Astronomy & Astrophysics

Papers
(The H4-Index of Astronomy & Astrophysics is 86. 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 2022-05-01 to 2026-05-01.)
ArticleCitations
Volatile-rich comets ejected early on during Solar System formation3683
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)917
Indications of magnetic accretion in Swift J0826.2−7033606
First detection of metric emission from a solar surge448
Categorization model of moving small-scale intensity enhancements in solar active regions422
Reduction of dust radial drift by turbulence in protoplanetary disks362
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes326
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity321
Massive pre-main-sequence stars in M17319
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?298
Reconciling concentration to virial mass relations279
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids269
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe258
The origin of the soft excess in the luminous quasar HE 1029-1401248
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1243
Ammonia characterisation of dense cores in the Rosette Molecular Cloud235
Post-Newtonian gravity and Gaia-like astrometry209
Multi-spacecraft observations of near-relativistic electron events at different radial distances202
Galaxies at the edges: A complete census of the MACS J0416.1–2403 cluster201
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d201
Calibration and performances of the integrated Mach—Zehnder wavefront sensor for extreme adaptive optics199
Transport of the magnetic flux away from a decaying sunspot via convective motions195
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts192
Euclid preparation185
The effect of dynamic temperatures on pebble dynamics and planet formation181
iNNterpol: High-precision interpolation of stellar atmospheres with a deep neural network using a 1D convolutional auto encoder for feature extraction178
Generative modelling of convergence maps based on predicted one-point statistics178
Probing the physical properties of the intergalactic medium using SRG/eROSITA spectra from blazars174
The XXL Survey172
CO enhancement by magnetohydrodynamic waves171
Parameter measurement based on photometric images171
What drives the corpulence of galaxies?167
Euclid preparation162
High-energy interstellar isomers: cis - N -methylformamide in the G+0.693-0.027 molecular cloud157
3D non-LTE Ca II line formation in metal-poor FGK stars156
Contribution of polycyclic aromatic hydrocarbon ionization to neutral gas heating in galaxies: model versus observations155
The shape of dark matter halos: A new fundamental cosmological invariance147
Detection of very high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage145
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments142
Number of stars in the Sun’s birth cluster revisited141
Probing methane in Uranus’ upper stratosphere using HST observations of the 1280 Å Raman feature140
Observational constraints on gas disc sizes in the protoplanetary discs of multiple systems in the Taurus region130
Edge-On Disk Study (EODS)129
Systematic evaluation of variability detection methods for eROSITA128
Exploring the Sagittarius stream with RR Lyrae stars from Gaia Data Release 3127
Noble gases neon and argon: A role for the chemical patterns of multiple populations in globular clusters?124
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles124
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models118
Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star ζ Oph from high-cadence ESPRESSO spectroscopy and TE116
Scale-invariant vacuum guided resolution of the 7Li BBN problem113
Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter112
Probing star formation and ISM properties using galaxy disk inclination112
HI-H2 transition: Exploring the role of the magnetic field110
Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies110
Unveiling a new extragalactic structure hidden by the Milky Way108
An idealized general circulation model for the atmospheric circulation on the ice giants108
Five methods for determining pattern speeds in galaxies107
Propeller effect in action: Unveiling quenched accretion in the transient X-ray pulsar 4U 0115+63107
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail106
Chromospherically active stars: Lithium and CNO abundances in northern RS CVn stars103
The GALAH survey: Improving chemical abundances using star clusters101
Detection of J -band photometric periodicity in the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-3338101
Exploring the origins of mega radio halos100
A solar rotation signature in cosmic dust observed in STEREO spacecraft data100
SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host98
Emission and absorption lines in the photospheric radius expansion bursts of 4U 1820–3098
Cosmic ray interactions with indene and adamantane seeded water ice mantles97
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy96
Age of (152830) Dinkinesh I Selam constrained by secular tidal-BYORP theory95
Dust-driven wind as a model of broad absorption line quasars95
Challenging historical novae: AT Cnc (1645), Te-11 (483), and M22 (BC 48) revisited95
Sub-stellar engulfment by a main-sequence star: Where is the lithium?95
The influence of planetesimal fragmentation on planet formation94
The cylindrical jet base of M 87 within 100 μas of the central engine93
The spectral energy distributions of very long-period Cepheids in the Milky Way, the Magellanic Clouds, M31, and M3390
Dynamics of trans-Neptunian objects near the 3/1 mean-motion resonance with Neptune90
Slow-mode rarefaction and compression fronts in the Hermean magnetosphere: From MESSENGER insights to future BepiColombo observations90
Survey of Orion Disks with ALMA (SODA)90
Identifying multiplets of IceCube alert events90
Constraining the formation history of the HAT-P-11 system using atmospheric abundances90
Astrometric mass measurement of compact companions in binary systems with Gaia90
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence89
X-ray polarization observations of NGC 2110 with IXPE87
Gas-phase reaction of fullerene monocations with 2,3-benzofluorene indicates the importance of charge exchanges87
Euclidpreparation87
Simulation of CH3OH ice UV photolysis under laboratory conditions86
The Snake filament: A study of polarization and kinematics86
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