Astronomy & Astrophysics

Papers
(The H4-Index of Astronomy & Astrophysics is 76. 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 2021-02-01 to 2025-02-01.)
ArticleCitations
Turnaround density evolution encodes cosmology in simulations2866
Rainy downdrafts in abyssal atmospheres1636
Shape models and spin states of Jupiter Trojans894
Analysis of the first coronagraphic multi-band observations of a sungrazing comet787
J-PLUS: The star formation main sequence and rate density at d  ≲  75 Mpc633
Detection of minute-timescale γ-ray variability in BL Lacertae by Fermi-LAT595
LHAASO J2226+6057 as a pulsar wind nebula487
Host galaxy and orientation differences between different AGN types474
Identification of late-type Class I stars using Gaia DR3 Apsis parameters389
Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars353
Vibrationally excited HCN transitions in circumstellar envelopes of carbon-rich AGB stars288
Polarization signatures of a high-velocity scatterer in nebular-phase spectra of Type II supernovae271
Magnetic and thermal acceleration in extragalactic jets251
Accelerated particle beams in a 3D simulation of the quiet Sun226
The first molecules in the intergalactic medium and halos of the Dark Ages and Cosmic Dawn225
Distribution of ionized, atomic, and PDR gas around S 1 in ρ Ophiuchus212
Sublimation origin of active asteroid P/2018 P3202
The miniJPAS survey: Maximising the photo-z accuracy from multi-survey datasets with probability conflation193
Exploring the dynamics of collisionless spherical stellar systems using the matrix method: Insights from the dilation mode155
How many suns are in the sky? A SPHERE multiplicity survey of exoplanet host stars154
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence152
The eccentric millisecond pulsar, PSR J0955−6150147
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state143
Photodynamical analysis of the nearly resonant planetary system WASP-148142
CRIRES-POP: A library of high resolution spectra in the near-infrared137
Parker Solar Probe observations of collisional effects on thermalizing the young solar wind128
Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernova126
FAUST124
New ex-OH maser detections in the northern celestial hemisphere124
SoloHI observations of coronal mass ejections observed by multiple spacecraft123
Follow-up of non-transiting planets detected by Kepler121
No detection of SO2, H2S, or OCS in the atmosphere of Mars from the first two Martian years of observations from TGO/ACS119
Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter118
Towards a fully consistent Milky Way disk model117
Hypervelocity star candidates from Gaia DR2 and DR3 proper motions and parallaxes117
The Arecibo Galaxy Environment Survey (AGES)114
The SEDIGISM survey: Molecular cloud morphology113
Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues112
Probing core overshooting using subgiant asteroseismology: The case of KIC10273246 (Corrigendum)109
The LOFAR Two Meter Sky Survey106
X-ray supernova remnants in the starburst region of M 82105
Retrieving the three-dimensional matter power spectrum and galaxy biasing parameters from lensing tomography (Corrigendum)104
Sapaki: Galactic O3If* star possibly born in isolation104
The nature of medium-period variables on the extreme horizontal branch103
REsolved ALMA and SMA Observations of Nearby Stars (REASONS)102
Gaia vbroad: Spectral-line broadening and binarity101
Mapping the spatial extent of H I-rich absorbers using Mg II absorption along gravitational arcs101
Non-local thermodynamic equilibrium (NLTE) abundances of europium (Eu) for a sample of metal-poor stars in the galactic halo and metal-poor disk with 1D and 〈3D〉 models100
ALMA observations of CO isotopologues towards six obscured post-asymptotic giant branch stars95
Planetary nebulae of the Large Magellanic Cloud II. The connection with the progenitors' properties95
Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys95
Continuous evolution of the polarization properties in the transient X-ray pulsar RX J0440.9+4431/LS V +44 1795
A nuclear spiral in a dusty star-forming galaxy at z = 2.7894
Unified multiwavelength data analysis workflow with gammapy93
Approaching ballistic motion in 3D simulations of gamma-ray burst jets in realistic binary neutron star merger environments92
A numerical study of unusual flux decreases for cosmic ray protons and electrons observed by Alpha Magnetic Spectrometer in 201792
Eclipse-mapping study of the eclipsing binary KIC 3858884 with a hybrid δ Sct/γ Dor component91
The polarisation behaviour of OJ 287 viewed through radio, millimetre, and optical observations between 2015 and 201791
Turbulent pressure support in galaxy clusters90
Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies89
Multiband embeddings of light curves89
Blue monsters at z>10: where all their dust has gone89
Euclid preparation89
Dust evolution by chemisputtering during protostellar formation88
A BCool survey of stellar magnetic cycles86
Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses86
Parameter measurement based on photometric images I: The method and the gas-phase metallicity of spiral galaxies85
Temperature and density profiles in the corona of main-sequence stars induced by stochastic heating in the chromosphere85
A Bond albedo map of Europa84
Frozen and β-equilibrated f and p modes of cold neutron stars: Nuclear metamodel predictions83
Radial evolution of interplanetary coronal mass ejection-associated particle acceleration observed by Solar Orbiter and ACE82
The ViCTORIA project81
Interaction between the supernova remnant W44 and the infrared dark cloud G034.77-00.55: Shock induced star formation80
Eppur si muove: Evidence of disc precession or a sub-milliparsec SMBH binary in the QPE-emitting galaxy GSN 06978
Time-integrated polarizations in the prompt phase of gamma-ray bursts via the multi-window interpretation76
Machine learning the gap between real and simulated nebulae. A domain-adaptation approach to classify ionised nebulae in nearby galaxies76
Modelling chemical clocks. Theoretical evidences of the space and time evolution of [s/α] in the Galactic disc with Gaia-ESO survey76
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