The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

Abstract

The Murchison Widefield Array (MWA) is one of three Square Kilometre Array Precursor telescopes and is located at the Murchison Radio-astronomy Observatory in the Murchison Shire of the mid-west of Western Australia, a location chosen for its extremely low levels of radio frequency interference. The MWA operates at low radio frequencies, 80-300 MHz, with a processed bandwidth of 30.72 MHz for both linear polarisations, and consists of 128 aperture arrays (known as tiles) distributed over a ~3 km diameter area. Novel hybrid hardware/software correlation and a real-time imaging and calibration systems comprise the MWA signal processing backend. In this paper the as-built MWA is described both at a system and sub-system level, the expected performance of the array is presented, and the science goals of the instrument are summarised.

Submitted to PASA. 11 figures, 2 tables

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• The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources
• Quantifying ionospheric effects on time-domain astrophysics with the Murchison Widefield Array
• Spectral performance of SKA Log-periodic Antennas I: Mitigating spectral artefacts in SKA1-LOW 21-cm cosmology experiments
• Hoinga: A supernova remnant discovered in the SRG/eROSITA All-Sky Survey eRASS1
• A method to determine the evolution history of the mean neutral Hydrogen fraction
• LOFAR early-time search for coherent radio emission from Short GRB 181123B
• The low-frequency characteristics of PSR J0437-4715 observed with the Murchison Widefield Array
• Inferring the properties of the sources of reionization using the morphological spectra of the ionized regions
• Cluster Mergers and the Origin of the ARCADE-2 Excess
• Quantifying weak non-thermal solar radio emission at low radio frequencies
• Primordial Non-Gaussianity Estimation using 21 cm Tomography from the Epoch of Reionization
• Baseline Dependent Averaging in Radio Interferometry
• The active region source of a type III radio storm observed by Parker Solar Probe during Encounter 2
• Pulsar revival in neutron star mergers: multi-messenger prospects for the discovery of pre-merger coherent radio emission
• Detecting the 21 cm Forest in the 21 cm Power Spectrum
• Canceling out intensity mapping foregrounds
• The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue
• The Murchison Widefield Array: solar science with the low frequency SKA Precursor
• A Census of Southern Pulsars at 185 MHz
• Improved treatments of the ionizing photon mean free path in semi-numerical simulations of reionization
• Modeling the afterglow of the possible Fermi-GBM event associated with GW150914
• Propagation Effects in Quiet Sun Observations at Meter Wavelengths
• Measuring the global 21-cm signal with the MWA-I: improved measurements of the Galactic synchrotron background using lunar occultation
• ARTIST: Fast radiative transfer for large-scale simulations of the epoch of reionisation
• Detection of Cosmic Structures using the Bispectrum Phase. II. First Results from Application to Cosmic Reionization Using the Hydrogen Epoch of Reionization Array
• A survey of spatially and temporally resolved radio frequency interference in the FM band at the Murchison Radio-astronomy Observatory
• The Morphology of Reionization in a Dynamically Clumpy Universe
• Noise Temperature of Phased Array Radio Telescope: The Murchison Widefield Array and the Engineering Development Array
• PySE: Software for Extracting Sources from Radio Images
• Exploring the evolution of Reionisation using a wavelet transform and the light cone effect
• Self-triggered radio detection and identification of cosmic air showers with the OVRO-LWA
• A study of halo and relic radio emission in merging clusters using the Murchison Widefield Array
• Inferring Astrophysics and Dark Matter Properties from 21cm Tomography using Deep Learning
• The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability
• Extracting the 21 cm EoR signal using MWA drift scan data
• The impact of non-Gaussianity on the Epoch of Reionization parameter forecast using 21-cm power spectrum measurements
• Modelling and peeling extended sources with shapelets: a Fornax A case study
• Measuring HERA's primary beam in-situ: methodology and first results
• A Halo Model Approach to the $21\mathrm{cm}$ and $\mathrm{Ly}\alpha$ Cross-correlation
• Astronomical verification of a stabilized frequency reference transfer system for the Square Kilometre Array
• Low-frequency pulse profile variation in PSR B2217+47: evidence for echoes from the interstellar medium
• Probing pulsar scattering between 120 and 280 MHz with the MWA
• 21cmfish: Fisher-matrix framework for fast parameter forecasts from the cosmic 21-cm signal
• Statistical recovery of 21cm visibilities and their power spectra with Gaussian constrained realisations and Gibbs sampling
• Ultra-Steep Spectrum Radio `Jellyfish' Uncovered in Abell 2877
• On the mechanism of polarised metrewave stellar emission
• Constraints on dark matter annihilation in dwarf spheroidal galaxies from low frequency radio observations
• Artificial intelligence for celestial object census: the latest technology meets the oldest science
• A unified framework for 21cm tomography sample generation and parameter inference with Progressively Growing GANs
• The Impact of Beam Variations on Power Spectrum Estimation for 21-cm Cosmology I: Simulations of Foreground Contamination for HERA
• Stars and Reionization: The Cross-Correlation of the 21cm Line and the Near Infrared Background
• Strategies for Finding Prompt Radio Counterparts to Gravitational Wave Transients with the Murchison Widefield Array
