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 2022-07-01 to 2026-07-01.)
ArticleCitations
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H i Disk of Galaxies4713
Double Shells of the Planetary Nebula NGC 7009 Minor Axis1184
The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity–Spectral Type Dependence in Taurus–Auriga YSOs821
Searching for Axion Dark Matter Gegenschein of the Vela Supernova Remnant with FAST514
H I Absorption Line and Anomalous Dispersion in the Radio Pulses of PSR B1937+21482
Parsec-scale SiO Emission in the Galactic Center411
Modeling the UV to Radio Spectral Energy Distribution of NGC 6946: Star Formation Rates and Dust Attenuation Properties300
Zonal Flow and Self-regulating Mechanism in a Hydrodynamic Disk293
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei267
Evaluating Non-LTE Spectral Inversions with ALMA and IBIS240
Evidence of the Alfvén Transition Layer and Particle Precipitation in the Cusp Region: 3D Global PIC Simulation of the Solar Wind–Earth Magnetosphere Interaction222
DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos214
Active Galactic Nucleus Variability in the Age of Rubin207
Weighing the Darkness. III. How Gaia Could, but Probably Will Not, Astrometrically Detect Free-floating Black Holes202
Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure195
Criss-cross Nebula: A Case Study of Shock Regions with Resolved Microstructures at Scales of ∼1000 au195
On the Width of a Collisionless Shock and the Index of the Cosmic Rays It Accelerates193
Dark Off-limb Gap: Manifestation of a Temperature Minimum and the Dynamic Nature of the Chromosphere192
Single-pulse Gamma-Ray Bursts Have Prevalent Hard-to-soft Spectral Evolution189
Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?189
Numerical Simulations of Oscillations in Solar Corona Excited by Vortex Shedding181
The Orion OB Association as a Generator for the Hot Circumgalactic Medium176
ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field171
Ultraviolet and Gravitational Wave Signatures of Magnetar Formation169
Scattering of Stellar Mass Black Holes and Gravitational-wave Bremsstrahlung Radiation in Active Galactic Nucleus Disks169
Geminga: A Window into the Role Played by the Local Halo in the Cosmic-Ray Propagation Process168
Electrostatic Transport Characteristics of Olivine Particles under Electron Irradiation in Vacuum161
A Holistic Exploration of the Potentially Recoverable Redshift Information of Stage IV Galaxy Surveys160
Including Neutrino-driven Convection in the Force Explosion Condition to Predict Explodability of Multidimensional Core-collapse Supernovae (FEC+)159
Small-scale Inhomogeneity Effects on Coherent Solar Radio Emission158
Gravitational Influence from Planets on the Measured Rates of Period Change of Pulsating White Dwarfs157
XMM-Newton and NuSTAR Observations of the Compact Millisecond Pulsar Binary PSR J1653–0158156
Binding Energies of Interstellar Complex Organic Molecules on Water Ice Surfaces: A Quantum Chemical Investigation154
Exploring the Evolution of a Dwarf Spheroidal Galaxy with Smoothed-particle Hydrodynamics Simulations. I. Stellar Feedback153
Improving the Low-energy Transient Sensitivity of AMEGO-X using Single-site Events152
Search for Kink Events in Variable Fermi-LAT Blazars151
Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation149
Modeling of Condensations in Coronal Loops Produced by Impulsive Heating with Variable Frequencies and Locations146
Spatiotemporal Evolution of the 2022 March Interplanetary Coronal Mass Ejection Revealed by Multipoint Observations of Forbush Decreases146
Evaluating the Limits of Rotation Period Recovery Through Gyrochronology Criteria145
Interaction of Inner Heliosheath Ions with Electromagnetic Ion Cyclotron Waves144
