Monthly Notices of the Royal Astronomical Society

Papers
(The TQCC of Monthly Notices of the Royal Astronomical Society is 12. 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 2022-06-01 to 2026-06-01.)
ArticleCitations
A partial isotopic decomposition for the Sculptor dSph399
Correction to: A blue depression in the optical spectra of M dwarfs309
Simulation of polarized emission from recollimation shocks in relativistic jets289
Time-series photometry and multiwavelength characterization of the young stellar cluster Mon R2267
Distribution of gamma-ray bursts on the T90–HR plane and their classification revisited258
Close encounters of the interstellar kind: exploring the capture of interstellar objects in near-Earth orbit252
Correction to: Strong CO absorption features in massive ETGs244
Correction to: Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z = 2−4 using JWST243
Data-driven scale identification in oscillatory dynamos217
A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization210
Correction to: Dynamical evolution of population III stellar systems and the resulting binary statistics206
Erratum: Stars in the local galactic thick disc and halo in Gaia EDR3:a catalogue of half a million local main-sequence stars with photometric metallicities202
MeerKAT observations of Herschel protocluster candidates187
Testing the transferability of machine learning techniques for determining photometric redshifts of galaxy catalogue populations187
Multifractality signatures in lensed quasars184
Extracting key information from spectroscopic galaxy surveys172
A joint investigation of Saturn’s deep zonal flow via its gravitational field and Ohmic dissipation170
Correction to: Pilot-WINGS: An extended MUSE view of the structure of Abell 370164
Correction to: Hyperbolic conduction: A fast, physical conduction model implemented in Smoothed Particle Hydrodynamics156
Correction to: Predicting the ages of galaxies with an artificial neural network155
Gap opening in protoplanetary discs: gas dynamics from global axisymmetric non-ideal MHD simulations with consistent thermochemistry153
Relating quasi-stationary one zone emission models to expanding relativistic shocks147
Correction to: Diagnosis of 3D magnetic field and mode composition in MHD turbulence with Y-parameter147
Revisiting a flux recovery systematic error arising from common deconvolution methods used in aperture-synthesis imaging143
CCD UBV(RI)KC photometry and dynamics of the open cluster NGC 1513139
Dynamical mass determination and partial eclipses of the heartbeat star HD 181793138
The dominant mechanism(s) for populating the outskirts of star clusters with neutron star binaries137
The colour evolution of magnetar-powered kilonova emission in merging neutron star–neutron star systems136
Commensal transient searches in eight short gamma-ray burst fields136
An improved time delay from VLA and ATCA monitoring of the gravitational lens system PKS 1830–211132
Matter power spectra in modified gravity: a comparative study of approximations and N-body simulations132
MeV neutrino flash from neutron star mergers viar-process nucleosynthesis131
NIGHT: A compact, near-infrared, high-resolution spectrograph to survey helium in exoplanet systems127
Correction to: MIGHTEE: the nature of the radio-loud AGN population122
Processing of hydroxylamine, NH2OH, an important prebiotic precursor, on interstellar ices120
Multiple photoionization for the 2s subshell in the iron atom119
Timing and spectral studies of Cen X-3 in multiple luminosity states using AstroSat118
Converting the sub-Jovian desert of exoplanets to a savanna with TESS, PLATO, and Ariel118
Decretion disc evolution and neutron star accretion in short-period eccentric Be/X-ray binaries117
Reddening and the shape of the variable component of the continua of active galactic nuclei from the optical to the far-ultraviolet – I111
Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties111
Boosting the evolutionary picture of galaxy clusters: a case study at intermediate-redshift of Cl 0024+17 and MS 0451−03110
On the correlation between X-rays and TeV gamma-rays in HBL Blazars110
Correction to: MaNGA AGN dwarf galaxies (MAD) – I. A new sample of AGNs in dwarf galaxies with spatially-resolved spectroscopy109
The luminosity functions of kilonovae from binary neutron star mergers under different equation of states109
Hubble’s Variable Nebula I. Ripples on a big screen107
Impact of inhomogeneous reionization on post-reionization 21-cm intensity mapping measurement of cosmological parameters106
Non-thermal radio emission from massive protostars in the SARAO MeerKAT Galactic Plane Survey106