• Extracting the 21-cm Power Spectrum and the reionization parameters from mock datasets using Artificial Neural Networks
• IslandFAST: A Semi-numerical Tool for Simulating the Late Epoch of Reionization
• LOFAR early-time search for coherent radio emission from GRB 180706A
• Expected constraints on models of the epoch of reionization with the variance and skewness in redshifted 21cm-line fluctuations
• Imaging-spectroscopy of a band-split type II solar radio burst with the Murchison Widefield Array
• A Serendipitous MWA Search for Narrow-band and Broad-band Low Frequency Radio Transmissions from 1I/2017 U1 'Oumuamua
• The most probable host of CHIME FRB 190425A, associated with binary neutron star merger GW190425, and a late-time transient search
• Low Radio Frequency Observations and Spectral Modelling of the Remnant of Supernova 1987A
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology
• Extreme scattering events from axisymmetric plasma lenses
• Learning from FITS: Limitations in use in modern astronomical research
• Improved Techniques for the Surveillance of the Near Earth Space Environment with the Murchison Widefield Array
• Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
• An Improved Statistical Point-Source Foreground Model for the Epoch of Reionization
• Optimal survey parameters: Ly$\alpha$ and H$\alpha$ intensity mapping for synergy with the 21cm signal during reionization
• MWA Tied-Array Processing I: Calibration and Beamformation
• Exploring the circular polarisation of low-frequency solar radio bursts with LOFAR
• A Generic and Efficient E-field Parallel Imaging Correlator for Next-Generation Radio Telescopes
• Murchison Widefield Array Observations of Anomalous Variability: A Serendipitous Night-time Detection of Interplanetary Scintillation
• Limits on radio emission from meteors using the MWA
• Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe
• New Limits on the Low-frequency Radio Transient Sky Using 31 hr of All-sky Data with the OVRO-LWA
• Spectral Structures and Their Generation Mechanisms for Solar Radio Type-I Bursts
• MeerTRAP: Twelve Galactic fast transients detected in a real-time, commensal MeerKAT survey
• The Electromagnetic Characteristics of the Tianlai Cylindrical Pathfinder Array
• Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization
• Low Frequency Carbon Radio Recombination Lines II: The Diffuse Interstellar Medium
• Galactic synchrotron distribution derived from 152 HII region absorption features in the full GLEAM survey
• Role of Thermal and Non-thermal Processes in the ISM of Magellanic Clouds
• The remnant radio galaxy associated with NGC 1534
• A search for Extraterrestrial Intelligence (SETI) toward the Galactic Anticenter with the Murchison Widefield Array
• The Hydrogen Epoch of Reionization Array Dish III: Measuring Chromaticity of Prototype Element with Reflectometry
• A MeerKAT-meets-LOFAR study of Abell 1413: a moderately disturbed non-cool-core cluster hosting a $\sim 500$ kpc 'mini'-halo
• Discovery of a steep-spectrum low-luminosity pulsar with the Murchison Widefield Array
• Evidence of Ultra-faint Radio Frequency Interference in Deep 21~cm Epoch of Reionization Power Spectra with the Murchison Widefield Array
• Interplanetary Scintillation with the Murchison Widefield Array V: An All-sky Survey of Compact Sources using a Modern Low-frequency Radio Telescope
• Methods of Error Estimation for Delay Power Spectra in $21\text{cm}$ Cosmology
• Discovering the Sky at the Longest Wavelengths with Small Satellite Constellations
• Discovery of correlated evolution in solar noise storm source parameters: Insights on magnetic field dynamics during a microflare
• Murchison Widefield Array Limits on Radio Emission from ANTARES Neutrino Events
• Characterising coronal turbulence using snapshot imaging of radio bursts in 80-200 MHz
• Controlling Rayleigh-Backscattering-Induced Distortion in Radio over Fiber Systems for Radioastronomic Applications
• Rates, Flux Densities, and Spectral Indices of Meteor Radio Afterglows
• Beamforming Errors in Murchison Widefield Array Phased Array Antennas and their effects on Epoch of Reionization Science
• Ionospheric modelling using GPS to calibrate the MWA. 1: Comparison of first order ionospheric effects between GPS models and MWA observations
• Detection of a Low-frequency Cosmic Radio Transient Using Two LWA Stations
• A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260< l <\340
• The merging galaxy cluster Abell 3266 at low radio frequencies
• Scalable precision wide-field imaging in radio interferometry: I. uSARA validated on ASKAP data
• Comparison of observing modes for statistical estimation of the 21cm signal from the Epoch of Reionisation
• High-resolution Observations of Low-luminosity Gigahertz-Peaked Spectrum and Compact Steep Spectrum Sources
• Tackling the Unique Challenges of Low-frequency Solar Polarimetry with the Square Kilometre Array Low Precursor: The Algorithm
• The spin-temperature dependence of the 21cm -- LAE cross-correlation
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Investigating ionospheric calibration for LOFAR 2.0 with simulated observations
• Low-frequency observations of the Giant Radio Galaxy NGC 6251
• 21cmSense v2: A modular, open-source 21cm sensitivity calculator
• A fast and exact $w$-stacking and $w$-projection hybrid algorithm for wide-field interferometric imaging
• Exploring the cosmic dawn and epoch of reionization with 21cm line
• Identifying Ionized Regions in Noisy Redshifted 21 cm Data Sets
• The Tianlai dish array low-z surveys forecasts
• Detecting the non-Gaussianity of the 21-cm signal during reionisation with the Wavelet Scattering Transform
