Astrophysical Journal

Papers
(The TQCC of Astrophysical Journal is 10. 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
Instability of Circumnuclear Gas Supply as an Origin of the “Changing-look” Phenomenon of Supermassive Black Holes145
Helium-deficient ER UMa-type Dwarf Nova below the Period Minimum with a Hot Secondary145
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
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
Observations of the X-Ray Millihertz Quasiperiodic Oscillations in Hercules X-1133
Magnetic Energy Conversion in Magnetohydrodynamics: Curvature Relaxation and Perpendicular Expansion of Magnetic Fields130
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow130
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
Rotational Fingerprints of Vinylketene for Astronomical Observations123
Zonal Flow and Self-regulating Mechanism in a Hydrodynamic Disk123
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
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
Global Non-ideal Magnetohydrodynamic Simulations of Protoplanetary Disks with Outer Truncation117
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters117
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
Evidence of the Alfvén Transition Layer and Particle Precipitation in the Cusp Region: 3D Global PIC Simulation of the Solar Wind–Earth Magnetosphere Interaction116
Two Analytic Relations Connecting the Hot Gas Astrophysics with the Cold Dark Matter Model for Galaxy Clusters115
Erratum: “Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration” (2022, ApJ, 940, 74)115
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
X-Ray-induced Diffusion and Mixing in Layered Astrophysical Ices109
DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos109
Merging Criteria for Planetesimal Collisions109
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
Active Galactic Nucleus Variability in the Age of Rubin106
Examining the Nature of the Starless Dark Matter Halo Candidate Cloud-9 with Very Large Array Observations106
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
Convolutional Neural Networks for Searching Superflares from Pixel-level Data of the Transiting Exoplanet Survey Satellite101
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets101
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
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
On the Width of a Collisionless Shock and the Index of the Cosmic Rays It Accelerates96
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
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
Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?94
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
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
Evolution of Magnetic Fields and Energy Release Processes during Homologous Eruptive Flares91
Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding90
New Spectroscopic Confirmations of Lyα Emitters at Z ∼ 7 from the LAGER Survey90
Angular Momentum and Morphological Sequence of Massive Galaxies through Dark Sage90
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
The Orion OB Association as a Generator for the Hot Circumgalactic Medium87
Magnetic Field of the Quasar 1604+159 from Parsec to Kiloparsec Scale87
Galactic Magnetic Fields. II. Applying the Model to Nearby Galaxies86
RRAT J2325–0530: A Rotating Radio Transient with an Atypical Waiting-time Distribution86
Streams and Bubbles: Tidal Shaping of Hydrodynamic Planetary Outflows86
Tilted Disk Precession and Negative Superhumps in HS 2325+8205: A Multiwindow Analysis84
Evidence of Continuous Reconnection along a Helmet Streamer Current Sheet Observed by WISPR on Parker Solar Probe84
Follow-up Investigation of 11 Pulsars Discovered in the Commensal Radio Astronomy FAST Survey84
Discovery of a Protocluster Core Associated with an Enormous Lya Nebula at z = 2.384
The Propagation of Fast Radio Bursts in the Magnetosphere Shapes Their Waiting-time and Flux Distributions84
UVIT Observations of the Small Magellanic Cloud: Point-source Catalog84
AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 81784
Measuring the H i Content of Individual Galaxies Out to the Epoch of Reionization with [C ii]82
Unusually Powerful Flare Phenomenon of the Water Maser in W51 and the Possibility of Detecting Gravitational Radiation from It82
XRISM Constrains Atmospheric Motion and Turbulent Dissipation in the Archetypal Radio-mode Feedback System Hydra-A81
Giant Planets, Tiny Stars: Producing Short-period Planets around White Dwarfs with the Eccentric Kozai–Lidov Mechanism81
