Datasets / Australian Government / CSIRO Data Access Portal
Australian Government CSIRO Data Access Portal open data
CSIRO Data Access Portal lists 1,133 datasets on data.gov.au. 0 of them have an open licence and a file or API we can read.
On the portal
1,133 datasets, newest 200 shownThese are the datasets CSIRO Data Access Portal lists on data.gov.au. A vote asks us to serialise one. Only the licence can stop us, so a dataset without an open licence cannot take a vote.
| Dataset | Formats | Licence | Updated | Votes |
|---|---|---|---|---|
| CASDA Virtual Observatory Tools v1.26CASDA VO Tools is a highly customizable Java web application developed to serve astronomy data via Virtual Observatory protocols. Currently Table Access (TAP), Simple Cone Search (SCS), Simple Spectral Access (SSA), Simple Image Access v1 (SIA1), Simple Image Access v2 (SIA2)… | HTML | none stated | 2025-12-17 | no licence stated |
| Indonesian Landscape MetricsThe Indonesian Landscape Metrics tool is an interactive web application, used by researchers to calculate and visualise metrics for describing and quantifying spatial patterns and ecological processes in landscapes in the Republic of Indonesia. These patterns can be relevant to… | none stated | 2025-12-17 | no licence stated | |
| Parkes observations for project P1032 semester 2022APRS_05This project aims to continue to perform rapid measurements of relativistic parameters of southern binary pulsar systems using data from the Parkes Ultra Wideband Low (UWL) receiver and the MeerKAT telescope thereby enabling measurement of their component masses and in some… | APPLICATION, FITS, TEXT, X-LOG | none stated | 2025-12-17 | no licence stated |
| Parkes observations for project P1139 semester 2022APRS_01We have made the first direct detection of an ultra-long period magnetar, using a low-frequency sky survey performed by the Murchison Widefield Array (MWA). Its radio emission is highly polarised and periodic on a timescale of ~20 minutes. Its dynamic spectrum shows high-fluence… | APPLICATION, FITS, TEXT, X-LOG | none stated | 2025-12-17 | no licence stated |
| Parkes observations for project P595 semester 2022APRS_07We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | APPLICATION, FITS, TEXT, X-LOG | none stated | 2025-12-17 | no licence stated |
| Updated regional sea-level projections for Australia based on IPCC AR6 and CMIP6Updated sea-level projections for Australia mainly based on the IPCC AR6 and CMIP6 climate models, under 5 Shared Socioeconomic Pathways (SSPs) over the period 2020-2150, as well as a few derived datasets such as sea-level projections along coastline and at tide gauge stations… | APPLICATION, X-NETCDF | none stated | 2025-12-17 | no licence stated |
| 3D vision pipeline data for ROSELLA frameworkThis data collection accompanies the DICTA'25 paper "ROSELLA: an Open Computer Vision and Measurement Toolkit for Advanced Manufacturing" and contains data streams from the hardware interface, including RGB images, depth maps, and (optionally) the corresponding robot/camera… | HTML, JSON, TXT | none stated | 2025-12-10 | no licence stated |
| Parkes observations for project P595 semester 2025OCTS_03We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-12-10 | no licence stated |
| Parkes observations for project P960 semester 2025OCTS_02We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and… | none stated | 2025-12-10 | no licence stated | |
| Parkes observations for project P1183 semester 2025OCTS_03After nearly three years of monitoring, comprising with the Parkes telescope and the FAST telescopes, FRB 20220529 is proven to be an extremely interesting repeater. It exhibits one of the longest activity durations and a potential ~200-day RM period. Due to frequent… | none stated | 2025-12-09 | no licence stated | |
| Parkes observations for project P630 semester 2011APRS_09We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-09 | no licence stated |
| Parkes observations for project P630 semester 2011APRS_17We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-09 | no licence stated |
| Data for backtracking microplastic sourcesCollection of proteomic and metabarcoding data characterising a microplastic ecocorona | BIN | none stated | 2025-12-03 | no licence stated |
| GLEAM-300: The GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey at 300 MHz catalogue and imagesThe source catalogue and mosaic images produced as part of the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey at 300 MHz (GLEAM-300). The mosaic images were produced by combining images from individual two-minute snapshot observations to create… | HTML | none stated | 2025-12-03 | no licence stated |
| Highest Astronomical Tide for estuaries adjacent to the Great Barrier ReefHydrodynamic model simulations using an estuary resolving unstructured mesh to estimate the Highest Astronomical Tide (HAT) for all estuaries of the Queensland coast from Cape York to Gold Coast. | none stated | 2025-12-03 | no licence stated | |
| Long-term project observations for project P1041 semester 2025OCTS_01Omega Cen is the largest globular cluster in the Milky Way. It contains at least 18 known MSPs, and there are solid hints for the presence of an even larger pulsar population. We propose a regular monthly follow-up to refine the timing solutions of the five Parkes discoveries… | none stated | 2025-12-03 | no licence stated | |
| Long-term project observations for project P1321 semester 2025OCTS_03The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-12-03 | no licence stated | |
| Long-term project observations for project P1361 semester 2025OCTS_01PSR J1227-6208 is a recycled pulsar in a binary with a massive white dwarf companion. A recent timing measurement from combined MeerKAT and Parkes observations shows the companion mass to be between 1.2 and 1.5 solar masses, very close to the Chandrasekhar limit, resulting in… | none stated | 2025-12-03 | no licence stated | |