• Probing early universe through redshifted 21-cm signal: Modelling and observational challenges
• Blazar jet evolution revealed by multi-epoch broadband radio polarimetry
• Hunting for radio emission from the intermittent pulsar J1107-5907 at low frequencies
• Direction Dependent Corrections in Polarimetric Radio Imaging II: A-Solver Methodology A low-order solver for the A-Term of the A-Projection algorithm
• Spectral performance of Square Kilometre Array Antennas II: Calibration performance
• The GLEAMing of the First Supermassive Black Holes
• Deep-Learning Study of the 21cm Differential Brightness Temperature During the Epoch of Reionization
• J1615+5452: a remnant radio galaxy in the ELAIS-N1 field
• The 21-cm signals from ultracompact minihalos as a probe of primordial small-scale fluctuations
• Dual Polarization Measurements of MWA Beampatterns at 137 MHz
• Cold-Source Noise Measurement of a Differential Input Single-Ended Output Low-Noise Amplifier Connected to a Low-Frequency Radio Astronomy Antenna
• Imaging Spectroscopy of CME-Associated Solar Radio Bursts
• On Solar Recurrent Coronal Jets: Coronal Geysers as Sources of Electron Beams and Interplanetary Type-III Radio Bursts
• The Impact of Realistic Foreground and Instrument Models on 21cm Epoch of Reionization Experiments
• Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA
• Physics Beyond The Standard Model with Circular Polarization in the CMB and CMB-21cm Cross-Correlation
• Quantifying Density-Ionization Correlations with the 21cm Power Spectrum
• Forecasts and Statistical Insights for Line Intensity Mapping Cross-Correlations: A Case Study with 21cm x [CII]
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• Density duct formation in the wake of a travelling ionospheric disturbance: Murchison Widefield Array observations
• The Expanded Giant Metrewave Radio Telescope
• Calibration Requirements for Epoch of Reionization 21-cm signal observations -- I. Effect of time-correlated gains
• Impact of instrument and data characteristics in the interferometric reconstruction of the 21 cm power spectrum
• Extracting the Global 21-cm signal from Cosmic Dawn and Epoch of Reionization in the presence of Foreground and Ionosphere
• Improved Sensitivity for Space Domain Awareness Observations with the Murchison Widefield Array
• Wide-Band Spectral Variability of Peaked Spectrum Sources
• Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
• Generating extremely large-volume reionisation simulations
• A polarimetric approach for constraining the dynamic foreground spectrum for cosmological global 21-cm measurements
• Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR
• Probing the magnetosphere of the M8.5 dwarf TVLM513-46546 by modelling its auroral radio emission. Hint of star exoplanet interaction?
• Detectability of 21cm-signal during the Epoch of Reionization with 21cm-Lyman-α emitter cross-correlation. II. Foreground contamination
• Persistent topology of the reionization bubble network. II: Evolution & Classification
• 21-cm signatures of residual HI inside cosmic HII regions during reionization
• Constraining the Radio Properties of the $z$=6.44 QSO VIK J2318$-$3113
• Simultaneous Observations of Giant Pulses from the Crab Pulsar, with the Murchison Widefield Array and Parkes Radio Telescope: Implications for the Giant Pulse Emission Mechanism
• The Role of the Instrumental Response in 21 cm EoR Power Spectrum Gridding Analyses
• LOFAR Deep Fields: Probing a broader population of polarized radio galaxies in ELAIS-N1
• Implications of the $z>5$ Lyman-$\alpha$ forest for the 21-cm power spectrum from the epoch of reionization
• Bayesian approach to constraining the properties of ionized bubbles during reionization
• Wavelet Based Statistics for Enhanced 21cm EoR Parameter Constraints
• Statistical Detection of IGM Structures during Cosmic Reionization using Absorption of the Redshifted 21 cm line by HI against Compact Background Radio Sources
• Extracting the Signal of Cosmic String Wakes from 21-cm Observations
• Exploring the consequences of chromatic data excision in 21-cm Epoch of Reionization power spectrum observations
• A Space-based Decametric Wavelength Radio Telescope Concept
• The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
• The spectacular cluster chain Abell 781 as observed with LOFAR, GMRT, and XMM-Newton
• A galaxy-free phenomenological model for the 21-cm power spectrum during reionization
• Multifrequency study of a double-double radio galaxy J0028+0035
• All Sky Modelling Requirements for Bayesian 21 cm Power Spectrum Estimation with BayesEoR
• Discovery of large-scale diffuse radio emission and of a new galaxy cluster in the surroundings of MACSJ0520.7-1328
• Ionospheric Modelling using GPS to Calibrate the MWA. II: Regional ionospheric modelling using GPS and GLONASS to estimate ionospheric gradients
• Probing the primordial Universe with 21-cm line from cosmic dawn/epoch of reionization
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• SKA-Low Intensity Mapping Pathfinder Updates: Deeper 21 cm Power Spectrum Limits from Improved Analysis Frameworks
• Reflections and Standing Waves on the Tianlai Cylinder Array
• MID-Radio Telescope, Single Pixel Feed Packages for the Square Kilometre Array: An Overview
• Detection of weak ubiquitous impulsive nonthermal emissions from the solar corona
• Investigating the Contribution of Extended Radio Sources to the Epoch of Reionisation Power Spectrum
• Covariant polarized radiative transfer on cosmological scales for investigating large-scale magnetic field structures
