Astronomy & Astrophysics

Papers
(The TQCC of Astronomy & Astrophysics 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 2021-08-01 to 2025-08-01.)
ArticleCitations
Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus (Corrigendum)2449
Indications of magnetic accretion in Swift J0826.2−70331221
First detection of metric emission from a solar surge653
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)476
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA431
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts348
Cosmology in the non-linear regime: the small scale miracle324
One Star to Tag Them All (OSTTA)276
Categorization model of moving small-scale intensity enhancements in solar active regions265
Reduction of dust radial drift by turbulence in protoplanetary disks241
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state207
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies195
The GAPS Programme at TNG189
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies188
From eruption to post-flare rain: A 2.5D MHD model184
Volatile-rich comets ejected early on during Solar System formation184
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)182
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves177
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD170
Timing and scintillation studies of PSR J1439−5501169
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission165
The LOFAR LBA Sky Survey: Deep Fields159
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field149
Properties of the ionisation glitch149
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 2022147
Stellar halo density with LAMOST K and M giants146
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources145
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole141
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation137
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST137
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility136
Improved source classification and performance analysis usingGaiaDR3134
Simulation of CH3OH ice UV photolysis under laboratory conditions132
Gamma-ray line emission from the Local Bubble128
Systematic evaluation of variability detection methods for eROSITA128
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY127
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars125
Massive pre-main-sequence stars in M17124
A solar rotation signature in cosmic dust observed in STEREO spacecraft data124
The effect of dynamic temperatures on pebble dynamics and planet formation123
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution122
Transient classifiers for Fink122
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?122
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids118
Reconciling concentration to virial mass relations118
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system117
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries113
The shape of dark matter halos: A new fundamental cosmological invariance110
Probing the interstellar medium of the quasar BRI 0952−0115110
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data107
The first spatio-spectral Bayesian imaging of SN1006 in X-rays105
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity104
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes104
Life cycle of cosmic-ray electrons in the intracluster medium102
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles102
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy102
Ultracool dwarfs identified using spectra in LAMOST DR7101
Dynamics of nanodust in the vicinity of a stellar corona: Effect of plasma corotation100
The origin of the soft excess in the luminous quasar HE 1029-140199
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies99
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe93
Non-linear dynamics of the minimal theory of massive gravity92
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail92
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments92
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf90
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey89
Carina High-contrast Imaging Project for massive Stars (CHIPS)89
Cosmic rays cannot explain the high ionisation rates in the Galactic centre88
Parameter measurement based on photometric images87
Exploring the origins of mega radio halos85
Black hole accretion and radiation variability in general relativistic magnetohydrodynamic simulations with Rezzolla–Zhidenko spacetime85
Link between star formation and the properties of supermassive black holes85
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs84
Unveiling a new extragalactic structure hidden by the Milky Way83
Evidence for stellar contamination in the transmission spectra of HAT-P-12b83
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data82
The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies80
SPICE connection mosaics to link the Sun’s surface and the heliosphere80
Multi-spacecraft observations of near-relativistic electron events at different radial distances79
zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks78
The PAU Survey: The quasar Lyα and UV luminosity functions at 2.7 < z < 5.378
The Disc Miner78
Five methods for determining pattern speeds in galaxies77
GaiaData Release 377
Ammonia characterisation of dense cores in the Rosette Molecular Cloud77
Cosmological measurement of the gravitational constant G using the CMB, BAO, and BBN76
Constraints on asteroid-mass primordial black holes in dwarf galaxies using Hubble Space Telescope photometry75
Very massive star models74
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy74
Backstreaming ions at a high Mach number interplanetary shock74
