Science with ASKAP - the Australian Square Kilometre Array Pathfinder

Abstract

[ABRIDGED VERSION] The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any existing radio facility. A majority of the key science for the SKA will be addressed through large-area imaging of the Universe at frequencies from 300 MHz to a few GHz. The Australian SKA Pathfinder (ASKAP) is aimed squarely in this frequency range, and achieves instantaneous wide-area imaging through the development and deployment of phase-array feed systems on parabolic reflectors. This large field-of-view makes ASKAP an unprecedented synoptic telescope poised to achieve substantial advances in SKA key science. The central core of ASKAP will be located at the Murchison Radio Observatory in inland Western Australia, one of the most radio-quiet locations on the Earth and one of the sites selected by the international community as a potential location for the SKA. Following an introductory description of ASKAP, this document contains 7 chapters describing specific science programmes for ASKAP. The combination of location, technological innovation and scientific program will ensure that ASKAP will be a world-leading radio astronomy facility, closely aligned with the scientific and technical direction of the SKA. A brief summary chapter emphasizes the point, and considers discovery space.

Accepted for publication in Experimental Astronomy. This submission contains only a summary of the full 120 page article which can be found at http://wwwatnf.atnf.csiro.au/projects/askap/newdocs/askap_expast08.pdf . Jasper Wall (UBC, Overall Editor)

References in corpus (184)

• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• The ATNF Pulsar Catalogue
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• The broken hierarchy of galaxy formation
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• How Do Galaxies Get Their Gas?
• A bright millisecond radio burst of extragalactic origin
• Hierarchical Galaxy Formation
• Galaxy Harassment and the Evolution of Clusters of Galaxies
• New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
• The Physics of Neutron Stars
• A statistical study of 233 pulsar proper motions
• A fundamental plane of black hole activity
• Interstellar Turbulence I: Observations and Processes
• Gravitational Wave Experiments and Early Universe Cosmology
• A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
• Origin of Galactic and Extragalactic Magnetic Fields
• A Radio Pulsar Spinning at 716 Hz
• SUMSS: A Wide-Field Radio Imaging Survey of the Southern Sky. II. The Source Catalogue
• Baryons in the Warm-Hot Intergalactic Medium
• Galaxy Star-Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey
• Birth and Evolution of Isolated Radio Pulsars
• The 2dF Galaxy Redshift Survey: The environmental dependence of galaxy star formation rates near clusters
• Faraday Rotation Measure Synthesis
• The Parkes Multibeam Pulsar Survey: I. Observing and Data Analysis Systems, Discovery and Timing of 100 Pulsars
• Transient radio bursts from rotating neutron stars
• The HIPASS Catalogue - I. Data Presentation
• SkyMapper and the Southern Sky Survey
• A primer on hierarchical galaxy formation: the semi-analytical approach
• A periodically active pulsar giving insight into magnetospheric physics
• The Low Redshift Lyman Alpha Forest in Cold Dark Matter Cosmologies
• The HIPASS catalogue: Omega_HI and environmental effects on the HI mass function of galaxies
• Damped Lyman Alpha Systems at z<1.65: The Expanded SDSS HST Sample
• The SDSS Damped Lya Survey: Data Release 3
• Pulsar rotation measures and the large-scale structure of Galactic magnetic field
• Science with the Square Kilometer Array: Motivation, Key Science Projects, Standards and Assumptions
• The Physics of Star Formation
• A correlation of the cosmic microwave sky with large scale structure
• The HI Content of Spirals. II. Gas Deficiency in Cluster Galaxies
• The Southern Galactic Plane Survey: HI Observations and Analysis
• A wide field Hubble Space Telescope study of the cluster CL0024+16 at z=0.4. I: morphological distributions to 5 Mpc radius
• DiFX: A software correlator for very long baseline interferometry using multi-processor computing environments
• Cosmic Star Formation History and its Dependence on Galaxy Stellar Mass
