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 2021-06-01 to 2025-06-01.)
ArticleCitations
Mid-infrared spectra of T Tauri disks: Modeling the effects of a small inner cavity on CO2 and H2O emission2222
Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus (Corrigendum)1147
Indications of magnetic accretion in Swift J0826.2−7033610
First detection of metric emission from a solar surge431
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)395
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA324
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts305
Cosmology in the non-linear regime: the small scale miracle259
One Star to Tag Them All (OSTTA)258
Generative models of astrophysical fields with scattering transforms on the sphere218
Categorization model of moving small-scale intensity enhancements in solar active regions194
The “C”: The large Chameleon-Musca-Coalsack cloud176
Reduction of dust radial drift by turbulence in protoplanetary disks175
Barred active galactic nucleus galaxies in paired systems: Exploring the impact on nuclear activity174
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state170
The GAPS Programme at TNG166
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies166
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies165
From eruption to post-flare rain: A 2.5D MHD model160
Volatile-rich comets ejected early on during Solar System formation160
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)158
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves153
Transport of the magnetic flux away from a decaying sunspot via convective motions150
Successive deuteration in low-mass star-forming regions: The case of D2-methanol (CHD2OH) in IRAS 16293-2422144
Slow-mode rarefaction and compression fronts in the Hermean magnetosphere: From MESSENGER insights to future BepiColombo observations140
Timing and scintillation studies of PSR J1439−5501140
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD140
Models of quasi-discontinuous solar-wind streams135
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission133
The LOFAR LBA Sky Survey: Deep Fields132
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field131
Evidence for stellar contamination in the transmission spectra of HAT-P-12b131
Properties of the ionisation glitch130
A highly dynamic small-scale jet in a polar coronal hole125
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz124
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 2022123
The MUSE-Faint survey121
Stellar halo density with LAMOST K and M giants120
Applicability of Taylor’s hypothesis during Parker Solar Probe perihelia119
Launching the asymmetric bipolar jet of DO Tau119
Clustered star formation toward Berkeley 87/ON2119
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole116
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources116
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation113
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST112
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility112
An analytical model for dust impact voltage signals and its application to STEREO/WAVES data110
The stable climate of KELT-9b108
Magnetic increases with central current sheets: observations with Parker Solar Probe107
Dark matter capture and annihilation in stars: Impact on the red giant branch tip105
Improved source classification and performance analysis usingGaiaDR3104
SPICE connection mosaics to link the Sun’s surface and the heliosphere104
Plasma dynamics in the flaring loop observed by RHESSI103
Simulation of CH3OH ice UV photolysis under laboratory conditions101
The PAU Survey: The quasar Lyα and UV luminosity functions at 2.7 < z < 5.3100
3He-rich solar energetic particle events observed on the first perihelion pass of Solar Orbiter100
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models99
Systematic evaluation of variability detection methods for eROSITA98
MUSE crowded field 3D spectroscopy in NGC 30097
Detection of iron emission lines and a temperature inversion on the dayside of the ultra-hot Jupiter KELT-20b96
Gamma-ray line emission from the Local Bubble96
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY93
Changing disc compositions via internal photoevaporation93
LIME: A LIne MEasuring library for large and complex spectroscopic data sets93
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars92
A solar rotation signature in cosmic dust observed in STEREO spacecraft data90
Massive pre-main-sequence stars in M1790
The effect of dynamic temperatures on pebble dynamics and planet formation90
Solar flares in the Solar Orbiter era: Short-exposure EUI/FSI observations of STIX flares89
Transient classifiers for Fink87
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution87
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?87
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d86
Reconciling concentration to virial mass relations86
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids85
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system84
Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies84
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries83
Probing the interstellar medium of the quasar BRI 0952−011581
The shape of dark matter halos: A new fundamental cosmological invariance80
The ANTARESS workflow78
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data78
The first spatio-spectral Bayesian imaging of SN1006 in X-rays77
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes76
Asymptotic giant branch stars in the eROSITA-DE eRASS1 catalog76
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity76