The longevity of the oldest open clusters74
Detection of very high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage73
Number of stars in the Sun’s birth cluster revisited72
Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter72
Core to ultracompact HII region evolution in the W49A massive protocluster72
Ammonia snow lines and ammonium salts desorption72
Velocity measurement in the extensive [OIII] emission region 1.2° south-east of M 3171
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz71
Central kiloparsec region of Andromeda70
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-170
Evolutionary tracks of binary neutron star progenitors across cosmic times70
Probing star formation and ISM properties using galaxy disk inclination70
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations70
Galaxy populations in the most distant SPT-SZ clusters70
The spectral energy distributions of very long-period Cepheids in the Milky Way, the Magellanic Clouds, M31, and M3369
Asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia69
Clumpy star formation and an obscured nuclear starburst in the luminous dusty z = 4 galaxy GN20 seen by MIRI/JWST69
Exploring non-thermal emission from the star-forming region NGC 3603 through a realistic modelling of its environment68
The impact of morphological quenching mechanisms on star formation activity at 0.2 < z < 1.2 in the COSMOS field67
Gas-phase reaction of fullerene monocations with 2,3-benzofluorene indicates the importance of charge exchanges66
Theoretical computations on the efficiency of acetaldehyde formation on interstellar icy grains66
Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter65
Euclid preparation65
Shaping physical properties of galaxy subtypes in the VIPERS survey: Environment matters65
Contribution of polycyclic aromatic hydrocarbon ionization to neutral gas heating in galaxies: model versus observations65
Predicting the surface age of chondritic S-type asteroids using the space weathering features in reflectance spectra: Small data machine learning65
Barred active galactic nucleus galaxies in paired systems: Exploring the impact on nuclear activity64
Modelling chemical clocks64
Supermassive Black Hole Winds in X-rays: SUBWAYS63
The preferential orientation of magnetic switchbacks and its implications for solar magnetic flux transport63
Quantifying observational projection effects with a simulation-based hot CGM model63
Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey63
Discovery of the luminous X-ray ignition eRASSt J234402.9−35264063
Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies62
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence62
Ultrasoft state of microquasar Cygnus X-3: X-ray polarimetry reveals the geometry of the astronomical puzzle62
Rotational equilibrium of C2 in diffuse interstellar clouds61
Anatomy of rocky planets formed by rapid pebble accretion61
Simulating the LOcal Web (SLOW)61
Changing disc compositions via internal photoevaporation61
Interstellar chemistry of CN radicals on ices: The formation of CH3CN and CH3NC and potential connection to acetamide61
12C/13C ratio and CNO abundances in the classical very old metal-poor dwarf HD 14028361
Reconstructing solar irradiance from historical Ca II K observations60
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models60
First look with JWST spectroscopy: Resemblance among z ∼ 8 galaxies and local analogs60
Plasma dynamics in the flaring loop observed by RHESSI60
Slow-mode rarefaction and compression fronts in the Hermean magnetosphere: From MESSENGER insights to future BepiColombo observations59
Atmospheric characterization of the ultra-hot Jupiter WASP-33b59
Fitting the light curves of Sagittarius A* with a hot-spot model59
Detection of iron emission lines and a temperature inversion on the dayside of the ultra-hot Jupiter KELT-20b59
The Low-Redshift Lyman Continuum Survey58
Double red giant branch and red clump features of Galactic disc stellar populations with Gaia GSP-Spec58
H2–H2O demixing in Uranus and Neptune: Adiabatic structure models58
K2 and Spitzer phase curves of the rocky ultra-short-period planet K2-141 b hint at a tenuous rock vapor atmosphere58
PARSEC V2.0: Stellar tracks and isochrones of low- and intermediate-mass stars with rotation58
Detection of a new sample of Galactic white dwarfs in the direction of the Small Magellanic Cloud58
What drives the corpulence of galaxies?58
The Gravitational Wave Universe Toolbox58
Comparing feature sets and machine-learning models for prediction of solar flares58
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars57
Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z  ∼  357
Kinematic properties of white dwarfs57
ASTRAEUS57
Generative models of astrophysical fields with scattering transforms on the sphere56
The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model56
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models56
ISPY: NACO Imaging Survey for Planets around Young stars55
Transport of the magnetic flux away from a decaying sunspot via convective motions55
JWST Observations of Young protoStars (JOYS)55
The EDGE-CALIFA Survey: An integral field unit-based integrated molecular gas database for galaxy evolution studies in the Local Universe55
N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift?55
Galaxies at the edges: A complete census of the MACS J0416.1 - 2403 cluster55
High-resolution APEX/LAsMA 12CO and 13CO (3-2) observation of the G333 giant molecular cloud complex55
Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes55
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA)55
HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars55
