{"elapsedTime":46,"totalResults":"10000+","page":1,"resultsPerPage":25,"next":{"relationship":"next","mediaType":null,"href":"https://data.csiro.au/dap/ws/v2/collections.json?p=2","fileUpload":false,"fileId":0},"previous":null,"first":{"relationship":"first","mediaType":null,"href":"https://data.csiro.au/dap/ws/v2/collections.json?p=1","fileUpload":false,"fileId":0},"last":{"relationship":"last","mediaType":null,"href":"https://data.csiro.au/dap/ws/v2/collections.json?p=400","fileUpload":false,"fileId":0},"query":"","criteria":null,"showOnlyUnrestrictedDataForUser":false,"sortBy":"RELEVANCE","complete":false,"dataCollections":[{"id":{"identifierType":"Fedora PID","identifier":"csiro:74183"},"dataCollectionId":74183,"self":"https://data.csiro.au/dap/ws/v2/collections/74183","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74183","fileUpload":false,"fileId":0},"title":"Optimising Canola Heterotic Pools project data sets","description":"SNP genotype data and trait data for the OzCanola diversity panel for use in the GRDC heterotic pools optimisation project","licence":"Creative Commons Attribution Noncommercial-Share Alike 4.0 Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1202","fileUpload":false,"fileId":0},"attributionStatement":"Dillon, Shannon; Mekkawy, Wagdy; Helliwell, Chris; Ahmed, Asif; Whish, Jeremy; Lilley, Julianne; Zwart, Alec; & Zheng, Bangyou (2026): Optimising Canola Heterotic Pools project data sets. v1. CSIRO. Data Collection. https://doi.org/10.25919/hhyf-jy79","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-20T03:02:44.007+10:00","leadResearcher":"Shannon Dillon","serviceCount":0,"contributors":["Wagdy Mekkawy","Chris Helliwell","Asif Ahmed","Jeremy Whish","Julianne Lilley","Alec Zwart","Bangyou Zheng"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/734407","doi":"10.25919/hhyf-jy79","project":{"irpHierarchy":true,"wbs":"R-22956","projectDescription":"GRDC: New Tools and knowledge for Optimising Heterotic Pools in Canola - CSP2512-009RTX"},"dataRestricted":"TRUE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:62180"},"dataCollectionId":74190,"self":"https://data.csiro.au/dap/ws/v2/collections/74190","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:62180","fileUpload":false,"fileId":0},"title":"Error-mitigated quantum computing SEMO Python dynamic module","description":"Qubit 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 true optimal solution (global optimal rather than local minima) decrease exponentially with increasing underlying problem complexity. A quantum computing error mitigation invention has been filed by CSIRO with IP Australia in Feb 2024. Based on the invention, a Python SEMO (spin-error mitigation for optimisation) software module has been developed.  The SEMO software module is available for collaboration for selected parties with a SEMO digital token issued from the CSIRO applied quantum computing project team. The token is authenticated online against the registration server at the beginning of each usage session. The SEMO software module can be evaluated without a digital token for small problems up to 100 spin variables and 200 couplings. \nInformation about CSIRO applied quantum computing and SEMO is available at http://research.csiro.au/aqc. Enquiries about accessing the SEMO software module, please email appliedquantumcomputing@csiro.au. ","licence":"CSIRO Binary Software Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1081","fileUpload":false,"fileId":0},"attributionStatement":"Yang, Sam; Chu, Clement; & Tyson, Peter (2026): Error-mitigated quantum computing SEMO Python dynamic module. CSIRO. v26. Software. https://doi.org/10.25919/2v3e-e927","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-19T07:05:53.721+10:00","leadResearcher":"Sam Yang","serviceCount":0,"contributors":["Clement Chu","Peter Tyson"],"activity":{"activityTitle":"Applied quantum computing"},"collectionType":"Software","domainType":"Everything Else","andsPid":"102.100.100/614516","doi":"10.25919/2v3e-e927","project":{"irpHierarchy":true,"wbs":"R-19618","projectDescription":"QT-FSP_Quantum Annealing for Materials and Processes"},"dataRestricted":"FALSE","dataVersionNumber":"26","softwareVersionNumber":"0.97"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74189"},"dataCollectionId":74189,"self":"https://data.csiro.au/dap/ws/v2/collections/74189","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74189","fileUpload":false,"fileId":0},"title":"Long-term project observations for project L126 semester 2026APRS_02","description":"We 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 properties provide a clear view of the impulse response of their magnetic fields. Second, understanding the links between magnetars the mysterious fast radio burst phenomenon through the discovery of rare emission and propagation effects, shared spectro-temporal phenomenology, and connections to high-energy (X-ray/gamma-ray) phenomena. Lastly, our continued monitoring has enormous benefit to the wider magnetar community, providing rapid alerts to changes in activity, adding context to unusual behaviour detected by high-energy observations, and a host of supplementary science through the teams extensive collaborative networks. The project and its precursors have been running since 2007 and have contributed to 22 publications since then. This is the first submission since the project was converted to long-term status.