{"elapsedTime":48,"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:75049"},"dataCollectionId":75049,"self":"https://data.csiro.au/dap/ws/v2/collections/75049","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75049","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1422 semester 2026APRS_06","description":"Interplanetery Scintillation (IPS) is a powerful observing technique for measuring the size and structure of radio sources, as well as characterising solar wind turbulence. Murriyang was used for IPS in the 1960 and 1980s for IPS observations. However, with the the UWL's ultra-wide bandwidth, we believe that Murriyang IPS observations can once again provide a unique science opportunity. Recent observations with the Five-hundred-metre Aperture Spherical Telescope revealed an unexpected trend of scintillation timescale with frequency. Murriyang is the perfect instrument to corroborate this finding. Furthermore, we believe this effect is due to the inner scale of the turbulence, which can be uniquely probed with the high sensitivity and bandwidth of Murriyang in unprecedented detail, with a modest amount of observing time. As well as providing the most detailed study of the Heliosphere's inner scale yet, we can also determine if it can act as a new and direct probe of heliospheric density: an important complement to IPS and extremely useful for understanding the impact of the solar wind to pulsar DM variations. Finally, these observations will also provide useful insights for instrumental systematics on timescales rather longer than pulsar periods (1-10s) but similar to the timescales of the new class of Ultra-long period magnetars. Thus we can better understand whether Murriyang has a role to play in this important discovery space.","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":"Morgan, John; Bignall, Hayley; Hobbs, George; Reynolds, Cormac; Zic, Andrew; Waszewski, Angelica; & Forte, Biagio (2026): Parkes observations for project P1422 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/afkh-yn67","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-14T20:46:34.433+10:00","leadResearcher":"John Morgan","serviceCount":0,"contributors":["Hayley Bignall","George Hobbs","Cormac Reynolds","Andrew Zic","Angelica Waszewski","Biagio Forte"],"activity":{"activityTitle":"P1422 - Measuring the inner scale of solar wind turbulence with ultra-wideband Interplanetary Scintillation Observations."},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735594","doi":"10.25919/afkh-yn67","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75046"},"dataCollectionId":75046,"self":"https://data.csiro.au/dap/ws/v2/collections/75046","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75046","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1398 semester 2026APRS_05","description":"Low-frequency (< ~1 GHz) Galactic-plane pulsar surveys are strongly limited by sky background noise, interstellar scattering, and dispersion smearing, leading to an incomplete census of the pulsar population. High-frequency (> 2 GHz) observations mitigate these effects and have recently enabled the discovery of pulsars that remain undetectable at low-frequency. We analyzed archival data from the 2008 Parkes 6.5-GHz pulsar survey using modern search techniques. This reprocessing has revealed four previously unknown millisecond pulsar candidates with spin periods of 3-11 ms and dispersion measures of 20-170 pc/cc. Two candidates exhibit significant line-of-sight acceleration, indicating likely membership in compact binary systems. We request a total of 8.4 hours of follow-up observations with the Parkes (Murriyang) Ultra-Wideband Low (UWL) receiver to confirm these candidates and characterize their emission across 704-4032 MHz. Confirming these sources would expand the population of high-frequency selected pulsars and demonstrate the continued importance of high-frequency searches for uncovering exotic systems obscured in conventional low-frequency surveys.","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":"Gao, Shi-Jie; Zhang, Songbo; Wang, Ziteng; & Li, Xiangdong (2026): Parkes observations for project P1398 semester 2026APRS_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/ypj9-kc58","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-14T20:45:42.893+10:00","leadResearcher":"Shi-Jie Gao","serviceCount":0,"contributors":["Songbo Zhang","Ziteng Wang","Xiangdong Li"],"activity":{"activityTitle":"P1398 - Confirmation of Four Pulsar Candidates Identified via Reprocessing of the Parkes 6.5 GHz Pulsar Survey"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735596","doi":"10.25919/ypj9-kc58","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75045"},"dataCollectionId":75045,"self":"https://data.csiro.au/dap/ws/v2/collections/75045","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75045","fileUpload":false,"fileId":0},"title":"Long-term project observations for project L124 semester 2026APRS_06","description":"We 