| Long-term project observations for project P885 semester 2025OCTS_03We propose a modest program to continue monitoring 4 of the 6 known radio magnetars in order to achieve three primary science goals. The first is to characterise magnetar outbursts over long timescales, for which tracking their rotational, flux density, and polarisation… | none stated | 2025-12-03 | no licence stated | |
| Mapping Australia's Coastal Defences Structures: Understanding the Gaps and the Need for a National DatasetThis dataset and accompanying RMarkdown notebook document the analysis and efforts to consolidate spatial data on coastal protection structures, such as sea walls, groynes, and wharfs, across Australia's coastline. The project addresses the urgent need for a national-level… | none stated | 2025-12-03 | no licence stated | |
| Motorbike frog (Litoria moorei) tissue untargeted metabolomicsUntargeted reversed-phase liquid chromatography high-resolution mass spectrometry profiling of four tissues (muscle, liver, fat and gonads/eggs) from wild-caught motorbike frogs (Litoria moorei) collected from 11 wetlands around Perth, Western Australia. The aim of collecting… | BIN, HTML, XML | none stated | 2025-12-03 | no licence stated |
| OzWheat V1.0 SNP data assetsSingle nucleotide polymorphism genotypes for ~300 varieties from the OzWheat diversity panel generated with alternative platforms combined in a single matrix. Original platform source files are also provided. Transcript SNPs: 63,222 SNP loci. 298 wheat lines. File=OzWheat… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1032 semester 2025OCTS_03With this proposal, we aim to continue P1032, the rapid measurements of relativistic parameters of southern binary pulsar systems using data from the Parkes Ultra Wideband Low (UWL) receiver. As the MeerTime project at the MeerKAT radio telescope ended in early 2024… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1349 semester 2025OCTS_01We propose a study of pulsars with interpulse (IP) emissions using the Ultra-Wideband Low (UWL) receiver on the Parkes radio telescope (Murriyang). This project aims to investigate the polarization and emission properties of these pulsars through detailed modeling using the… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1349 semester 2025OCTS_02We propose a study of pulsars with interpulse (IP) emissions using the Ultra-Wideband Low (UWL) receiver on the Parkes radio telescope (Murriyang). This project aims to investigate the polarization and emission properties of these pulsars through detailed modeling using the… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1349 semester 2025OCTS_04We propose a study of pulsars with interpulse (IP) emissions using the Ultra-Wideband Low (UWL) receiver on the Parkes radio telescope (Murriyang). This project aims to investigate the polarization and emission properties of these pulsars through detailed modeling using the… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1380 semester 2025OCTS_04The association of FRB 200428 with the Galactic magnetar SGR 1935+2154 confirms that magnetars can power fast radio bursts (FRBs). However, FRB 200428 is 4 to 8 orders of magnitude less energetic than the typical population of cosmological FRBs. This discrepancy is likely due to… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1380 semester 2025OCTS_05The association of FRB 200428 with the Galactic magnetar SGR 1935+2154 confirms that magnetars can power fast radio bursts (FRBs). However, FRB 200428 is 4 to 8 orders of magnitude less energetic than the typical population of cosmological FRBs. This discrepancy is likely due to… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1380 semester 2025OCTS_06The association of FRB 200428 with the Galactic magnetar SGR 1935+2154 confirms that magnetars can power fast radio bursts (FRBs). However, FRB 200428 is 4 to 8 orders of magnitude less energetic than the typical population of cosmological FRBs. This discrepancy is likely due to… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1382 semester 2025OCTS_09The prevalence of millisecond pulsars (MSPs) in and around the Galactic center and the bulge has been one of the key questions in pulsar astronomy. In addition to finding more exotic and interesting binary systems at and around the Galactic center and bulge due to the enhanced… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1382 semester 2025OCTS_10The prevalence of millisecond pulsars (MSPs) in and around the Galactic center and the bulge has been one of the key questions in pulsar astronomy. In addition to finding more exotic and interesting binary systems at and around the Galactic center and bulge due to the enhanced… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P1382 semester 2025OCTS_11The prevalence of millisecond pulsars (MSPs) in and around the Galactic center and the bulge has been one of the key questions in pulsar astronomy. In addition to finding more exotic and interesting binary systems at and around the Galactic center and bulge due to the enhanced… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P630 semester 2011APRS_11We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-03 | no licence stated |
| Parkes observations for project P630 semester 2011APRS_12We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-03 | no licence stated |
| Parkes observations for project P630 semester 2011APRS_13We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-03 | no licence stated |
| Parkes observations for project P630 semester 2011APRS_14We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-03 | no licence stated |
| Parkes observations for project P630 semester 2011APRS_15We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-03 | no licence stated |
| Parkes observations for project P630 semester 2011APRS_16We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future… | HTML | none stated | 2025-12-03 | no licence stated |
| Parkes observations for project P960 semester 2025OCTS_01We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and… | none stated | 2025-12-03 | no licence stated | |
| Parkes observations for project P960 semester 2025OCTS_03We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and… | none stated | 2025-12-03 | no licence stated | |