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Camilo, Fernando; Sarkissian, John; Reynolds, John; Scholz, Paul; Lower, Marcus; & Younes, George (2026): Long-term project observations for project L126 semester 2026APRS_02. v1. CSIRO. Data Collection. https://doi.org/10.25919/dx06-wt87","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T21:06:02.599+10:00","leadResearcher":"Fernando Camilo","serviceCount":0,"contributors":["John Sarkissian","John Reynolds","Paul Scholz","Marcus Lower","George Younes"],"activity":{"activityTitle":"L126 - Understanding the Remarkable Behaviour of Radio Magnetars"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734406","doi":"10.25919/dx06-wt87","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74185"},"dataCollectionId":74185,"self":"https://data.csiro.au/dap/ws/v2/collections/74185","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74185","fileUpload":false,"fileId":0},"title":"Long-term project observations for project L134 semester 2026APRS_01","description":"Omega 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 from 2020, and to find timing solutions for the 13 MeerKAT discoveries from 2023, in combination with six MeerKAT observations between 2021 and 2023, and future MeerKAT observations. These timing solutions should enable the detection of derivatives of the spin periods of these pulsars, allowing us to probe the dynamics of Omega Cen and the presence of a possible IMBH at its centre. Timing solutions will also enable the search for X-ray and gamma-ray pulsations in the multiple sources detected in this cluster. This study will allow us to better understand the populations of this globular cluster and its formation history. We request observations until 2030, when we expect to have measurements of the second period derivative of the five brighter discoveries, and first period derivative measurements for the later discoveries. These observations will also contribute to the study of eclipsing binaries, and may include future discoveries from pending searches in MeerKAT data.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Colom I Bernadich, Miquel; Possenti, Andrea; Kramer, Michael; Burgay, Marta; Bailes, Matthew; Stappers, Benjamin; Keane, Evan; Dai, Shi; Ridolfi, Alessandro; Chen, Weiwei; & Abbate, Federico (2026): Long-term project observations for project L134 semester 2026APRS_01. v1. CSIRO. Data Collection. https://doi.org/10.25919/7zn6-pz61","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T21:05:51.429+10:00","leadResearcher":"Miquel Colom I Bernadich","serviceCount":0,"contributors":["Andrea Possenti","Michael Kramer","Marta Burgay","Matthew Bailes","Benjamin Stappers","Evan Keane","Shi Dai","Alessandro Ridolfi","Weiwei Chen","Federico Abbate"],"activity":{"activityTitle":"L134 - LONG-TERM TIMING OF MILLISECOND PULSARS IN GLOBULAR CLUSTER OMEGA CENTAURI"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734405","doi":"10.25919/7zn6-pz61","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74186"},"dataCollectionId":74186,"self":"https://data.csiro.au/dap/ws/v2/collections/74186","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74186","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1054 semester 2026APRS_07","description":"With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fiftythree sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 27 in the Magellanic Clouds, 109 in Globular Clusters and 96 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including a few relativistic systems, a pulsar with a planetary companion and  several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing for the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Burgay, Marta; Possenti, Andrea; Kramer, Michael; Freire, Paulo; Stappers, Benjamin; Levin, Lina; Champion, David; Buchner, Sarah; Barr, Ewan; Venkatraman Krishnan, Vivek; Karuppusamy, Ramesh; Clark, Colin James; Breton, Rene; Ridolfi, Alessandro; Cognard, Ismaël; Grießmeier, Jean-Mathias; Colom I Bernadich, Miquel; Thongmeearkom, Tinn; Carli, Emma;...Sergio, Belmonte Dìaz (2026): Parkes observations for project P1054 semester 2026APRS_07. v1. CSIRO. Data Collection. https://doi.org/10.25919/4znk-4728","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T21:05:17.527+10:00","leadResearcher":"Marta Burgay","serviceCount":0,"contributors":["Andrea Possenti","Michael Kramer","Paulo Freire","Benjamin Stappers","Lina Levin","David Champion","Sarah Buchner","Ewan Barr","Vivek Venkatraman Krishnan","Ramesh Karuppusamy","Colin James Clark","Rene Breton","Alessandro Ridolfi","Ismaël Cognard","Jean-Mathias Grießmeier","Miquel Colom I Bernadich","Tinn Thongmeearkom","Emma Carli","James Turner","Venu Prayag","Belmonte Dìaz Sergio"],"activity":{"activityTitle":"P1054 - Follow-up of pulsar discoveries from MeerKAT searches"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734404","doi":"10.25919/4znk-4728","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74187"},"dataCollectionId":74187,"self":"https://data.csiro.au/dap/ws/v2/collections/74187","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74187","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1413 semester 2026APRS_03","description":"We request 75 hours of Parkes observing time for dedicated radio follow-up observations of PSR J1635-5134, a promising candidate pulsar-subdwarf B (sdB) star binary system. PSR J1635-5134 is a non-recycled 340 ms pulsar in a nearly circular 18-hour orbit with a minimum companion mass of 0.26 solar mass. It lies in a sparsely populated region of binary-pulsars parameter space and may represent a short-lived