Hydrogen-triggered X-Ray Bursts from SAX J1808.4−3658? The Onset of Nuclear Burning81
Dark Matter in Fractional Gravity. I. Astrophysical Tests on Galactic Scales81
The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud80
Examining the Rotation Period Distribution of the 40 Myr Tucana–Horologium Association with TESS79
GASP. XLV. Stellar Bars in Jellyfish Galaxies: Analysis of Ionized Gas and Stellar Populations79
Photochemical Hazes Dramatically Alter Temperature Structure and Atmospheric Circulation in 3D Simulations of Hot Jupiters78
Azimuthal Size Scales of Solar Wind Periodic Density Structures78
Toward a More Complete Optical Census of Active Galactic Nuclei via Spatially Resolved Spectroscopy78
Improving the Low-energy Transient Sensitivity of AMEGO-X using Single-site Events78
Surface Brightness Profile of Lyman-α Halos out to 320 kpc in HETDEX78
What Are the Pillars of Reionization? Revising the AGN Luminosity Function at z ∼ 578
The Relevance of Ram Pressure Stripping for the Evolution of Blue Cluster Galaxies as Seen at Optical Wavelengths77
The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGL⃗E Sample77
Erratum: “Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains” (2021, ApJ, 919, 65)77
Repeating Nuclear Transients from Repeating Partial Tidal Disruption Events: Reproducing ASASSN-14ko and AT2020vdq76
Clustercentric Distance or Local Density? It Depends on Galaxy Morphology76
Inverse MultiView. II. Microarcsecond Trigonometric Parallaxes for Southern Hemisphere 6.7 GHz Methanol Masers G232.62+00.99 and G323.74–00.2675
Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph75
Spectral Evolution of the X-Ray Remnant of SN 1987A: A High-resolution Chandra HETG Study75
Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus74
Observations of Magnetospheric Solar Wind Charge Exchange74
Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey73
Gone with the Wind: JWST-MIRI Unveils a Strong Outflow from the Quiescent Stellar-mass Black Hole A0620-0073
Planetary Nebulae in the eROSITA eRASS1 Catalog72
A Monte Carlo Simulation on the Scattering Coefficients of Solar Radio Wave Propagation72
Steep Balmer Decrement in Weak AGNs May Not Be Caused by Dust Extinction: Clues from Low-luminosity AGNs and Changing-look AGNs71
Milky Way's Eccentric Constituents with Gaia, APOGEE, and GALAH71
Efficiency of Nonthermal Pulsed Emission from Eight MeV Pulsars71
When is a Bulge Not a Bulge? Revealing the Satellite Nature of NGC 5474’s Bulge70
COCONUT, a Novel Fast-converging MHD Model for Solar Corona Simulations. III. Impact of the Preprocessing of the Magnetic Map on the Modeling of the Solar Cycle Activity and Comparison with Observatio70
The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes69
On the Onset Delays of Solar Energetic Electrons and Protons: Evidence for a Common Accelerator69
A Detailed Survey of the Parallel Mean Free Path of Solar Energetic Particle Protons and Electrons69
Modeling of Condensations in Coronal Loops Produced by Impulsive Heating with Variable Frequencies and Locations69
The Effect of Spatially Varying Collision Frequency on the Development of the Rayleigh–Taylor Instability68
Distances to Recent Near-Earth Supernovae from Geological and Lunar 60Fe68
First Measurement of 87Rb(αxn) Cross Sections at Weak r-process Energies in Supernova ν-driven Ejecta to Investigate Elemental Abundances in Low-metallicity St68
Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension68
Mass-ratio and Magnetic Flux Dependence of Modulated Accretion from Circumbinary Disks67
To Be or Not To Be: The Role of Rotation in Modeling Galactic Be X-Ray Binaries67
Intensity and Polarization Characteristics of Extended Neutron Star Surface Regions67
Recovering Cosmic Microwave Background Polarization Signals with Machine Learning67
Binary Vision: The Mass Distribution of Merging Binary Black Holes via Iterative Density Estimation66
Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts66
Prospects for Measuring Off-axis Spins of Binary Black Holes with Plus-era Gravitational-wave Detectors65
HSTPROMO Internal Proper-motion Kinematics of Dwarf Spheroidal Galaxies. I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco65
Search for Lensing Signatures from the Latest Fast Radio Burst Observations and Constraints on the Abundance of Primordial Black Holes65
Nucleosynthesis Conditions in Outflows of White Dwarfs Collapsing to Neutron Stars64
Solution to the Conflict between the Estimations of Resolved and Unresolved Galaxy Stellar Mass from the Perspective of JWST64