| Scripts and data associated with the techno-economic analysis of fugitive methane abatement from Australian landfillsCollection contains scripts and data associated with the techno-economic analysis of fugitive methane abatement from Australian landfills Authors: Andy Wilkins, Jun-Seok Bae, Courtney M Regan This report directory holds scripts and data associated with the 2025 CSIRO Report "A… | CSV, HTML, JSON, MARKDOWN +5 | none stated | 2025-12-03 | no licence stated |
| Drastic index map for the Fitzroy BasinThis dataset represents the intrinsic aquifer vulnerability to contamination evaluated for unconfined aquifers in Fitzroy, based on the DRASTIC method (Aller et al. 1987). This semi-quantitative but spatially distributed method is especially suited for regional investigations… | BIN | none stated | 2025-12-01 | no licence stated |
| Drastic index map for the Pilbara regionThis dataset represents the intrinsic aquifer vulnerability to contamination evaluated for unconfined aquifers in Fitzroy, based on the DRASTIC method (Aller et al. 1987). This semi-quantitative but spatially distributed method is especially suited for regional investigations… | BIN | none stated | 2025-12-01 | no licence stated |
| Drastic index map for the Upper Spencer Gulf regionThis dataset represents the intrinsic aquifer vulnerability to contamination evaluated for unconfined aquifers in Fitzroy, based on the DRASTIC method (Aller et al. 1987). This semi-quantitative but spatially distributed method is especially suited for regional investigations… | BIN | none stated | 2025-12-01 | no licence stated |
| ECL BuilderUI components that help you build SNOMED CT ECL expressions. | ZIP | none stated | 2025-12-01 | no licence stated |
| FHIR Bulk Client for JavaA Java client for the Bulk Data Export operation within the FHIR Bulk Data Access IG. | ZIP | none stated | 2025-12-01 | no licence stated |
| FHIR Terminology EncoderA tool for encoding FHIR terminology concepts for machine learning applications. | ZIP | none stated | 2025-12-01 | no licence stated |
| FHIR Validation on Apache SparkA tool for executing FHIR validation over a set of resources using Apache Spark. | ZIP | none stated | 2025-12-01 | no licence stated |
| Long-term project observations for project P1321 semester 2025APRS_11The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-12-01 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_12The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-12-01 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_13The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-12-01 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_14The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-12-01 | no licence stated | |
| Long-term project observations for project P1361 semester 2025APRS_06PSR J1227-6208 is a recycled pulsar in a bianry with a massive white dwarf companion. A recent timing measurement from combined MeerKAT and Parkes observations shows the companion mass to be between 1.2 and 1.5 $M \odot$, very close to the Chandrasekhar, resulting in potential… | none stated | 2025-12-01 | no licence stated | |
| Long-term project observations for project P885 semester 2025APRS_10We propose a modest program to continue monitoring 4 of the 6 known radio magnetars in order to achieve three primary science goals. The first is to characterise magnetar outbursts over long timescales, for which tracking their rotational, flux density, and polarisation… | none stated | 2025-12-01 | no licence stated | |
| MCP FHIR ToolsA collection of tools for working with FHIR data, designed to be used with Large Language Models via the Model Context Protocol. | ZIP | none stated | 2025-12-01 | no licence stated |
| NVCL Case Study: South Gawler Craton (MDSP11)This is a .tdg file of a HyLogger Dataset for drill hole MSDP11 from the South Gawler Craton of South Australia. It is for training purposes and allows full TSG capability without a TSG license. | ZIP | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P1054 semester 2025APRS_15With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourtytwo sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 19 in the Magellanic… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_12After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_13After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_14After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1211 semester 2024APRS_21Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary systems), extremely fast spinning pulsars (e.g., sub-MSPs), and high dispersion measure (DM) pulsars. Such a… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1211 semester 2024APRS_22Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary systems), extremely fast spinning pulsars (e.g., sub-MSPs), and high dispersion measure (DM) pulsars. Such a… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_46Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_47Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_48Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1357 semester 2025APRS_09MeerKAT has already discovered a number of Galactic transients, which are most likely to be Rotating Radio Transients (RRATs). Previous observations of a few of these sources with the Parkes UWL receiver have proven its utility in follow-up timing observations of MeerKAT… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P1363 semester 2025APRS_12We propose to monitor the bursts from the hyperactive repeating fast radio burst FRB 20240619D over six months using the Murriyang UWL receiver. The primary aim is to study the evolution of burst activity and polarization properties with frequency and time, and to discover any… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project P512 semester 2005OCTS_01A methanol multibeam pulsar survey | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P512 semester 2005OCTS_02A methanol multibeam pulsar survey | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P512 