evolutionary stage immediately following inefficient spin-up, thereby providing a missing link between canonical binaries and the millisecond pulsar-WD population. The system exhibits peculiar, orbital-phase-dependent dispersion-measure (DM) variability, with DM variations exceeding 30 pc/cc, indicating substantial ionised material plausibly associated with an outflow from the companion. Moreover, during prior monitoring with Parkes, the DM variations shifted from being predominantly modest to being persistently large, implying an evolving plasma environment that cannot be characterised with sparse or irregular observations. Determining whether these high-DM variations are intermittent or long-lived, and mapping how the excess material varies with orbital phase and epoch, are essential for constraining the origin and geometry of the plasma and for testing the hypothesis that an sdB wind supplies the required electron column. Through this proposal, we aim to (i) extend the timing baseline to improve astrometric precision to sub-arcsecond accuracy, enabling secure identification of the optical counterpart in a crowded field, and (ii) perform phase-targeted observations during eclipse/DM variation phases to understand the temporal behavior of excess DM.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Sengar, Rahul; Bailes, Matthew; Tauris, Thomas; Kaplan, David; & Clark, Colin James (2026): Parkes observations for project P1413 semester 2026APRS_03. v1. CSIRO. Data Collection. https://doi.org/10.25919/mf4m-ra22","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T21:05:16.948+10:00","leadResearcher":"Rahul Sengar","serviceCount":0,"contributors":["Matthew Bailes","Thomas Tauris","David Kaplan","Colin James Clark"],"activity":{"activityTitle":"P1413 - Follow up of a Missing-Link Binary: PSR J1635-5134 as a Potential Pulsar-sdB Binary System"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734403","doi":"10.25919/mf4m-ra22","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74188"},"dataCollectionId":74188,"self":"https://data.csiro.au/dap/ws/v2/collections/74188","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74188","fileUpload":false,"fileId":0},"title":"Parkes observations for project P595 semester 2026APRS_04","description":"We 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 space missions, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Hobbs, George; Hollow, Robert; Dai, Shi; Zic, Andrew; Mandow, Rami; Kaur, Dilpreet; Ling, Wenhua; & Pritchard, Joshua (2026): Parkes observations for project P595 semester 2026APRS_04. v1. CSIRO. Data Collection. https://doi.org/10.25919/rhr8-rh06","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T21:05:17.817+10:00","leadResearcher":"George Hobbs","serviceCount":0,"contributors":["Robert Hollow","Shi Dai","Andrew Zic","Rami Mandow","Dilpreet Kaur","Wenhua Ling","Joshua Pritchard"],"activity":{"activityTitle":"P595 - PULSE@Parkes (Pulsar Student Exploration online at Parkes)"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734402","doi":"10.25919/rhr8-rh06","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:CASDA-ATOA-P1407-2026APRS"},"dataCollectionId":74191,"self":"https://data.csiro.au/dap/ws/v2/collections/74191","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:CASDA-ATOA-P1407-2026APRS","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1407 semester 2026APRS","description":"The study of low-mass dwarf galaxies plays a key role in understanding the formation, star formation, and chemical evolution of galaxies in the Universe. In this project, we propose a survey of 47 nearby southern sky dwarf galaxies that have not previously been observed in HI. This will allow us to measure fundamental HI properties, determine their redshifts, HI fluxes, and HI line-widths. These measurements will enable us to extend the HI mass function into the faint-end region. More than half of the sample is composed of recently discovered Local Volume galaxy candidates that were identified through a visual search of a large region of the sky in DESI Legacy Surveys. Each of the other galaxies in the sample resides outside the FASHI survey area and has not previously been observed in HI. These dwarfs are characterized by irregular morphology and sizes of about 1 arcmin, suggesting that they are low-mass galaxies within ~10 Mpc. The blue colors of the stellar populations indicate recent star formation and the presence of a significant amount of neutral HI. Observations of these galaxies will allow us to determine the properties of the interstellar medium (ISM) for the first time and will motivate future interferometric observations","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Marine, Joshua; Cannon, John; & Codd, Jackson (2026): Parkes observations for project P1407 semester 2026APRS. v1. CSIRO. Data Collection. http://hdl.handle.net/102.100.100/734401?index=1","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T17:48:40.353+10:00","leadResearcher":"Joshua Marine","serviceCount":0,"contributors":["John Cannon","Jackson Codd"],"activity":{"activityTitle":"P1407 - The HI Content of Candidate Local Volume Low-Mass Galaxies"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734401","doi":null,"project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"TRUE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74161"},"dataCollectionId":74161,"self":"https://data.csiro.au/dap/ws/v2/collections/74161","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74161","fileUpload":false,"fileId":0},"title":"Parkes