• Antenna Design and Implementation for the Future Space Ultra-Long Wavelength Radio Telescope
• Two-dimensional Topology of Cosmological Reionization
• Radio Sources Segmentation and Classification with Deep Learning
• A First Look for Molecules between 103 and 133 MHz using the Murchison Widefield Array
• A Matched Filter Technique For Slow Radio Transient Detection And First Demonstration With The Murchison Widefield Array
• The Zadko Telescope: Exploring the transient Universe
• The MHz-peaked radio spectrum of the unusual gamma-ray source PMN J1603-4904
• Insights from snapshot spectroscopic radio observations of a weak Type I noise storm
• Detection and Characterisation of a Coronal Mass Ejection using Interplanetary Scintillation measurements from the Murchison Widefield Array
• Optimal, fast, and robust inference of reionization-era cosmology with the 21cmPIE-INN
• Synergizing 21 cm and sub-millimetre surveys during reionization: new empirical insights
• MeerKAT follow-up of enigmatic GLEAM 4-Jy (G4Jy) sources
• Probing delayed-end reionization histories with the 21cm-LAE cross-power spectrum
• The HI Bias during the Epoch of Reionization
• The Murchison Widefield Array Transients Survey (MWATS). A search for low frequency variability in a bright Southern hemisphere sample
• Fisher Matrix Based Predictions for Measuring the z = 3.35 Binned 21-cm Power Spectrum using the Ooty Wide Field Array (OWFA)
• Sensitivity of a Low-Frequency Polarimetric Radio Interferometer
• LOFAR 144-MHz follow-up observations of GW170817
• Detection of Cosmic Structures using the Bispectrum Phase. I. Mathematical Foundations
• A Search for Technosignatures toward the Galactic Centre at 150 MHz
• MWA tied-array processing III: Microsecond time resolution via a polyphase synthesis filter
• Contribution of Radio Halos to the Foreground for SKA EoR Experiments
• Robust absolute solar flux density calibration for the Murchison Widefield Array
• Characterization of unresolved and unclassified sources detected in radio continuum surveys of the Galactic plane
• Low(er) frequency follow-up of 28 candidate, large-scale synchrotron sources
• Radio Galaxy Zoo EMU: Towards a Semantic Radio Galaxy Morphology Taxonomy
• Working Principle of the Calibration Algorithm for High Dynamic Range Solar Imaging with Square Kilometre Array Precursor
• Redundant interferometric calibration as a complex optimization problem
• First measurement of interplanetary scintillation with the ASKAP radio telescope: implications for space weather
• Calculating transient rates from surveys
• Non-Gaussianity of diffuse Galactic synchrotron emission at 408 MHz
• Modeling the Ionosphere with GPS and Rotation Measure Observations
• The precision and accuracy of early Epoch of Reionization foreground models: comparing MWA and PAPER 32-antenna source catalogs
• LEAP: An Innovative Direction Dependent Ionospheric Calibration Scheme for Low Frequency Arrays
• A high time resolution study of the millisecond pulsar J2241-5236 at frequencies below 300 MHz
• Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < δ< +55o
• The EDGES measurement disfavors an excess radio background during the cosmic dawn
• A multi-resolution, multi-epoch low radio frequency survey of the Kepler K2 mission Campaign 1 field
• The Growing Impact of Unintended Starlink Broadband Emission on Radio Astronomy in the SKA-Low Frequency Range
• Upper Limits on the 21 cm Power Spectrum at z = 5.9 from Quasar Absorption Line Spectroscopy
• Building models for extended radio sources: implications for Epoch of Reionisation science
• An analytical method to simulate the HI 21-cm visibility signal for intensity mapping experiments
• Astrophysical information from the Rayleigh-Jeans Tail of the CMB
• Study of Redshifted HI from the Epoch of Reionization with Drift scan
• An Image-based Tapered Gridded Estimator (ITGE) for the angular power spectrum
• Interplanetary Scintillation studies with the Murchison Wide-field Array IV: The hosts of sub-arcsecond compact sources at low radio frequencies
• Direct Optimal Mapping for 21cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization Array
• A VOEvent based automatic trigger system for the Murchison Widefield Array
• Tackling the Unique Challenges of Low-frequency Solar Polarimetry with the Square Kilometre Array Low Precursor: Pipeline Implementation
• Estimation of HII Bubble Size Distribution from 21cm Power Spectrum with Artificial Neural Networks
• Interactions between the jet and disk wind in a nearby radio intermediate quasar III Zw 2
• Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array
• Detection of fast transients with radio interferometric arrays
• An Iterative Reconstruction Algorithm for Faraday Tomography
• A fast method of reionization parameter space exploration using GPR trained SCRIPT
• Probing the intergalactic medium during the Epoch of Reionization using 21-cm signal power spectra
• Predicting 21cm-line map from Lyman $\alpha$ emitter distribution with Generative Adversarial Networks
• Antisymmetric cross-correlation of line-intensity maps as a probe of reionization
• Collimation of the kiloparsec-scale radio jets in NGC 2663
• Effects of model incompleteness on the drift-scan calibration of radio telescopes
• Detectability of 21cm signal during the Epoch of Reionization with 21cm-Lyman-$\alpha$ emitter cross-correlation. III. Model dependence
• Wide-band Rotation Measure Synthesis
• On the optical counterparts of radio transients and variables
• Challenging interferometric imaging: Machine learning-based source localization from uv-plane observations
• Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experiment
• Strategies for Maximizing Detection Rate in Radio SETI