semester 2005OCTS_03A methanol multibeam pulsar survey | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_21We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_22We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_23We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_24We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project P960 semester 2025APRS_10We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project PX500 semester 2025APRS_26This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading. The primary reason for… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project PX500 semester 2025APRS_27This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading. The primary reason for… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project PX500 semester 2025APRS_28This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading. The primary reason for… | none stated | 2025-12-01 | no licence stated | |
| Parkes observations for project PX600 semester 2020APRS_124The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project PX600 semester 2020APRS_125The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-12-01 | no licence stated |
| Parkes observations for project PX600 semester 2020APRS_126The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-12-01 | no licence stated |
| RV Investigator Voyage IN2025_E02 End of Voyage (EOV) ArchiveThis record describes the End of Voyage (EOV) data archive from the Marine National Facility (MNF) RV Investigator voyage IN2025 E02, titled "IN2025 E02 Trials and Calibrations." The voyage took place between July 26, 2025 and August 02, 2025 (AEST), departing from Hobart and… | none stated | 2025-12-01 | no licence stated | |
| Spatial causal network for green hydrogen production in the Fitzroy region, QueenslandThis dataset was compiled by the Water for Sustainable Hydrogen project from source data referenced within the dataset and/or metadata. The spatial causal network comprises a rigorous and comprehensive scientific assessment of potential causal pathways by which hydrogen and… | BIN, HTML, XLSX | none stated | 2025-12-01 | no licence stated |
| Spatial causal network for green hydrogen production in the Upper Spencer Gulf region, South AustraliaThis dataset was compiled by the Water for Sustainable Hydrogen project from source data referenced within the dataset and/or metadata. The spatial causal network comprises a rigorous and comprehensive scientific assessment of potential causal pathways by which hydrogen and… | BIN, HTML, TIFF, XLSX +1 | none stated | 2025-12-01 | no licence stated |
| Spatial causal network for hydrogen production in the Pilbara region, Western AustraliaThis dataset was compiled by the Water for Sustainable Hydrogen project from source data referenced within the dataset and/or metadata. The spatial causal network comprises a rigorous and comprehensive scientific assessment of potential causal pathways by which hydrogen and… | BIN, HTML, XLSX | none stated | 2025-12-01 | no licence stated |
| Tipuana tipu distribution and climatic nicheThe dataset includes locations of Tipuana tipu, assembled to undertake species distribution modelling and climatic niche analysis. The results of this analysis are appended to the data, and R code for the analysis of results. | CSV, HTML | none stated | 2025-12-01 | no licence stated |
| A Standard Metadata Template for Representing Mineral Spectral Reference SamplesThis dataset contains a standard template for representing the metadata of mineral spectral reference specimens in the CSIRO Mineral Resources Discovery program. The template includes core properties of samples such as their name, identifier, type, and location, as well as… | XLSX | none stated | 2025-11-30 | no licence stated |
| A Standard Metadata Template For Representing Rock SpecimensThis dataset contains a standard template for representing the metadata of rock specimens (e.g., core, microanalysis, hand grab) in the CSIRO Mineral Resources Discovery program. The template includes core properties of samples such as their name, identifier, type, and location… | XLSX | none stated | 2025-11-30 | no licence stated |
| A Standard Metadata Template for Representing Soil SpecimensThis dataset contains a standard template for representing the metadata of soil specimens in the CSIRO Mineral Resources Discovery program. The template includes core properties of samples such as their name, identifier, type, and location, as well as associated metadata such as… | XLSX | none stated | 2025-11-30 | no licence stated |
| Agricultural climate metrics for the National Climate Risk AssessmentAgricultural climate metrics were derived for the National Climate Risk Assessment. This data collection describes the agricultural climate metrics derived from projections of climate variables across Australia from 8 CMIP6 global climate models, as well as a historical baseline… | BIN, DOCX | none stated | 2025-11-30 | no licence stated |
| BERI v2: Bioclimatic Ecosystem Resilience Index: 30s global time seriesCSIRO Bioclimatic Ecosystem Resilience Index (BERI v2) is a global 30 arc-second product for the years 2000, 2005, 2010, 2015 and 2020. BERI measures the capacity of natural ecosystems to retain species diversity in the face of climate change, as a function of ecosystem area… | HTML, PDF, PNG, TIFF +1 | none stated | 2025-11-30 | no licence stated |
| BHI v2: Biodiversity Habitat Index: 30s global time seriesCSIRO Biodiversity Habitat Index (BHI v2) is a global 30 arc-second product for 2000,2005,2010,2015 and 2020. BHI estimates the level of species diversity expected to be retained within any given spatial reporting unit (e.g., a country, a broad ecosystem type, or the entire… | HTML, PDF, PNG, TIFF +1 | none stated | 2025-11-30 | no licence stated |
| Blue Carbon Ecosystems of Papua New Guinea (PNG)This spatial data represents outputs from the Pacific Blue Carbon project for Papua New Guinea (PNG). Here we map Blue Carbon Ecosystems (BCE) for PNG using Earth observation data for 2020. This research project aimed to evaluate Living Earth for obtaining consistent and… | HTML, TIFF | none stated | 2025-11-30 | no licence stated |