observations for project P595 semester 2026APRS_03","description":"We 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 space missions, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Hobbs, George; Hollow, Robert; Dai, Shi; Zic, Andrew; Mandow, Rami; Kaur, Dilpreet; Ling, Wenhua; & Pritchard, Joshua (2026): Parkes observations for project P595 semester 2026APRS_03. v1. CSIRO. Data Collection. https://doi.org/10.25919/kvt9-p955","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T06:29:11.931+10:00","leadResearcher":"George Hobbs","serviceCount":0,"contributors":["Robert Hollow","Shi Dai","Andrew Zic","Rami Mandow","Dilpreet Kaur","Wenhua Ling","Joshua Pritchard"],"activity":{"activityTitle":"P595 - PULSE@Parkes (Pulsar Student Exploration online at Parkes)"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734400","doi":"10.25919/kvt9-p955","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74162"},"dataCollectionId":74162,"self":"https://data.csiro.au/dap/ws/v2/collections/74162","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74162","fileUpload":false,"fileId":0},"title":"Parkes observations for project PX144 semester 2026APRS_01","description":"Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"CSIRO; & Sengar, Rahul (2026): Parkes observations for project PX144 semester 2026APRS_01. v1. CSIRO. Data Collection. https://doi.org/10.25919/x570-2w90","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T06:29:11.708+10:00","leadResearcher":"CSIRO","serviceCount":0,"contributors":["Rahul Sengar"],"activity":{"activityTitle":"PUNDEF - Pulsar projects (undefined in OPAL)"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734399","doi":"10.25919/x570-2w90","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:62968"},"dataCollectionId":74184,"self":"https://data.csiro.au/dap/ws/v2/collections/74184","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:62968","fileUpload":false,"fileId":0},"title":"OzWheat v1.0 GWAS platform datasets","description":"Genomic/pedigree and marker-trait association data associated with the following publication; Hyles, J., Eagles, H., et al. (2024). OzWheat; a genome-to-phenome platform to resolve complex traits for wheat pre-breeding and research. ","licence":"Creative Commons Attribution-Noncommercial 4.0 Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1181","fileUpload":false,"fileId":0},"attributionStatement":"Hyles, Jessica; Eagles, Howard; Ramm, Kerrie; Sherman, Bjorg; Gock, Andrew; Stops, Sandra; Phongkham, Tanya; Leyne, Emmett; Rathjen, Tina; Suchecki, Rad; Stevens, Lauren; Ord, Louise; Fradgley, Nick; McNeil, Meredith; Marquardt, Annelie; Andrew, Sam; Forrest, Kerrie; Eastwood, Russell; Norman, Adam;...Dillon, Shannon (2026): OzWheat v1.0 GWAS platform datasets. v1. CSIRO. Data Collection. https://doi.org/10.25919/v1x6-9q97","rights":"All Rights (including copyright) CSIRO 2024.","published":"2026-04-18T04:32:46.834+10:00","leadResearcher":"Jessica Hyles","serviceCount":0,"contributors":["Howard Eagles","Kerrie Ramm","Bjorg Sherman","Andrew Gock","Sandra Stops","Tanya Phongkham","Emmett Leyne","Tina Rathjen","Rad Suchecki","Lauren Stevens","Louise Ord","Nick Fradgley","Meredith McNeil","Annelie Marquardt","Sam Andrew","Kerrie Forrest","Russell Eastwood","Adam Norman","Annette Tredrea","Richard Trethowan","Ben Trevaskis","Shannon Dillon"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/636950","doi":"10.25919/v1x6-9q97","project":{"irpHierarchy":true,"wbs":"R-15556","projectDescription":"SIP020_Genome to phenome platforms V2.0"},"dataRestricted":"TRUE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:73142"},"dataCollectionId":74098,"self":"https://data.csiro.au/dap/ws/v2/collections/74098","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:73142","fileUpload":false,"fileId":0},"title":"National data for Australia's ecosystem services: groundwater fraction of the total irrigation water use by state/territory, Australia: 2002-03 to 2023-24","description":"This collection was developed primarily to support national ecosystem accounting. It provides annual estimates of the groundwater fraction of irrigation water use for each Australian state and territory. The reported series covers financial years 2002–03 to 2023–24, with each reporting year defined from 1 July to 30 June.\n\nThe groundwater fraction is defined as the proportion of irrigation water use sourced from groundwater within a given state or territory in a given financial year. Estimates are reported as dimensionless fractions (0–1) and include associated standard errors to indicate uncertainty.\n\nThe primary estimates were generated using state- and territory-specific statistical models calibrated with data from 2010–11 to 2020–21 and then applied to reconstruct the full 2002–03 to 2023–24 series. Additional estimates based on temporal-block cross-validation (Temporal-block CV) and leave-one-out cross-validation (LOOCV) were generated using model building over 2005–06 to 2020–21 and are included for methodological comparison and robustness assessment.\n\nThe collection is provided as an Excel workbook with three worksheets:\n\nEstimated groundwater fraction of irrigation water use by state/territory, Australia, 2002–03 to 2023–24\nPrimary model-based estimates.\nEstimated groundwater fraction of irrigation water use by state/territory, Australia, 2005–06 to 2020–21 using the temporal-block cross-validation method\nEstimates derived using temporal-block cross-validation (Temporal-block CV).