• Galactic and extragalactic magnetic fields
• Thermal condensation in a turbulent atomic hydrogen flow
• VLA HI Observations of Gas Stripping in the Virgo Cluster Spiral NGC 4522
• Spitzer Observations of Massive Red Galaxies at High Redshift
• Interstellar Turbulence II: Implications and Effects
• The Nature and Evolution of Classical Double Radio Sources from Complete Samples
• Discovery of an Unusual Dwarf Galaxy in the Outskirts of the Milky Way
• The evolution of the star formation activity in galaxies and its dependence on environment
• The Far- and Mid-Infrared/Radio Correlations in the Spitzer Extragalactic First Look Survey
• The radio luminosity function from the low-frequency 3CRR, 6CE & 7CRS complete samples
• The Magellanic Stream, High-Velocity Clouds and the Sculptor Group
• Looking for $\Lambda$ with the Rees-Sciama Effect
• Searches for Fast Radio Transients
• The Millennium Arecibo 21-cm Absorption Line Survey. IV. Statistics of Magnetic Field, Column Density, and Turbulence
• Reviving Fossil Radio Plasma in Clusters of Galaxies by Adiabatic Compression in Environmental Shock Waves
• Detecting the stochastic gravitational wave background using pulsar timing
• The Properties of Poor Groups of Galaxies: II. X-ray and Optical Comparisons
• Cosmological Magnetic Fields Limits in an Inhomogeneous Universe
• Explosive reconnection in magnetars
• Hot Bubbles from Active Galactic Nuclei as a Heat Source in Cooling Flow Clusters
• Observations of 20 millisecond pulsars in 47 Tucanae at 20 cm
• Surveys for z > 3 Damped Lyman-alpha Absorption Systems
• The evolution of Omega(HI) and the epoch of formation of damped Lyman-alpha absorbers
• Joint Formation of QSOs and Spheroids: QSOs as clocks of star formation in Spheroids
• Radio Observations of a Large Sample of Late-M, L, and T Dwarfs: The Distribution of Magentic Field Strengths
• Radio and X-ray Signatures of Merging Neutron Stars
• Evidence for alignment of the rotation and velocity vectors in pulsars
• The HI Mass Function of Galaxies from a Deep Survey in the 21cm Line
• Rotation Measures of Extragalactic Sources Behind the Southern Galactic Plane: New Insights into the Large-Scale Magnetic Field of the Inner Milky Way
• SPH compressible turbulence
• The 1000 Brightest HIPASS Galaxies: HI Mass Function and Omega_HI
• Integrated Sachs-Wolfe effect from the cross correlation of WMAP3 year and the NRAO VLA sky survey data: New results and constraints on dark energy
• VLBA Measurement of Nine Pulsar Parallaxes
• Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
• The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State
• Effects of the Equation of State on the Formation of Star Clusters
• Strong-Field Tests of Gravity Using Pulsars and Black Holes
• Deep ATLAS radio observations of the CDFS-SWIRE field
• A powerful bursting radio source towards the Galactic Centre
• Bubbles, feedback and the intra-cluster medium: three-dimensional hydrodynamic simulations
• The Millennium Arecibo 21-cm Absorption Line Survey. I. Techniques and Gaussian Fits
• An absolutely calibrated survey of polarized emission from the northern sky at 1.4 GHz
• The dependence of Star Formation on Galaxy Stellar Mass
• Detection of ionized gas in the globular cluster 47 Tucanae
• Constraints on Cosmic Neutrino Fluxes from the ANITA Experiment
• Jet-Induced Emission-Line Nebulosity and Star Formation in the High-Redshift Radio Galaxy 4C41.17
• Detection of the velocity dipole in the radio galaxies of the NRAO VLA Sky Survey
• The HI content of star-forming galaxies at z = 0.24
• Velocity and density spectra of the Small Magellanic Cloud
• Extragalactic radio source evolution under the dual-population unification scheme
• HI Narrow Line Absorption in Dark Clouds
• On the origin of the galaxy luminosity function
• Specific star formation rates to redshift 5 from the FORS Deep Field and the GOODS-S Field
• Orphan GRB radio afterglows: Candidates and constraints on beaming
• HI Narrow Self-Absorption in Dark Clouds: Correlations with Molecular Gas and Implications for Cloud Evolution and Star Formation
• The WSRT wide-field HI survey: II. Local Group features
• A Faraday Rotation Search for Magnetic Fields in Large Scale Structure
• PKS 0405--385: the smallest radio quasar?
