Astronomy & Astrophysics

Papers
(The median citation count of Astronomy & Astrophysics is 3. 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 2021-05-01 to 2025-05-01.)
ArticleCitations
Mid-infrared spectra of T Tauri disks: Modeling the effects of a small inner cavity on CO2 and H2O emission2111
Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus (Corrigendum)1110
Indications of magnetic accretion in Swift J0826.2−7033580
First detection of metric emission from a solar surge419
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data372
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)317
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models291
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA252
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts251
Cosmology in the non-linear regime: the small scale miracle214
One Star to Tag Them All (OSTTA)206
Generative models of astrophysical fields with scattering transforms on the sphere181
Categorization model of moving small-scale intensity enhancements in solar active regions171
Solar extreme ultraviolet variability as a proxy for nanoflare heating diagnostics171
The “C”: The large Chameleon-Musca-Coalsack cloud168
Barred active galactic nucleus galaxies in paired systems: Exploring the impact on nuclear activity165
Reduction of dust radial drift by turbulence in protoplanetary disks165
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state164
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies160
The GAPS Programme at TNG158
Transient obscuration event captured in NGC 3227152
Volatile-rich comets ejected early on during Solar System formation151
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies151
From eruption to post-flare rain: A 2.5D MHD model147
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)143
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves142
Atmospheric characterization of the ultra-hot Jupiter WASP-33b135
Transport of the magnetic flux away from a decaying sunspot via convective motions135
Self-gravity in thin-disc simulations of protoplanetary discs: The smoothing length rectified and generalised to bi-fluids132
Successive deuteration in low-mass star-forming regions: The case of D2-methanol (CHD2OH) in IRAS 16293-2422132
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD130
The SRG/eROSITA All-Sky Survey129
Timing and scintillation studies of PSR J1439−5501126
Slow-mode rarefaction and compression fronts in the Hermean magnetosphere: From MESSENGER insights to future BepiColombo observations125
Tracking active nests in solar-type pulsators: Ensemble starspot modelling of Kepler asteroseismic targets124
Optical emission lines in the most massive galaxies: Morphology, kinematics, and ionisation properties123
Models of quasi-discontinuous solar-wind streams123
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission121
STEPARSYN: A Bayesian code to infer stellar atmospheric parameters using spectral synthesis117
The LOFAR LBA Sky Survey: Deep Fields116
The first GeV flare of the radio-loud narrow-line Seyfert 1 galaxy PKS 2004–447115
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field115
Evidence for stellar contamination in the transmission spectra of HAT-P-12b115
Shaping physical properties of galaxy subtypes in the VIPERS survey: Environment matters113
Properties of the ionisation glitch112
HI-H2 transition: Exploring the role of the magnetic field110
A highly dynamic small-scale jet in a polar coronal hole110
Exploring the radial evolution of interplanetary coronal mass ejections using EUHFORIA109
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz109
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 2022109
The MUSE-Faint survey106
Stellar halo density with LAMOST K and M giants105
Algebraic quantification of an active region contribution to the solar cycle103
Peculiar X-ray transient SRGA J043520.9+552226/AT2019wey discovered with SRG/ART-XC102
Clustered star formation toward Berkeley 87/ON2101
Launching the asymmetric bipolar jet of DO Tau99
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole97
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources97
Applicability of Taylor’s hypothesis during Parker Solar Probe perihelia97
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation95
Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey95
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST94
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility93
The stable climate of KELT-9b91
An analytical model for dust impact voltage signals and its application to STEREO/WAVES data91
Dark matter capture and annihilation in stars: Impact on the red giant branch tip90
Magnetic increases with central current sheets: observations with Parker Solar Probe90
SPICE connection mosaics to link the Sun’s surface and the heliosphere89
Improved source classification and performance analysis usingGaiaDR387
The PAU Survey: The quasar Lyα and UV luminosity functions at 2.7 < z < 5.386
Plasma dynamics in the flaring loop observed by RHESSI86
3He-rich solar energetic particle events observed on the first perihelion pass of Solar Orbiter86
Simulation of CH3OH ice UV photolysis under laboratory conditions86
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models85
Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images85
The XXL Survey85
Systematic evaluation of variability detection methods for eROSITA84
Gamma-ray line emission from the Local Bubble83
MUSE crowded field 3D spectroscopy in NGC 30083
Detection of iron emission lines and a temperature inversion on the dayside of the ultra-hot Jupiter KELT-20b82
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY79
LIME: A LIne MEasuring library for large and complex spectroscopic data sets78
Changing disc compositions via internal photoevaporation77
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars77