| Data - Modelling Sectoral Technology and Emissions Pathways to 2035 and Net ZeroData and charts for figures of CSIRO's 'Modelling Sectoral Technology and Emissions Pathways to 2035 and Net Zero Emissions - Final Report' To assist the Australian Government in developing a national net zero emissions by 2050 plan, the parliament requested that the Climate… | PDF, XLSX | none stated | 2025-11-30 | no licence stated |
| Data and code for "Larval seedboxes: a modular and effective tool for scaling coral reef restoration"This dataset contains the experimental data underpinning the development and field testing of the larval seedbox, a modular and passive delivery system designed to scale coral reef restoration. Data include larval culturing, seedbox deployments, and coral settlement surveys… | ZIP | none stated | 2025-11-30 | no licence stated |
| Deep sea coral chemical composition data used in Thresher et al. "Southern Ocean overturning presages historical and recent changes in the North Atlantic meridional overturning circulation"Chemical composition of deep sea corals | CSV | none stated | 2025-11-30 | no licence stated |
| Fisheries and aquaculture data for the National Climate Risk AssessmentWhat is the data? Projections of marine climate hazards, and marine exploitable animal biomass across Australia's Exclusive Economic Zone and regional areas. Hazard data were supplied by the Australian Climate Service (ACS) from data stored on the National Computational… | BIN | none stated | 2025-11-30 | no licence stated |
| Impact of environmental gradients on juvenile coral demography across the Great Barrier Reef and Torres StraitThis study spanned 14° of latitude from the southern to northern Great Barrier Reef and Torres Strait. The southernmost reef was Lady Musgrave (latitude 23.9°S), while the northernmost reef was Masig Island (Masig = 9.45°S). Across this latitudinal gradient, reefs were situated… | XLSX | none stated | 2025-11-30 | no licence stated |
| Long-term project observations for project P1101 semester 2025APRS_08We propose a long-term project to monitor a very active repeater, FRB 20190520B, with Murriyang's UWL system. Our previous observations show that FRB 20190520B is not only among the most active FRBs that can be observed with Murriyang, but also shows extreme rotation measure… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_15The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_16The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_17The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_18The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_19The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1321 semester 2025APRS_20The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this Tiny-Scale Atomic Structure (TSAS) has significant implications, potentially calling into question our… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P1361 semester 2025APRS_07PSR J1227-6208 is a recycled pulsar in a bianry with a massive white dwarf companion. A recent timing measurement from combined MeerKAT and Parkes observations shows the companion mass to be between 1.2 and 1.5 $M \odot$, very close to the Chandrasekhar, resulting in potential… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P455 semester 2025APRS_04This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Important results published in our 53-page Phys. Rev. X paper (2021) include the first measurements of higher-order light-propagation effects… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P455 semester 2025APRS_05This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Important results published in our 53-page Phys. Rev. X paper (2021) include the first measurements of higher-order light-propagation effects… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P456 semester 2025APRS_10The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. We are now in an exciting regime… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P574 semester 2025APRS_10We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what disrupts this process, how and why their profiles vary with time, whether they precess or have planetary… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P574 semester 2025APRS_11We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what disrupts this process, how and why their profiles vary with time, whether they precess or have planetary… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P574 semester 2025APRS_12We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what disrupts this process, how and why their profiles vary with time, whether they precess or have planetary… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P574 semester 2025APRS_13We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what disrupts this process, how and why their profiles vary with time, whether they precess or have planetary… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P574 semester 2025APRS_14We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what disrupts this process, how and why their profiles vary with time, whether they precess or have planetary… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P885 semester 2025APRS_11We propose a modest program to continue monitoring 4 of the 6 known radio magnetars in order to achieve three primary science goals. The first is to characterise magnetar outbursts over long timescales, for which tracking their rotational, flux density, and polarisation… | none stated | 2025-11-30 | no licence stated | |
| Long-term project observations for project P885 semester 2025APRS_12We propose a modest program to continue monitoring 4 of the 6 known radio magnetars in order to achieve three primary science goals. The first is to characterise magnetar outbursts over long timescales, for which tracking their rotational, flux density, and polarisation… | none stated | 2025-11-30 | no licence stated | |