Parameter distributions of binary black hole mergers near supermassive black holes as seen by advanced gravitational wave detectors106
An enigmatic 380 kpc long linear collimated galactic tail105
Magnetic burial in millisecond magnetars and late GRB afterglow signatures105
Cooling and instabilities in colliding radiative flows with toroidal magnetic fields104
Accreting neutron stars: composition of the upper layers of the inner crust104
A fuzzy situation eased: cold dark matter with multipoles can explain the double radio quad lens HS 0810+2554103
Epicyclic frequencies of spheroidal stars with non-uniform density101
Stellar spots cause measurable variations in atmospheric metallicity100
MOCCA-Survey Database: extra galactic globular clusters – III. The population of black holes in Milky Way and Andromeda-like galaxies99
Correction to: a revised age greater than 50 Myr for the young cluster IC 466597
Boosting line intensity map signal-to-noise ratio with the Ly-α forest cross-correlation97
On the gamma-ray emission from the core of the Sagittarius dwarf galaxy96
A covariant formulation for cosmological radiative transfer of the 21-cm line96
An X-rays-to-radio investigation of the nuclear polarization from the radio-galaxy Centaurus A93
X-ray surface brightness fluctuations in smooth galaxy cluster atmospheres92
From particles to orbits: precise dark matter density profiles using dynamical information92
Structure functions with higher-order stencils as a probe to separate small- and large-scale magnetic fields92
Multistream radial structure of cold dark matter haloes from particle trajectories: deep inside splashback radius92
Star formation rate density as a function of galaxy mass at z < 0.2 with MUSE and GAMA surveys91
The multizone chemical evolution of the Galactic bulge: predicting abundances for different radial zones91
H i-rich but low star formation galaxies in MaNGA: physical properties and comparison to control samples89
The progenitor galaxies of stellar haloes as ‘failed’ Milky Ways89
4U 1210−64: a new member of the rare intermediate-mass X-ray binary subclass88
Self-similar mass accretion history in scale-free simulations88
The loneliest galaxies in the Universe: a GAMA and Galaxy Zoo study on void galaxy morphology88
General relativistic moving-mesh hydrodynamic simulations with arepo and applications to neutron star mergers87
A mutually embedded perception model for solar corona87
Cosmological forecast of the void size function measurement from the CSST spectroscopic survey85
Magnetically driven coupling in relativistic radiation-mediated shocks84
On non-detection of gamma-ray bursts in three compact binary merger events detected by LIGO84
The abundance of core-collapsed subhaloes in SIDM: insights from structure formation in ΛCDM83
The evolution of the Milky Way’s thin disc radial metallicity gradient with K2 asteroseismic ages83
Explaining prolonged fluctuations in light curves of classical novae via modelling83
Chemical abundance analysis of symbiotic giants. Metallicity and CNO abundance patterns in 14 northern S-type systems81
Isophote shape analysis and the unfortunate subtlety of dwarf galaxy structure80
The redshift evolution of the S0 fraction for z < 1 in COSMOS80
PyLMT : a transient detection pipeline for the 4-m International Liquid Mirror Telescope80
The EBLM project – XIV. TESS light curves for eclipsing binaries with very low mass companions80
Solar coronal heating: role of kinetic and inertial Alfvén waves in heating and charged particle acceleration80
Energy equipartition in multiple-population globular clusters80
The chemical compositions of multiple stellar populations in the globular cluster NGC 280879
The Three Hundred: cluster dynamical states and relaxation period78
Multi-cloud crushing – the collective survival of cold clouds in galactic outflows78
Non-parametric attenuation curves in local star-forming galaxies: geometry effect, dust evolution, and intermediate-scale structures78
White dwarf constraints on geological processes at the population level78
Large, fast, and accurate H  i intensity maps with latent overlap diffusion77
Proximal boulders and momentum transfer from DART-scale 3D impact simulations on asteroid Dimorphos77
Fundamental effective temperature measurements for eclipsing binary stars – VII. The solar twin in LL Aquarii77
OGLE-2015-BLG-0845L: a low-mass M dwarf from the microlensing parallax and xallarap effects77
A high-resolution spectroscopic search for multiple populations in the 2 Gyr old cluster NGC 184677
Infrared and Optical Emission-line Diagnostics76
HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 8542676
Revisiting the formaldehyde masers – II. Effects of an H ii region and beaming76