Multiline Stokes Synthesis of Ellerman Bombs: Obtaining Seamless Information from Photosphere to Chromosphere143
Mitigating Polarization Leakage in Gas Pixel Detectors through Hybrid Machine Learning and Analytic Event Reconstruction142
The Propagation of Fast Radio Bursts in the Magnetosphere Shapes Their Waiting-time and Flux Distributions141
Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus138
A Monte Carlo Simulation on the Scattering Coefficients of Solar Radio Wave Propagation136
Planetary Nebulae in the eROSITA eRASS1 Catalog133
Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph133
Observations of Magnetospheric Solar Wind Charge Exchange133
When is a Bulge Not a Bulge? Revealing the Satellite Nature of NGC 5474’s Bulge130
Searching for Propionamide (C2H5CONH2) toward Sagittarius B2 at Centimeter Wavelengths129
Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts125
Spectral Evolution of Ultraluminous X-Ray Pulsar NGC 300 ULX-1124
The “Canonical” White Dwarf Cooling Sequence of M5122
Global Distribution of the Key Species on the Surface of Europa122
Dark Matter in Fractional Gravity. I. Astrophysical Tests on Galactic Scales121
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters121
Evolution of Magnetic Fields and Energy Release Processes during Homologous Eruptive Flares121
Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter120
The 230 GHz Variability of Numerical Models of Sagittarius A*. II. The Physical Origins of the Variability119
How Does the Critical Torus Instability Height Vary with the Solar Cycle?117
Suprathermal Population Associated with Stream Interaction Regions Observed by STEREO-A: New Insights117
Characterizing Stellar and Gas Properties in NGC 628: Spatial Distributions, Radial Gradients, and Resolved Scaling Relations117
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow117
Inferring Line-of-sight Velocities and Doppler Widths from Stokes Profiles of GST/NIRIS Using Stacked Deep Neural Networks115
Effects of Alpha Particle Fraction on Kinetic Plasma Turbulence115
Search for Fast Radio Bursts and Radio Pulsars from Pulsing Ultraluminous X-Ray Sources114
Spectro-polarimetric Properties of Sunquake Sources in X1.5 Flare and Evidence for Electron and Proton Beam Impacts112
Reconstruction of Coronal Magnetic Fields Using a Poloidal–Toroidal Representation112
The Complex Multiwavelength Morphology of the Peculiar Compact Galaxy Group IC 2431112
Internal 1000 au Scale Structures of the R CrA Cluster-forming Cloud. I. Filamentary Structures112
When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multiband Imaging Data111
What if the Universe Expands Linearly? A Local General Relativity to Solve the “Zero Active Mass” Problem111
Coherent Imaging with Photonic Lanterns111
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 Progenitors109
Identifying Signatures of Inflow onto Face-on Galaxies Using the Balmer Decrement108
The Effects of Turbulent Electrical Resistivity on the Response of the Solar Atmosphere to Flare Energy Input. I. Results of Radiative Hydrodynamic Simulations108
Interplanetary Type III Radio Emission Locations Deduced from the Underlying Electron Exciter Beam Kinematics104
Testing the Physical Parameter Constraining Power of HCN and HNC with Neural Networks103
Possibility of Using 3.3 μm Polycyclic Aromatic Hydrocarbon Luminosity as a Molecular Gas Mass Estimator103
A Novel Blast Wave Solution for the Propagation of Coronal And Interplanetary Shocks103
Rotational Fingerprints of Vinylketene for Astronomical Observations102
Statistical Study of the Timing of the Appearance of H α Postflare Loops: Simple Scaling Law Based on Radiative Cooling102
The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud101
COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey100