Testing f(R) Gravity from Cosmic Shear Measurements64
Revealing the Dynamic Magnetoionic Environments of Repeating Fast Radio Burst Sources through Multiyear Polarimetric Monitoring with CHIME/FRB64
Deep Two-phase, Hemispherical Magma Oceans on Lava Planets63
Photometric and Spectroscopic Observations of GRB 210104A: Bright Reverse-shock Emission and Dense Circumburst Environment63
Dust Properties of 870 μm-selected Galaxies in GOODS-S63
The Use of Binary Black Holes Merging in Active Galactic Nuclei Disks for Hubble Constant Measurements63
Is the Radio Source Dipole from NVSS Consistent with the Cosmic Microwave Background and ΛCDM?63
Active Galactic Nuclei Continuum Reverberation Mapping Based on Zwicky Transient Facility Light Curves63
A Babcock–Leighton-type Solar Dynamo Operating in the Bulk of the Convection Zone63
First-principles-integrated Study of Blazar Synchrotron Radiation and Polarization Signatures from Magnetic Turbulence62
The Structure of the Local Interstellar Medium. VII. Additional New Mg ii, Fe ii, and Mn ii Observations toward Stars within 100 pc62
The Effects of Turbulent Electrical Resistivity on the Response of the Solar Atmosphere to Flare Energy Input. I. Results of Radiative Hydrodynamic Simulations62
Methods for Incorporating Model Uncertainty into Exoplanet Atmospheric Analysis62
Erratum: “Wave Generation by Flare-accelerated Ions and Implications for 3 He Acceleration” (2024, ApJ, 964, 97)62
Global Distribution of the Key Species on the Surface of Europa62
APOGEE Chemical Abundance Patterns of the Massive Milky Way Satellites62
Investigating the Time Evolution of the Thermal Emission from the Putative Neutron Star in SN 1987A for 50+ Years62
Implications of NICER for Neutron Star Matter: The QHC21 Equation of State61
The Discovery of the Faintest Known Milky Way Satellite Using UNIONS61
Spectral Evolution of Ultraluminous X-Ray Pulsar NGC 300 ULX-161
Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping61
Multimessenger Constraints on Magnetic Fields in Merging Black Hole–Neutron Star Binaries61
Light-curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers60
MINDS: Detection of an Inner Gas Disk Caused by Evaporating Bodies around HD 17255560
Updated Low-temperature Gas Opacities with ÆSOPUS 2.060
The Diffusion Tensor of Protons at 1 au: Comparing Simulation, Observation, and Theory60
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification60
Massive Debris Disks May Hinder Secular Stirring by Planetary Companions: An Analytic Proof of Concept60
Solar Eruptive Phenomena Associated with Solar Energetic Electron Spectral Types60
Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger60
Evolution of the Mass–Metallicity Relation from Redshift z ≈ 8 to the Local Universe60
Two Intermittent Eruptions of a Minifilament Triggered by a Two-step Magnetic Reconnection Within a Fan-spine Configuration60
H i HOD. I. The Halo Occupation Distribution of H i Galaxies60
The Density Distribution of Compressively Forced, Supersonic Turbulence Depends on the Driving Correlation Time59
The 230 GHz Variability of Numerical Models of Sagittarius A*. II. The Physical Origins of the Variability59
Mapping the Skies of Ultracool Worlds: Detecting Storms and Spots with Extremely Large Telescopes59
Spin and Obliquity Evolution of Hot Jupiter Hosts from Resonance Locks58
The Local Group L-band Survey: The First Measurements of Localized Cold Neutral Medium Properties in the Low-metallicity Dwarf Galaxy NGC 682258
DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy58
ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field58
Numerical Simulation of Hot Accretion Flow around Bondi Radius57
Nucleosynthesis of Binary-stripped Stars57
A Universal Equation to Predict Ωm from Halo and Galaxy Catalogs57
A Heating Mechanism via Magnetic Pumping in the Intracluster Medium57
AGILE Observations of the LIGO-Virgo Gravitational-wave Events of the GWTC-1 Catalog57
Scattering of Stellar Mass Black Holes and Gravitational-wave Bremsstrahlung Radiation in Active Galactic Nucleus Disks57
Methyl Isocyanate Formation from Oxygen Insertion in Methyl Cyanide Ices57
Spectropolarimetry of GRB 180427A: Evidence for Distinct Emission Sites with Varying Polarization57
Igneous Rim Accretion on Chondrules in Low-velocity Shock Waves56
Mode Mixing and Rotational Splittings. II. Reconciling Different Approaches to Mode Coupling 56
CLASSY VII Lyα Profiles: The Structure and Kinematics of Neutral Gas and Implications for LyC Escape in Reionization-era Analogs*56
