Monthly Notices of the Royal Astronomical Society

Papers
(The H4-Index of Monthly Notices of the Royal Astronomical Society is 73. 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 2020-04-01 to 2024-04-01.)
ArticleCitations
The GALAH+ survey: Third data release284
Unresolved stellar companions with Gaia DR2 astrometry218
Bayesian inference for compact binary coalescences with bilby: validation and application to the first LIGO–Virgo gravitational-wave transient catalogue207
A million binaries from Gaia eDR3: sample selection and validation of Gaia parallax uncertainties204
Gaia EDR3 view on galactic globular clusters196
Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: inferences in the stochastic gravitational-wave background search184
The milky way total mass profile as inferred from Gaia DR2182
The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background176
Possible periodic activity in the repeating FRB 121102165
The biggest splash159
Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST, and literature data158
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies155
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function 151
The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging146
Kraken reveals itself – the merger history of the Milky Way reconstructed with the E-MOSAICS simulations142
Systematic opacity calculations for kilonovae140
To H0 or not to H0?137
A unified picture of Galactic and cosmological fast radio bursts134
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the quasar sample in configuration space between redshift 0.8 a134
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum betwee132
Simulating cosmic structure formation with the gadget-4 code129
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2126
Tango for three: Sagittarius, LMC, and the Milky Way125
A catalogue of white dwarfs in Gaia EDR3121
Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST ERO SMACS 0723 Field119
hmcode-2020: improved modelling of non-linear cosmological power spectra with baryonic feedback118
On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference113
Repeating behaviour of FRB 121102: periodicity, waiting times, and energy distribution109
Updated parameters of 1743 open clusters based on Gaia DR2108
Distances to PHANGS galaxies: New tip of the red giant branch measurements and adopted distances106
The Uchuu simulations: Data Release 1 and dark matter halo concentrations105
The [O iii]+H β equivalent width distribution at z ≃ 7: implications for the contribution of galaxies to reionization103
Evidence from APOGEE for the presence of a major building block of the halo buried in the inner Galaxy103
Revealing galaxy candidates out to z ∼ 16 with JWST observations of the lensing cluster SMACS0723102
Massively parallel Bayesian inference for transient gravitational-wave astronomy102
The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8100
Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies99
Properties of the circumgalactic medium in cosmic ray-dominated galaxy haloes98
Resolving small-scale cold circumgalactic gas in TNG5098
A Volume-limited Sample of Cataclysmic Variables from Gaia DR2: Space Density and Population Properties97
Arbitrating the S8 discrepancy with growth rate measurements from redshift-space distortions97
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues for cosmological analysis94
High time resolution and polarization properties of ASKAP-localized fast radio bursts92
Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up, and 12C(α, γ)16O rate on the pair-instability black hole mass gap92
Parameter estimation of hairy Kerr black holes from its shadow and constraints from M87*90
Binary black holes in young star clusters: the impact of metallicity89
The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function, and binary evolution89
Binary black holes in the pair instability mass gap87
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum betwe87
High-redshift cosmography: auxiliary variables versus Padé polynomials85
Unveiling the planet population at birth84
Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing84
The clustering of DESI-like luminous red galaxies using photometric redshifts83
Black hole, neutron star, and white dwarf merger rates in AGN discs83
Monte Carlo simulations of black hole mergers in AGN discs: Low χeff mergers and predictions for LIGO83
Cosmic Dawn II (CoDa II): a new radiation-hydrodynamics simulation of the self-consistent coupling of galaxy formation and reionization83
Impact of massive binary star and cosmic evolution on gravitational wave observations I: black hole–neutron star mergers82
Hydrogen reionization ends by z = 5.3: Lyman-α optical depth measured by the XQR-30 sample82
Large-scale poloidal magnetic field dynamo leads to powerful jets in GRMHD simulations of black hole accretion with toroidal field81
SPIRou: NIR velocimetry and spectropolarimetry at the CFHT80
ProSpect: generating spectral energy distributions with complex star formation and metallicity histories80
Introducing the thesan project: radiation-magnetohydrodynamic simulations of the epoch of reionization79
How to tell an accreting boson star from a black hole79
Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions77
The completed SDSS-IV extended baryon oscillation spectroscopic survey: growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 fo76
Three-dimensional models of core-collapse supernovae from low-mass progenitors with implications for Crab75
On the nature of massive helium star winds and Wolf–Rayet-type mass-loss75
A combined analysis of the H0 late time direct measurements and the impact on the Dark Energy sector75
Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta, and kilonova signals75
VINTERGATAN – I. The origins of chemically, kinematically, and structurally distinct discs in a simulated Milky Way-mass galaxy74
Giant molecular cloud catalogues for PHANGS-ALMA: methods and initial results74
The BACCO simulation project: exploiting the full power of large-scale structure for cosmology74
Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties74
Ionized outflows in local luminous AGN: what are the real densities and outflow rates?73
A thousand days after the merger: Continued X-ray emission from GW17081773
FETCH: A deep-learning based classifier for fast transient classification73
Dark energy survey year 3 results: weak lensing shape catalogue73
The Universe at z > 10: predictions for JWST from the universemachine DR173
STARFORGE: Towards a comprehensive numerical model of star cluster formation and feedback73
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