Unexpected stratification in the equivalent-duration distributions of flare stars75
Unveiling the main sequence of galaxies at z ≥ 5 with the JWST: predictions from simulations75
Massive young stellar objects in the Local Group spiral galaxy M 33 identified using machine learning75
Probing dark matter substructures with free-form modelling: a case study of the ‘Jackpot’ strong lens74
Cloud properties and star formation in M3173
White dwarf pollution: one star or two?73
Blending-induced beating and emission in the symbiotic star Terz V 251373
Deciphering cometary outbursts: linking gas composition changes to trigger mechanisms73
A detailed chemical study of the extreme velocity stars in the galaxy73
Searching for globular clusters in the inner halo of the Circinus galaxy73
Partially ionized two-fluid shocks with collisional and radiative ionization and recombination – multilevel hydrogen model73
The H α luminosity and stellar mass dependent clustering of star-forming galaxies at 0.7 < z < 1.5 with 3D-HST72
Formation of millisecond pulsars with wide orbits72
Inferring system parameters from the bursts of the accretion-powered pulsar IGR J17498–292172
A differentiable perturbation-based weak lensing shear estimator71
Correction to: Galaxy source counts at 7.7 μm, 10 μm and 15 μm with the james webb space telescope71
Spectroscopic confirmation of high-amplitude eruptive YSOs and dipping giants from the VVV survey71
Revisiting multiwavelength data on the supersoft X-ray source CAL 8371
Simulating the deposition of angular momentum by jets in common envelope evolution71
Modelling solar coronal magnetic fields with physics-informed neural networks70
Effects of feedback on galaxies in the VELA simulations: elongation, clumps, and compaction70
XMM–Newton: X-ray emission analysis of SNR N63A and surrounding regions in the LMC70
Bondi–Hoyle–Lyttleton accretion flow in a stratified layer70
StarUnLink: identifying and mitigating signals from communication satellites in stellar spectral surveys70
The PARADIGM project – I. How early merger histories shape the present-day sizes of Milky-Way-mass galaxies70
Phase curve wavelength dependency as revealed by shape- and geometry- corrected asteroid phase curves70
Kinematics of supernova remnants in the galaxy NGC 694669
The Tully–Fisher relation and the Bosma effect69
Identifying evolutionary stages of molecular clumps through unsupervised and supervised machine learning69
Did Kepler-444 have a long-lived convective core?69
Eclipse timing variations in seven post-common envelope binaries: an update and analysis of their recently proposed circumbinary models69
Insights into the 21 cm field from the vanishing cross-power spectrum at the epoch of reionization68
A fast-cadenced search for gamma-ray burst orphan afterglows with the Deeper, Wider, Faster programme68
Imaging and spectroscopic observations of a confined solar filament eruption with two-stage evolution68
JWST /MIRI coronagraphic search for planets in systems with gapped exoKuiper belts and proper-motion anomalies68
Observational signatures of circumbinary discs – I. Kinematics68
In situ ionospheric observations near lunar south pole by the Langmuir Probe on Chandrayaan-3 lander67
Investigation on the orbital period variations of NN Ser: implications for the hypothetical planets, the Applegate mechanism, and the orbital stability67
A pristine view of galactic globular clusters and their peripheries: Omega Centauri66
On the origin of the evolution of the halo occupation distribution66
Machine-learning enhanced photometric analysis of the extremely bright GRB 210822A66
The missing radial velocities of Gaia: a catalogue of Bayesian estimates for DR366
Mixing bispectrum multipoles under geometric distortions66
Cometary ion drift energy and temperature at comet 67P/Churyumov–Gerasimeko66
Opacities of dense gas tracers in galactic massive star-forming regions66
I Zw 1 and H0557-385: the dusty tori of two high Eddington AGNs observed in the MATISSE LM bands65
Analysis of a thermal correction method for infrared spectroscopy: preparation for the future observations of the Martian moons Phobos and Deimos with the MIRS instrument65
Decoding the thermal history of the merging cluster Cygnus A65
GRB 201015A: from seconds to months of optical monitoring and supernova discovery65
Resistive heating induced by streaming cosmic rays around a galaxy in the early Universe65
Evidence of extended cold molecular gas and dust haloes around z ~ 2.3 extremely red quasars with ALMA64
Constraining SN Ia progenitors from the observed Fe-peak elemental abundances in the Milky Way dwarf galaxy satellites64
