Publications of the Astronomical Society of Australia

Papers
(The TQCC of Publications of the Astronomical Society of Australia is 3. 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 2021-05-01 to 2025-05-01.)
ArticleCitations
Multimessenger astronomy with a kHz-band gravitational-wave observatory115
Evolution of the magnetic field and flows of solar active regions with persistent magnetic bipoles before emergence57
Low-frequency pulse-jitter measurement with the uGMRT I: PSR J0437–471554
The Evolutionary Map of the Universe Pilot Survey – ADDENDUM53
A search for 3-mm molecular absorption line transitions in the magellanic stream47
Comparison of Gaia and Hipparcos parallaxes of close visual binary stars and the impact on determinations of their masses – ADDENDUM35
The dusty aftermath of a rapid nova: V5579 Sgr34
A commensal Fast Radio Burst search pipeline for the Murchison Widefield Array29
EMU/GAMA: A technique for detecting active galactic nuclei in low mass systems27
Adaptive particle refinement for compressible smoothed particle hydrodynamics22
The Rapid ASKAP Continuum Survey V: Cataloguing the sky at 1 367.5 MHz and the second data release of RACS-mid18
Measuring the global 21-cm signal with the MWA-II: improved characterisation of lunar-reflected radio frequency interference16
A geometric view of closure phases in interferometry16
The Rapid ASKAP Continuum Survey III: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) first data release14
Understanding the impact of diffusion of CO in the astrochemical models14
VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies12
Searching for the Synchrotron Cosmic Web Again: A replication attempt – ADDENDUM12
Second-generation planet formation after tidal disruption from common envelope evolution12
On the existence of ‘Maia variables’11
Investigating unusual Hα features towards the Scutum Supershell11
Beamforming approaches towards detecting the 21-cm global signal from Cosmic Dawn with radio array telescopes11
FIGARO Simulation: FIlaments & GAlactic RadiO Simulation – ADDENDUM10
New radio continuum study of the large magellanic cloud supernova remnant N4910
Long-term spin-down and low luminosity regime in the Be/X-ray binary pulsar GX 304-110
The thermal history of the intergalactic medium at 3.9 ≤ z ≤ 4.310
On the collisional sensitivity of polarised Mg II solar lines10
Fast as Potoroo: Radio continuum detection of a bow-shock pulsar wind nebula powered by pulsar J1638–471310
Predicting the scaling relations between the dark matter halo mass and observables from generalised profiles I: Kinematic tracers9
A search for annihilating dark matter in 47 Tucanae and Omega Centauri8
SimSpin v2.6.0—constructing synthetic spectral IFU cubes for comparison with observational surveys8
Orbit determination of visual binary systems observed with CST telescope in 2010–20138
21-cm Epoch of reionisation power spectrum with closure phase using the Murchison Widefield Array8
Self-supervised contrastive learning of radio data for source detection, classification and peculiar object discovery7
MWA rapid follow-up of gravitational wave transients: Prospects for detecting prompt radio counterparts7
The Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys7
WALLABY pilot survey: Public release of H i data for almost 600 galaxies from phase 1 of ASKAP pilot observations7
The angular correlation function as measured by the GLEAM-X survey7
RadioGalaxyNET: Dataset and novel computer vision algorithms for the detection of extended radio galaxies and infrared hosts7
WALLABY Pilot Survey: Public release of HI kinematic models for more than 100 galaxies from phase 1 of ASKAP pilot observations7
Intensity correlation functions of microwave maser sources7
The non-thermal emission from the colliding-wind binary Apep6
Estimating stellar parameters and identifying very metal-poor stars for low-resolution spectra (R∼ 200)6
Design of a high-resolution antenna array solar observing system for radio frequencies of 25–110 MHz6
The First Large Absorption Survey in Hi(FLASH): I. Science goals and survey design5
Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Lyα forest data5
The MAGPI Survey: Insights into the Lyα line widths and the size of ionised bubbles at the edge of cosmic reionisation5
Probing the soft X-ray properties and multi-wavelength variability of SN2023ixf and its progenitor5
Intranight optical monitoring of the rare quasar J0950+5128, the brightest known candidate for transition from radio-quiet to radio-loud state5
Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation – CORRIGENDUM5
The global structure of astrospheres: Effect of Knudsen number5
A jet-induced shock in a young, powerful radio galaxy at z = 3.005
Studying the internal structures of the central region of prestellar core L1517B in Taurus molecular cloud using ammonia (NH3) (1,1) and (2,2) lines4
Galaxy 3D shape recovery using mixture density network4
Baseline correction for FAST radio recombination lines: A modified penalised least squares smoothing technique4
The transience and persistence of high optical polarisation state in beamed radio quasars4
Strategy for mitigation of systematics for EoR experiments with the Murchison Widefield Array4
Dashing through the cluster: An X-ray to radio view of UGC 10420 undergoing ram-pressure stripping4
A measurement of small-scale features using ionospheric scintillation. Comparison with refractive shift measurements4
Predicting Sunyaev-Zel’dovich effect observations of galaxy cluster cavities with the Square Kilometre Array4
Semi-empirical calibration of the oxygen abundance for LINER galaxies based on SDSS-IV MaNGA – The case for strong and weak AGN4
Deblending overlapping galaxies in DECaLS using transformer-based algorithm: A method combining multiple bands and data types4
Constraining the link between the 2175Å dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI4
Inviscid protostellar disc ring formation and high-density ring edges due to the ejection and subsequent infall of material onto a protostellar disc3
System design and validation of Central Redundant Array Mega-tile (CRAM)3
Modelling DSA, FAST, and CRAFT surveys in a z-DM analysis and constraining a minimum FRB energy3
Spectral analysis of 22 radio pulsars using SKA-Low precursor stations3
Angular momentum and energy transport in disc–jet systems: Unravelling the contribution of saturated thermal conduction3
When models fail: An introduction to posterior predictive checks and model misspecification in gravitational-wave astronomy3
Less wound and more asymmetric: JWST confirms the evolution of spiral structure in galaxies at $z \lesssim 3$3
Hydra II: Characterisation of Aegean, Caesar, ProFound, PyBDSF, and Selavy source finders3
Altitude estimation of radio frequency interference sources via interferometric near-field corrections3
A search for technosignatures toward the Galactic Centre at 150 MHz3
Statistical analysis of kicked black holes from TNG300 simulation3
Non-Gaussianity of optical emission lines in SDSS star-forming galaxies and its implications on galactic outflows3
Thefhdpolarised imaging pipeline: A new approach to widefield interferometric polarimetry3
GNOMES II: Analysis of the Galactic diffuse molecular ISM in all four ground state hydroxyl transitions usingAmoeba3
Bayesian evidence-driven diagnosis of instrumental systematics for sky-averaged 21-cm cosmology experiments3
WALLABY Pilot Survey: HI source-finding with a machine learning framework3
High-time resolution GPU imager for FRB searches at low radio frequencies3
System design and calibration of SITARA—a global 21 cm short spacing interferometer prototype3
Classical novae in the ASKAP pilot surveys3
Discovery of peculiar radio morphologies with ASKAP using unsupervised machine learning3
Effects of angular scattering and H+p, H+H collisions on the properties of interstellar atoms in the heliosphere3
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