Astronomy & Astrophysics

Papers
(The TQCC of Astronomy & Astrophysics is 11. 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
A solar rotation signature in cosmic dust observed in STEREO spacecraft data100
Exploring the origins of mega radio halos100
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
Sub-stellar engulfment by a main-sequence star: Where is the lithium?95
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
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
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission85
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field85
The longevity of the oldest open clusters85
Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk84
Gamma-ray line emission from the Local Bubble84
MOCKA – A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators84
Tracing the Galactic disk with planetary nebulae using Gaia DR384
Coronal rain formation in a two-fluid approximation82
Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z  ∼  382
Discovery of the luminous X-ray ignition eRASSt J234402.9−35264082
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations82
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations81
Dynamical modelling and the origin of gas turbulence in z ∼ 4.5 galaxies81
PDRs4All80
X-ray pulsar GRO J1008−57 as an orthogonal rotator80
Changing disc compositions via internal photoevaporation79
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries79
Data span and frequency coverage requirements for robust detection and inference in pulsar timing arrays. A case study with EPTA DR279
The Arecibo Galaxy Environment Survey (AGES)79
The MUSE-Faint survey79
Constraints on asteroid-mass primordial black holes in dwarf galaxies using Hubble Space Telescope photometry77
Tracking active nests in solar-type pulsators: Ensemble starspot modelling of Kepler asteroseismic targets76
Cosmology in the non-linear regime: the small scale miracle76
Probing the interstellar medium of the quasar BRI 0952−011576
[Mg/Fe] ratios in the solar neighbourhood: Stellar yields and chemical evolution scenarios76
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries76
The supermassive black hole population from seeding via collisions in nuclear star clusters76
Models of quasi-discontinuous solar-wind streams76
Improved source classification and performance analysis usingGaiaDR375
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy75
The drastic impact of Eddington-limit induced mass ejections on massive star populations75
A highly dynamic small-scale jet in a polar coronal hole74
Strong lensing in UNIONS: Toward a pipeline from discovery to modeling74
Planet formation around intermediate-mass stars74
The GAPS Programme at TNG74
Quasars behind the disk of M31 galaxy73
JOYS: JWST MIRI/MRS spectra of the inner 500 au region of the L1527 IRS bipolar outflow73
Characterisation of starspot structure and differential rotation of Kepler-41173
A search for new symbiotic stars in the Milky Way73
Classical Cepheids in the Galactic thin disk72
Exploring non-thermal emission from the star-forming region NGC 3603 through a realistic modelling of its environment72
Cataclysmic variables and the disc instability model in the Gaia DR3 colour–magnitude diagram71
A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS71
Magnetic properties of orphan penumbrae71
Exploring self-consistent 2.5D flare simulations with MPI-AMRVAC71
Discovery of a strong rotation of the X-ray polarization angle in the galactic burster GX 13+170
The SLACS strong lens sample, debiased70
Standardizing the gamma-ray burst as a standard candle and applying it to cosmological probes: Constraints on the two-component dark energy model70
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY69
Timing and scintillation studies of PSR J1439−550169
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz69
Globules and pillars in Cygnus X69
Velocity measurement in the extensive [OIII] emission region 1.2° south-east of M 3169
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars68
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey67
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation66
Deep imaging of the galaxy Malin 2 shows new faint structures and a candidate satellite dwarf galaxy66
Solar flares in the Solar Orbiter era: Short-exposure EUI/FSI observations of STIX flares66
Detection of a new sample of Galactic white dwarfs in the direction of the Small Magellanic Cloud66
The impact of morphological quenching mechanisms on star formation activity at 0.2 < z < 1.2 in the COSMOS field66
JWST reveals a supernova following a gamma-ray burst at z ≃ 7.366
Shaping physical properties of galaxy subtypes in the VIPERS survey: Environment matters66
Molecular hydrogen in filaments at high Galactic latitudes66
Fast-rotating blue straggler stars in the globular cluster NGC 185166
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data65
zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks65
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models64
Implications of a turbulent convection model for classical Cepheids64
The SPAr burning: Proton captures powering carbon–oxygen shell mergers in massive stars63
From eruption to post-flare rain: A 2.5D MHD model63
Bi-directional reflectance, polarization, and spectroscopic measurements of the Chang'e-5 regolith sample63
Validating a non-local stellar convection model with 3D hydrodynamics simulations63
Simulating the LOcal Web (SLOW)63
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution62
The spatial distribution of dwarf and giant galaxies in and around the Virgo cluster62
Transient classifiers for Fink62
Instabilities at recollimation shocks in magnetohydrodynamic jets62
An effective model for magnetic field amplification by the magnetorotational and parasitic instabilities62
An efficient spectral Poisson solver for the NIRVANA-III code: The shearing box case with vertical vacuum boundary conditions62
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies62
