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 2021-09-01 to 2025-09-01.)
ArticleCitations
Indications of magnetic accretion in Swift J0826.2−70332581
First detection of metric emission from a solar surge687
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)491
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA450
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts363
Cosmology in the non-linear regime: the small scale miracle339
One Star to Tag Them All (OSTTA)286
Categorization model of moving small-scale intensity enhancements in solar active regions271
Reduction of dust radial drift by turbulence in protoplanetary disks253
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state218
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies205
The GAPS Programme at TNG202
Volatile-rich comets ejected early on during Solar System formation196
From eruption to post-flare rain: A 2.5D MHD model195
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)193
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves188
Timing and scintillation studies of PSR J1439−5501185
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission178
The LOFAR LBA Sky Survey: Deep Fields176
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field173
Properties of the ionisation glitch172
Stellar halo density with LAMOST K and M giants153
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources152
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole152
Improved source classification and performance analysis usingGaiaDR3151
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation151
Simulation of CH3OH ice UV photolysis under laboratory conditions150
Gamma-ray line emission from the Local Bubble147
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY142
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars142
Massive pre-main-sequence stars in M17140
A solar rotation signature in cosmic dust observed in STEREO spacecraft data139
The effect of dynamic temperatures on pebble dynamics and planet formation138
Transient classifiers for Fink136
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?135
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution134
Reconciling concentration to virial mass relations133
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids133
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries132
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system132
Probing the interstellar medium of the quasar BRI 0952−0115127
The shape of dark matter halos: A new fundamental cosmological invariance124
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data123
The first spatio-spectral Bayesian imaging of SN1006 in X-rays120
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes116
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity115
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy112
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles111
Ultracool dwarfs identified using spectra in LAMOST DR7110
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies109
The origin of the soft excess in the luminous quasar HE 1029-1401107
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe105
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail104
Non-linear dynamics of the minimal theory of massive gravity103
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments102
Carina High-contrast Imaging Project for massive Stars (CHIPS)101
Parameter measurement based on photometric images97
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey97
Exploring the origins of mega radio halos97
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs95
Evidence for stellar contamination in the transmission spectra of HAT-P-12b93
Unveiling a new extragalactic structure hidden by the Milky Way93
Spectroflat: A generic spectrum and flat-field calibration library for spectro-polarimetric data92
zELDA II: Reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks92
SPICE connection mosaics to link the Sun’s surface and the heliosphere92
The PAU Survey: The quasar Lyα and UV luminosity functions at 2.7 < z < 5.391
Ammonia characterisation of dense cores in the Rosette Molecular Cloud88
GaiaData Release 388
Five methods for determining pattern speeds in galaxies87
Constraints on asteroid-mass primordial black holes in dwarf galaxies using Hubble Space Telescope photometry87
Multi-iron subpopulations in Liller 1 from high-resolution H-band spectroscopy85
The longevity of the oldest open clusters85
Detection of very high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passage83
Core to ultracompact HII region evolution in the W49A massive protocluster83
Number of stars in the Sun’s birth cluster revisited82
Velocity measurement in the extensive [OIII] emission region 1.2° south-east of M 3182
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz82
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-181
Probing star formation and ISM properties using galaxy disk inclination81
Galaxy populations in the most distant SPT-SZ clusters80
Evolutionary tracks of binary neutron star progenitors across cosmic times80
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