The Sonora Substellar Atmosphere Models. VI. Red Diamondback: Extending Diamondback with SPHINX for Brown Dwarf Early Evolution99
Streams and Bubbles: Tidal Shaping of Hydrodynamic Planetary Outflows99
Radio Emission From a z = 10.1 Black Hole in UHZ198
Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content97
Detection of the Extended γ-Ray Emission around TeV Source 1LHAASO J0249+6022 with Fermi-LAT97
Solar Eruptive Phenomena Associated with Solar Energetic Electron Spectral Types97
Gone with the Wind: JWST-MIRI Unveils a Strong Outflow from the Quiescent Stellar-mass Black Hole A0620-0096
Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-353795
Accretion from a Shock-inflated Companion: Spinning Down Neutron Stars to Hour-long Periods94
Dust Properties of 870 μm-selected Galaxies in GOODS-S93
Disentangling Magnetic Fields in NGC 6946 with Wide-band Polarimetry92
Radiative Signatures of Magnetic Reconnection: An Approach to Remote Probing of Reconnection Dynamics92
Galactic Magnetic Fields. II. Applying the Model to Nearby Galaxies91
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets91
Investigating the Time Evolution of the Thermal Emission from the Putative Neutron Star in SN 1987A for 50+ Years90
Spin and Obliquity Evolution of Hot Jupiter Hosts from Resonance Locks90
Wave Emission of Nonthermal Electron Beams Generated by Magnetic Reconnection89
Constraints on Evolutions of Fundamental Constants from Clustering of Fast Radio Burst Dispersion Measure87
S-type Stars: Line List for the A2Π–X2Σ+ Band System of LaO87
Magnetic Field of the Quasar 1604+159 from Parsec to Kiloparsec Scale87
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)86
Asymptotic Normalization Coefficient Investigation of the 17 O( d , p 85
Erratum: “Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains” (2021, ApJ, 919, 65)85
Erratum: “Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration” (2022, ApJ, 940, 74)85
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 )85
Erratum: “Wave Generation by Flare-accelerated Ions and Implications for 3 He Acceleration” (2024, ApJ, 964, 97)84
Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 with Radiant Energies of 1042.5±1.6 erg84
The Imprint of Dark Matter on the Galactic Acceleration Field83
A High-resolution Far-infrared Survey to Probe Black Hole–Galaxy Co-evolution83
Mergers and Recoil in Triple Massive Black Hole Systems from Illustris82
Photospheric Horizontal Magnetic Field Decrease Preceding a Major Solar Eruption82
Spatially Resolved Modeling of Galactic Hα Emission for Galaxy Clustering81
A Systematic Search of Distant Superclusters with the Subaru Hyper Suprime-Cam Survey81
Tidally Driven Inertial Waves Enhance Eccentricity Damping and Spin Evolution in Planets and Stars81
Efficiency of Nonthermal Pulsed Emission from Eight MeV Pulsars81
Discovery of a Rapidly Evolving Global Magnetic Field in the M Dwarf YZ Cet and Constraints on the Magnetic Field of Its Planet YZ Cet b81
Magnetization Factors of Gamma-Ray Burst Jets Revealed by a Systematic Analysis of the Fermi Sample80
Precise Mass, Orbital Motion, and Stellar Properties of the M-dwarf Binary LP 349−25AB80
Photometric and Spectroscopic Studies of Two Early-type Eclipsing Binaries80
Dissecting the Multiple Component Outflow in NGC 5548 with Absorption Line Variability80
Statistical Plasma Properties of the Planar and Nonplanar ICME Magnetic Clouds during Solar Cycles 23 and 2480
The Use of Binary Black Holes Merging in Active Galactic Nuclei Disks for Hubble Constant Measurements78
Stratified Evolution of Ryugu’s Regolith Revealed by Spectroscopic Analyses of Two Hayabusa2 Collected Particles78
Continued PSP/WISPR Observations of a Phaethon-related Dust Trail77
Pulsed, Polarized X-Ray Emission from Neutron Star Surfaces: The Effects of Vacuum Birefringence in the Magnetosphere77