Gravitational potential drives the concentration dependence of the stellar mass–halo mass relation64
Activity in white dwarf debris discs I: Spitzer legacy reveals variability incompatible with the canonical model64
On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 − 280764
Narrowing the discovery space of the cosmological 21-cm signal using multi-wavelength constraints64
The evolution of radial gradients of MaNGA quiescent elliptical galaxies: inside-out quenching or outer mass growth?64
A multizone view on the multiwavelength emission of blazars64
Galaxy assembly bias in cosmological hydrodynamical simulations – a comparison between SIMBA and illustris TNG63
Chromosome maps of globular clusters from wide-field ground-based photometry63
The LOFAR Two-metre Sky Survey: The nature of the faint source population and SFR–radio luminosity relation using prospector 63
Detection of 125.5-day optical periodic modulation of the neutron star M51 ULX-863
Imprints of supermassive black hole evolution on the spectral and spatial anisotropy of nano-hertz stochastic gravitational-wave background63
A flash of polarized optical light points to an aspherical ‘cow’63
Chemical evolution of fluorine in the Milky Way63
Chemical abundances of LINER galaxies – nitrogen abundance estimations63
MeerKAT radio observations of the neutron star low-mass X-ray binary Cen X–4 at low accretion rates62
Machine-guided exploration and calibration of astrophysical simulations62
The nature of very-faint X-ray binaries: near-infrared spectroscopy of 1RXH J173523.7−354013 reveals a giant companion62
The MAGPI survey: evidence against the bulge–halo conspiracy62
KURVS: the outer rotation curve shapes and dark matter fractions of z ∼ 1.5 star-forming galaxies61
γ-ray detection from occasional flares in T Tauri stars of NGC 2071 – I. Observational connection61
Improving and extending non-Poissonian distributions for satellite galaxies sampling in HOD: applications to eBOSS ELGs61
Testing colour–magnitude pattern as a method in the search for changing-look AGNs61
The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA61
The integrated radio spectrum of G2.4+1.460
Evolution of parsec-scale jet directions in active galaxies60
Spectroscopy of a sample of unidentified gamma-ray Fermi sources60
Constraining a relativistic mean field model using neutron star mass–radius measurements I: nucleonic models60
Radiation hydrodynamic simulations for the origin of quasi-periodic oscillations for accretion onto supermassive black holes59
OzDES Reverberation Mapping Program: Stacking analysis with Hβ, Mg ii, and C iv59
Dynamical instabilities in post-disc evolution: hot Jupiters left isolated59
Long-time 2D simulations of fallback supernovae: a systematic investigation of explosions dynamics and mass ejection59
A bright wideband radio burst from the isolated neutron star 2XMM J104608.7−59430659
Constraining modified gravity with weak-lensing peaks58
Improved constraints on Galactic Centre ejection of hypervelocity stars based on novel search method58
Gaseous methanol in cold environments: is thermal desorption from low binding energy sites the explanation?58
Investigation of the correlation between optical and γ-ray flux variations in the blazar Ton 59958
On the role of minor neutrals in determining the characteristic features of the Venus ionosphere at low altitudes58
Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations58
Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ∼ 0.8 with BOSS and DESI58
An ancient system hidden in the Galactic plane?58
Population synthesis of hot subdwarf B stars with COMPAS: on the observed Galactic population58
The progenitors of the intra-cluster light and intra-cluster globular clusters in galaxy groups and clusters58
Zonal winds in the gas planets driven by convection above a stably stratified layer58
Restoring cosmological concordance with early dark energy and massive neutrinos?58
Observation of a propagating slow magnetoacoustic wave in a coronal plasma fan with SDO/AIA and SolO/EUI58
BayeSN and SALT: a comparison of dust inference across SN Ia light-curve models with DES5YR57
A simple method to measure νmax for asteroseismology: application to 16 000 oscillating Kepler red giants57
The dark energy survey 5-yr photometrically identified type Ia supernovae57
A regularization technique to precisely infer limb darkening using transit measurements: can we estimate stellar surface magnetic fields?57
Measuring Galactic dark matter through unsupervised machine learning57
The bright end of the galaxy luminosity function at z ≃ 7 from the VISTA VIDEO survey56
Carbon–oxygen ultra-massive white dwarfs in general relativity56
