Astrophysical Journal

Papers
(The H4-Index of Astrophysical Journal is 88. 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 2021-11-01 to 2025-11-01.)
ArticleCitations
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H i Disk of Galaxies3265
Thermal Damping of Weak Magnetosonic Turbulence in the Interstellar Medium792
XMM-Newton Perspective of the Unique Magnetic Binary-ϵ Lupi554
Periodic Variable Stars Modulated by Time-varying Parameters312
A Parkes “Murriyang” Search for Pulsars and Fast Transients in the Large Magellanic Cloud288
Double Shells of the Planetary Nebula NGC 7009 Minor Axis238
SDSS J1059+4251, a Highly Magnified z ∼ 2.8 Star-forming Galaxy: ESI Observations of the Rest-frame UV Spectrum225
The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity–Spectral Type Dependence in Taurus–Auriga YSOs206
Searching for Axion Dark Matter Gegenschein of the Vela Supernova Remnant with FAST192
Constraining the Milky Way Halo Accretion History with Simulated Stellar Halos: Designing the HALO7D-X Survey191
Evidence for YORP-induced Spin Deceleration in Asteroid (433) Eros186
H I Absorption Line and Anomalous Dispersion in the Radio Pulses of PSR B1937+21173
Caught in the Act: A Metal-rich High-velocity Cloud in the Inner Galaxy169
Detecting Atmospheric CO2 Trends as Population-level Signatures for Long-term Stable Water Oceans and Biotic Activity on Temperate Terrestrial Exoplanets164
ALMASOP. A Rotating Feature Rich in Complex Organic Molecules in a Protostellar Core156
Enhanced Star Formation and Black Hole Accretion Rates in Galaxy Mergers in IllustrisTNG50155
Acceleration and Spectral Redistribution of Cosmic Rays in Radio-jet Shear Flows151
Anomalously Fast Core and Envelope Rotation in Red Giants150
Parsec-scale SiO Emission in the Galactic Center149
Experimental and Numerical Studies of the Collapse of Dense Clouds Induced by Herbig–Haro Stellar Jets148
Helium-deficient ER UMa-type Dwarf Nova below the Period Minimum with a Hot Secondary145
Instability of Circumnuclear Gas Supply as an Origin of the “Changing-look” Phenomenon of Supermassive Black Holes145
Ultrahigh-energy γ-Rays from Past Explosions in Our Galaxy144
Investigating Mass Segregation of the Binary Stars in the Open Cluster NGC 6819141
The Central 300 pc of the Galaxy Probed by Infrared Spectra of H3 + and CO. III. Locations of Sgr B2 and Star Iota139
Landau Modes are Eigenmodes of Stellar Systems in the Limit of Zero Collisions137
Observations of the X-Ray Millihertz Quasiperiodic Oscillations in Hercules X-1133
A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed Out by High-z Radio Galaxies at z ∼ 4133
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow130
Magnetic Energy Conversion in Magnetohydrodynamics: Curvature Relaxation and Perpendicular Expansion of Magnetic Fields130
Discovery of Extraplanar H i Clouds and a H i Tail in the M101 Galaxy Group with FAST129
Modeling the UV to Radio Spectral Energy Distribution of NGC 6946: Star Formation Rates and Dust Attenuation Properties128
Empirical Evidence of Nonminimally Coupled Dark Matter in the Dynamics of Local Spiral Galaxies?126
Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae125
Core-collapse Supernova Simulations with Reduced Nucleosynthesis Networks125
XMM-Newton and NuSTAR Observations of the Compact Millisecond Pulsar Binary PSR J1653–0158123
Constraints on Evolutions of Fundamental Constants from Clustering of Fast Radio Burst Dispersion Measure123
Rotational Fingerprints of Vinylketene for Astronomical Observations123
Zonal Flow and Self-regulating Mechanism in a Hydrodynamic Disk123
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei122
Evaluating Non-LTE Spectral Inversions with ALMA and IBIS121
Exploring the Evolution of a Dwarf Spheroidal Galaxy with Smoothed-particle Hydrodynamics Simulations. I. Stellar Feedback119
Disentangling Magnetic Fields in NGC 6946 with Wide-band Polarimetry119