| Modelled quantification plausible impacts of Biological Nitrification Inhibition in Australian cropping systemsThis collection consists of the model set-up used to develop an initial capability for modelling biological nitrification inhibition (BNI) in APSIM Next Generation and a preliminary evaluation of BNI in wheat, canola, sorghum and maize systems across Australian grain regions. To… | none stated | 2025-11-30 | no licence stated | |
| NEMX.jlNEMX.jl is an open source package developed in Julia using JuMP based on PowerModelsACDC.jl that provides physics-based co-optimized electricity and frequency control ancillary services (FCAS) market clearing models for the Australian National Electricty Market (NEM)… | ZIP | none stated | 2025-11-30 | no licence stated |
| PARC: Protected Area Representativeness Index: 30s global time seriesCSIRO Protected Area Representativeness Index (PARC: Representativeness) is a global 30 arc-second product for 1970,1980,1990,2000,2005,2010,2015, 2020, and 2024. The Protected Area Representativeness and Connectedness (PARC) indices measure the extent to which terrestrial… | HTML, PDF, PNG, TIFF +1 | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P1054 semester 2025APRS_16With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourtytwo sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 19 in the Magellanic… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1165 semester 2025APRS_06We recently discovered two new pulsars J1849+1001 (35.1 ms) and J1839+0542 (57.9 ms) in a FAST pulsar survey at intermediate Galactic latitudes (PT2020 0141). Follow-up timing observations show that they are in circular orbits with massive companions. This suggests that PSR… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_15After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_16After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_17After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_18After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_19After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_20After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_21After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1183 semester 2025APRS_22After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1211 semester 2024APRS_23Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary systems), extremely fast spinning pulsars (e.g., sub-MSPs), and high dispersion measure (DM) pulsars. Such a… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1211 semester 2024APRS_24Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary systems), extremely fast spinning pulsars (e.g., sub-MSPs), and high dispersion measure (DM) pulsars. Such a… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1219 semester 2025APRS_10Magnetic fields are fundamental in regulating star formation and the evolution of molecular clouds. Zeeman splitting offers a unique method to directly measure line-of-sight magnetic field strengths in interstellar environments, from the diffuse ISM to dense cores. Observations… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1219 semester 2025APRS_11Magnetic fields are fundamental in regulating star formation and the evolution of molecular clouds. Zeeman splitting offers a unique method to directly measure line-of-sight magnetic field strengths in interstellar environments, from the diffuse ISM to dense cores. Observations… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1219 semester 2025APRS_12Magnetic fields are fundamental in regulating star formation and the evolution of molecular clouds. Zeeman splitting offers a unique method to directly measure line-of-sight magnetic field strengths in interstellar environments, from the diffuse ISM to dense cores. Observations… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1325 semester 2025APRS_07We request 15 hours of observing time with the Parkes UWL receiver (700-4000 MHz) to investigate frequency-dependent eclipsing in three spider millisecond pulsars (MSPs): one redback and two black widows. Spider MSPs commonly exhibit frequency-dependent eclipsing, which provides… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1325 semester 2025APRS_08We request 15 hours of observing time with the Parkes UWL receiver (700-4000 MHz) to investigate frequency-dependent eclipsing in three spider millisecond pulsars (MSPs): one redback and two black widows. Spider MSPs commonly exhibit frequency-dependent eclipsing, which provides… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1328 semester 2025APRS_16Fast radio bursts are peculiar micro-millisecond duration transients, which have been seen to be extragalactic in origin. Since their discovery, a dichotomy has emerged in their population. Some FRBs have been seen to be repeating, while others have not been seen to be… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1328 semester 2025APRS_17Fast radio bursts are peculiar micro-millisecond duration transients, which have been seen to be extragalactic in origin. Since their discovery, a dichotomy has emerged in their population. Some FRBs have been seen to be repeating, while others have not been seen to be… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_49Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_50Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_51Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_52Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_53Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_54Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_55Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_56Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1338 semester 2025APRS_58Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1343 semester 2025APRS_06Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1343 semester 2025APRS_07Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1343 semester 2025APRS_08Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1345 semester 2025APRS_16This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade (CRACO) system. Over the past 12-months of commissioning, CRACO discovered and precisely