• Understanding the Impact of Semi-numeric Reionization Models when using CNNs
• A Simultaneous Dual-site Technosignature Search Using International LOFAR Stations
• Multiple Regions of Nonthermal Quasi-Periodic Pulsations during the Impulsive Phase of a Solar Flare
• Testing afterglow models of FRB 200428 with early post-burst observations of SGR 1935+2154
• Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia's Role
• Multi-frequency angular power spectrum of the 21~cm signal from the Epoch of Reionisation using the Murchison Widefield Array
• Exoplanet Radio Transits as a Probe for Exoplanetary Magnetic Fields -- Time-dependent MHD Simulations
• A search for short-term hard X-ray bursts in the direction of the repeating FRB 121102
• Holographic Calibration of Phased Array Telescopes
• Analysing the Epoch of Reionization with three-point correlation functions and machine learning techniques
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• Discovery and follow-up of a quasiperiodically nulling and sub-pulse drifting pulsar with the Murchison Widefield Array
• Unlocking Sensitivity for Visibility-based Estimators of the 21 cm Reionization Power Spectrum
• Measuring the Earth's Synchrotron Emission from Radiation Belts with a Lunar Near Side Radio Array
• Detection of frequency-dependent dispersion measure toward the millisecond pulsar PSR J2241-5236 from contemporaneous wide-band observations
• Pulsar Scintillation Studies with LOFAR: II. Dual-frequency scattering study of PSR J0826+2637 with LOFAR and NenuFAR
• Black holes at cosmic dawn in the redshifted 21cm signal of HI
• Contribution of Galactic free-free emission to the foreground for EoR signal in SKA experiments
• On-sky calibration of a SKA1-low station in the presence of mutual coupling
• Powerful Radio Sources in the Southern Sky. I. Optical Identifications
• Revealing the Unusual Structure of the KAT-7-Discovered Giant Radio Galaxy J0133$-$1302
• Radio Astronomy transformed: Aperture Arrays - Past, Present and Future
• Calibration requirements for Epoch of Reionization 21-cm signal observations -- II. Analytical estimation of the bias and variance with time-correlated residual gains
• A Low Frequency Pilot Survey of Southern HII Regions in the Vela Constellation
• Prospects for Observing High-redshift Radio-loud Quasars in the SKA Era: Paving the Way for 21-cm Forest Observations
• Deciphering Faint Gyrosynchrotron Emission from Coronal Mass Ejection using Spectro-polarimetric Radio Imaging
• Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator II: Cross-polarization power spectrum
• Spectropolarimetric Radio Imaging of Faint Gyrosynchrotron Emission from a CME : A Possible Indication of the Insufficiency of Homogeneous Models
• Dark Ages Radio Explorer Mission: Probing the Cosmic Dawn
• LOFAR detectability of prompt low-frequency radio emission during gamma-ray burst X-ray flares
• Peculiar Radio Structures in the Central Regions of Galaxy Cluster Abell 585
• Line of sight anisotropies in the Cosmic Dawn and EoR 21-cm power spectrum
• Stacking the Synchrotron Cosmic Web with FIGARO
• Comprehensive view on a $z\sim 6.5$ radio-loud QSO: from the radio to the optical/NIR to the X-ray band
• Panoramic optical and near-infrared SETI instrument: optical and structural design concepts
• On improving analytical models of cosmic reionization for matching numerical simulation
• Limits on the validity of the thin-layer model of the ionosphere for radio interferometric calibration
• Robust statistics toward detection of the 21 cm signal from the Epoch of Reionisation
• Message in a Bottle: Unveiling the Magneto-Ionic Complexity of AGNs through the Stokes QU-Fitting Technique
• Imaging results from the legacy GMRT Galaxy Cluster Key Project
• Constraining the 21cm brightness temperature of the IGM at $z$=6.6 around LAEs with the Murchison Widefield Array
• Radio-astronomical Image Reconstruction with Conditional Denoising Diffusion Model
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• The ultimate frontier of 21cm cosmology
• Radiative transfer of Lyman-$\alpha$ photons at cosmic dawn with realistic gas physics
• Resolving moving heliospheric structures using interplanetary scintillation observations with the Murchison Widefield Array
• Radio spectral properties of cores and extended regions in blazars in the MHz regime
• The Redshift Dependence of the Radio Flux of Gamma-Ray Bursts and Their Host Galaxies
• Lyman Alpha Emitters and the 21cm Power Spectrum as Probes of Density-Ionization Correlation in the Epoch of Reionization
• Delay-Weighted Calibration: Precision Calibration for 21 cm Cosmology with Resilience to Sky Model Error
• Optimization and Commissioning of the EPIC Commensal Radio Transient Imager for the Long Wavelength Array
• Why and When to Expect Gaussian Error Distributions in Epoch of Reionization 21-cm Power Spectrum Measurements
• Searching for the largest bound atoms in space
• Design, operation and performance of the PAON4 prototype transit interferometer
• Probing the ionosphere by the pulsar B0950+08 with help of RadioAstron ground-space baselines
• Pre-selection of the Candidate Fields for Deep Imaging of the Epoch of Reionization with SKA1-Low
• Signal of Cosmic Strings in Cross-Correlation of 21-cm Redshift and CMB Polarization Maps
• High time resolution search for prompt radio emission from the long GRB 210419A with the Murchison Widefield Array
• Preparing for Solar and Heliospheric Science with the SKAO: An Indian Perspective
• The Tracking Tapered Gridded Estimator (TTGE) for the power spectrum from drift scan observations
• Is the X-ray bright z = 5.5 quasar SRGE J170245.3+130104 a blazar?