JADES: comprehensive census of broad-line AGN from reionization to cosmic noon revealed by JWST56
All-sky three-dimensional dust density and extinction Maps of the Milky Way out to 2.8 kpc56
Reconstructing cosmological initial conditions from late-time structure with convolutional neural networks56
Stellar cluster formation in a Milky Way-sized galaxy at z > 4 – I. The proto-globular cluster population and the imposter amongst us56
Galactic seismology: can the Gaia ‘phase spiral’ co-exist with a clumpy, turbulent interstellar medium?56
A chemodynamical analysis of bright metal-poor stars from the HESP-GOMPA survey – indications of a non-prevailing site for light r-process elements56
Mapping the Milky Way with LAMOST – IV. The large Galactic disc extending to 35 kpc56
Alleviating the Hubble tension using the Barrow holographic dark energy cosmology with Granda–Oliveros IR cut-off56
The critical role of nuclear heating rates, thermalization efficiencies, and opacities for kilonova modelling and parameter inference56
The Pristine Inner Galaxy Survey (PIGS) – IV. A photometric metallicity analysis of the Sagittarius dwarf spheroidal galaxy56
On the interaction of pebble accreting embryos with the gaseous disc: importance of thermal forces55
Measuring and unbiasing the BAO shift in the Ly α forest with AbacusSummit55
PM2.5 as a proxy for aerosol optical depth in night sky brightness models55
Partition function approach to non-Gaussian likelihoods: formalism and expansions for weakly non-Gaussian cosmological inference55
The Herschel-SPIRE Dark Field I: the deepest Herschel image of the submillimetre Universe55
Jellyfish galaxies with the IllustrisTNG simulations - No enhanced population-wide star formation according to TNG5055
Wind-fed GRMHD simulations of Sagittarius A*: tilt and alignment of jets and accretion discs, electron thermodynamics, and multiscale modelling of the rotation measure55
Photometric characterization and trajectory accuracy of Starlink satellites: implications for ground-based astronomical surveys55
Emission line tracers of galactic outflows driven by stellar feedback in simulations of isolated disc galaxies55
ExoMol photodissociation cross-sections – III. Temperature-dependent photodissociation and photoabsorption spectra for NH55
X-ray absorption lines in FUV-detected quasars – II. Cosmological density and properties of the missing baryons55
Survey of radiative, two-temperature magnetically arrested simulations of the black hole M87* I: turbulent electron heating55
A universal relationship between the variability time-scale and black hole mass in black hole jetted and non-jetted accreting systems54
Revisiting the properties of GW190814 and its formation history54
Direct collapse of exceptionally heavy black holes in the merger-driven scenario54
Optical spectroscopy of blazars for the Cherenkov Telescope Array – II54
AGN flares as counterparts to LIGO/Virgo mergers: no confident causal connection in spatial correlation analysis54
Global asteroseismology of 19 000 red giants in the TESS Continuous Viewing Zones54
When, where, and how many planets end up in first-order resonances?54
Lofting of low-speed ejecta produced in the DART experiment and production of a dust cloud54
Diversity of SEDs among the star-forming regions in NGC 136554
Dwarf galaxy discoveries from the KMTNet supernova programme – III. The Milky-Way analogue NGC 2997 group54
Shedding far-ultraviolet light on the donor star and evolutionary state of the neutron-star LMXB Swift J1858.6−081453
The stability of Prendergast magnetic fields53
Probing cosmic isotropy in the Local Universe53
Evidence for relativistic Sunyaev–Zeldovich effect in Planck CMB maps with an average electron-gas temperature of Te ≃ 5 keV53
Gas-phase formation route for trans-HC(O)SH and its isomers under interstellar conditions: a state-of-the-art quantum-chemical study53
A multiwavelength study of nearby star-forming spiral galaxies and the clustering of star formation in M6353
Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy53
Influence of planets on debris discs in star clusters – II. The impact of stellar density53
The no-hair theorems at work in M87*53
Time-varying Na iD absorption in ILRTs as a probe of circumstellar material53
Isolated and dynamical black hole mergers withB-POP: the role of star formation and dynamics, star cluster evolution, natal kicks, mass and spins, and hierarchical mergers52
Under the glare of a luminous quasar, the FIR continuum is still an excellent tracer of the ISM down to the central kiloparsec52
Merger histories of brightest group galaxies from MUSE stellar kinematics52
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