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 2021-11-01 to 2025-11-01.)
ArticleCitations
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state2823
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies746
The GAPS Programme at TNG484
Volatile-rich comets ejected early on during Solar System formation380
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)368
Timing and scintillation studies of PSR J1439−5501301
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission285
The LOFAR LBA Sky Survey: Deep Fields283
Properties of the ionisation glitch234
Indications of magnetic accretion in Swift J0826.2−7033228
First detection of metric emission from a solar surge222
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA208
One Star to Tag Them All (OSTTA)206
Cosmology in the non-linear regime: the small scale miracle206
Categorization model of moving small-scale intensity enhancements in solar active regions204
Reduction of dust radial drift by turbulence in protoplanetary disks201
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes198
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy196
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity196
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars189
Massive pre-main-sequence stars in M17186
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?182
Stellar halo density with LAMOST K and M giants165
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation162
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole162
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources162
Improved source classification and performance analysis usingGaiaDR3161
Gamma-ray line emission from the Local Bubble160
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution154
Reconciling concentration to virial mass relations153
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids152
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system151
The shape of dark matter halos: A new fundamental cosmological invariance149
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data147
The first spatio-spectral Bayesian imaging of SN1006 in X-rays146
Ultracool dwarfs identified using spectra in LAMOST DR7145
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail140
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies139
The origin of the soft excess in the luminous quasar HE 1029-1401138
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe138
Implications of a turbulent convection model for classical Cepheids137
The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies125
High-resolution APEX/LAsMA 12CO and 13CO (3-2) observation of the G333 giant molecular cloud complex123
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs123
The EDGE-CALIFA Survey: An integral field unit-based integrated molecular gas database for galaxy evolution studies in the Local Universe123
Exploring the origins of mega radio halos122
Evidence for multiple types of post-starburst galaxies120
Volatile enrichment in low-mass planets as signatures of past planetary disruption118
Three hot Jupiters transiting K-dwarfs with significant heavy element masses118
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1113
Evolutionary tracks of binary neutron star progenitors across cosmic times111
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility111
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models108
Carina High-contrast Imaging Project for massive Stars (CHIPS)106
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey104
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy103
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data103
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz103
Ammonia characterisation of dense cores in the Rosette Molecular Cloud102
Evidence for stellar contamination in the transmission spectra of HAT-P-12b102
Five methods for determining pattern speeds in galaxies100
Post-Newtonian gravity and Gaia-like astrometry98
Modelling chemical clocks98
Cosmological measurement of the gravitational constant G using the CMB, BAO, and BBN97
Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS97
Modeling the 2020 November 29 solar energetic particle event using EUHFORIA and iPATH models96
The supermassive black hole population from seeding via collisions in nuclear star clusters94
Backstreaming ions at a high Mach number interplanetary shock92
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments92
Multi-spacecraft observations of near-relativistic electron events at different radial distances92
Standardizing the gamma-ray burst as a standard candle and applying it to cosmological probes: Constraints on the two-component dark energy model90
Scale-invariant vacuum guided resolution of the 7Li BBN problem90
Central kiloparsec region of Andromeda89
Probing star formation and ISM properties using galaxy disk inclination87
Core to ultracompact HII region evolution in the W49A massive protocluster87
Galaxy populations in the most distant SPT-SZ clusters87
Hunting for complex cyanides in protostellar ices with the JWST85
Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter84
Asymptotic giant branch stars in the eROSITA-DE eRASS1 catalog83
FAUST82
Detection of J-band photometric periodicity in the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-333882
Bayesian inference of three-dimensional gas maps81
Feedback from low-to-moderate-luminosity radio-active galactic nuclei with MaNGA80
Exploring the intermittency of magnetohydrodynamic turbulence by synchrotron polarization radiation80
Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies80
Magnetic properties of orphan penumbrae80
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)79
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph79
JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H2 in the radio galaxy 3C 326 N79