• Rapid Variability and Annual Cycles in the Characteristic Time-scale of the Scintillating Source PKS 1257-326
• Interstellar scintillation as the origin of rapid radio variability in the quasar J1819+3845
• The Southern Galactic Plane Survey: Polarized Radio Continuum Observations and Analysis
• A Complete Survey of the Transient Radio Sky and Implications for Gamma-Ray Bursts, Supernovae, and other Relativistic Explosions
• First Results from MASIV: The Micro-Arcsecond Scintillation-Induced Variability Survey
• Giant Pulses from PSR B0540-69 in the Large Magellanic Cloud
• The Origin and Evolution of Cosmic Magnetism
• Discovery of a Young Radio Pulsar in a Relativistic Binary Orbit
• SubmilliJansky Transients in Archival Radio Observations
• Structures in the RM sky
• A deep Chandra observation of the Centaurus cluster: bubbles, filaments and edges
• Molecular gas at high redshift: jet-induced star formation?
• Discovery of 14 radio pulsars in a survey of the Magellanic Clouds
• Quiescent Radio Emission from Southern Late-type M Dwarfs and a Spectacular Radio Flare from the M8 Dwarf DENIS 1048-3956
• Timing the millisecond pulsars in 47 Tucanae
• Measurement of the angular correlation function of radio galaxies from the NRAO VLA Sky Survey
• A search for distant radio galaxies from SUMSS and NVSS: III. radio spectral energy distributions and the z-alpha correlation
• Extragalactic Zeeman Detections in OH Megamasers
• Discovery of a Population of HI Clouds in the Galactic Halo
• Predictions on high frequency polarization properties of extragalactic radio sources and implications for CMB polarization measurements
• Pulsar Birthrate from Parkes Multi-beam Survey
• Implications for unified schemes from the quasar fraction and emission-line luminosities in radio-selected samples
• The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds
• Orphan Afterglows of Collimated Gamma-Ray Bursts: Rate Predictions and Prospects for Detection
• Observations of magnetic fields in the Milky Way and in nearby galaxies with a Square Kilometre Array
• The SDSS Damped Lya Survey: Data Release 1
• FIRST J102347.6+003841: The First Radio-Selected Cataclysmic Variable
• Morphology, Environment, and the HI Mass Function
• Evidence that powerful radio jets have a profound influence on the evolution of galaxies
• Rapid interstellar scintillation of PKS B1257-326: two-station pattern time delays and constraints on scattering and microarcsecond source structure
• Quantifying angular clustering in wide-area radio surveys
• Submillimetre photometry of X-ray absorbed QSOs: their formation and evolutionary status
• Optimal Radio Window for the Detection of Ultra-High-Energy Cosmic Rays and Neutrinos off the Moon
• The evolution of submillimetre galaxies: two populations and a redshift cut-off
• Implications of 21cm observations for damped Ly-$\alpha$ systems
• SN 1993J VLBI (III): The Evolution of the Radio Shell
• Ultra High Energy Cosmic Rays
• The Exploration of the Unknown
• Weak Lensing by Large-Scale Structure with the FIRST Radio Survey
• Variability of sub-mJy radio sources
• Chandra Observation of the Central Region of the Cooling Flow Cluster Abell 262: A Radio Source that is a Shadow of its Former Self?
• The Weak Clustering of Gas-Rich Galaxies
• Radio Polarimetry of the ELAIS N1 Field: Polarized Compact Sources
• Extending the infrared radio correlation
• Coupled spheroid and black-hole formation, and the multifrequency detectability of active galactic nuclei and submillimetre sources
• The VSOP 5-GHz AGN Survey: IV. The Angular Size/Brightness Temperature Distribution
• Deep H I observations of the compact high-velocity cloud HVC125+41-207
• Lensing of Stars by Spherical Gas Clouds
• SN 1993J VLBI (IV): A Geometric Determination of the Distance to M81 with the Expanding Shock Front Method
• Reconstructing Deconstruction: High-Velocity Cloud Distance Through Disruption Morphology
• APERTIF, a focal plane array for the WSRT
• Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
• Polarization Properties of Extragalactic Radio Sources and Their Contribution to Microwave Polarization Fluctuations
• The Sub-parsec Scale Radio Properties of Southern Starburst Galaxies. I. Supernova Remnants, the Supernova Rate, and the Ionised Medium in the NGC 253 Starburst
• Determination of the Primordial Magnetic Field Power Spectrum by Faraday Rotation Correlations
• A Laboratory for Constraining Cosmic Evolution of the Fine Structure Constant: Conjugate 18 cm OH Lines Toward PKS 1413+135 at z=0.2467
• 21 cm Absorption Studies with the Square Kilometer Array
• Turbulent dissipation in the ISM: the coexistence of forced and decaying regimes and implications for galaxy formation and evolution
• Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids with HI galaxies?