Next-generation Improvements in Giant-exoplanet Evolutionary and Structural Models77
Constraining the Effects of Pre- and Post-accretionary Processes on Ryugu Insoluble Organic Matter76
XMM-Newton Perspective of the Unique Magnetic Binary-ϵ Lupi76
A New Galaxy Cluster Merger Capable of Probing Dark Matter: A5676
Hydrogen-triggered X-Ray Bursts from SAX J1808.4−3658? The Onset of Nuclear Burning76
Unusually Powerful Flare Phenomenon of the Water Maser in W51 and the Possibility of Detecting Gravitational Radiation from It76
A Universal Equation to Predict Ωm from Halo and Galaxy Catalogs75
High-resolution, High-sensitivity, Low-frequency uGMRT View of Coma Cluster of Galaxies75
Thermal Baroclinic Instabilities in Accretion Disks. I. Combined Dispersion Relation for Goldreich–Schubert–Fricke Instability and Convective Overstability in Disks around Young Stars74
A Comprehensive Study on the Relation between the Metal Enrichment of Ionized and Atomic Gas in Star-forming Galaxies74
Binary Vision: The Mass Distribution of Merging Binary Black Holes via Iterative Density Estimation74
The Lively Accretion Disk in NGC 2992. III. Tentative Evidence of Rapid Ultrafast Outflow Variability74
Enhanced Star Formation and Black Hole Accretion Rates in Galaxy Mergers in IllustrisTNG5073
The Discovery of the Faintest Known Milky Way Satellite Using UNIONS73
Unveiling Bifurcated Blue Straggler Sequences in NGC 2173: Insights from Binary Evolution73
Uncalibrated Cosmic Standards as a Robust Test on Late-time Cosmological Models73
Investigation of the Microquasar SS 433 with VERITAS73
Constraints on the Galaxy Formation Models during the Epoch of Reionization with High-redshift Observations73
Light-curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers73
Silicon, Sulfur, and Iron in the Interstellar Medium: A High-resolution X-Ray Spectral Study of GX 340+073
Properties of the Magellanic Corona72
Analysis of Thermal Emissions of Exoplanets with Axially Symmetric Temperature Gradients72
Electron Acceleration by Multiple Fast Fermi Reflections at Earth’s Bow Shock72
Forming Gas Giants around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability72
Two High-amplitude δ Scuti–γ Doradus Hybrids Constrained by the Radial Fundamental p and Equally Spaced g Modes71
Coordinated JWST Imaging of Three Distance Indicators in a Supernova Host Galaxy and an Estimate of the Tip of the Red Giant Branch Color Dependence71
Mapping the z  ∼  2 Circumgalactic Medium with KBSS Galaxy Pairs *71
Large Variations Seen in First Ultraviolet Spectroscopic M33 Dust Extinction Curves70
Sensitivity of Simulations of Double-detonation Type Ia Supernovae to Integration Methodology70
A Census of Star Formation Histories of Massive Galaxies at 0.6 < z < 1 from Spectrophotometric Modeling Using Bagpipes and Prospector70
Discovery of Two Ultra-diffuse Galaxies with Unusually Bright Globular Cluster Luminosity Functions via a Mark-dependently Thinned Point Process (MATHPOP)69
Star Formation in the Lopsided Galaxy Arp 29169
The Local Group L-band Survey: The First Measurements of Localized Cold Neutral Medium Properties in the Low-metallicity Dwarf Galaxy NGC 682269
The Impact of Cosmic Filaments on the Abundance of Satellite Galaxies69
Self-consistent Spin, Tidal, and Dynamical Equations of Motion in the REBOUNDx Framework69
Quantitative Sensitivity Assessment of Martian Geodetic Parameters to Interior Model: Implications for Joint Inversion68
The Internal Proper Motion Kinematics of NGC 346: Past Formation and Future Evolution68
Quantifying the High Early Solar Cosmic-Ray Flux with Cosmogenic Neon Isotopes in Refractory Minerals68
Impact of Current Uncertainties in the 12C+12C Nuclear Reaction Rate on Intermediate-mass Stars and Massive White Dwarfs68
H i HOD. I. The Halo Occupation Distribution of H i Galaxies67