The Snake filament: A study of polarization and kinematics55
PRODIGE – envelope to disk with NOEMA54
Strong lensing in UNIONS: Toward a pipeline from discovery to modeling54
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d54
Probing quadratic gravity with the Event Horizon Telescope54
Forming Planets Around Stars With Non-Solar Elemental Composition54
Implications of a turbulent convection model for classical Cepheids54
Mid-infrared spectra of T Tauri disks: Modeling the effects of a small inner cavity on CO2 and H2O emission54
[Mg/Fe] ratios in the solar neighbourhood: Stellar yields and chemical evolution scenarios54
The Arecibo Galaxy Environment Survey (AGES)53
χ1 Fornacis cluster DANCe53
Carbon envelopes around merging galaxies at z ∼ 4.553
Emission and absorption lines in the photospheric radius expansion bursts of 4U 1820–3053
The origin of X-ray emission in 3CRR sources: Hints from mid-infrared Spitzer observations53
Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations53
Doppler shifts of spectral lines formed in the solar transition region and corona53
The outflowing ionised gas of I Zw 1 observed by HST COS53
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries53
JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H2 in the radio galaxy 3C 326 N53
Age of (152830) Dinkinesh I Selam constrained by secular tidal-BYORP theory53
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph52
Making the unmodulated pyramid wavefront sensor smart52
Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters52
The influence of planetesimal fragmentation on planet formation52
The cylindrical jet base of M 87 within 100 μas of the central engine52
Constraining the formation history of the HAT-P-11 system using atmospheric abundances52
An effective model for magnetic field amplification by the magnetorotational and parasitic instabilities52
Spinning nano-carbon grains: Viable origin for anomalous microwave emission52
Sub-stellar engulfment by a main-sequence star: Where is the lithium?51
On-sky validation of image-based adaptive optics wavefront sensor referencing51
Survey of Orion Disks with ALMA (SODA)51
A phase-resolvedFermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere51
Exploring self-consistent 2.5D flare simulations with MPI-AMRVAC50
MeerKAT view of Hickson Compact Groups50
A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies50
Post-Newtonian gravity and Gaia-like astrometry50
Astrometric mass measurement of compact companions in binary systems with Gaia50
Identifying multiplets of IceCube alert events49
Clustering of magnetic reconnection exhausts in the solar wind: An automated detection study49
Euclid: Searches for strong gravitational lenses using convolutional neural nets in Early Release Observations of the Perseus field49
A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies49
Dust-driven wind as a model of broad absorption line quasars49
Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk49
Cyano radical emission at small spatial scales towards massive protostars49
Spatially resolved spectroscopic analysis of Lyα haloes49
Cataclysmic variables and the disc instability model in the Gaia DR3 colour–magnitude diagram48
Multi-step reconstruction of radio-interferometric images48
The jet and circumstellar environment of the young binary DF Tau48
Cosmic-ray electron transport in the galaxy M 5148
Discovery of a strong rotation of the X-ray polarization angle in the galactic burster GX 13+148
Euclid48
Observational constraints on gas disc sizes in the protoplanetary discs of multiple systems in the Taurus region48
The EXOD search for faint transients in XMM-Newton observations48
Planetesimal and planet formation in transient dust traps48
3D non-LTE Ca II line formation in metal-poor FGK stars48
Euclid preparation48
Abundance analysis of stars hosting gas-rich debris discs48
The SLACS strong lens sample, debiased48
Irradiation-driven escape of primordial planetary atmospheres48
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases47
Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images47
MUSE crowded field 3D spectroscopy in NGC 30047
Probing the galactic cosmic-ray density with current and future γ-ray instruments47
Measuring chemical abundances with infrared nebular lines: HII-CHI-MISTRY-IR47
Sublimation of refractory minerals in the gas envelopes of accreting rocky planets47
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations47
Assessing the accuracy of star formation rate measurements by direct star count in molecular clouds47
An analytical model for dust impact voltage signals and its application to STEREO/WAVES data47
HI-H2 transition: Exploring the role of the magnetic field46
Dynamics of trans-Neptunian objects near the 3/1 mean-motion resonance with Neptune46
Planet formation around intermediate-mass stars46
Testing refracted gravity with the kinematics of galaxy clusters46
eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS246
Detection of J-band photometric periodicity in the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-333846
The SRG/eROSITA All-Sky Survey46
A new way to measure the distance to NGC1052-DF246
The EDGES measurement disfavors an excess radio background during the cosmic dawn46
OGLE-2002-BLG-360: a dusty anomaly among red nova remnants46
Feedback from low-to-moderate-luminosity radio-active galactic nuclei with MaNGA46
SUPER46
Modeling the 2020 November 29 solar energetic particle event using EUHFORIA and iPATH models46
X-ray polarization observations of NGC 2110 with IXPE46
Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing46
Coronal rain formation in a two-fluid approximation46
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