• An interference detection strategy for Apertif based on AOFlagger 3
• Pipeline Collector: gathering performance data for distributed astronomical pipelines
• Search for the Epoch of Reionisation with HERA: Upper Limits on the Closure Phase Delay Power Spectrum
• A Molecular Line Survey around Orion at Low Frequencies with the MWA
• Study of systematics effects on the Cross Power Spectrum of 21 cm Line and Cosmic Microwave Background using Murchison Widefield Array Data
• Aliasing from Galactic Plane Setting in Widefield Radio Interferometry
• A Multi-Frequency Study of the Milky Way-like Spiral Galaxy NGC 6744
• Reionization and Cosmic Dawn: theory and simulations
• A Multifrequency Census of 100 Pulsars below 100 MHz with LWA: A Systematic Study of Flux Density, Spectra, Timing, Dispersion, Polarization, and Its Variation from a Decade of Observations
• The statistics of radio frequency interference propagating from long distances to the Murchison Radio-astronomy Observatory
• Rapid and Late Cosmic Reionization Driven by Massive Galaxies: a Joint Analysis of Constraints from 21-cm, Lyman Line & CMB Data Sets
• Plausible association of distant late M dwarfs with low-frequency radio emission
• Studying the Multi-frequency Angular Power Spectrum of the Cosmic Dawn 21-cm Signal
• The Effect of Interplanetary Scintillation on Epoch of Reionisation Power Spectra
• A prototype for pulsar observations at low radio frequencies using log periodic dipole antennas
• The Low Frequency Perspective on Fast Radio Bursts
• Gamma-ray burst radio afterglows from Population III stars: Simulation methods and detection prospects with SKA precursors
• LOFAR imaging of the solar corona during the 2015 March 20 solar eclipse
• Direct Parameter Inference from Global EoR Signal with Bayesian Statistics
• A search for extended radio emission from selected compact galaxy groups
• Correcting for the solar wind in pulsar timing observations: the role of simultaneous a nd l ow-frequency observations
• A Supernova Remnant Counterpart for HESS J1832-085
• Understanding spectral artefacts in SKA-LOW 21-cm cosmology experiments: the impact of cable reflections
• Characterizing Beam Errors for Radio Interferometric Observations of Reionization
• Spectroscopic Imaging of the Sun with MeerKAT: Opening a New Frontier in Solar Physics
• New Insights into Type-I Solar Noise Storms from High Angular Resolution Spectroscopic Imaging with the Upgraded Giant Metrewave Radio Telescope
• Discovery of X-shaped Morphology of the Giant Radio Galaxy GRG 0503-286
• A statistical framework for recovering intensity mapping autocorrelations from crosscorrelations
• Statistical estimation of full-sky radio maps from 21cm array visibility data using Gaussian constrained realizations
• The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
• Deep learning approach for identification of HII regions during reionization in 21-cm observations -- III. image recovery
• Linear Polarization of the 21 cm Line from the Epoch of Reionization
• A new angle for probing field-aligned irregularities with the Murchison Widefield Array
• Powerful Radio Sources in the Southern Sky. II. A SWIFT X-Ray Perspective
• Study of radio transients from the quiet Sun during an extremely quiet time
• The Impact of ionization Morphology and X-ray Heating on the Cosmological 21cm Skew Spectrum
• A strong broadband 21 cm cosmological signal from dark matter spin-flip interactions
• Enhanced detection and identification of satellites using an all-sky multi-frequency survey with prototype SKA-Low stations
• Signature of the interaction between dark sectors in the reionization process
• The population of Galactic supernova remnants in the TeV range
• G321.3-3.9: A new supernova remnant observed with multi-band radio data and in the SRG/eROSITA All-Sky Surveys
• System equivalent flux density of a low-frequency polarimetric phased array interferometer
• Automated Detection of Antenna Malfunctions in Large-N Interferometers: A Case Study with the Hydrogen Epoch of Reionization Array
• Correcting Bandwidth Depolarization by Extreme Faraday Rotation
• Efficient Photo-heating Algorithms in Time-dependent Photo-ionization Simulations
• A targeted search for repeating fast radio bursts with the MWA
• Future Radio Continuum Cosmology Clustering Surveys
• Calibration Schemes with $\mathcal{O}(N\log N)$ Scaling for Large-N Radio Interferometers Built on a Regular Grid
• Supernova remnant candidates identified using MWA Galactic Plane Monitoring over 285deg < l < 70deg and |b| < 16deg
• One of Everything: The Breakthrough Listen Exotica Catalog
• A Bayesian Method to Mitigate the Effects of Unmodelled Time-Varying Systematics for 21-cm Cosmology Experiments
• Spectroscopy with the Engineering Development Array: cold H${}^{+}$ at 63 MHz towards the Galactic Centre