localised 15 new… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1345 semester 2025APRS_17This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade (CRACO) system. Over the past 12-months of commissioning, CRACO discovered and precisely localised 15 new… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1345 semester 2025APRS_18This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade (CRACO) system. Over the past 12-months of commissioning, CRACO discovered and precisely localised 15 new… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1345 semester 2025APRS_19This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade (CRACO) system. Over the past 12-months of commissioning, CRACO discovered and precisely localised 15 new… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1349 semester 2025APRS_04We propose an investigation of pulsars with interpulse (IP) emissions using the Ultra-wide-bandwidth Low (UWL) receiver at the Parkes (Murriyang) telescope. We aim to explore the polarization and emission properties of these pulsars through the application of the rotating vector… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1349 semester 2025APRS_05We propose an investigation of pulsars with interpulse (IP) emissions using the Ultra-wide-bandwidth Low (UWL) receiver at the Parkes (Murriyang) telescope. We aim to explore the polarization and emission properties of these pulsars through the application of the rotating vector… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1349 semester 2025APRS_06We propose an investigation of pulsars with interpulse (IP) emissions using the Ultra-wide-bandwidth Low (UWL) receiver at the Parkes (Murriyang) telescope. We aim to explore the polarization and emission properties of these pulsars through the application of the rotating vector… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1349 semester 2025APRS_07We propose an investigation of pulsars with interpulse (IP) emissions using the Ultra-wide-bandwidth Low (UWL) receiver at the Parkes (Murriyang) telescope. We aim to explore the polarization and emission properties of these pulsars through the application of the rotating vector… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1356 semester 2025APRS_13Magnetars are neutron stars with exceptionally high magnetic fields. From the 30 known magnetars, only six have had radio emission detected so far. The remaining 24 magnetars are generally only searched for radio emission after an X-ray outburst. This added a strong selection… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1356 semester 2025APRS_14Magnetars are neutron stars with exceptionally high magnetic fields. From the 30 known magnetars, only six have had radio emission detected so far. The remaining 24 magnetars are generally only searched for radio emission after an X-ray outburst. This added a strong selection… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1356 semester 2025APRS_15Magnetars are neutron stars with exceptionally high magnetic fields. From the 30 known magnetars, only six have had radio emission detected so far. The remaining 24 magnetars are generally only searched for radio emission after an X-ray outburst. This added a strong selection… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1357 semester 2025APRS_10MeerKAT has already discovered a number of Galactic transients, which are most likely to be Rotating Radio Transients (RRATs). Previous observations of a few of these sources with the Parkes UWL receiver have proven its utility in follow-up timing observations of MeerKAT… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1362 semester 2025APRS_05PSR J1757-1854 is the most relativistic galactic double neutron star system. Its eccentricity makes it an ideal playground for gravity experiments with pulsar timing. Via observations of its profile evolution, we can constraint its rate of geodetic precession. Currently, there… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1363 semester 2025APRS_13We propose to monitor the bursts from the hyperactive repeating fast radio burst FRB 20240619D over six months using the Murriyang UWL receiver. The primary aim is to study the evolution of burst activity and polarization properties with frequency and time, and to discover any… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P1363 semester 2025APRS_14We propose to monitor the bursts from the hyperactive repeating fast radio burst FRB 20240619D over six months using the Murriyang UWL receiver. The primary aim is to study the evolution of burst activity and polarization properties with frequency and time, and to discover any… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project P512 semester 2006APRS_01We propose to undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the spiral arms… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2006APRS_02We propose to undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the spiral arms… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2006APRS_03We propose to undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the spiral arms… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2006OCTS_01We propose to continue undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2006OCTS_02We propose to continue undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2007APRS_01We propose to continue undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2007APRS_02We propose to continue undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P512 semester 2007APRS_03We propose to continue undertake a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower frequency surveys. The scientific aims of this survey are (a) to discover young pulsars in the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_25We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_26We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_27We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_28We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_29We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P595 semester 2025APRS_30We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P737 semester 2025APRS_04Instrumental Commissioning | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project P960 semester 2025APRS_11We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project PX500 semester 2025APRS_29This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading. The primary reason for… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project PX500 semester 2025APRS_30This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading. The primary reason for… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project PX500 semester 2025APRS_31This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading. The primary reason for… | none stated | 2025-11-30 | no licence stated | |