Planetesimal and planet formation in transient dust traps78
Interstellar chemistry of CN radicals on ices: The formation of CH3CN and CH3NC and potential connection to acetamide78
Shaping physical properties of galaxy subtypes in the VIPERS survey: Environment matters78
HI-H2 transition: Exploring the role of the magnetic field78
[Mg/Fe] ratios in the solar neighbourhood: Stellar yields and chemical evolution scenarios77
The behaviour of eccentric sub-pc massive black hole binaries embedded in massive discs77
Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters77
M-type (22) Kalliope: A tiny Mercury76
Life cycle of cosmic-ray electrons in the intracluster medium76
Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey75
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD74
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy73
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA)73
Detection of very high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage73
Models of quasi-discontinuous solar-wind streams72
3He-rich solar energetic particle events observed on the first perihelion pass of Solar Orbiter72
Comparing feature sets and machine-learning models for prediction of solar flares72
The GALAH survey: Improving chemical abundances using star clusters71
Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing71
JWST MIRI reveals the diversity of nuclear mid-infrared spectra of nearby type 2 quasars71
Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star ζ Oph from high-cadence ESPRESSO spectroscopy and TESS photometry70
Discovery of the luminous X-ray ignition eRASSt J234402.9−35264070
eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS270
The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model70
Black hole accretion and radiation variability in general relativistic magnetohydrodynamic simulations with Rezzolla–Zhidenko spacetime70
Supermassive Black Hole Winds in X-rays: SUBWAYS69
Discovery of a strong rotation of the X-ray polarization angle in the galactic burster GX 13+168
Euclid68
Anatomy of rocky planets formed by rapid pebble accretion67
SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host67
The Low-Redshift Lyman Continuum Survey67
Reconstructing the epoch of reionisation with Planck PR467
K2 and Spitzer phase curves of the rocky ultra-short-period planet K2-141 b hint at a tenuous rock vapor atmosphere67
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases67
ASTRAEUS66
HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars66
Fitting the light curves of Sagittarius A* with a hot-spot model66
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations66
Probing the interstellar medium of the quasar BRI 0952−011566
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf65
Sublimation of refractory minerals in the gas envelopes of accreting rocky planets65
Deep imaging of the galaxy Malin 2 shows new faint structures and a candidate satellite dwarf galaxy65
The New Generation Planetary Population Synthesis (NGPPS)65
The EDGES measurement disfavors an excess radio background during the cosmic dawn64
Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z  ∼  364
Hydrogenated atmospheres of lava planets: Atmospheric structure and emission spectra64
Observability of evaporating lava worlds64
Carbon envelopes around merging galaxies at z ∼ 4.564
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field63
First look with JWST spectroscopy: Resemblance among z ∼ 8 galaxies and local analogs63
Unveiling a new extragalactic structure hidden by the Milky Way63
Strong lensing in UNIONS: Toward a pipeline from discovery to modeling62
Irradiation-driven escape of primordial planetary atmospheres62
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations62
An idealized general circulation model for the atmospheric circulation on the ice giants61
Cosmic ray interactions with indene and adamantane seeded water ice mantles61
Dynamics of tidal spiral arms: Machine learning-assisted identification of equations and application to the Milky Way61
The preferential orientation of magnetic switchbacks and its implications for solar magnetic flux transport61
Systematic evaluation of variability detection methods for eROSITA61
Propeller effect in action: Unveiling quenched accretion in the transient X-ray pulsar 4U 0115+6361
PRODIGE – envelope to disk with NOEMA61
Quantifying observational projection effects with a simulation-based hot CGM model60
Binary neutron star merger offsets from their host galaxies60
Euclid: Searches for strong gravitational lenses using convolutional neural nets in Early Release Observations of the Perseus field60
Solar extreme ultraviolet variability as a proxy for nanoflare heating diagnostics59
MOCKA – A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators59
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d59
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries59
Radio outburst from a massive (proto)star59
Self-gravity in thin-disc simulations of protoplanetary discs: The smoothing length rectified and generalised to bi-fluids59
Time-resolved spectro-polarimetric analysis of extremely bright GRB 230307A: Possible evidence of evolution from photospheric to synchrotron dominated emission58
The MUSE-Faint survey58
Little impact of mergers and galaxy morphology on the production and escape of ionizing photons in the early Universe58
Galaxies at the edges: A complete census of the MACS J0416.1–2403 cluster57
Transport of the magnetic flux away from a decaying sunspot via convective motions57
Calibration and performances of the integrated Mach—Zehnder wavefront sensor for extreme adaptive optics57
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts57
Multi-step reconstruction of radio-interferometric images57
Euclid preparation56
