Astronomy & Astrophysics

Papers
(The H4-Index of Astronomy & Astrophysics is 80. 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 2021-10-01 to 2025-10-01.)
ArticleCitations
Indications of magnetic accretion in Swift J0826.2−70332699
First detection of metric emission from a solar surge712
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA472
Cosmology in the non-linear regime: the small scale miracle374
One Star to Tag Them All (OSTTA)359
Categorization model of moving small-scale intensity enhancements in solar active regions297
Reduction of dust radial drift by turbulence in protoplanetary disks278
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state270
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies226
The GAPS Programme at TNG220
Volatile-rich comets ejected early on during Solar System formation209
From eruption to post-flare rain: A 2.5D MHD model201
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)200
Timing and scintillation studies of PSR J1439−5501197
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission193
The LOFAR LBA Sky Survey: Deep Fields190
Properties of the ionisation glitch185
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field185
Stellar halo density with LAMOST K and M giants184
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources180
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole179
Improved source classification and performance analysis usingGaiaDR3159
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation159
Simulation of CH3OH ice UV photolysis under laboratory conditions158
Gamma-ray line emission from the Local Bubble158
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars155
Massive pre-main-sequence stars in M17154
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?153
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution149
Reconciling concentration to virial mass relations147
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids144
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system143
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries142
Probing the interstellar medium of the quasar BRI 0952−0115142
The shape of dark matter halos: A new fundamental cosmological invariance140
The first spatio-spectral Bayesian imaging of SN1006 in X-rays138
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data138
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes136
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity133
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy131
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles128
Ultracool dwarfs identified using spectra in LAMOST DR7123
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies121
The origin of the soft excess in the luminous quasar HE 1029-1401118
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe117
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail116
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments114
Carina High-contrast Imaging Project for massive Stars (CHIPS)113
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey112
Parameter measurement based on photometric images111
Exploring the origins of mega radio halos110
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs109
Evidence for stellar contamination in the transmission spectra of HAT-P-12b106
Five methods for determining pattern speeds in galaxies103
Ammonia characterisation of dense cores in the Rosette Molecular Cloud103
The longevity of the oldest open clusters101
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy100
Unveiling a new extragalactic structure hidden by the Milky Way99
SPICE connection mosaics to link the Sun’s surface and the heliosphere98
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data98
WEAVE-StePS: A stellar population survey using WEAVE at WHT97
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz97
Modelling chemical clocks95
Modeling the 2020 November 29 solar energetic particle event using EUHFORIA and iPATH models94
Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at z  ∼  393
Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS92
Multi-spacecraft observations of near-relativistic electron events at different radial distances89
Fitting the light curves of Sagittarius A* with a hot-spot model89
Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies89
The supermassive black hole population from seeding via collisions in nuclear star clusters88
Cosmological measurement of the gravitational constant G using the CMB, BAO, and BBN87
Post-Newtonian gravity and Gaia-like astrometry87
HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars86
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models86
Black hole accretion and radiation variability in general relativistic magnetohydrodynamic simulations with Rezzolla–Zhidenko spacetime85
Cosmic rays cannot explain the high ionisation rates in the Galactic centre85
Hydrogenated atmospheres of lava planets: Atmospheric structure and emission spectra84
The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies83
OGLE-2002-BLG-360: A dusty anomaly among red nova remnants81
High-resolution APEX/LAsMA 12CO and 13CO (3-2) observation of the G333 giant molecular cloud complex80
The EDGE-CALIFA Survey: An integral field unit-based integrated molecular gas database for galaxy evolution studies in the Local Universe80
Reconstructing the epoch of reionisation with Planck PR480
Implications of a turbulent convection model for classical Cepheids80
0.12820196151733