• ISOCAM observations of the Ursa Major cirrus: Evidence for large abundance variations of small dust grains
• The thinnest cold HI clouds in the diffuse interstellar medium?
• The Supernova Remnant CTB104A : Magnetic Field Structure and Interaction with the Environment
• Tiny HI Clouds in the Local ISM
• Dependence of Dust Obscuration on Star Formation Rates in Galaxies
• Cross correlation of Lyman-alpha absorbers with gas-rich galaxies
• Emergence and disappearance of micro-arcsecond structure in the scintillating quasar J1819+3845
• VLBI detection of an Infrared-Faint Radio Source
• Two New Low Redshift 21cm Absorbers
• A new twist to an old story: HE 0450-2958, and the ULIRG$\to$(optically bright QSO) transition hypothesis
• The Fragmenting Superbubble Associated with the HII Region W4
• A search for distant radio galaxies from SUMSS and NVSS: II. Optical Spectroscopy
• Detection of 21 Centimeter HI Absorption at z = 0.78 in a Survey of Radio Continuum Sources
• Pulsars and Gravitational Wave Detection
• A Survey for Transient Astronomical Radio Emission at 611 MHz
• Deep Radio Continuum Studies with the SKA: Evolution of Radio AGN Populations
• A Search for 6.7 GHz Methanol Masers in OH Megamaser Galaxies at 0.11<z<0.27
• Using SKA to observe relativistic jets from X-ray binary systems
• SGRS J0515-8100: a Fat-Double giant radio galaxy
• Absorption of the Linear Polarization of the Galactic Background Radiation by the $\lambda$21-cm Line of HI
• MHD Simulations of the ISM: The Importance of the Galactic Magnetic Field on the ISM "Phases"
• A new 21-cm absorber identified with an $L\sim L^{\star }$ galaxy
• Limits on Turbulent HI Fluctuations Towards PSR B0329+54 On Scales Between 0.0025 and 12.5 AU

Cited by in corpus (305)

• Short-Duration Gamma-Ray Bursts
• The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures
• DSPSR: Digital Signal Processing Software for Pulsar Astronomy
• Holographic Dark Energy
• A single fast radio burst localized to a massive galaxy at cosmological distance
• Fundamental Physics with the Square Kilometre Array
• The Australia Telescope Compact Array Broadband Backend (CABB)
• Late-time cosmology with 21cm intensity mapping experiments
• The Last of FIRST: The Final Catalog and Source Identifications
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Radio and Millimeter Continuum Surveys and their Astrophysical Implications
• Shark: introducing an open source, free and flexible semi-analytic model of galaxy formation
• Cosmic evolution of the atomic and molecular gas content of galaxies
• Compact continuum source-finding for next generation radio surveys
• The Westerbork SINGS Survey II. Polarization, Faraday Rotation, and Magnetic Fields
• On the origin of a highly-dispersed coherent radio burst
• WALLABY -- An SKA Pathfinder HI Survey
• The cold interstellar medium of galaxies in the Local Universe
• Radio Properties of Tidal Disruption Events
• Evolution of the atomic and molecular gas content of galaxies
• The Rapid ASKAP Continuum Survey Paper II: First Stokes I Source Catalogue Data Release
• Source finding in the era of the SKA (precursors): Aegean 2.0
• On the impact of empirical and theoretical star formation laws on galaxy formation
• The detection of an extremely bright fast radio burst in a phased array feed survey
• A Survey of Extragalactic Faraday Rotation at High Galactic Latitude: The Vertical Magnetic Field of the Milky Way towards the Galactic Poles
• Cosmic microwave background constraints on the duration and timing of reionization from the South Pole Telescope
• Predictions for ASKAP Neutral Hydrogen Surveys
• Surveying the reach and maturity of machine learning and artificial intelligence in astronomy
• BLOBCAT: Software to Catalogue Flood-Filled Blobs in Radio Images of Total Intensity and Linear Polarization
• Modelling the Galactic Magnetic Field on the Plane in 2D
• The Caltech-NRAO Stripe 82 Survey (CNSS) Paper I: The Pilot Radio Transient Survey In 50 deg${}^2$
• Revisiting the radio interferometer measurement equation. II. Calibration and direction-dependent effects
• On using angular cross-correlations to determine source redshift distributions
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• Variation of galactic cold gas reservoirs with stellar mass
• The Local Volume HI Survey (LVHIS)
• Are peculiar velocity surveys competitive as a cosmological probe?
