Astronomy & Astrophysics

Papers
(The median citation count of Astronomy & Astrophysics is 4. 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 2022-01-01 to 2026-01-01.)
ArticleCitations
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state3095
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies795
The GAPS Programme at TNG536
Volatile-rich comets ejected early on during Solar System formation407
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)386
Timing and scintillation studies of PSR J1439−5501314
Indications of magnetic accretion in Swift J0826.2−7033295
First detection of metric emission from a solar surge260
Cosmology in the non-linear regime: the small scale miracle258
One Star to Tag Them All (OSTTA)246
Categorization model of moving small-scale intensity enhancements in solar active regions242
Reduction of dust radial drift by turbulence in protoplanetary disks231
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes226
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity222
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy216
Massive pre-main-sequence stars in M17215
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?211
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources201
Stellar halo density with LAMOST K and M giants201
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation199
Improved source classification and performance analysis usingGaiaDR3177
Reconciling concentration to virial mass relations176
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution176
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids174
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system173
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe171
The origin of the soft excess in the luminous quasar HE 1029-1401170
Implications of a turbulent convection model for classical Cepheids168
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs162
Evidence for multiple types of post-starburst galaxies157
Three hot Jupiters transiting K-dwarfs with significant heavy element masses156
Volatile enrichment in low-mass planets as signatures of past planetary disruption154
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1153
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility150
Carina High-contrast Imaging Project for massive Stars (CHIPS)144
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models144
Ammonia characterisation of dense cores in the Rosette Molecular Cloud137
Five methods for determining pattern speeds in galaxies137
Post-Newtonian gravity and Gaia-like astrometry132
Cosmological measurement of the gravitational constant G using the CMB, BAO, and BBN131
Multi-spacecraft observations of near-relativistic electron events at different radial distances129
The supermassive black hole population from seeding via collisions in nuclear star clusters129
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments124
A new way to measure the distance to NGC1052-DF2122
Constraints on asteroid-mass primordial black holes in dwarf galaxies using Hubble Space Telescope photometry118
Spatially resolved spectroscopic analysis of Lyα haloes117
Noble gases neon and argon: A role for the chemical patterns of multiple populations in globular clusters?114
The stable climate of KELT-9b112
Primordial black holes as dark matter candidates111
Euclid110
Changing disc compositions via internal photoevaporation110
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles110
Cosmic rays cannot explain the high ionisation rates in the Galactic centre108
Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star ζ Oph from high-cadence ESPRESSO spectroscopy and TE107
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models107
Scale-invariant vacuum guided resolution of the 7Li BBN problem105
Central kiloparsec region of Andromeda104
Probing star formation and ISM properties using galaxy disk inclination103
Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter102
Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies101
Exploring the intermittency of magnetohydrodynamic turbulence by synchrotron polarization radiation98
[Mg/Fe] ratios in the solar neighbourhood: Stellar yields and chemical evolution scenarios98
Models of quasi-discontinuous solar-wind streams96
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy94
Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing94
eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS293
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph92
JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H2 in the radio galaxy 3C 326 N91
Planetesimal and planet formation in transient dust traps88
Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters87
Carbon envelopes around merging galaxies at z ∼ 4.586
HI-H2 transition: Exploring the role of the magnetic field86
Reconstructing the epoch of reionisation with Planck PR486
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations86
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations85
An idealized general circulation model for the atmospheric circulation on the ice giants85
Unveiling a new extragalactic structure hidden by the Milky Way85
Dynamics of tidal spiral arms: Machine learning-assisted identification of equations and application to the Milky Way83
Propeller effect in action: Unveiling quenched accretion in the transient X-ray pulsar 4U 0115+6383
Systematic evaluation of variability detection methods for eROSITA82
Solar extreme ultraviolet variability as a proxy for nanoflare heating diagnostics82
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries82
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d82
Self-gravity in thin-disc simulations of protoplanetary discs: The smoothing length rectified and generalised to bi-fluids82
Galaxies at the edges: A complete census of the MACS J0416.1–2403 cluster81
