OOIR: Observatory of International Research

Papers

(The H4-Index of Astronomy & Astrophysics is 82. 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 2022-01-01 to 2026-01-01.)

Article	Citations
Optical and near-infrared spectroscopy of the black hole transient 4U 1543–47 during its 2021 ultra-luminous state	3095
Cosmic insights from galaxy clusters: Exploring magnification bias on sub-millimetre galaxies	795
The GAPS Programme at TNG	536
Volatile-rich comets ejected early on during Solar System formation	407
Numerical simulations of turbulence in prominence threads induced by torsional oscillations (Corrigendum)	386
Timing and scintillation studies of PSR J1439−5501	314
Indications of magnetic accretion in Swift J0826.2−7033	295
First detection of metric emission from a solar surge	260
Cosmology in the non-linear regime: the small scale miracle	258
One Star to Tag Them All (OSTTA)	246
Categorization model of moving small-scale intensity enhancements in solar active regions	242
Reduction of dust radial drift by turbulence in protoplanetary disks	231
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes	226
Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity	222
Hidden in plain sight: UVIT and MUSE discovery of a large, diffuse star-forming galaxy	216
Massive pre-main-sequence stars in M17	215
The massive galaxy cluster CL0238.3+2005 (the Peanut cluster) at z = 0.42: A merger just after pericenter passage?	211
Stellar halo density with LAMOST K and M giants	201
Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources	201
A pair of early- and late-forming galaxy cluster samples: A novel way of studying halo assembly bias assisted by a constrained simulation	199
Improved source classification and performance analysis usingGaiaDR3	177
Reconciling concentration to virial mass relations	176
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution	176
Large main-belt asteroids are generally not Maclaurin or Jacobi ellipsoids	174
Estimation of the lateral mis-registrations of the GRAVITY₊adaptive optics system	173

Constraints on the variable nature of the slow solar wind with the Wide-Field Imager on board the Parker Solar Probe	171
The origin of the soft excess in the luminous quasar HE 1029-1401	170
Implications of a turbulent convection model for classical Cepheids	168
A search for ionised gas outflows in an Hα imaging atlas of nearby LINERs	162
Evidence for multiple types of post-starburst galaxies	157
Three hot Jupiters transiting K-dwarfs with significant heavy element masses	156
Volatile enrichment in low-mass planets as signatures of past planetary disruption	154
Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1	153
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility	150
Challenges in modeling the dark matter halo of NGC 1052–DF2: Cored versus cuspy halo models	144
Carina High-contrast Imaging Project for massive Stars (CHIPS)	144
Five methods for determining pattern speeds in galaxies	137
Ammonia characterisation of dense cores in the Rosette Molecular Cloud	137
Post-Newtonian gravity and Gaia-like astrometry	132
Cosmological measurement of the gravitational constant G using the CMB, BAO, and BBN	131
Multi-spacecraft observations of near-relativistic electron events at different radial distances	129
The supermassive black hole population from seeding via collisions in nuclear star clusters	129
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments	124
A new way to measure the distance to NGC1052-DF2	122
Constraints on asteroid-mass primordial black holes in dwarf galaxies using Hubble Space Telescope photometry	118
Spatially resolved spectroscopic analysis of Lyα haloes	117
Noble gases neon and argon: A role for the chemical patterns of multiple populations in globular clusters?	114
The stable climate of KELT-9b	112
Primordial black holes as dark matter candidates	111
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles	110
Euclid	110
Changing disc compositions via internal photoevaporation	110
Cosmic rays cannot explain the high ionisation rates in the Galactic centre	108
Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star ζ Oph from high-cadence ESPRESSO spectroscopy and TE	107
A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models	107
Scale-invariant vacuum guided resolution of the ⁷Li BBN problem	105
Central kiloparsec region of Andromeda	104
Probing star formation and ISM properties using galaxy disk inclination	103
Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter	102
Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies	101
[Mg/Fe] ratios in the solar neighbourhood: Stellar yields and chemical evolution scenarios	98
Exploring the intermittency of magnetohydrodynamic turbulence by synchrotron polarization radiation	98
Models of quasi-discontinuous solar-wind streams	96
Constraints on primordial non-Gaussianity from the cross-correlation of DESI luminous red galaxies and Planck CMB lensing	94
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy	94
eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2	93
New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph	92
JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H₂ in the radio galaxy 3C 326 N	91
Planetesimal and planet formation in transient dust traps	88
Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters	87
H_I-H₂ transition: Exploring the role of the magnetic field	86
Reconstructing the epoch of reionisation with Planck PR4	86
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations	86
Carbon envelopes around merging galaxies at z ∼ 4.5	86
An idealized general circulation model for the atmospheric circulation on the ice giants	85

Unveiling a new extragalactic structure hidden by the Milky Way	85
Dissecting the emission from LHAASO J0341+5258: Implications for future multiwavelength observations	85
Propeller effect in action: Unveiling quenched accretion in the transient X-ray pulsar 4U 0115+63	83
Dynamics of tidal spiral arms: Machine learning-assisted identification of equations and application to the Milky Way	83
Self-gravity in thin-disc simulations of protoplanetary discs: The smoothing length rectified and generalised to bi-fluids	82
Systematic evaluation of variability detection methods for eROSITA	82
Solar extreme ultraviolet variability as a proxy for nanoflare heating diagnostics	82
Carbon enrichment in APOGEE disk stars as evidence of mass transfer in binaries	82
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d	82