• The fundamental plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
• Automated Kinematic Modelling of Warped Galaxy Discs in Large Hi Surveys: 3D Tilted Ring Fitting of HI Emission Cubes
• MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey
• 2MTF VI. Measuring the velocity power spectrum
• Radio Counterparts of Compact Binary Mergers detectable in Gravitational Waves: A Simulation for an Optimized Survey
• Magnetic Fields in the Milky Way
• Radio Galaxy populations and the multi-tracer technique: pushing the limits on primordial non-Gaussianity
• Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421
• H${}_2$-based star formation laws in hierarchical models of galaxy formation
• HIGHz: A Survey of the Most HI-Massive Galaxies at z~0.2
• Which galaxies dominate the neutral gas content of the Universe?
• Kinematics and physical conditions of HI in nearby radio sources. The last survey of the old Westerbork Synthesis Radio Telescope
• Synthetic off-axis light curves for low energy gamma-ray bursts
• A Revised View of the Transient Radio Sky
• The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
• Radio Halos in future surveys in the radio continuum
• The SVOM Mission
• Variable and Transient Radio Sources in the FIRST Survey
• The mid-life crisis of the Milky Way and M31
• The variability timescales and brightness temperatures of radio flares from stars to supermassive black holes
• Gas Dynamics and Star Formation in the Galaxy Pair NGC1512/1510
• Cosmological Forecasts for Combined and Next Generation Peculiar Velocity Surveys
• ATLAS - I. Third Release of 1.4 GHz Mosaics and Component Catalogues
• The radio afterglow of Swift J1644+57 reveals a powerful jet with fast core and slow sheath
• A Broadband Polarization Catalog of Extragalactic Radio Sources
• Extragalactic Radio Continuum Surveys and the Transformation of Radio Astronomy
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• LUNASKA experiments using the Australia Telescope Compact Array to search for ultra-high energy neutrinos and develop technology for the lunar Cherenkov technique
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• An ASKAP search for a radio counterpart to the first high-significance neutron star-black hole merger LIGO/Virgo S190814bv
• Scientific Visualization in Astronomy: Towards the Petascale Astronomy Era
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• Theoretical and observational constraints on the HI intensity power spectrum
• Cosmological Measurements with Forthcoming Radio Continuum Surveys
• Study of galaxies in the Lynx-Cancer void. I. Sample description
• ASKAP HI imaging of the galaxy group IC 1459
• V-FASTR: The VLBA Fast Radio Transients Experiment
• A circular polarisation survey for radio stars with the Australian SKA Pathfinder
• Gas accretion from minor mergers in local spiral galaxies
• ASKAP Detection of Periodic and Elliptically Polarized Radio Pulses from UV Ceti
• A complete sample of 21-cm absorbers at z~1.3: Giant Metrewave Radio Telescope Survey Using MgII Systems
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales
• Toward a Direct Measurement of the Cosmic Acceleration
• Cataloging the radio-sky with unsupervised machine learning: a new approach for the SKA era
• A compression scheme for radio data in high performance computing
• The Australia Telescope Large Area Survey: Spectroscopic Catalogue and Radio Luminosity Functions
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• The FIRST Classifier: Compact and Extended Radio Galaxy Classification using Deep Convolutional Neural Networks
• 2D Bayesian automated tilted-ring fitting of disk galaxies in large HI galaxy surveys: 2DBAT
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• WALLABY Early Science - III. An HI Study of the Spiral Galaxy NGC 1566
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• Radio observations of the merging galaxy cluster system Abell 3391-Abell 3395
• Fanaroff-Riley classification of radio galaxies using group-equivariant convolutional neural networks
• First constraints on the AGN X-ray luminosity function at $z\sim 6$ from an eROSITA-detected quasar
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• Detectability of Torsion Gravity via Galaxy Clustering and Cosmic Shear Measurements
• Quantified HI Morphology III: Merger Visibility Times from HI in Galaxy Simulations
• An accurate low-redshift measurement of the cosmic neutral hydrogen density
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• Probing the gas content of radio galaxies through HI absorption stacking
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