• Effects of Small-Scale Absorption Systems on Neutral Islands during the Late Epoch of Reionization
• Antenna array characterization via radio interferometry observation of astronomical sources
• First Robust Detection of Linear Polarization from Metric Solar Emissions: Challenging Established Paradigms
• Type IV Radio Bursts and Associated Active Regions in the Sunspot Cycle 24
• The SKA Particle Array Prototype: The First Particle Detector at the Murchison Radio-astronomy Observatory
• Field-level Reconstruction from Foreground-Contaminated 21-cm Maps
• The Statistics of Negative Power Spectrum Systematics in some 21 cm Analyses
• Radio Observations as a Probe of Cosmic Web Magnetism
• A catalogue of complex radio sources in the Rapid ASKAP Continuum Survey created using a Self-Organising Map
• Strategy for mitigation of systematics for EoR experiments with the Murchison Widefield Array
• A LOFAR prompt search for radio emission accompanying X-ray flares in GRB 210112A
• The impact of lossy data compression on the power spectrum of the high redshift 21-cm signal with LOFAR
• Evolution of the cold gas fraction and the star formation history: Prospects with current and future radio facilities
• Singular spectrum analysis of time series data from low frequency radiometers, with an application to SITARA data
• Probing self-interacting ultrahigh-energy neutrinos with the cosmic 21-cm signal
• An Ultra-High Time Resolution Cosmic Ray Detection Mode for the Murchison Widefield Array
• Low-Frequency Radio Recombination Lines Away From the Inner Galactic Plane
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• Radio jets: properties, life and impact
• History of Astronomy in Australia: Big-Impact Astronomy from World War II until the Lunar Landing (1945-1969)
• Synthetic Observations with the Square Kilometre Array (SKA) -- development towards an end-to-end pipeline
• Einstein Probe discovery of the short period intermediate polar EP J115415.8-501810
• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• Prospects of detecting HI using redshifted 21 cm radiation at z ~ 3
• Wavelets and sparsity for Faraday tomography
• Type II radio bursts and space weather phenomena: A statistical study
• Detecting 21 cm EoR Signal using Drift Scans: Correlation of Time-ordered Visibilities
• Beam Maps of the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Measured with a Drone
• Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-Point Statistics
• Reionization Parameter Inference from 3D Minkowski Functionals of the 21 cm Signals
• Differentiating Warm Dark Matter Models through 21cm Line Intensity Mapping: A Convolutional Neural Network Approach
• Practical Limits in the Sensitivity-Linearity Trade-off for Radio Telescope Front Ends in the HF and VHF-low Bands
• Astroinformatics Challenges from Next-generation Radio Continuum Surveys
• CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
• Performance of the Segment Anything Model in Various RFI/Events Detection in Radio Astronomy
• A Formalism for Calibrating the Instrumental Polarization of Radio Interferometric Arrays at Meter Wavelengths using Unpolarized Sky: A Demonstration using the MWA Observations
• The Subparsec-scale Structure and Evolution of Centaurus A. III. A Multi-Epoch Spectral And Polarimetric VLBA Study
• The Lockman Hole with LOFAR - Searching for GPS and CSS sources at low frequencies
• Application of Physics-Informed Neural Networks in Removing Telescope Beam Effects
• Probing magneto-ionic microstructure towards the Vela pulsar using a prototype SKA-Low station
• Detection of the extended $\gamma$-ray emission from the new supernova remnant G321.3-3.9 with Fermi-LAT
• A Digital Calibration Source for 21cm Cosmology Telescopes
• Primary Beam Chromaticity in HIRAX: I. Characterization from Simulations and Power Spectrum Implications
• Design and Commissioning of an LWA Swarm Station: The Long Wavelength Array -- North Arm
• Measurement of the Primary Beam of the Tianlai Cylindrical Antenna Using an Unmanned Aerial Vehicle
• Investigating four new candidate redback pulsars discovered in the image plane
• Mapping Diffuse Radio Sources Using TUNA: A Transformer-Based Deep Learning Approach
• Solar Observation with MeerKAT: Demonstration of Technical Readiness and Initial Science Highlight
• Fast response electromagnetic follow-ups from low latency GW triggers
• A Swift X-ray view of the SMS4 sample -- II: X-ray properties of 17 bright radio sources
• An Extragalactic Widefield Search for Technosignatures with the Murchison Widefield Array
• A Matched Survey for the Enigmatic Low Radio Frequency Transient ILT J225347+862146
• Somewhere in between: Tracing the Radio Emission from Galaxy Groups (or Why Does the Future of Observing Galaxy Groups with Radio Telescopes Look Promising?)