Azimuthal Size Scales of Solar Wind Periodic Density Structures67
GASP. XLV. Stellar Bars in Jellyfish Galaxies: Analysis of Ionized Gas and Stellar Populations67
The JWST Resolved Stellar Populations Early Release Science Program. VII. Stress Testing the NIRCam Exposure Time Calculator67
The Role of Magnetic and Rotation Axis Alignment in Driving Fast Radio Burst Phenomenology67
The Density Distribution of Compressively Forced, Supersonic Turbulence Depends on the Driving Correlation Time67
Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope67
Constraining the Milky Way Halo Accretion History with Simulated Stellar Halos: Designing the HALO7D-X Survey67
Impact of Multimessenger Spectral Modeling on Blazar–Neutrino Associations66
Discovery of Evolution of the Temporal Features of X-Ray Bursts from SGR J1935+215466
UVIT Observations of the Small Magellanic Cloud: Point-source Catalog65
Revealing the CME Impact on the Martian Nightside Ionosphere Based on MAVEN and Tianwen-1 Observations65
Caught in the Act: A Metal-rich High-velocity Cloud in the Inner Galaxy64
Experimental and Numerical Studies of the Collapse of Dense Clouds Induced by Herbig–Haro Stellar Jets64
Delayed Thermal Relaxation of Rapid Cooling Neutron Stars: Nucleon Superfluidity and Nonnucleon Particles64
Total Power and Low-energy Cutoff Time Evolution of Solar Flare Accelerated Electrons Using X-Ray Observations and Warm-target Model64
Is the Radio Source Dipole from NVSS Consistent with the Cosmic Microwave Background and ΛCDM?64
Methyl Isocyanate Formation from Oxygen Insertion in Methyl Cyanide Ices63
An SMA Survey of Chemistry in Disks Around Herbig AeBe Stars63
An Elemental Abundance Diagnostic for Coordinated Solar Orbiter/SPICE and Hinode/EIS Observations62
The Importance of Heat Flux in Low-Mach-number, Quasi-parallel Collisionless Shocks62
No Sign of a Magnetar Remnant Following the Kilonova-producing Long GRB 211211A ∼1.7 yr Later62
Bell Instability and Cosmic-Ray Acceleration in Active Galactic Nuclei Ultrafast Outflow Shocks62
The Structure of the Local Interstellar Medium. VII. Additional New Mg ii, Fe ii, and Mn ii Observations toward Stars within 100 pc62
Galaxies Caught in Transition: The Role of Group Environment in Shaping the Mass–Size Relation in the Local Universe61
The ALMA-QUARKS Survey: Evidence of a Candidate High-mass Prestellar Core Aside a Bright-rimmed Cloud IRAS 18290-092461
Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II. Spectroscopic and Environmental Analysis of Thorne–Żytkow Object and Super-AGB Star Candidates61
The Observable Properties of Galaxy Accretion Events in Milky Way–like Galaxies in the FIRE-2 Cosmological Simulations61
Investigation of Phase Shift and Travel Time of Acoustic Waves in the Lower Solar Atmosphere Using Multiheight Velocities60
Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension60
Discovery of a 21 cm Absorption System at z = 2.327 with CHIME60
Assessing the Observability of Deep Meridional Flow Cells in the Solar Interior60
A Unified Photometric Redshift Calibration for Weak Lensing Surveys Using the Dark Energy Spectroscopic Instrument60
Convolutional Neural Networks for Searching Superflares from Pixel-level Data of the Transiting Exoplanet Survey Satellite60
Differential Rotation of CoRoT Stars and a Kepler Binary Star from Starspot Transit Mapping59
Properties of Type Iax Supernova 2019muj in the Late Phase: Existence, Nature, and Origin of the Iron-rich Dense Core59
Iron-peak Element Abundances in Warm Very Metal-poor Stars59
Two Intermittent Eruptions of a Minifilament Triggered by a Two-step Magnetic Reconnection Within a Fan-spine Configuration59
Stellar Mergers or Truly Young? Intermediate-age Stars on Highly Radial Orbits in the Milky Way’s Stellar Halo59