\nEstimated groundwater fraction of irrigation water use by state/territory, Australia, 2005–06 to 2020–21 using the leave-one-out cross-validation method\nEstimates derived using leave-one-out cross-validation (LOOCV).","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Liu, Ning; Smith, Greg; Evans, David; McVicar, Tim; Pena Arancibia, Jorge; Tetreault Campbell, Sally; & Pascoe, Sean (2026): National data for Australia's ecosystem services: groundwater fraction of the total irrigation water use by state/territory, Australia: 2002-03 to 2023-24. v3. CSIRO. Data Collection. https://doi.org/10.25919/mwke-2z30","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-18T02:24:56.313+10:00","leadResearcher":"Ning Liu","serviceCount":0,"contributors":["Greg Smith","David Evans","Tim McVicar","Jorge Pena Arancibia","Sally Tetreault Campbell","Sean Pascoe"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/734398","doi":"10.25919/mwke-2z30","project":{"irpHierarchy":true,"wbs":"R-19972","projectDescription":"National Ecosystem Accounting Project"},"dataRestricted":"FALSE","dataVersionNumber":"3"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:65932"},"dataCollectionId":74019,"self":"https://data.csiro.au/dap/ws/v2/collections/74019","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:65932","fileUpload":false,"fileId":0},"title":"Basic Spatial Units (BSU) at 100 m resolution for national ecosystem accounts","description":"This data collection defines the BSUs for the National Ecosystem Accounts, experimental estimates, 2022–23 financial year (released in April 2026), at a resolution of 100 m in GDA2020 / Australian Albers (EPSG:9473) projection, and includes the coverage fraction of each pixel of the Ecosystem Accounting Area (EAA). For the national ecosystem accounts, the base grid has been revised from 250 m to 100 m, with the Vegetation Information System (NVIS) version 7.0 data (NVIS, 2017) defining both the spatial resolution and grid origin. ","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Liu, Ning; Newnham, Glenn; Richards, Anna; Pascoe, Sean; & Tetreault Campbell, Sally (2026): Basic Spatial Units (BSU) at 100 m resolution for national ecosystem accounts. v2. CSIRO. Data Collection. https://doi.org/10.25919/ncen-jf51","rights":"All Rights (including copyright) CSIRO 2005.","published":"2026-04-17T19:25:48.026+10:00","leadResearcher":"Ning Liu","serviceCount":0,"spatialParameters":{"projection":"WGS84","northLatitude":"-6.098251944444444","southLatitude":"-47.902521944444445","westLongitude":"104.30321611111111","eastLongitude":"167.85181027777776"},"contributors":["Glenn Newnham","Anna Richards","Sean Pascoe","Sally Tetreault Campbell"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/734382","doi":"10.25919/ncen-jf51","project":{"irpHierarchy":true,"wbs":"R-19972","projectDescription":"National Ecosystem Accounting Project"},"dataRestricted":"FALSE","dataVersionNumber":"2"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74177"},"dataCollectionId":74177,"self":"https://data.csiro.au/dap/ws/v2/collections/74177","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74177","fileUpload":false,"fileId":0},"title":"ASKAP Data Products for Project AS331 (Radio monitoring of the Rubin Deep Drilling Fields): catalogues","description":"The Vera C. Rubin Observatory will begin full survey operations in early 2026. It will carry out a paradigm shifting survey of the sky and detect time-variable objects such as Active Galactic Nuclei, Tidal Disruption Events and kilonovae at an unprecedented rate, as well as being one of the deepest widefield optical surveys ever undertaken. Studying the objects discovered by Rubin will require comprehensive multi-wavelength observations, but the sheer number of sources to observe makes dedicated follow-up inefficient. In this project we propose regular monitoring of the five Rubin ``Deep Drilling Fields'' with ASKAP. These observations will provide efficient coverage of a large number of optical transients and form a legacy\n  product that is useful to the wider astronomical community. We will make the raw data products publicly available immediately and release value-added data products regularly throughout the survey.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Dobie, Dougal; Sadler, Elaine; Deller, Adam; Freeburn, James; de Ruiter, Iris; Moller, Anais; & Sarin, Nikhil (2026): ASKAP Data Products for Project AS331 (Radio monitoring of the Rubin Deep Drilling Fields): catalogues. v1. CSIRO. Data Collection. http://hdl.handle.net/102.100.100/734375?index=1","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-17T00:35:40.881+10:00","leadResearcher":"Dougal Dobie","serviceCount":0,"contributors":["Elaine Sadler","Adam Deller","James Freeburn","Iris de Ruiter","Anais Moller","Nikhil Sarin"],"activity":{"activityTitle":"AS331 - Radio monitoring of the Rubin Deep Drilling Fields"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734375","doi":null,"project":{"irpHierarchy":true,"wbs":"","projectDescription":"ASKAP"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74178"},"dataCollectionId":74178,"self":"https://data.csiro.au/dap/ws/v2/collections/74178","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74178","fileUpload":false,"fileId":0},"title":"ASKAP Data Products for Project AS331 (Radio monitoring of the Rubin Deep Drilling Fields): images and visibilities","description":"The Vera C. Rubin Observatory will begin full survey operations in early 2026. It will carry out a paradigm shifting survey of the sky and detect time-variable objects such as Active Galactic Nuclei, Tidal Disruption Events and kilonovae at an unprecedented rate, as well as being one of the deepest widefield optical surveys ever undertaken. Studying the objects discovered by Rubin will require comprehensive multi-wavelength observations, but the sheer number of sources to observe makes dedicated follow-up inefficient. In this project we propose regular monitoring of the five Rubin ``Deep Drilling Fields'' with ASKAP. These observations will provide efficient coverage of a large number of optical transients and form a legacy\n  product that is useful to the wider astronomical community. We will make the raw data products publicly available immediately and release value-added data products regularly throughout the survey.