• Low-Frequency Carbon Recombination Lines in the Orion Molecular Cloud Complex
• Confronting global 21-cm signal with ${\mathbb{Z}}_3$ symmetric dark matter models
• Extracting 21cm signal by frequency and angular filtering
• Single-pulse analysis and average emission characteristics of PSR J1820-0427 from observations made with the MWA and uGMRT
• Testing the circularity of PSR B0818-41's carousel
• The Aperture Array Verification System 1: System overview and early commissioning results
• Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 Field
• VLBI properties of compact interplanetary scintillators detected by the Murchison Widefield Array
• System equivalent flux density of Stokes I, Q, U, V of a polarimetric interferometer
• Murchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1
• Multi-epoch Low Radio Frequency Surveys of the Kepler K2 Mission Campaign Fields 3, 4, and 5 with the Murchison Widefield Array
• Mapping our Universe in 3D with MITEoR
• Revisiting Hybrid Interferometry with Low-Frequency Radio Astronomy Arrays
• Mapping Large-Scale-Structure Evolution over Cosmic Times
• AlgoSCR: An algorithm for Solar Contamination Removal from radio interferometric data
• Distributed and parallel sparse convex optimization for radio interferometry with PURIFY
• Reassessment of an origin of the radio structure of J1420-0545
• Constraining the Rate of Primordial Black-Hole Explosions and Extra Dimension Scale using a Low-Frequency Radio Antenna Array
• Drone Beam Mapping of the TONE Radio Dish Array
• A FLASH on Blazars: Capturing the Radio Realm of 4FGL Blazars with SKAO Pathfinders
• MeerKAT discovery of GHz radio emission extending from Abell 3017 toward Abell 3016
• Absorption variability as a probe of the multiphase interstellar media surrounding active galaxies
• Simulations of orbital debris clouds due to breakup events and their characterisation using the Murchison Widefield Array radio telescope
• De-distorting ionospheric effects in the image plane
• A Multi-Mechanism Hybrid Model of Peaked-Spectrum Radio Sources
• The Evolving Power Spectrum for the light cone Epoch of Reionization (EoR) 21-cm signal
• Low radio frequency detections of known pulsars and identification of new candidates with GLEAM-X: GP
• Noise Reduction Method for Radio Astronomy Single Station Observation Based on Wavelet Transform and Mathematical Morphology
• Concept of an Experimental Ultra Long-wavelength Radio Array
• A Search for Low-frequency Radio Pulses from Long Gamma-ray Bursts with the Murchison Widefield Array
• Real-time imaging of density ducts between the plasmasphere and ionosphere
• Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography
• Radio Halo Detection in MWA Data using Deep Neural Networks and Generative Data Augmentation
• Fast in-database cross-matching of high-cadence, high-density source lists with an up-to-date sky model
• BLINK: an End-To-End GPU High Time Resolution Imaging Pipeline for Fast Radio Burst Searches with the Murchison Widefield Array
• Characterizing the Spectral Structure of Weak Impulsive Narrowband Quiet Sun Emissions
• Impact of astrophysical effects on the dark matter mass constraint with 21cm intensity mapping
• Enabling pulsar and fast transient searches using coherent dedispersion
• The Effect of Large Optical Depths on the Non-Gaussian 21-cm signal from Cosmic Dawn
• Radiative transfer of 21-cm line through ionised cavities in an expanding universe
• Optimal Dithering Configuration Mitigating Rayleigh-Backscattering-Induced Distortion in Radioastronomic Optical Fiber Systems
• 50-250 MHz Pulsar Census with an SKA-Low prototype station: Spectra and Polarization
• Clustering properties of TGSS radio sources
• Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
• Foreground Subtraction with a Tensor-Based Oriented Singular Value Decomposition Method for HI Experiments
• The GLEAM 4-Jy (G4Jy) Sample: IV. Multiwavelength data and analysis
• Transformer-Based Source Detection and Morphological Classification in LOFAR Deep-Field Continuum Images
• Bayes-SCF: A Bayesian filter to mitigate foreground leakage in the 21-cm power spectrum
• Extremely Large Images: Considerations for Contemporary Approach
• Optimizing Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling
• Accelerating reionization constraints: An ANN-emulator framework for the SCRIPT Semi-numerical Model
• Multi-tracer analysis of straight depolarisation canals in the surroundings of the 3C 196 field
• Realisation of a low frequency SKA Precursor: The Murchison Widefield Array
• On the accuracy of posterior recovery with neural network emulators
• Uncertainty-Aware Neural Networks for Fuzzy Dark Matter Model Selection from \texorpdfstring{$x_{\mathrm{HI}}$}{x_HI} Measurements
• Direction-Dependent Polarised Primary Beams in Wide-Field Synthesis Imaging
• Simulating a full-sky high resolution Galactic synchrotron spectral index map using neural networks
• Using low-frequency pulsar observations to study the 3-D structure of the Galactic magnetic field
• Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations
• Deep ASKAP EMU Survey of the GAMA23 field: Properties of radio sources
• Low frequency observations of radio relics and halos
• The Correlation Calibration of PAPER-64 data
• Power spectrum multipoles and clustering wedges during the Epoch of Reionization
• Communication protocol for a satellite-swarm interferometer
• First Look Murchison Widefield Array observations of Abell 3667
• Independent discovery of a nulling pulsar with unusual sub-pulse drifting properties with the Murchison Widefield Array
• A Cloud-native Agile approach to cyber platform prototyping and integration for astronomy: the ENGAGE SKA case
• It's Always Darkest Before the Cosmic Dawn: Early Results from Novel Tools and Telescopes for 21 cm Cosmology
• Are the modern computer simulations a substitute for physical models? The SKA case
• A novel algorithm for high fidelity spectro-polarimetric snapshot imaging of the low-frequency radio Sun using SKA-low precursor
• Direct reconstruction of the Reionization history from 21cm 2D Power Spectra
• Direct Wide-Field Radio Imaging in Real-Time at High Time Resolution using Antenna Electric Fields
• Radio Burst and Circular Polarization Studies of the Solar Corona at Low Frequencies
• Solar Radio-Frequency Reflectivity and Localization of FRB from Solar Reflection
• Establishing a relationship between the cosmological 21 cm power spectrum and interferometric closure phases