Digging into the Interior of Hot Cores with ALMA (DIHCA). VI. The Formation of Low-mass Multiple Systems in High-mass Cluster-forming Regions59
LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results59
Distances to Recent Near-Earth Supernovae from Geological and Lunar 60Fe59
On the Onset Delays of Solar Energetic Electrons and Protons: Evidence for a Common Accelerator59
SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z  > 6 Quasar Host Galaxies Using the JWST NIRSpec Fixed Slit58
Prospects of Detecting Nonthermal Protons in Solar Flares via Lyman Line Spectroscopy: Revisiting the Orrall–Zirker Effect58
Asymptotic Giant Branch Mass-loss Rates and Metal Yields from Scaled Mixing-length and Mass-loss Parameters58
Determining the Spatial Origin of X-Ray and Optical Emission in the z = 3.1 Strongly Lensed Radio-quiet Quasar GraL J065904.1+162909 to Hundreds of Parse58
The DESI Single Fiber Lens Search. I. Four Thousand Spectroscopically Selected Galaxy–Galaxy Gravitational Lens Candidates58
The Effect of Spatially Varying Collision Frequency on the Development of the Rayleigh–Taylor Instability58
The Role of the Third Dredge-up and Mass Loss in Shaping the Initial–Final Mass Relation of White Dwarfs58
The Carbon Isotopic Ratio and Planet Formation57
Numerical Simulation of Hot Accretion Flow around Bondi Radius57
Updated Low-temperature Gas Opacities with ÆSOPUS 2.057
A Study of the Kinematic and Volumetric Coevolution of Earth-directed Coronal Mass Ejections57
An NGC 1068-informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+05657
Lyα Emission at z = 7–13: Clear Evolution of Lyα Equivalent Width Indicating a Late Cosmic Reionization History57
Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm57
The BoRG-JWST Survey: Analogs at z ∼ 8 to the UV-luminous Galaxy Population at z ≳ 1057
A Data-driven Approach for Star Formation Parameterization Using Symbolic Regression57
RRAT J2325–0530: A Rotating Radio Transient with an Atypical Waiting-time Distribution56
New Spectroscopic Confirmations of Lyα Emitters at Z ∼ 7 from the LAGER Survey56
VERITAS Observations Contemporaneous with the LHAASO Detection of NGC 427856
Radial and Vertical Constraints on the Icy Origin of H2CO in the HD 163296 Protoplanetary Disk56
Igneous Rim Accretion on Chondrules in Low-velocity Shock Waves56
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. IV. Heavy Element Enhanced Stars56
Extinction Values toward Embedded Planets in Protoplanetary Disks Estimated from Hydrodynamic Simulations56
Discovering High- z BL Lacs Using Swift/UVOT and SARA Observations with the Dropout Technique56
XRISM Constrains Atmospheric Motion and Turbulent Dissipation in the Archetypal Radio-mode Feedback System Hydra-A56
Investigating the Impact of Vertically Extended Coronae on X-Ray Reverberation Mapping56
The Study of Jet Formation Mechanism in Fermi Blazars55
Balmer Decrement Anomalies in Galaxies at z ∼ 6 Found by JWST Observations: Density-bounded Nebulae or Excited H i Clouds?55
A Tale of Three Dwarfs: No Extreme Cluster Formation in Extreme Star-forming Galaxies55
Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling55
Anomalously Fast Core and Envelope Rotation in Red Giants55
Quiet Sun Center to Limb Variation of the Linear Polarization Observed by CLASP2 Across the Mg ii h and k Lines55
The Kinematic Signature of the Warp and Waves in the Milky Way Disk55
Coronal Heating and Solar Wind Generation by Flux Cancellation Reconnection55
Mode Mixing and Rotational Splittings. II. Reconciling Different Approaches to Mode Coupling 55
A Comparison of Three Neodymium Atomic Data Sets for Kilonova Modeling55
Ab Initio Quantum Dynamics as a Scalable Solution to the Exoplanet Opacity Challenge: A Case Study of CO2 in a Hydrogen Atmosphere55
Model-independent Approach of the JUNO 8B Solar Neutrino Program55
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