The Active Optics System on the Vera C. Rubin Observatory: Optimal Control of Degeneracy among the Large Number of Degrees of Freedom117
Effect of Dust in Circumgalactic Halos on the Cosmic Shear Power Spectrum117
Global Non-ideal Magnetohydrodynamic Simulations of Protoplanetary Disks with Outer Truncation117
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters117
Evidence of the Alfvén Transition Layer and Particle Precipitation in the Cusp Region: 3D Global PIC Simulation of the Solar Wind–Earth Magnetosphere Interaction116
Erratum: “Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration” (2022, ApJ, 940, 74)115
Two Analytic Relations Connecting the Hot Gas Astrophysics with the Cold Dark Matter Model for Galaxy Clusters115
Late Afterglow Bump/Plateau around the Jet Break: Signature of a Free-to-shocked Wind Environment in Gamma-Ray Burst112
Properties of Type Iax Supernova 2019muj in the Late Phase: Existence, Nature, and Origin of the Iron-rich Dense Core110
Merging Criteria for Planetesimal Collisions109
X-Ray-induced Diffusion and Mixing in Layered Astrophysical Ices109
DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos109
STag: Supernova Tagging and Classification108
Subgalactic Scaling Relations with T e-based Metallicities of Low-metallicity Regions in Galaxies: Metal-poor Gas Inflow May Have Important Effects?107
Analysis of Thermal Emissions of Exoplanets with Axially Symmetric Temperature Gradients107
Examining the Nature of the Starless Dark Matter Halo Candidate Cloud-9 with Very Large Array Observations106
Active Galactic Nucleus Variability in the Age of Rubin106
Weighing the Darkness. III. How Gaia Could, but Probably Will Not, Astrometrically Detect Free-floating Black Holes105
Criss-cross Nebula: A Case Study of Shock Regions with Resolved Microstructures at Scales of ∼1000 au104
Two High-amplitude δ Scuti–γ Doradus Hybrids Constrained by the Radial Fundamental p and Equally Spaced g Modes103
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)102
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets101
Convolutional Neural Networks for Searching Superflares from Pixel-level Data of the Transiting Exoplanet Survey Satellite101
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 erg97
On the Width of a Collisionless Shock and the Index of the Cosmic Rays It Accelerates96
An SMA Survey of Chemistry in Disks Around Herbig AeBe Stars96
The ISM in the z = 6.9 Interacting Galaxies of SPT0311-5896
Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure96
Assessing the Observability of Deep Meridional Flow Cells in the Solar Interior95
Dark Off-limb Gap: Manifestation of a Temperature Minimum and the Dynamic Nature of the Chromosphere95
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 )95
Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?94
Investigation of Phase Shift and Travel Time of Acoustic Waves in the Lower Solar Atmosphere Using Multiheight Velocities94
S-type Stars: Line List for the A2Π–X2Σ+ Band System of LaO94
Single-pulse Gamma-Ray Bursts Have Prevalent Hard-to-soft Spectral Evolution93
Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm92
Evolution of Magnetic Fields and Energy Release Processes during Homologous Eruptive Flares91
Multiple Rebrightenings in the Optical Afterglow of GRB 210731A: Evidence for an Asymmetric Jet91
The Formation of Filaments and Dense Cores in the Cocoon Nebula (IC 5146)91
Angular Momentum and Morphological Sequence of Massive Galaxies through Dark Sage90
Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding90
New Spectroscopic Confirmations of Lyα Emitters at Z ∼ 7 from the LAGER Survey90
Evidence for Centrifugal Breakout around the Young M Dwarf TIC 23428455689
A Monte Carlo Method for Evaluating Empirical Gyrochronology Models and Its Application to Wide Binary Benchmarks88
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