Effects on Coherent Solar Radio Emission169
Gravitational Influence from Planets on the Measured Rates of Period Change of Pulsating White Dwarfs168
Exploring the Evolution of a Dwarf Spheroidal Galaxy with Smoothed-particle Hydrodynamics Simulations. I. Stellar Feedback167
Search for Kink Events in Variable Fermi-LAT Blazars165
Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation164
Modeling of Condensations in Coronal Loops Produced by Impulsive Heating with Variable Frequencies and Locations161
Spatiotemporal Evolution of the 2022 March Interplanetary Coronal Mass Ejection Revealed by Multipoint Observations of Forbush Decreases160
Evaluating the Limits of Rotation Period Recovery Through Gyrochronology Criteria159
Interaction of Inner Heliosheath Ions with Electromagnetic Ion Cyclotron Waves158
A Monte Carlo Simulation on the Scattering Coefficients of Solar Radio Wave Propagation157
The Propagation of Fast Radio Bursts in the Magnetosphere Shapes Their Waiting-time and Flux Distributions157
Planetary Nebulae in the eROSITA eRASS1 Catalog154
Observations of Magnetospheric Solar Wind Charge Exchange154
Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph151
When is a Bulge Not a Bulge? Revealing the Satellite Nature of NGC 5474’s Bulge151
Searching for Propionamide (C2H5CONH2) toward Sagittarius B2 at Centimeter Wavelengths148
Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts145
Spectral Evolution of Ultraluminous X-Ray Pulsar NGC 300 ULX-1145
Global Distribution of the Key Species on the Surface of Europa142
The “Canonical” White Dwarf Cooling Sequence of M5140
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters135
Evolution of Magnetic Fields and Energy Release Processes during Homologous Eruptive Flares132
The 230 GHz Variability of Numerical Models of Sagittarius A*. II. The Physical Origins of the Variability132
Dark Matter in Fractional Gravity. I. Astrophysical Tests on Galactic Scales132
Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter132
Suprathermal Population Associated with Stream Interaction Regions Observed by STEREO-A: New Insights131
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow131
Characterizing Stellar and Gas Properties in NGC 628: Spatial Distributions, Radial Gradients, and Resolved Scaling Relations128
How Does the Critical Torus Instability Height Vary with the Solar Cycle?126
Inferring Line-of-sight Velocities and Doppler Widths from Stokes Profiles of GST/NIRIS Using Stacked Deep Neural Networks126
The Complex Multiwavelength Morphology of the Peculiar Compact Galaxy Group IC 2431125
Search for Fast Radio Bursts and Radio Pulsars from Pulsing Ultraluminous X-Ray Sources125
Reconstruction of Coronal Magnetic Fields Using a Poloidal–Toroidal Representation124
Internal 1000 au Scale Structures of the R CrA Cluster-forming Cloud. I. Filamentary Structures124
Spectro-polarimetric Properties of Sunquake Sources in X1.5 Flare and Evidence for Electron and Proton Beam Impacts124
When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multiband Imaging Data123
What if the Universe Expands Linearly? A Local General Relativity to Solve the “Zero Active Mass” Problem123
Coherent Imaging with Photonic Lanterns122
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 Progenitors121
The Effects of Turbulent Electrical Resistivity on the Response of the Solar Atmosphere to Flare Energy Input. I. Results of Radiative Hydrodynamic Simulations117
Identifying Signatures of Inflow onto Face-on Galaxies Using the Balmer Decrement117
Testing the Physical Parameter Constraining Power of HCN and HNC with Neural Networks116
Interplanetary Type III Radio Emission Locations Deduced from the Underlying Electron Exciter Beam Kinematics116
A Novel Blast Wave Solution for the Propagation of Coronal And Interplanetary Shocks115
Statistical Study of the Timing of the Appearance of H α Postflare Loops: Simple Scaling Law Based on Radiative Cooling114
Possibility of Using 3.3 μm Polycyclic Aromatic Hydrocarbon Luminosity as a Molecular Gas Mass Estimator114
Rotational Fingerprints of Vinylketene for Astronomical Observations112
Streams and Bubbles: Tidal Shaping of Hydrodynamic Planetary Outflows111
The Sonora Substellar Atmosphere Models. VI. Red Diamondback: Extending Diamondback with SPHINX for Brown Dwarf Early Evolution110
Radio Emission From a z = 10.1 Black Hole in UHZ1108
Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content107
Detection of the Extended γ-Ray Emission around TeV Source 1LHAASO J0249+6022 with Fermi-LAT107
Gone with the Wind: JWST-MIRI Unveils a Strong Outflow from the Quiescent Stellar-mass Black Hole A0620-00106
Accretion from a Shock-inflated Companion: Spinning Down Neutron Stars to Hour-long Periods105
Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537105
Disentangling Magnetic Fields in NGC 6946 with Wide-band Polarimetry104
Radiative Signatures of Magnetic Reconnection: An Approach to Remote Probing of Reconnection Dynamics104
Dust Properties of 870 μm-selected Galaxies in GOODS-S104
Galactic Magnetic Fields. II. Applying the Model to Nearby Galaxies103
Spin and Obliquity Evolution of Hot Jupiter Hosts from Resonance Locks102
Investigating the Time Evolution of the Thermal Emission from the Putative Neutron Star in SN 1987A for 50+ Years101
S-type Stars: Line List for the A2Π–X2Σ+ Band System of LaO100
Constraints on Evolutions of Fundamental Constants from Clustering of Fast Radio Burst Dispersion Measure99
Magnetic Field of the Quasar 1604+159 from Parsec to Kiloparsec Scale98
Erratum: “Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains” (2021, ApJ, 919, 65)98
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)98
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 )97
Erratum: “Wave Generation by Flare-accelerated Ions and Implications for 3 He Acceleration” (2024, ApJ, 964, 97)95
Asymptotic Normalization Coefficient Investigation of the 17 O( d , p 95
Erratum: “Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration” (2022, ApJ, 940, 74)95
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