A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS75
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy74
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles74
Ultracool dwarfs identified using spectra in LAMOST DR774
Life cycle of cosmic-ray electrons in the intracluster medium74
Dynamics of nanodust in the vicinity of a stellar corona: Effect of plasma corotation73
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence73
Unveiling a new extragalactic structure hidden by the Milky Way72
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies70
The origin of the soft excess in the luminous quasar HE 1029-140170
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail69
Probing the galactic cosmic-ray density with current and future γ-ray instruments69
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe69
Non-linear dynamics of the minimal theory of massive gravity69
Radio outburst from a massive (proto)star68
Ammonia characterisation of dense cores in the Rosette Molecular Cloud68
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments68
Carina High-contrast Imaging Project for massive Stars (CHIPS)67
Backstreaming ions at a high Mach number interplanetary shock67
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf67
The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model67
Probing the physical properties of the intergalactic medium using SRG/eROSITA spectra from blazars66
The kinematics of 30 Milky Way globular clusters and the multiple stellar populations within66
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey66
Cosmic rays cannot explain the high ionisation rates in the Galactic centre66
Link between star formation and the properties of supermassive black holes65
Parameter measurement based on photometric images65
Black hole accretion and radiation variability in general relativistic magnetohydrodynamic simulations with Rezzolla–Zhidenko spacetime65
Modelling chemical clocks65
Ammonia snow lines and ammonium salts desorption64
Exploring the origins of mega radio halos64
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs63
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-163
Velocity measurement in the extensive [OIII] emission region 1.2° south-east of M 3163
Standard solar models: Perspectives from updated solar neutrino fluxes and gravity-mode period spacing62
Probing star formation and ISM properties using galaxy disk inclination62
Evolutionary tracks of binary neutron star progenitors across cosmic times62
The supermassive black hole population from seeding via collisions in nuclear star clusters62
Galaxy populations in the most distant SPT-SZ clusters61
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations60
JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H2 in the radio galaxy 3C 326 N60
Central kiloparsec region of Andromeda60
χ1 Fornacis cluster DANCe60
Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations60
Age of (152830) Dinkinesh I Selam constrained by secular tidal-BYORP theory59
Doppler shifts of spectral lines formed in the solar transition region and corona59
Carbon envelopes around merging galaxies at z ∼ 4.559
Double red giant branch and red clump features of Galactic disc stellar populations with Gaia GSP-Spec59
The origin of X-ray emission in 3CRR sources: Hints from mid-infrared Spitzer observations58
Emission and absorption lines in the photospheric radius expansion bursts of 4U 1820–3058
H2–H2O demixing in Uranus and Neptune: Adiabatic structure models58
Kinetic electrostatic waves and their association with current structures in the solar wind58
The Arecibo Galaxy Environment Survey (AGES)58
Bayesian inference of three-dimensional gas maps58
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries58
The outflowing ionised gas of I Zw 1 observed by HST COS58
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy58
Clumpy star formation and an obscured nuclear starburst in the luminous dusty z = 4 galaxy GN20 seen by MIRI/JWST58
Jupiter’s “cold” formation in the protosolar disk shadow58
Making the unmodulated pyramid wavefront sensor smart57
Euclid preparation57
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph57
The influence of planetesimal fragmentation on planet formation57
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations57
An effective model for magnetic field amplification by the magnetorotational and parasitic instabilities57
Constraining the formation history of the HAT-P-11 system using atmospheric abundances57
Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters56
The cylindrical jet base of M 87 within 100 μas of the central engine56
Spinning nano-carbon grains: Viable origin for anomalous microwave emission56
Core to ultracompact HII region evolution in the W49A massive protocluster56
Sub-stellar engulfment by a main-sequence star: Where is the lithium?55
Survey of Orion Disks with ALMA (SODA)55
Strong lensing in UNIONS: Toward a pipeline from discovery to modeling55
Testing the magnetic flux paradigm for AGN radio loudness with a radio-intermediate quasar55
Simulating observable structures due to a perturbed interstellar medium in front of astrospheric bow shocks in 3D MHD55
A phase-resolvedFermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere54
Physical properties of the Didymos system before and after the DART impact54
What drives the corpulence of galaxies?54
CAPOS: The bulge Cluster APOgee Survey53
Post-Newtonian gravity and Gaia-like astrometry53
Tracing the Galactic disk with planetary nebulae using Gaia DR353
Kinematic properties of white dwarfs53
The near-Sun streamer belt solar wind: turbulence and solar wind acceleration53