Time-resolved spectro-polarimetric analysis of extremely bright GRB 230307A: Possible evidence of evolution from photospheric to synchrotron dominated emission81
Radio outburst from a massive (proto)star81
Calibration and performances of the integrated Mach—Zehnder wavefront sensor for extreme adaptive optics80
Transport of the magnetic flux away from a decaying sunspot via convective motions79
Multi-step reconstruction of radio-interferometric images79
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts79
Negative polarization properties of regolith simulants78
The “C”: The large Chameleon-Musca-Coalsack cloud77
The effect of dynamic temperatures on pebble dynamics and planet formation77
Euclid preparation77
Exploring the Sagittarius stream with RR Lyrae stars from Gaia Data Release 375
Generative modelling of convergence maps based on predicted one-point statistics75
Don’t torque like that74
The Milky Way’s middle-aged inner ring74
iNNterpol: High-precision interpolation of stellar atmospheres with a deep neural network using a 1D convolutional auto encoder for feature extraction74
A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS73
Non-radial oscillations mimicking a brown dwarf orbiting the cluster giant NGC 4349 No. 12773
Probing the physical properties of the intergalactic medium using SRG/eROSITA spectra from blazars73
Selected open cluster sample for validating atmospheric parameters: Application to Gaia and other surveys73
Parameter measurement based on photometric images73
The XXL Survey73
Anatomy of rocky planets formed by rapid pebble accretion72
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies71
CO enhancement by magnetohydrodynamic waves71
Beyond monoculture: Polydisperse moment methods for sub-stellar atmosphere cloud microphysics. II. A three-moment gamma distribution formulation for GCM applications71
M-type (22) Kalliope: A tiny Mercury71
Core to ultracompact HII region evolution in the W49A massive protocluster71
WEAVE-StePS: A stellar population survey using WEAVE at WHT71
Comparing feature sets and machine-learning models for prediction of solar flares71
What drives the corpulence of galaxies?70
Detection of very high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage70
Euclid preparation70
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies69
High-energy interstellar isomers: cis - N -methylformamide in the G+0.693-0.027 molecular cloud69
Ultrasoft state of microquasar Cygnus X-3: X-ray polarimetry reveals the geometry of the astronomical puzzle69
Fitting the light curves of Sagittarius A* with a hot-spot model69
Stochastic excitation of waves in magnetic stars68
High-resolution APEX/LAsMA 12CO and 13CO (3-2) observation of the G333 giant molecular cloud complex68
Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey67
Temperature of quiet Sun small scale brightenings observed by EUI on board Solar Orbiter: Evidence for a cooler component67
Numerical simulations of prominence oscillations triggered by external perturbations67
The EDGES measurement disfavors an excess radio background during the cosmic dawn67
GaiaData Release 366
A low mass, binary-stripped envelope for the Type IIb SN 2024abfo66
Fast-rotating blue straggler stars in the globular cluster NGC 185165
The fate of the progenitors of luminous red novae: Infrared detection of LRNe years after the outburst65
The Arecibo Galaxy Environment Survey (AGES)64
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 202264
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries63
The influence of planetesimal fragmentation on planet formation63
The outflowing ionised gas of I Zw 1 observed by HST COS63
Spinning nano-carbon grains: Viable origin for anomalous microwave emission63
Testing refracted gravity with the kinematics of galaxy clusters63
The SLACS strong lens sample, debiased63
Making the unmodulated pyramid wavefront sensor smart62
The cylindrical jet base of M 87 within 100 μas of the central engine62
The EXOD search for faint transients in XMM-Newton observations62
Survey of Orion Disks with ALMA (SODA)62
Constraining the formation history of the HAT-P-11 system using atmospheric abundances62
Cosmic-ray electron transport in the galaxy M 5161
Euclid preparation61
Identifying multiplets of IceCube alert events61
The spectral energy distributions of very long-period Cepheids in the Milky Way, the Magellanic Clouds, M31, and M3361
MeerKAT view of Hickson Compact Groups61
Exploring non-thermal emission from the star-forming region NGC 3603 through a realistic modelling of its environment61
Dynamics of trans-Neptunian objects near the 3/1 mean-motion resonance with Neptune61
Clustering of magnetic reconnection exhausts in the solar wind: An automated detection study61
Observational constraints on gas disc sizes in the protoplanetary discs of multiple systems in the Taurus region60
Astrometric mass measurement of compact companions in binary systems with Gaia60
Probing the galactic cosmic-ray density with current and future γ-ray instruments60
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence59
Slow-mode rarefaction and compression fronts in the Hermean magnetosphere: From MESSENGER insights to future BepiColombo observations59
Rotational equilibrium of C2 in diffuse interstellar clouds59
zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks59
MUSE crowded field 3D spectroscopy in NGC 30059
Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter59
Detection of a new sample of Galactic white dwarfs in the direction of the Small Magellanic Cloud58
Simulating the LOcal Web (SLOW)58
Euclidpreparation58
X-ray polarization observations of NGC 2110 with IXPE58
Gas-phase reaction of fullerene monocations with 2,3-benzofluorene indicates the importance of charge exchanges58
Plasma dynamics in the flaring loop observed by RHESSI58
The Snake filament: A study of polarization and kinematics58