Similar Signatures of Coplanar Gas Inflow and Disk Warps in Galactic Gas Kinematic Maps56
MOSEL Survey: Spatially Offset Lyman-continuum Emission in a New Emitter at z = 3.088 Can Explain the Low Number Density of Observed LyC Leakers56
Self-consistent Spin, Tidal, and Dynamical Equations of Motion in the REBOUNDx Framework56
Quantifying the High Early Solar Cosmic-Ray Flux with Cosmogenic Neon Isotopes in Refractory Minerals56
Probing the Heights and Depths of Y Dwarf Atmospheres: A Retrieval Analysis of the JWST Spectral Energy Distribution of WISE J035934.06–540154.656
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
Balmer Decrement Anomalies in Galaxies at z ∼ 6 Found by JWST Observations: Density-bounded Nebulae or Excited H i Clouds?56
Continued PSP/WISPR Observations of a Phaethon-related Dust Trail56
The Atmospheric Response to High Nonthermal Electron-beam Fluxes in Solar Flares. II. Hydrogen-broadening Predictions for Solar Flare Observations with the Daniel K. Inouye Solar Telescope56
Simultaneous Evidence of Edge Collapse and Hub-filament Configurations: A Rare Case Study of a Giant Molecular Filament, G45.3+0.155
Quiet Sun Center to Limb Variation of the Linear Polarization Observed by CLASP2 Across the Mg ii h and k Lines55
How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-dust Geometry Model in Spectral Energy Distribution Fitting55
Discovery of Evolution of the Temporal Features of X-Ray Bursts from SGR J1935+215455
Ultraviolet and Gravitational Wave Signatures of Magnetar Formation55
JWST Observations of the Enigmatic Y-Dwarf WISE 1828+2650. I. Limits to a Binary Companion55
A High-resolution Far-infrared Survey to Probe Black Hole–Galaxy Co-evolution55
Electrostatic Transport Characteristics of Olivine Particles under Electron Irradiation in Vacuum55
A New Galaxy Cluster Merger Capable of Probing Dark Matter: A5655
Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope55
Geminga: A Window into the Role Played by the Local Halo in the Cosmic-Ray Propagation Process55
RELICS: Small-scale Star Formation in Lensed Galaxies at z = 6–1055
Convective Mixing in Gas Giant Planets with Primordial Composition Gradients55
Including Neutrino-driven Convection in the Force Explosion Condition to Predict Explodability of Multidimensional Core-collapse Supernovae (FEC+)54
Anomalous Orbital Characteristics of the AQ Col (EC 05217-3914) System54
Forming Gas Giants around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability54
Discovery of Two Ultra-diffuse Galaxies with Unusually Bright Globular Cluster Luminosity Functions via a Mark-dependently Thinned Point Process (MATHPOP)54
The Study of Jet Formation Mechanism in Fermi Blazars54
Investigating the Impact of Atomic Data Uncertainties on the Measured Physical Parameters of the Perseus Galaxy Cluster54
Iron-peak Element Abundances in Warm Very Metal-poor Stars54
The Complex Infrared Dust Continuum Emission of NGC 1068: Ground-based N- and Q-band Spectroscopy and New Radiative Transfer Models54
Stellar Mergers or Truly Young? Intermediate-age Stars on Highly Radial Orbits in the Milky Way’s Stellar Halo54
A Holistic Exploration of the Potentially Recoverable Redshift Information of Stage IV Galaxy Surveys54
A Systematic Search of Distant Superclusters with the Subaru Hyper Suprime-Cam Survey54
Small-scale Inhomogeneity Effects on Coherent Solar Radio Emission54
Spectroscopically Identified Emission Line Galaxy Pairs in the WISP Survey*54
Identifying Galaxy Mergers in Simulated CEERS NIRCam Images Using Random Forests54
The Cooling of the Central Compact Object in Cas A from 2006 to 202053
CO(2–1)/CO(1–0) Line Ratio on a ∼100 Parsec Scale in the Nearby Barred Galaxy NGC 130053
Delayed Thermal Relaxation of Rapid Cooling Neutron Stars: Nucleon Superfluidity and Nonnucleon Particles53
Suppression of the TeV Pair-beam–Plasma Instability by a Tangled Weak Intergalactic Magnetic Field53
The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method53
Gravitational Influence from Planets on the Measured Rates of Period Change of Pulsating White Dwarfs53
The Dependence of Joy’s Law and Mean Tilt as a Function of Flux Emergence Phase53
The Arizona Molecular ISM Survey with the SMT: Variations in the CO(2–1)/CO(1–0) Line Ratio across the Galaxy Population53
FAST Drift-scan Survey for H i Intensity Mapping: Simulation on Hunting H i Filament with Pairwise Stacking53
Plausible Constraints on the Range of Bulk Terrestrial Exoplanet Compositions in the Solar Neighborhood53
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