| Parkes observations for project PX600 semester 2020APRS_127The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project PX600 semester 2020APRS_128The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project PX600 semester 2020APRS_129The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-11-30 | no licence stated |
| Parkes observations for project PX600 semester 2020APRS_130The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most… | HTML | none stated | 2025-11-30 | no licence stated |
| Penaeus monodon whole genome sequenceWhole genome sequence from Penaeus monodon obtained at various geographical locations | GZ | none stated | 2025-11-30 | no licence stated |
| Population genomics of Cape ivy (Delairea odorata)Collection contains Single Nucleotide Polymorphism (SNP) population genomic data for populations of Cape ivy from its native range of South Africa and its introduced ranges of Australia, France, New Zealand, and United States. In total, SNP data for 921 cape ivy samples across… | CSV, TSV | none stated | 2025-11-30 | no licence stated |
| RV Investigator Voyage IN2025_V04 End of Voyage (EOV) ArchiveThis record describes the End of Voyage (EOV) data archive from the Marine National Facility (MNF) RV Investigator voyage IN2025 V04, titled "Untangling the causes of change over 25 years in the southeast marine ecosystem - Voyage IV (SEA-MES Voyage 4)." The voyage took place… | none stated | 2025-11-30 | no licence stated | |
| Simulation output for baseline monitoring design of Crown-of-thorns starfish (COTS) in the Great Barrier Reef (GBR)This data collection contains simulation output from GBR-based models used for the analysis for Lawrence et al. (2025). The data contain Crown-of-thorns starfish and coral cover output from 500 simulations of (i) CoConet (Condie et al., 2021) and (ii) ReefMod-GBR (Mumby et al… | CSV | none stated | 2025-11-30 | no licence stated |
| Surface swabs outperform most traditional honeybee (Apis mellifera) hive samples for recovery of eDNA and eRNARaw data files, analysis scripts and input files to generate data presented in the manuscript | CSV, HTML, PDF, TXT +2 | none stated | 2025-11-30 | no licence stated |
| Vegetation (BOTANAL) data for four control and four treatment (gully) remediation sites in the Burdekin catchmentThis Collection contains vegetation measurements analysed and published in the paper: Bartley, R., Abbott, B., Murray, B., Kinsey-Henderson, A., Hawdon, A., 2025. Rehabilitating vegetation and demonstrating co-benefits in highly degraded rangelands draining to the Great Barrier… | CSV | none stated | 2025-11-30 | no licence stated |
| Annual vegetation height for Australia for 2019 to 2024This product provides an annual estimate of vegetation height (top of canopy) for 2019 to 2024 at a 30m pixel size. These images are created using an extreme gradient boosting regressor (XGBoost) machine learning model which was training using GEDI vegetation height (from the… | PDF, TIFF | none stated | 2025-11-29 | no licence stated |
| CSIRO Laterite Geochemistry Data CompilationThis dataset comprises geochemical data from laterite samples collected during CSIRO projects led by Ray Smith between 1983 and 2000. The samples include various forms of lateritic material, such as lateritic duricrust (both nodular and pisolitic), loose lateritic pisoliths, and… | XLSX | none stated | 2025-11-29 | no licence stated |
| Error-mitigated quantum computing SEMO Python dynamic moduleQubit noise is one of the major barriers limiting broad adoption of quantum computing in solving complex real-word problems, such as optimisation. The qubit noise and the local minima in the underlying optimisation objective function often make the probability of obtaining the… | HTML, PDF, TXT | none stated | 2025-11-29 | no licence stated |
| Geomorphic change detection between 2018 and 2024 for the Fitzroy River Basin Queensland AustraliaThis dataset shows geomorphic change in the Fitzroy River Basin Queensland, Australia. The change is determined by the difference in elevation in the overlapping areas of two co-registered airborne laser scanning (ALS) point cloud datasets, collected in 2018 and 2024. The change… | CSV, HTML, TIFF, ZIP | none stated | 2025-11-29 | no licence stated |
| Long-term project observations for project P1041 semester 2025APRS_06Omega Cen is the largest globular cluster in the Milky Way. I contains at least 18 known MPSs, and there are solid hints for the presence of an even larger pulsar population. We propose a regular monthly follow-up to refine the timing solutions of the five Parkes discoveries… | none stated | 2025-11-29 | no licence stated | |
| Long-term project observations for project P1101 semester 2025APRS_09We propose a long-term project to monitor a very active repeater, FRB 20190520B, with Murriyang's UWL system. Our previous observations show that FRB 20190520B is not only among the most active FRBs that can be observed with Murriyang, but also shows extreme rotation measure… | none stated | 2025-11-29 | no licence stated |
The full list of 1,133 is in catalogue.json.
Listed from the portals' own catalogues, read 28 September 2026. CSIRO Data Access Portal has not endorsed this site. Every dataset here keeps its publisher's licence and attribution. catalogue.json has this list as data.