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Dobie, Dougal; Sadler, Elaine; Deller, Adam; Freeburn, James; de Ruiter, Iris; Moller, Anais; & Sarin, Nikhil (2026): ASKAP Data Products for Project AS331 (Radio monitoring of the Rubin Deep Drilling Fields): images and visibilities. v1. CSIRO. Data Collection. http://hdl.handle.net/102.100.100/734374?index=1","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-17T00:35:40.954+10:00","leadResearcher":"Dougal Dobie","serviceCount":0,"contributors":["Elaine Sadler","Adam Deller","James Freeburn","Iris de Ruiter","Anais Moller","Nikhil Sarin"],"activity":{"activityTitle":"AS331 - Radio monitoring of the Rubin Deep Drilling Fields"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734374","doi":null,"project":{"irpHierarchy":true,"wbs":"","projectDescription":"ASKAP"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:73771"},"dataCollectionId":74175,"self":"https://data.csiro.au/dap/ws/v2/collections/74175","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:73771","fileUpload":false,"fileId":0},"title":"Annual vegetation height for Australia for 2019 to 2025 release 2.0","description":"This product provides an annual estimate of vegetation height (top of canopy) for 2019 to 2025 at a 30m pixel size. These images are created using an extreme gradient boosting regressor (XGBoost) machine learning model which was trained using GEDI vegetation height (from the 98th percentile height) with spatially complete earth observation data as independent variables: Landsat annual surface reflectance, Landsat annual fractional cover percentiles, PALSAR backscatter (HV polarised) annual mosaic, along with a Digital Elevation Model (DEM) as well as long-term average temperature and rainfall. This release (no. 2.0) has had minor updates to the model, and includes 2025. Further details are provided in (Ticehurst et al. (in review)). This product was created as part of the National Bushfire Intelligence Capability (NBIC) and supported by the Terrestrial Ecosystem Research Network (TERN).\n\nTicehurst C, Joshi R, Hussain S, Walker S, Opie K, Donohue R (in review) Developing a nation-wide vegetation height layer for bushfire fuel classification.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Ticehurst, Catherine; Joshi, Rakesh; Hussain, Shehza; Walker, Simon; Opie, Kimberley; & Donohue, Randall (2026): Annual vegetation height for Australia for 2019 to 2025 release 2.0. v2. CSIRO. Data Collection. https://doi.org/10.25919/xas0-qh56","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T23:09:50.616+10:00","leadResearcher":"Catherine Ticehurst","serviceCount":0,"spatialParameters":{"projection":"WGS84","northLatitude":"-9.8","southLatitude":"-43.8","westLongitude":"112.8","eastLongitude":"154.0"},"contributors":["Rakesh Joshi","Shehza Hussain","Simon Walker","Kimberley Opie","Randall Donohue"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/733718","doi":"10.25919/xas0-qh56","project":{"irpHierarchy":true,"wbs":"R-19830","projectDescription":"ACS NBIC Stage 2"},"dataRestricted":"FALSE","dataVersionNumber":"2"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:34440"},"dataCollectionId":34440,"self":"https://data.csiro.au/dap/ws/v2/collections/34440","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:34440","fileUpload":false,"fileId":0},"title":"Transcriptome of Aedes albopictus infected with CHIKV","description":"Fasta files from RNASeq analysis of Albopictus mosquito tissue, infected with Chikunugnya virus.","licence":"Creative Commons Attribution-Noncommercial 4.0 Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1181","fileUpload":false,"fileId":0},"attributionStatement":"Vedururu, Ravikiran (2026): Transcriptome of Aedes albopictus infected with CHIKV. v1. CSIRO. Data Collection. https://doi.org/10.25919/n4aa-nj09","rights":"All Rights (including copyright) CSIRO 2018.","published":"2026-04-16T20:37:47.486+10:00","leadResearcher":"Ravikiran Vedururu","serviceCount":0,"contributors":[],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/734363","doi":"10.25919/n4aa-nj09","project":{"irpHierarchy":true,"wbs":"R-08799","projectDescription":"CLSD - RO Postgrad - Ravikiran Vedururu"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:54520"},"dataCollectionId":74166,"self":"https://data.csiro.au/dap/ws/v2/collections/74166","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:54520","fileUpload":false,"fileId":0},"title":"IMOS Biological Ocean Observer - sysdata.rda","description":"This is the sysdata.rda file that is used to populate the IMOS Biological Ocean Observer (BOO) Shiny App. The IMOS biological and supporting data is accessed directly from the AODN, processed and reformatted to the requirements of the Shiny App and stored in this location.