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• An automated archival VLA transients survey
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• Synchrotron Emission from Dark Matter Annihilation: Predictions for Constraints from Non-detections of Galaxy Clusters with New Radio Surveys
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• Morphological classification of compact and extended radio galaxies using convolutional neural networks and data augmentation techniques
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• Quantified HI Morphology II : Lopsidedness and Interaction in WHISP Column Density Maps
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• Statistical Properties of Radio Halos in Galaxy Clusters and Origin of Seed Electrons for Reacceleration
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• The cosmic atomic hydrogen mass density as a function of mass and galaxy hierarchy from spectral stacking
• Constraining properties of neutron star merger outflows with radio observations
• A pilot ASKAP survey for radio transients towards the Galactic Centre
• ASKAP Commissioning Observations of the GAMA 23 Field
• Radio Afterglows from Compact Binary Coalescences: Prospects for Next-Generation Telescopes
• Optimal Multiwavelength Source Detection: Experience Gained from the WISE Mission
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• Optimising commensality of radio continuum and spectral line observations in the era of the SKA
• Evolutionary Map of the Universe (EMU):Compact radio sources in the SCORPIO field towards the Galactic plane
• Large-scale comparative visualisation of sets of multidimensional data
• A new approach for short-spacing correction of radio interferometric data sets
• Quantified HI Morphology V: HI Disks in the Virgo Cluster
• Search for high-energy neutrinos in coincidence with Fast Radio Bursts with the ANTARES neutrino telescope
• First Results from the REAL-time Transient Acquisition backend (REALTA) at the Irish LOFAR station
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• Spectropolarimetry with the Giant Metrewave Radio Telescope at 610 MHz: a case study of two Southern Compact Group fields
• Discovery of large-scale diffuse radio emission and of a new galaxy cluster in the surroundings of MACSJ0520.7-1328
• Unusual displacement of HI due to tidal interaction in Arp 181
• First Study of the Supernova Remnant Population in the Large Magellanic Cloud with eROSITA
• FLASH Pilot Survey: Detections of associated 21 cm HI absorption in GAMA galaxies at 0.42 < z <1.00
• Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass
• The Caltech-NRAO Stripe 82 Survey (CNSS) Paper II: On-The-Fly Mosaicing Methodology
• Beyond Stacking: A Maximum-Likelihood Method to Constrain Radio Source Counts Below the Detection Threshold
• The 2-degree Field Lensing Survey: photometric redshifts from a large new training sample to r<19.5
• Analyzing the Galactic pulsar distribution with machine learning
• Dark Matter Fraction in z~1 Star-Forming Galaxies
• The Thousand-Pulsar-Array programme on MeerKAT VII: Polarisation properties of pulsars in the Magellanic Clouds
• Radio Galaxy Zoo EMU: Towards a Semantic Radio Galaxy Morphology Taxonomy
• The radio spectral energy distribution of infrared-faint radio sources
• SAMI-HI: The HI view of the H$\alpha$ Tully-Fisher relation and data release
• Radio Transients from Newborn Black Holes
• A method for reconstructing the Galactic magnetic field using dispersion of fast radio bursts and Faraday rotation of radio galaxies
• Observing superluminous supernovae and long gamma ray bursts as potential birthplaces of repeating fast radio bursts
• Radio data challenge the broadband modelling of GRB160131A afterglow
• A VOEvent based automatic trigger system for the Murchison Widefield Array
• Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array
• A consistent model for both the HI and stellar mass functions of galaxies
• Baseline-dependent sampling and windowing for radio interferometry: data compression, field-of-interest shaping and outer field suppression
• Upper Limits on Pulsed Radio Emission from the 6.85 s X-ray Pulsar XTE J0103-728 in the Small Magellanic Cloud
• Improved CLEAN reconstructions for rotation measure synthesis with maximum likelihood estimation
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Finding AGN remnant candidates based on radio morphology with machine learning
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• On the optical counterparts of radio transients and variables
• Collimation of the kiloparsec-scale radio jets in NGC 2663