The “C”: The large Chameleon-Musca-Coalsack cloud56
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies56
Negative polarization properties of regolith simulants56
Generative modelling of convergence maps based on predicted one-point statistics55
The effect of dynamic temperatures on pebble dynamics and planet formation55
iNNterpol: High-precision interpolation of stellar atmospheres with a deep neural network using a 1D convolutional auto encoder for feature extraction55
Exploring the Sagittarius stream with RR Lyrae stars from Gaia Data Release 355
A solar rotation signature in cosmic dust observed in STEREO spacecraft data55
Dynamical modelling and the origin of gas turbulence in z ∼ 4.5 galaxies54
Sub-stellar engulfment by a main-sequence star: Where is the lithium?54
LIME: A LIne MEasuring library for large and complex spectroscopic data sets54
The Milky Way’s middle-aged inner ring54
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY54
Generative models of astrophysical fields with scattering transforms on the sphere54
Probing the physical properties of the intergalactic medium using SRG/eROSITA spectra from blazars53
Euclid preparation53
The XXL Survey53
Peculiar X-ray transient SRGA J043520.9+552226/AT2019wey discovered with SRG/ART-XC53
Selected open cluster sample for validating atmospheric parameters: Application to Gaia and other surveys53
Don’t torque like that53
Non-radial oscillations mimicking a brown dwarf orbiting the cluster giant NGC 4349 No. 12753
A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS53
Planet formation around intermediate-mass stars52
The kinematics of 30 Milky Way globular clusters and the multiple stellar populations within52
Parameter measurement based on photometric images52
Forming Planets Around Stars With Non-Solar Elemental Composition52
The Mantis Network52
The ANTARESS workflow52
A3COSMOS: Measuring the cosmic dust-attenuated star formation rate density at 4 < z < 552
Kinematic properties of white dwarfs52
TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE52
Tracking active nests in solar-type pulsators: Ensemble starspot modelling of Kepler asteroseismic targets52
Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images52
Spinning nano-carbon grains: Viable origin for anomalous microwave emission51
Testing refracted gravity with the kinematics of galaxy clusters51
The outflowing ionised gas of I Zw 1 observed by HST COS51
On-sky validation of image-based adaptive optics wavefront sensor referencing51
Temperature of quiet Sun small scale brightenings observed by EUI on board Solar Orbiter: Evidence for a cooler component51
A highly dynamic small-scale jet in a polar coronal hole51
The Arecibo Galaxy Environment Survey (AGES)51
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries51
Age of (152830) Dinkinesh I Selam constrained by secular tidal-BYORP theory51
SPICE connection mosaics to link the Sun’s surface and the heliosphere51
The influence of planetesimal fragmentation on planet formation51
Emission and absorption lines in the photospheric radius expansion bursts of 4U 1820–3051
The cylindrical jet base of M 87 within 100 μas of the central engine51
Making the unmodulated pyramid wavefront sensor smart50
The SLACS strong lens sample, debiased50
The EXOD search for faint transients in XMM-Newton observations50
Survey of Orion Disks with ALMA (SODA)50
An effective model for magnetic field amplification by the magnetorotational and parasitic instabilities50
Euclid preparation50
Cataclysmic variables and the disc instability model in the Gaia DR3 colour–magnitude diagram50
Constraining the formation history of the HAT-P-11 system using atmospheric abundances50
Abundance analysis of stars hosting gas-rich debris discs50
The impact of morphological quenching mechanisms on star formation activity at 0.2 < z < 1.2 in the COSMOS field49
Cosmic-ray electron transport in the galaxy M 5149
Exploring non-thermal emission from the star-forming region NGC 3603 through a realistic modelling of its environment49
3D non-LTE Ca II line formation in metal-poor FGK stars49
The spectral energy distributions of very long-period Cepheids in the Milky Way, the Magellanic Clouds, M31, and M3349
The jet and circumstellar environment of the young binary DF Tau49
Identifying multiplets of IceCube alert events48
Clustering of magnetic reconnection exhausts in the solar wind: An automated detection study48
Dynamics of trans-Neptunian objects near the 3/1 mean-motion resonance with Neptune48
Probing the galactic cosmic-ray density with current and future γ-ray instruments48
A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies48
Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk48
Observational constraints on gas disc sizes in the protoplanetary discs of multiple systems in the Taurus region48
Assessing the accuracy of star formation rate measurements by direct star count in molecular clouds48
MeerKAT view of Hickson Compact Groups48
Astrometric mass measurement of compact companions in binary systems with Gaia48
Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations48
A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies48
The PAU Survey: The quasar Lyα and UV luminosity functions at 2.7 < z < 5.347
An analytical model for dust impact voltage signals and its application to STEREO/WAVES data47
MUSE crowded field 3D spectroscopy in NGC 30047
zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks47
Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter47
Plasma dynamics in the flaring loop observed by RHESSI46
Simulating the LOcal Web (SLOW)46
ISPY: NACO Imaging Survey for Planets around Young stars46
Simulations of radio-wave anisotropic scattering to interpret type III radio burst data from Solar Orbiter, Parker Solar Probe, STEREO, and Wind46
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