Massive pre-main-sequence stars in M1777
Simulating the LOcal Web (SLOW)76
Ultrasoft state of microquasar Cygnus X-3: X-ray polarimetry reveals the geometry of the astronomical puzzle76
A solar rotation signature in cosmic dust observed in STEREO spacecraft data75
The effect of dynamic temperatures on pebble dynamics and planet formation74
Solar flares in the Solar Orbiter era: Short-exposure EUI/FSI observations of STIX flares74
Stochastic excitation of waves in magnetic stars74
Properties of intermediate- to high-mass stars in the young cluster M1773
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?72
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d72
Transient classifiers for Fink72
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution72
Reconciling concentration to virial mass relations70
iNNterpol: High-precision interpolation of stellar atmospheres with a deep neural network using a 1D convolutional auto encoder for feature extraction70
Multi-step reconstruction of radio-interferometric images69
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids69
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system69
Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies69
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data68
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries68
The shape of dark matter halos: A new fundamental cosmological invariance68
Probing the interstellar medium of the quasar BRI 0952−011568
Asymptotic giant branch stars in the eROSITA-DE eRASS1 catalog67
The ANTARESS workflow67
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes67
The first spatio-spectral Bayesian imaging of SN1006 in X-rays67
Non-radial oscillations mimicking a brown dwarf orbiting the cluster giant NGC 4349 No. 12767
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity66
A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS66
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles65
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy65
Life cycle of cosmic-ray electrons in the intracluster medium65
Ultracool dwarfs identified using spectra in LAMOST DR764
Unveiling a new extragalactic structure hidden by the Milky Way63
eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS263
Dynamics of nanodust in the vicinity of a stellar corona: Effect of plasma corotation63
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence63
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies62
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail62
Discovery of the luminous X-ray ignition eRASSt J234402.9−35264062
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe62
The origin of the soft excess in the luminous quasar HE 1029-140162
The Gravitational Wave Universe Toolbox61
Negative polarization properties of regolith simulants61
Non-linear dynamics of the minimal theory of massive gravity60
Probing the galactic cosmic-ray density with current and future γ-ray instruments60
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments59
Radio outburst from a massive (proto)star59
Multi-spacecraft observations of near-relativistic electron events at different radial distances59
Detection of very high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage58
Backstreaming ions at a high Mach number interplanetary shock58
Ammonia characterisation of dense cores in the Rosette Molecular Cloud58
The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model57
Carina High-contrast Imaging Project for massive Stars (CHIPS)57
The jet collimation profile at high resolution in BL Lacertae57
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf57
Constraining the intrinsic population of long gamma-ray bursts: Implications for spectral correlations, cosmic evolution, and their use as tracers of star formation57
Cosmic rays cannot explain the high ionisation rates in the Galactic centre56
Probing the physical properties of the intergalactic medium using SRG/eROSITA spectra from blazars56
M-type (22) Kalliope: A tiny Mercury56
Exploring the origins of mega radio halos56
Parameter measurement based on photometric images56
Modelling chemical clocks56
A nuclear spiral in a dusty star-forming galaxy at z = 2.7856
Black hole accretion and radiation variability in general relativistic magnetohydrodynamic simulations with Rezzolla–Zhidenko spacetime56
Ammonia snow lines and ammonium salts desorption56
The kinematics of 30 Milky Way globular clusters and the multiple stellar populations within56
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey56
Machine learning the gap between real and simulated nebulae56
Link between star formation and the properties of supermassive black holes56
Exploring the intermittency of magnetohydrodynamic turbulence by synchrotron polarization radiation56
The Milky Way’s middle-aged inner ring55
Euclid preparation55
ISPY: NACO Imaging Survey for Planets around Young stars55
Dynamical modelling and the origin of gas turbulence in z ∼ 4.5 galaxies55
The supermassive black hole population from seeding via collisions in nuclear star clusters54
Velocity measurement in the extensive [OIII] emission region 1.2° south-east of M 3154
Gas-phase reaction of fullerene monocations with 2,3-benzofluorene indicates the importance of charge exchanges54
Probing star formation and ISM properties using galaxy disk inclination54
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs54
Evolutionary tracks of binary neutron star progenitors across cosmic times54
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-154
[Mg/Fe] ratios in the solar neighbourhood: Stellar yields and chemical evolution scenarios53
Revisiting the tension between fast bars and the ΛCDM paradigm53
Galaxy populations in the most distant SPT-SZ clusters53
Standard solar models: Perspectives from updated solar neutrino fluxes and gravity-mode period spacing53