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Davies, Claire; & Everett, Jason (2026): IMOS Biological Ocean Observer - sysdata.rda. v39. 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CSIRO. v1. Software. https://doi.org/10.25919/76hb-3917","rights":"All Rights (including copyright) CSIRO 2025.","published":"2026-04-16T16:52:46.612+10:00","leadResearcher":"Marcela Cespedes","serviceCount":0,"contributors":[],"activity":{},"collectionType":"Software","domainType":"Everything Else","andsPid":"102.100.100/711338","doi":"10.25919/76hb-3917","project":{"irpHierarchy":true,"wbs":"R-16491","projectDescription":"BIG - AIBL Biostatistics/Bioinformatics Support"},"dataRestricted":"FALSE","dataVersionNumber":"1","softwareVersionNumber":"1.0"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74157"},"dataCollectionId":74157,"self":"https://data.csiro.au/dap/ws/v2/collections/74157","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74157","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1386 semester 2026APRS_06","description":"J0045-7319 is a B star/pulsar binary in the Small Magellanic Cloud (SMC) with an orbital period of 51 days. The system is highly eccentric, with a closest approach of only 6 B-star radii, and it offers an unusual probe into massive stars in the SMC. Although similar systems exhibit strong dispersion measure (DM) variation during periastron arising from the stellar wind, observations in 1996 on the Parkes 70 cm receiver found no evidence of a wind from the B star. We request an additional 15 hours of observations on J0045-7319 to follow up on our current project.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Squillace, Reynier; & Ransom, Scott (2026): Parkes observations for project P1386 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/wx8c-7x92","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T07:34:48.033+10:00","leadResearcher":"Reynier Squillace","serviceCount":0,"contributors":["Scott Ransom"],"activity":{"activityTitle":"P1386 - Further Parkes Observations of a Pulsar-B Star Binary in the Small Magellanic Cloud"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734358","doi":"10.25919/wx8c-7x92","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74155"},"dataCollectionId":74155,"self":"https://data.csiro.au/dap/ws/v2/collections/74155","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74155","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1054 semester 2026APRS_05","description":"With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fiftythree sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 27 in the Magellanic Clouds, 109 in Globular Clusters and 96 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including a few relativistic systems, a pulsar with a planetary companion and  several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing for the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Burgay, Marta; Possenti, Andrea; Kramer, Michael; Freire, Paulo; Stappers, Benjamin; Levin, Lina; Champion, David; Buchner, Sarah; Barr, Ewan; Venkatraman Krishnan, Vivek; Karuppusamy, Ramesh; Clark, Colin James; Breton, Rene; Ridolfi, Alessandro; Cognard, Ismaël; Grießmeier, Jean-Mathias; Colom I Bernadich, Miquel; Thongmeearkom, Tinn; Carli, Emma;...Sergio, Belmonte Dìaz (2026): Parkes observations for project P1054 semester 2026APRS_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/29r5-jq92","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T07:28:09.286+10:00","leadResearcher":"Marta Burgay","serviceCount":0,"contributors":["Andrea Possenti","Michael Kramer","Paulo Freire","Benjamin Stappers","Lina Levin","David Champion","Sarah Buchner","Ewan Barr","Vivek Venkatraman Krishnan","Ramesh Karuppusamy","Colin James Clark","Rene Breton","Alessandro Ridolfi","Ismaël Cognard","Jean-Mathias Grießmeier","Miquel Colom I Bernadich","Tinn Thongmeearkom","Emma Carli","James Turner","Venu Prayag","Belmonte Dìaz Sergio"],"activity":{"activityTitle":"P1054 - Follow-up of pulsar discoveries from MeerKAT searches"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734356","doi":"10.25919/29r5-jq92","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74160"},"dataCollectionId":74160,"self":"https://data.csiro.au/dap/ws/v2/collections/74160","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74160","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1102 semester 2026APRS_06","description":"We request a triggered, high-cadence observation campaign to fully capture abrupt radiative and timing changes in the pulsed radio emission of a sample of four actively monitored magnetars. Magnetars are excellent laboratories for exploring the response of a neutron star magnetosphere to sudden, often times cataclysmic, changes in magnetic structure. Catching a radio-loud magnetar during the early stages of a sudden change in radiative behaviour, whether switching on after an outburst or displaying signs of a rapidly varying magnetic topology, is key to understanding both the short- and long-term evolution of their ultra-strong magnetic fields. The excellent sensitivity of the Ultra-Wideband Low (UWL) receiver system provides us with the means to capture high-quality, phase resolved polarisation spectra of these objects.