Astrophysical Journal

Papers
(The H4-Index of Astrophysical Journal is 82. 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 2021-06-01 to 2025-06-01.)
ArticleCitations
The Cross-sectional Shape and Height Expansion of Coronal Loops: High-resolution Coronal Imager (Hi-C) Analysis of AR 127122565
Toward a More Complete Optical Census of Active Galactic Nuclei via Spatially Resolved Spectroscopy597
The Role of Magnetic and Rotation Axis Alignment in Driving Fast Radio Burst Phenomenology399
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H i Disk of Galaxies388
XMM-Newton Perspective of the Unique Magnetic Binary-ϵ Lupi245
Asymptotic Normalization Coefficient Investigation of the 17O(d, p) Transfer for Astrophysical Application to the 17O(n, α)14C Reaction at Low Energies219
The Effect of Spatially Varying Collision Frequency on the Development of the Rayleigh–Taylor Instability202
Magnetization Factors of Gamma-Ray Burst Jets Revealed by a Systematic Analysis of the Fermi Sample190
AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 817186
Model-independent Approach of the JUNO 8B Solar Neutrino Program184
Efficiency of Nonthermal Pulsed Emission from Eight MeV Pulsars174
Massive Debris Disks May Hinder Secular Stirring by Planetary Companions: An Analytic Proof of Concept152
Electrostatic Transport Characteristics of Olivine Particles under Electron Irradiation in Vacuum147
On the Hard Gamma-Ray Spectrum of the Potential PeVatron Supernova Remnant G106.3 + 2.7144
Forming Gas Giants around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability144
Periodic Variable Stars Modulated by Time-varying Parameters142
A Parkes “Murriyang” Search for Pulsars and Fast Transients in the Large Magellanic Cloud136
Double Shells of the Planetary Nebula NGC 7009 Minor Axis132
The Dependence of Joy’s Law and Mean Tilt as a Function of Flux Emergence Phase131
Late Afterglow Bump/Plateau around the Jet Break: Signature of a Free-to-shocked Wind Environment in Gamma-Ray Burst130
Merging Criteria for Planetesimal Collisions128
Properties of Type Iax Supernova 2019muj in the Late Phase: Existence, Nature, and Origin of the Iron-rich Dense Core128
DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos128
The Crab Nebula as a Calibrator for Wide-beam Cosmic Microwave Background Polarization Surveys127
X-Ray-induced Diffusion and Mixing in Layered Astrophysical Ices123
Core-collapse Supernova Simulations with Reduced Nucleosynthesis Networks118
Study of Temporal and Spectral variability for Blazar PKS 1830-211 with Multiwavelength Data115
STag: Supernova Tagging and Classification115
CO(2–1)/CO(1–0) Line Ratio on a ∼100 Parsec Scale in the Nearby Barred Galaxy NGC 1300115
Quantifying Wave–Particle Interactions in Collisionless Plasmas: Theory and Its Application to the Alfvén-mode Wave114
Analysis of Thermal Emissions of Exoplanets with Axially Symmetric Temperature Gradients113
Active Galactic Nucleus Variability in the Age of Rubin112
High-resolution, High-sensitivity, Low-frequency uGMRT View of Coma Cluster of Galaxies112
Subgalactic Scaling Relations with T e-based Metallicities of Low-metallicity Regions in Galaxies: Metal-poor Gas Inflow May Have Important Effects?112
Examining the Nature of the Starless Dark Matter Halo Candidate Cloud-9 with Very Large Array Observations111
Interstellar Objects Follow the Collapse of Molecular Clouds109
Weighing the Darkness. III. How Gaia Could, but Probably Will Not, Astrometrically Detect Free-floating Black Holes109
Reconstruction of Coronal Magnetic Fields Using a Poloidal–Toroidal Representation108
Criss-cross Nebula: A Case Study of Shock Regions with Resolved Microstructures at Scales of ∼1000 au107
Mode Mixing and Rotational Splittings. II. Reconciling Different Approaches to Mode Coupling 106
Two High-amplitude δ Scuti–γ Doradus Hybrids Constrained by the Radial Fundamental p and Equally Spaced g Modes106
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)104
The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud103
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets103
ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field102
Post-AO High-resolution Imaging Using the Kraken Multi-frame Blind Deconvolution Algorithm102
An Elemental Abundance Diagnostic for Coordinated Solar Orbiter/SPICE and Hinode/EIS Observations102
Convolutional Neural Networks for Searching Superflares from Pixel-level Data of the Transiting Exoplanet Survey Satellite101
Multiple Measurements of Gravitational Waves Acting as Standard Probes: Model-independent Constraints on the Cosmic Curvature with DECIGO101
Precise Mass, Orbital Motion, and Stellar Properties of the M-dwarf Binary LP 349−25AB100
Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 with Radiant Energies of 1042.5±1.6 erg99
Searching for Propionamide (C2H5CONH2) toward Sagittarius B2 at Centimeter Wavelengths96
Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure96
Searching for Anisotropic Stochastic Gravitational-wave Backgrounds with Constellations of Space-based Interferometers96
GASP. XLV. Stellar Bars in Jellyfish Galaxies: Analysis of Ionized Gas and Stellar Populations94
Investigating the Impact of Atomic Data Uncertainties on the Measured Physical Parameters of the Perseus Galaxy Cluster94
An SMA Survey of Chemistry in Disks Around Herbig AeBe Stars93
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification93
JWST Observations of the Enigmatic Y-Dwarf WISE 1828+2650. I. Limits to a Binary Companion92
Nodal Precession and Tidal Evolution of Two Hot Jupiters: WASP-33 b and KELT-9 b92
DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy91
Photon Ring Polarimetry with Next-generation Black Hole Imaging. I. M87*90
On the Width of a Collisionless Shock and the Index of the Cosmic Rays It Accelerates90
The Local Group L-band Survey: The First Measurements of Localized Cold Neutral Medium Properties in the Low-metallicity Dwarf Galaxy NGC 682290
Dark Off-limb Gap: Manifestation of a Temperature Minimum and the Dynamic Nature of the Chromosphere89
The ISM in the z = 6.9 Interacting Galaxies of SPT0311-5889
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 )89
Igneous Rim Accretion on Chondrules in Low-velocity Shock Waves88
Recovering Cosmic Microwave Background Polarization Signals with Machine Learning88
Unusually Powerful Flare Phenomenon of the Water Maser in W51 and the Possibility of Detecting Gravitational Radiation from It88
Do Hα Stokes V Profiles Probe the Chromospheric Magnetic Field? An Observational Perspective*86
Assessing the Observability of Deep Meridional Flow Cells in the Solar Interior86
Disentangling Magnetic Fields in NGC 6946 with Wide-band Polarimetry85
S-type Stars: Line List for the A2Π–X2Σ+ Band System of LaO85
Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?85
The Active Optics System on the Vera C. Rubin Observatory: Optimal Control of Degeneracy among the Large Number of Degrees of Freedom84
Dark Matter in Fractional Gravity. I. Astrophysical Tests on Galactic Scales84
Exploring the Evolution of a Dwarf Spheroidal Galaxy with Smoothed-particle Hydrodynamics Simulations. I. Stellar Feedback84
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters84
The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method83
A High-resolution Far-infrared Survey to Probe Black Hole–Galaxy Co-evolution82
Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey82
0.14395213127136