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 2021-07-01 to 2025-07-01.)
ArticleCitations
Mid-infrared spectra of T Tauri disks: Modeling the effects of a small inner cavity on CO2 and H2O emission2327
Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus (Corrigendum)1186
Indications of magnetic accretion in Swift J0826.2−7033632
First detection of metric emission from a solar surge459
High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)416
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-z lensed dusty star-forming galaxies using ALMA334
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts319
Cosmology in the non-linear regime: the small scale miracle271
One Star to Tag Them All (OSTTA)262
Generative models of astrophysical fields with scattering transforms on the sphere229
Categorization model of moving small-scale intensity enhancements in solar active regions201
Reduction of dust radial drift by turbulence in protoplanetary disks186
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state178
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies177
The GAPS Programme at TNG174
Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies173
Volatile-rich comets ejected early on during Solar System formation172
From eruption to post-flare rain: A 2.5D MHD model168
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)167
Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves163
Successive deuteration in low-mass star-forming regions: The case of D2-methanol (CHD2OH) in IRAS 16293-2422160
Moment expansion of polarized dust SED: A new path towards capturing the CMB B-modes with LiteBIRD158
Timing and scintillation studies of PSR J1439−5501152
Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing Hα emission146
The LOFAR LBA Sky Survey: Deep Fields144
Origin of eclipsing time variations: Contributions of different modes of the dynamo-generated magnetic field144
Properties of the ionisation glitch142
Evidence for flare-accelerated particles in large scale loops in the behind-the-limb gamma-ray solar flare of September 29, 2022139
Stellar halo density with LAMOST K and M giants137
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources136
Particle acceleration and radiation reaction in a strongly magnetised rotating dipole135
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation131
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST128
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility127
The stable climate of KELT-9b124
Improved source classification and performance analysis usingGaiaDR3123
Systematic evaluation of variability detection methods for eROSITA121
Plasma dynamics in the flaring loop observed by RHESSI121
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models121
Simulation of CH3OH ice UV photolysis under laboratory conditions121
Gamma-ray line emission from the Local Bubble120
Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY116
Changing disc compositions via internal photoevaporation115
Study of oxygen-rich post-AGB stars in the Milky Way as a means to explain the production of silicates among evolved stars114
Massive pre-main-sequence stars in M17113
A solar rotation signature in cosmic dust observed in STEREO spacecraft data112
The effect of dynamic temperatures on pebble dynamics and planet formation110
Transient classifiers for Fink109
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?107
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution106
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d105
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids103
Reconciling concentration to virial mass relations103
Estimation of the lateral mis-registrations of the GRAVITY+adaptive optics system102
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries101
Probing the interstellar medium of the quasar BRI 0952−0115101
The shape of dark matter halos: A new fundamental cosmological invariance100
The ANTARESS workflow98
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data98
The first spatio-spectral Bayesian imaging of SN1006 in X-rays97
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes97
A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS96
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity96
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles91
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy91
Ultracool dwarfs identified using spectra in LAMOST DR790
Life cycle of cosmic-ray electrons in the intracluster medium90
Tailoring galaxies: Size–luminosity–surface brightness relations of bulges and disks along the morphological sequence89
Dynamics of nanodust in the vicinity of a stellar corona: Effect of plasma corotation88
Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies88
The origin of the soft excess in the luminous quasar HE 1029-140187
Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe86
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail85
Non-linear dynamics of the minimal theory of massive gravity84
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments83
Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf82
Carina High-contrast Imaging Project for massive Stars (CHIPS)81
Probable brown dwarf companions detected in binary microlensing events during the 2018–2020 seasons of the KMTNet survey80
Probing the physical properties of the intergalactic medium using SRG/eROSITA spectra from blazars79
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