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Lower, Marcus; Johnston, Simon; Camilo, Fernando; Bailes, Matthew; & Shannon, Ryan (2026): Parkes observations for project P1102 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/rhs3-9q61","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T07:27:15.673+10:00","leadResearcher":"Marcus Lower","serviceCount":0,"contributors":["Simon Johnston","Fernando Camilo","Matthew Bailes","Ryan Shannon"],"activity":{"activityTitle":"P1102 - A movie of a dynamic magnetar magnetosphere"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734361","doi":"10.25919/rhs3-9q61","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74159"},"dataCollectionId":74159,"self":"https://data.csiro.au/dap/ws/v2/collections/74159","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74159","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1054 semester 2026APRS_06","description":"With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fiftythree sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 27 in the Magellanic Clouds, 109 in Globular Clusters and 96 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including a few relativistic systems, a pulsar with a planetary companion and  several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing for the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Burgay, Marta; Possenti, Andrea; Kramer, Michael; Freire, Paulo; Stappers, Benjamin; Levin, Lina; Champion, David; Buchner, Sarah; Barr, Ewan; Venkatraman Krishnan, Vivek; Karuppusamy, Ramesh; Clark, Colin James; Breton, Rene; Ridolfi, Alessandro; Cognard, Ismaël; Grießmeier, Jean-Mathias; Colom I Bernadich, Miquel; Thongmeearkom, Tinn; Carli, Emma;...Sergio, Belmonte Dìaz (2026): Parkes observations for project P1054 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/xk2n-yc25","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T07:26:45.242+10:00","leadResearcher":"Marta Burgay","serviceCount":0,"contributors":["Andrea Possenti","Michael Kramer","Paulo Freire","Benjamin Stappers","Lina Levin","David Champion","Sarah Buchner","Ewan Barr","Vivek Venkatraman Krishnan","Ramesh Karuppusamy","Colin James Clark","Rene Breton","Alessandro Ridolfi","Ismaël Cognard","Jean-Mathias Grießmeier","Miquel Colom I Bernadich","Tinn Thongmeearkom","Emma Carli","James Turner","Venu Prayag","Belmonte Dìaz Sergio"],"activity":{"activityTitle":"P1054 - Follow-up of pulsar discoveries from MeerKAT searches"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734360","doi":"10.25919/xk2n-yc25","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74158"},"dataCollectionId":74158,"self":"https://data.csiro.au/dap/ws/v2/collections/74158","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74158","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1386 semester 2026APRS_07","description":"J0045-7319 is a B star/pulsar binary in the Small Magellanic Cloud (SMC) with an orbital period of 51 days. The system is highly eccentric, with a closest approach of only 6 B-star radii, and it offers an unusual probe into massive stars in the SMC. Although similar systems exhibit strong dispersion measure (DM) variation during periastron arising from the stellar wind, observations in 1996 on the Parkes 70 cm receiver found no evidence of a wind from the B star. We request an additional 15 hours of observations on J0045-7319 to follow up on our current project.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Squillace, Reynier; & Ransom, Scott (2026): Parkes observations for project P1386 semester 2026APRS_07. v1. CSIRO. Data Collection. https://doi.org/10.25919/gm9n-eh82","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T07:26:15.157+10:00","leadResearcher":"Reynier Squillace","serviceCount":0,"contributors":["Scott Ransom"],"activity":{"activityTitle":"P1386 - Further Parkes Observations of a Pulsar-B Star Binary in the Small Magellanic Cloud"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734359","doi":"10.25919/gm9n-eh82","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74154"},"dataCollectionId":74154,"self":"https://data.csiro.au/dap/ws/v2/collections/74154","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74154","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1386 semester 2026APRS_05","description":"J0045-7319 is a B star/pulsar binary in the Small Magellanic Cloud (SMC) with an orbital period of 51 days. The system is highly eccentric, with a closest approach of only 6 B-star radii, and it offers an unusual probe into massive stars in the SMC. Although similar systems exhibit strong dispersion measure (DM) variation during periastron arising from the stellar wind, observations in 1996 on the Parkes 70 cm receiver found no evidence of a wind from the B star. We request an additional 15 hours of observations on J0045-7319 to follow up on our current project.","licence":"Creative Commons Attribution 4.0 International Licence","licenceLink":{"relationship":"licence","mediaType":"text/html","href":"https://data.csiro.au/dap/ws/v2/licences/1121","fileUpload":false,"fileId":0},"attributionStatement":"Squillace, Reynier; & Ransom, Scott (2026): Parkes observations for project P1386 semester 2026APRS_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/n8hq-y018","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-04-16T07:25:45.543+10:00","leadResearcher":"Reynier Squillace","serviceCount":0,"contributors":["Scott Ransom"],"activity":{"activityTitle":"P1386 - Further Parkes Observations of a Pulsar-B Star Binary in the Small Magellanic Cloud"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/734357","doi":"10.25919/n8hq-y018","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"}]}