• Redshift evolution of the HI detection rate in radio-loud active galactic nuclei
• The Atomic Hydrogen Content of Galaxies as a function of Group-Centric Radius
• A search for short-term hard X-ray bursts in the direction of the repeating FRB 121102
• The Weizmann Fast Astronomical Survey Telescope (W-FAST): System Overview
• Interferometric Cubelet Stacking to Recover H\,\textsc{i} Emission from Distant Galaxies
• Real-time colouring and filtering with graphics shaders
• Commensal Transient Searches in Eight Short Gamma Ray Burst Fields
• Searching for stellar flares from low mass stars using ASKAP and TESS
• Source finding, parametrization and classification for the extragalactic Effelsberg-Bonn HI Survey
• SPT-CL J2215-3537: A Massive Starburst at the Center of the Most Distant Relaxed Galaxy Cluster
• The SARAO MeerKAT Galactic Plane Survey extended source catalogue
• The Redshift Dependence of the Radio Flux of Gamma-Ray Bursts and Their Host Galaxies
• Methods for detection and analysis of weak radio sources with single-dish radio telescopes
• WALLABY Pilot Survey: Hydra Cluster Galaxies UV and HI morphometrics
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• No strong radio absorption detected in the low-frequency spectra of radio-loud quasars at z > 5.6
• Noise reduction on single-shot images using an autoencoder
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Central radio galaxies in galaxy clusters: Joint surveys by eROSITA and ASKAP
• The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
• Disc galaxy resolved in HI absorption against the radio lobe of 3C 433: Case study for future surveys
• Modeling the Initial Conditions of Interacting Galaxy Pairs Using Identikit
• MeerKAT reveals a ghostly thermal radio ring towards the Galactic Centre
• Enhanced detection and identification of satellites using an all-sky multi-frequency survey with prototype SKA-Low stations
• On the use of variability time-scales as an early classifier of radio transients and variables
• SCORPIO-II: Spectral indices of weak Galactic radio sources
• A Quantitative Assessment of Communicating Extra-Terrestrial Intelligent Civilizations in the Galaxy and the Case of FRB-like Signals
• The ISM scaling relations using inner HI and an application of estimating dust mass
• X-ray Observations of Radio Transients without Optical Hosts
• Are there radio-loud and radio-quiet Gamma-Ray Bursts?
• Diverse Properties of Molecular Gas in the Host Galaxies of Fast Radio Bursts
• Sports stars: analyzing the performance of astronomers at visualization-based discovery
• The Local Universe: Galaxies in 3D
• Cold and Warm Gas Outflows in Radio AGN
• Application of Physics-Informed Neural Networks in Removing Telescope Beam Effects
• A self-supervised, physics-aware, Bayesian neural network architecture for modelling galaxy emission-line kinematics
• Correction of Radio Interferometric Imaging for Antenna Patterns
• Astroinformatics Challenges from Next-generation Radio Continuum Surveys
• Collaborative visual analytics of radio surveys in the Big Data era
• The First Detection of Neutral Hydrogen in Emission in a Strong Spiral Lens
• Deep Extragalactic VIsible Legacy Survey (DEVILS): DR1 Blended Spectra Search for Candidate Strong Gravitational Lenses
• Characterisation of Long Baseline Calibrators at 2.3 GHz
• The localization of single pulse in VLBI observation
• HI asymmetries in spatially resolved SIMBA galaxies
• Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
• iDaVIE v1.0: A virtual reality tool for interactive analysis of astronomical data cubes
• Cold gas and the disruptive effect of a young radio jet
• MeerKAT discovery of 164 compact radio rings toward the Galactic Plane
• MeerKAT 21-cm HI imaging of Abell 2626 and beyond
• Absorption variability as a probe of the multiphase interstellar media surrounding active galaxies
• First Search for Low-Frequency CH with a Square Kilometre Array Precursor Telescope
• Evolutionary Map of the Universe
• Radio Galaxy Zoo: Giant Radio Galaxy Classification using Multi-Domain Deep Learning
• MUSE-ALMA Haloes XIV: The ALMA Large Programme Data Release
• Interstellar filament detection and characterization: methods and implications for studies of magnetized interstellar medium
• 3-D interactive visualisation tools for HI spectral line imaging
• First studies of the diffuse X-ray emission in the Large Magellanic Cloud with eROSITA
• Exploring the Link between Fast Radio Burst and Binary Neutron Star Origins with Spaceborne Gravitational Wave Observations
• Spectroscopic Characterization of LOFAR Radio-emitting M dwarfs