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations53
Age of (152830) Dinkinesh I Selam constrained by secular tidal-BYORP theory52
Carbon envelopes around merging galaxies at z ∼ 4.552
Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line52
JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H2 in the radio galaxy 3C 326 N52
Five methods for determining pattern speeds in galaxies52
Double red giant branch and red clump features of Galactic disc stellar populations with Gaia GSP-Spec52
Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations52
χ1 Fornacis cluster DANCe52
Doppler shifts of spectral lines formed in the solar transition region and corona52
Central kiloparsec region of Andromeda52
Simulations of radio-wave anisotropic scattering to interpret type III radio burst data from Solar Orbiter, Parker Solar Probe, STEREO, and Wind52
Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes51
The origin of X-ray emission in 3CRR sources: Hints from mid-infrared Spitzer observations51
Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z  ∼  351
Catalogue of exoplanets accessible in reflected starlight to theNancy Grace RomanSpace Telescope51
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy51
N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift?51
Emission and absorption lines in the photospheric radius expansion bursts of 4U 1820–3050
H2–H2O demixing in Uranus and Neptune: Adiabatic structure models50
The outflowing ionised gas of I Zw 1 observed by HST COS50
Cosmic-ray electron transport in the galaxy M 5150
Magnetic helicity and energy budget around large confined and eruptive solar flares50
WEAVE-StePS: A stellar population survey using WEAVE at WHT50
Clumpy star formation and an obscured nuclear starburst in the luminous dusty z = 4 galaxy GN20 seen by MIRI/JWST50
The Arecibo Galaxy Environment Survey (AGES)50
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries50
Bayesian inference of three-dimensional gas maps50
Asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia50
Kinetic electrostatic waves and their association with current structures in the solar wind49
The behaviour of eccentric sub-pc massive black hole binaries embedded in massive discs49
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph49
GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisation49
Number of stars in the Sun’s birth cluster revisited49
The EXOD search for faint transients in XMM-Newton observations. Part II49
The influence of planetesimal fragmentation on planet formation49
Constraining the formation history of the HAT-P-11 system using atmospheric abundances49
Jupiter’s “cold” formation in the protosolar disk shadow49
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations49
Euclid preparation49
Planetesimal and planet formation in transient dust traps49
The cylindrical jet base of M 87 within 100 μas of the central engine48
Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters48
The SLACS strong lens sample, debiased. II. Lensing-only constraints on the stellar initial mass function and dark matter contraction in early-type galaxies48
Testing the magnetic flux paradigm for AGN radio loudness with a radio-intermediate quasar48
Making the unmodulated pyramid wavefront sensor smart48
Core to ultracompact HII region evolution in the W49A massive protocluster48
Quantifying Observational Projection Effects with a Simulation-based hot CGM model48
Survey of Orion Disks with ALMA (SODA)48
CO enhancement by magnetohydrodynamic waves48
An effective model for magnetic field amplification by the magnetorotational and parasitic instabilities48
Spinning nano-carbon grains: Viable origin for anomalous microwave emission48
A state-of-the-art strong-lensing model of MACS J0416.1−2403 with the largest sample of spectroscopic multiple images48
A new way to measure the distance to NGC1052-DF248
What drives the corpulence of galaxies?47
Sub-stellar engulfment by a main-sequence star: Where is the lithium?47
Submillimeter imaging of the Galactic Center starburst Sgr B247
HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars47
Simulating observable structures due to a perturbed interstellar medium in front of astrospheric bow shocks in 3D MHD47
A phase-resolvedFermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere47
Temperature of quiet Sun small scale brightenings observed by EUI on board Solar Orbiter: Evidence for a cooler component47
TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE47
Strong lensing in UNIONS: Toward a pipeline from discovery to modeling47
The longevity of the oldest open clusters47
Physical properties of the Didymos system before and after the DART impact46
Abundance analysis of stars hosting gas-rich debris discs46
The near-Sun streamer belt solar wind: turbulence and solar wind acceleration46
Tracing the Galactic disk with planetary nebulae using Gaia DR346
First look with JWST spectroscopy: Resemblance among z ∼ 8 galaxies and local analogs46
On-sky validation of image-based adaptive optics wavefront sensor referencing46
Bayesian test of Brans–Dicke theories with planetary ephemerides: Investigating the strong equivalence principle46
Post-Newtonian gravity and Gaia-like astrometry46
3D non-LTE Ca II line formation in metal-poor FGK stars. I. Abundance corrections, radial velocity corrections, and synthetic spectra46
A3COSMOS: Measuring the cosmic dust-attenuated star formation rate density at 4 < z < 546
Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS46
Theoretical computations on the efficiency of acetaldehyde formation on interstellar icy grains45
ASTRAEUS45
Supermassive Black Hole Winds in X-rays: SUBWAYS45
A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies45
Numerical simulations of prominence oscillations triggered by external perturbations45
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