Predicting the surface age of chondritic S-type asteroids using the space weathering features in reflectance spectra: Small data machine learning58
Simulation of CH3OH ice UV photolysis under laboratory conditions58
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field58
Assessing the accuracy of star formation rate measurements by direct star count in molecular clouds57
The first spatio-spectral Bayesian imaging of SN1006 in X-rays57
Quantifying observational projection effects with a simulation-based hot CGM model57
The SPAr burning: Proton captures powering carbon–oxygen shell mergers in massive stars57
Doppler shifts of spectral lines formed in the solar transition region and corona57
Machine learning the gap between real and simulated nebulae57
SPICE connection mosaics to link the Sun’s surface and the heliosphere56
Very massive star models56
Bayesian test of Brans–Dicke theories with planetary ephemerides: Investigating the strong equivalence principle56
A catalogue of low-mass X-ray binaries in the Galaxy: From the INTEGRAL to the Gaia era56
Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS56
Bayesian inference of three-dimensional gas maps56
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)55
Peculiar X-ray transient SRGA J043520.9+552226/AT2019wey discovered with SRG/ART-XC55
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail55
An analytical model for dust impact voltage signals and its application to STEREO/WAVES data55
MOCKA – A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators55
Kinematic properties of white dwarfs55
Standardizing the gamma-ray burst as a standard candle and applying it to cosmological probes: Constraints on the two-component dark energy model55
Chromospherically active stars: Lithium and CNO abundances in northern RS CVn stars54
ISPY: NACO Imaging Survey for Planets around Young stars54
Evolutionary tracks of binary neutron star progenitors across cosmic times54
The PAU Survey: The quasar Lyα and UV luminosity functions at 2.7 < z < 5.354
A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies54
Discovery of a strong rotation of the X-ray polarization angle in the galactic burster GX 13+154
The GALAH survey: Improving chemical abundances using star clusters54
Detection of J -band photometric periodicity in the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-333853
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission53
A solar rotation signature in cosmic dust observed in STEREO spacecraft data53
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases53
X-ray pulsar GRO J1008−57 as an orthogonal rotator53
Exploring the origins of mega radio halos53
The jet and circumstellar environment of the young binary DF Tau53
Ultracool dwarfs identified using spectra in LAMOST DR752
Asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia52
SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host52
Emission and absorption lines in the photospheric radius expansion bursts of 4U 1820–3052
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD52
A nuclear spiral in a dusty star-forming galaxy at z = 2.7852
Cosmic ray interactions with indene and adamantane seeded water ice mantles52
Cataclysmic variables and the disc instability model in the Gaia DR3 colour–magnitude diagram52
OGLE-2002-BLG-360: A dusty anomaly among red nova remnants52
A comprehensive radio study of narrow-line Seyfert 1 galaxies52
Tracking active nests in solar-type pulsators: Ensemble starspot modelling of Kepler asteroseismic targets51
A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies51
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole51
A phase-resolvedFermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere51
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy51
LIME: A LIne MEasuring library for large and complex spectroscopic data sets51
A highly dynamic small-scale jet in a polar coronal hole51
Dynamical modelling and the origin of gas turbulence in z ∼ 4.5 galaxies51
Dust-driven wind as a model of broad absorption line quasars51
Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk51
The behaviour of eccentric sub-pc massive black hole binaries embedded in massive discs50
STEPARSYN: A Bayesian code to infer stellar atmospheric parameters using spectral synthesis50
Discovery of the luminous X-ray ignition eRASSt J234402.9−35264050
The Mantis Network50
Multiple short-term cycles in star KIC 6876668 Kepler50
LOFAR high-band antenna observations of the Perseus cluster50
The origin of B-type runaway stars based on kinematics50
Bi-directional reflectance, polarization, and spectroscopic measurements of the Chang’e-5 regolith sample50
The MALATANG survey: Star formation, dense gas, and active galactic nucleus feedback in NGC 106850
Probing the interstellar medium of the quasar BRI 0952−011550
Edge-On Disk Study (EODS)50
The Disc Miner49
H2–H2O demixing in Uranus and Neptune: Adiabatic structure models49
TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE49
Link between star formation and the properties of supermassive black holes49
On-sky validation of image-based adaptive optics wavefront sensor referencing49
Planet formation around intermediate-mass stars49
Asymptotic giant branch stars in the eROSITA-DE eRASS1 catalog49
Sub-stellar engulfment by a main-sequence star: Where is the lithium?49
Physical properties of the Didymos system before and after the DART impact48
Atmospheric characterization of the ultra-hot Jupiter WASP-33b48
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data48
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf48
JWST reveals a supernova following a gamma-ray burst at z ≃ 7.348
Challenging historical novae: AT Cnc (1645), Te-11 (483), and M22 (BC 48) revisited48
Instabilities at recollimation shocks in magnetohydrodynamic jets48
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