Astronomy & Astrophysics

Papers
(The H4-Index of Astronomy & Astrophysics is 79. 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 2021-08-01 to 2025-08-01.)
ArticleCitations
Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus (Corrigendum)2449
Indications of magnetic accretion in Swift J0826.2−70331221
First detection of metric emission from a solar surge653
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)476
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA431
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts348
Cosmology in the non-linear regime: the small scale miracle324
One Star to Tag Them All (OSTTA)276
Categorization model of moving small-scale intensity enhancements in solar active regions265
Reduction of dust radial drift by turbulence in protoplanetary disks241
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state207
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies195
The GAPS Programme at TNG189
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies188
From eruption to post-flare rain: A 2.5D MHD model184
Volatile-rich comets ejected early on during Solar System formation184
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)182
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves177
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD170
Timing and scintillation studies of PSR J1439−5501169
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission165
The LOFAR LBA Sky Survey: Deep Fields159
Properties of the ionisation glitch149
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field149
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 2022147
Stellar halo density with LAMOST K and M giants146
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources145
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole141
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST137
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation137
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility136
Improved source classification and performance analysis usingGaiaDR3134
Simulation of CH3OH ice UV photolysis under laboratory conditions132
Gamma-ray line emission from the Local Bubble128
Systematic evaluation of variability detection methods for eROSITA128
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY127
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars125
A solar rotation signature in cosmic dust observed in STEREO spacecraft data124
Massive pre-main-sequence stars in M17124
The effect of dynamic temperatures on pebble dynamics and planet formation123
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?122
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution122
Transient classifiers for Fink122
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids118
Reconciling concentration to virial mass relations118
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system117
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries113
Probing the interstellar medium of the quasar BRI 0952−0115110
The shape of dark matter halos: A new fundamental cosmological invariance110
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data107
The first spatio-spectral Bayesian imaging of SN1006 in X-rays105
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes104
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity104
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles102
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy102
Life cycle of cosmic-ray electrons in the intracluster medium102
Ultracool dwarfs identified using spectra in LAMOST DR7101
Dynamics of nanodust in the vicinity of a stellar corona: Effect of plasma corotation100
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies99
The origin of the soft excess in the luminous quasar HE 1029-140199
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe93
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments92
Non-linear dynamics of the minimal theory of massive gravity92
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail92
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf90
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey89
Carina High-contrast Imaging Project for massive Stars (CHIPS)89
Cosmic rays cannot explain the high ionisation rates in the Galactic centre88
Parameter measurement based on photometric images87
Link between star formation and the properties of supermassive black holes85
Exploring the origins of mega radio halos85
Black hole accretion and radiation variability in general relativistic magnetohydrodynamic simulations with Rezzolla–Zhidenko spacetime85
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs84
Evidence for stellar contamination in the transmission spectra of HAT-P-12b83
Unveiling a new extragalactic structure hidden by the Milky Way83
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data82
SPICE connection mosaics to link the Sun’s surface and the heliosphere80
The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies80
Multi-spacecraft observations of near-relativistic electron events at different radial distances79
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