Exploring self-consistent 2.5D flare simulations with MPI-AMRVAC53
Forming Planets Around Stars With Non-Solar Elemental Composition53
On-sky validation of image-based adaptive optics wavefront sensor referencing53
Bayesian test of Brans–Dicke theories with planetary ephemerides: Investigating the strong equivalence principle53
Detection of a new sample of Galactic white dwarfs in the direction of the Small Magellanic Cloud53
A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies52
Standardizing the gamma-ray burst as a standard candle and applying it to cosmological probes: Constraints on the two-component dark energy model52
Hydrogenated atmospheres of lava planets: Atmospheric structure and emission spectra52
Numerical simulations of prominence oscillations triggered by external perturbations52
Probing quadratic gravity with the Event Horizon Telescope52
Astrometric mass measurement of compact companions in binary systems with Gaia52
MeerKAT view of Hickson Compact Groups52
MOCKA – A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators51
Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk51
Identifying multiplets of IceCube alert events51
Cyano radical emission at small spatial scales towards massive protostars51
Dust-driven wind as a model of broad absorption line quasars51
A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies51
The preferential orientation of magnetic switchbacks and its implications for solar magnetic flux transport51
Clustering of magnetic reconnection exhausts in the solar wind: An automated detection study51
Assessing the accuracy of star formation rate measurements by direct star count in molecular clouds50
Very massive star models50
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA)50
JWST MIRI reveals the diversity of nuclear mid-infrared spectra of nearby type 2 quasars50
Spatially resolved spectroscopic analysis of Lyα haloes50
Euclid: Searches for strong gravitational lenses using convolutional neural nets in Early Release Observations of the Perseus field50
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases50
Cataclysmic variables and the disc instability model in the Gaia DR3 colour–magnitude diagram50
Measuring chemical abundances with infrared nebular lines: HII-CHI-MISTRY-IR50
Observational constraints on gas disc sizes in the protoplanetary discs of multiple systems in the Taurus region50
Feedback from low-to-moderate-luminosity radio-active galactic nuclei with MaNGA50
Euclid50
Observability of evaporating lava worlds49
Multi-spacecraft observations of near-relativistic electron events at different radial distances49
Euclid preparation49
Multi-step reconstruction of radio-interferometric images49
Number of stars in the Sun’s birth cluster revisited49
Sublimation of refractory minerals in the gas envelopes of accreting rocky planets49
zELDA. II. Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks49
Testing refracted gravity with the kinematics of galaxy clusters49
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy49
Periodicities in an active region correlated with Type III radio bursts observed by Parker Solar Probe49
Abundance analysis of stars hosting gas-rich debris discs48
WEAVE-StePS: A stellar population survey using WEAVE at WHT48
Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS48
The EDGES measurement disfavors an excess radio background during the cosmic dawn48
The jet and circumstellar environment of the young binary DF Tau48
The SLACS strong lens sample, debiased48
Cosmological measurement of the gravitational constant G using the CMB, BAO, and BBN48
Asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia48
3D non-LTE Ca II line formation in metal-poor FGK stars48
Algebraic quantification of an active region contribution to the solar cycle48
Coronal rain formation in a two-fluid approximation47
STEPARSYN: A Bayesian code to infer stellar atmospheric parameters using spectral synthesis47
Comparing feature sets and machine-learning models for prediction of solar flares47
Planetesimal and planet formation in transient dust traps47
The EXOD search for faint transients in XMM-Newton observations47
HI-H2 transition: Exploring the role of the magnetic field47
Cosmic-ray electron transport in the galaxy M 5147
M-type (22) Kalliope: A tiny Mercury47
Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing47
12C/13C ratio and CNO abundances in the classical very old metal-poor dwarf HD 14028347
N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift?47
Planet formation around intermediate-mass stars47
Dynamics of trans-Neptunian objects near the 3/1 mean-motion resonance with Neptune46
The longevity of the oldest open clusters46
Contribution of polycyclic aromatic hydrocarbon ionization to neutral gas heating in galaxies: model versus observations46
FAUST46
Supermassive Black Hole Winds in X-rays: SUBWAYS46
Fitting the light curves of Sagittarius A* with a hot-spot model46
SUPER46
The Gravitational Wave Universe Toolbox46
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data46
Gas-phase reaction of fullerene monocations with 2,3-benzofluorene indicates the importance of charge exchanges46
Shaping physical properties of galaxy subtypes in the VIPERS survey: Environment matters46
Irradiation-driven escape of primordial planetary atmospheres45
A state-of-the-art strong-lensing model of MACS J0416.1−2403 with the largest sample of spectroscopic multiple images45
Transient obscuration event captured in NGC 322745
Discovery of the luminous X-ray ignition eRASSt J234402.9−35264045
The SRG/eROSITA All-Sky Survey45
HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars45
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