Life cycle of cosmic-ray electrons in the intracluster medium61
Planetesimal and planet formation in transient dust traps61
The EDGES measurement disfavors an excess radio background during the cosmic dawn61
The Gravitational Wave Universe Toolbox61
Generative models of astrophysical fields with scattering transforms on the sphere60
Negative polarization properties of regolith simulants60
The preferential orientation of magnetic switchbacks and its implications for solar magnetic flux transport60
Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing59
Rotational equilibrium of C2 in diffuse interstellar clouds59
The attempted polarity reversal and evolving magnetic environment of AD Leo59
Cosmic rays cannot explain the high ionisation rates in the Galactic centre59
Radio outburst from a massive (proto)star58
The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model58
Euclid58
An Earth-sized planet on a 5.4 h orbit around a nearby K dwarf58
Backstreaming ions at a high Mach number interplanetary shock58
Volatile enrichment in low-mass planets as signatures of past planetary disruption58
A rotation-based census of blue lurker candidates in open clusters58
Predicting the surface age of chondritic S-type asteroids using the space weathering features in reflectance spectra: Small data machine learning58
Spinning nano-carbon grains: Viable origin for anomalous microwave emission58
Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 135158
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole57
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system57
The ESO SupJup Survey57
Bayesian test of Brans–Dicke theories with planetary ephemerides: Investigating the strong equivalence principle57
TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE57
Very massive star models57
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data57
Anatomy of rocky planets formed by rapid pebble accretion57
LOFAR high-band antenna observations of the Perseus cluster56
The X-ray properties of the most luminous quasars with strong emission-line outflows56
Double red giant branch and red clump features of Galactic disc stellar populations with Gaia GSP-Spec56
The AIDA-TNG project: Abundance, radial distribution, and clustering properties of halos in alternative dark matter models56
Quantifying observational projection effects with a simulation-based hot CGM model56
Euclid : The first statistical census of dusty and massive objects in the ERO/Perseus field56
Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies56
Stochastic excitation of waves in magnetic stars56
Multi-step reconstruction of radio-interferometric images55
A3COSMOS: Measuring the cosmic dust-attenuated star formation rate density at 4 < z < 555
Euclid: Searches for strong gravitational lenses using convolutional neural nets in Early Release Observations of the Perseus field55
The jet and circumstellar environment of the young binary DF Tau55
Temperature of quiet Sun small scale brightenings observed by EUI on board Solar Orbiter: Evidence for a cooler component55
The MALATANG survey: Star formation, dense gas, and active galactic nucleus feedback in NGC 106855
M-type (22) Kalliope: A tiny Mercury55
A nuclear spiral in a dusty star-forming galaxy at z = 2.7855
Star-forming compact groups: Tracing the early evolutionary stages of compact group environments55
Extreme line profile variations in the repeating changing-look active galactic nucleus IRAS 23226-384354
Carbon envelopes around merging galaxies at z ∼ 4.554
Core to ultracompact HII region evolution in the W49A massive protocluster54
Barred active galactic nucleus galaxies in paired systems: Exploring the impact on nuclear activity54
Clumpy star formation and an obscured nuclear starburst in the luminous dusty z = 4 galaxy GN20 seen by MIRI/JWST54
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph54
Properties of intermediate- to high-mass stars in the young cluster M1754
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 202253
Multiple short-term cycles in Kepler star KIC 687666853
Non-radial oscillations mimicking a brown dwarf orbiting the cluster giant NGC 4349 No. 12753
The stable climate of KELT-9b53
SPICE connection mosaics to link the Sun’s surface and the heliosphere53
The outflowing ionised gas of I Zw 1 observed by HST COS53
A phase-resolvedFermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere53
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA53
Numerical simulations of prominence oscillations triggered by external perturbations53
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies53
Time-resolved spectro-polarimetric analysis of extremely bright GRB 230307A: Possible evidence of evolution from photospheric to synchrotron dominated emission53
Galaxy populations in the most distant SPT-SZ clusters53
Stellar halo density with LAMOST K and M giants53
Clustering of magnetic reconnection exhausts in the solar wind: An automated detection study53
Probing quadratic gravity with the Event Horizon Telescope52
A new way to measure the distance to NGC1052-DF252
Selected open cluster sample for validating atmospheric parameters: Application to Gaia and other surveys52
The “C”: The large Chameleon-Musca-Coalsack cloud52
The origin of B-type runaway stars based on kinematics52
MUSE crowded field 3D spectroscopy in NGC 30052
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)52
SHAPE52
Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes52
ISPY: NACO Imaging Survey for Planets around Young stars52
The SRG/eROSITA All-Sky Survey52
GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisation51
Evolutionary tracks of binary neutron star progenitors across cosmic times51
Self-gravity in thin-disc simulations of protoplanetary discs: The smoothing length rectified and generalised to bi-fluids51
A low mass, binary-stripped envelope for the Type IIb SN 2024abfo51
Modeling the 2020 November 29 solar energetic particle event using EUHFORIA and iPATH models51
0.15112495422363