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 (RM) and dispersion measure (DM) evolution, along with distinctive behavior at 3GHz frequency. This makes the UWL receiver uniquely suited for detailed studies and long-term monitoring of this repeating FRB. Through this program, we anticipate detecting a large sample of bursts from this FRB. In collaboration with FAST, we aim to investigate the time evolution of various properties of FRB 20190520B, enhance our understanding of polarisation across an extremely wide bandwidth with high sensitivity, and gain deeper insights into the local environment and emission mechanisms of FRBs.","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":"Dai, Shi; Hobbs, George; Li, Di; Wang, Pei; Zhang, Lei; Zhu, Weiwei; Feng, Yi; Xue, Mengyao; Yang, Yuanpei; Zhang, YongKun; Niu, Chenhui; Xu, Jiaying; Zhu, Yuhao; & Zhang, Jiaheng (2026): Long-term project observations for project L124 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/pas1-6v96","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-14T20:45:45.013+10:00","leadResearcher":"Shi Dai","serviceCount":0,"contributors":["George Hobbs","Di Li","Pei Wang","Lei Zhang","Weiwei Zhu","Yi Feng","Mengyao Xue","Yuanpei Yang","YongKun Zhang","Chenhui Niu","Jiaying Xu","Yuhao Zhu","Jiaheng Zhang"],"activity":{"activityTitle":"L124 - Long-term monitoring of FRB 20190520B with the Ultra-Wideband Low receiver"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735597","doi":"10.25919/pas1-6v96","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75048"},"dataCollectionId":75048,"self":"https://data.csiro.au/dap/ws/v2/collections/75048","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75048","fileUpload":false,"fileId":0},"title":"Long-term project observations for project L134 semester 2026APRS_05","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_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/ws53-q981","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-14T20:45:07.735+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":"102.100.100/735593","doi":"10.25919/ws53-q981","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75050"},"dataCollectionId":75050,"self":"https://data.csiro.au/dap/ws/v2/collections/75050","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75050","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1032 semester 2026APRS_08","description":"With 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, observations with the UWL receiver now form the backbone for extending the timing baselines of many pulsars that have been part of this project. Since the source selection in the previous semesters was tailored such that the UWL receiver is the most (versatile and) suited instrument to achieve the proposed scientific goals for the chosen pulsars, we propose to continue these observations. We will use the UWL data to obtain significant orbital coverage and timing baselines on these pulsars and obtain important constraints on orbital and temporal DM variations that will help in identifying the nature of the companion stars. Increasing the number of measured Neutron Star (NS) masses, as well as improving on current constraints has profound implications for NS internal structure and for stellar and binary evolution physics.","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":"Grunthal, Kathrin; Possenti, Andrea; Kramer, Michael; Burgay, Marta; Freire, Paulo; Bailes, Matthew; Bhat, Ramesh; Venkatraman Krishnan, Vivek; Lower, Marcus; Colom I Bernadich, Miquel; Pillay, Denisha; Geyer, Marisa; Dutta, Arunima; Senzel, Robert; & Bhatnagar, Devika (2026): Parkes observations for project P1032 semester 2026APRS_08. v1. CSIRO. Data Collection. https://doi.org/10.25919/97hy-s377","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-14T20:45:07.863+10:00","leadResearcher":"Kathrin Grunthal","serviceCount":0,"contributors":["Andrea Possenti","Michael Kramer","Marta Burgay","Paulo Freire","Matthew Bailes","Ramesh Bhat","Vivek Venkatraman Krishnan","Marcus Lower","Miquel Colom I Bernadich","Denisha Pillay","Marisa Geyer","Arunima Dutta","Robert Senzel","Devika Bhatnagar"],"activity":{"activityTitle":"P1032 - Timing southern binary pulsar systems"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735595","doi":"10.25919/97hy-s377","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:69115"},"dataCollectionId":69115,"self":"https://data.csiro.au/dap/ws/v2/collections/69115","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:69115","fileUpload":false,"fileId":0},"title":"Image Collection - RV Investigator Voyage IN2024_V03 - SEA-MES: Untangling the causes of change over 25 years in the southeast marine ecosystem - Voyage 2","description":"This data set contains the imagery collected on the Marine National Facility (MNF) RV Investigator voyage IN2024_V03, titled ‘Untangling the causes of change over 25 years in the southeast marine ecosystem (SEA-MES Voyage 2) .\" The voyage took place between May 01, 2024 and May 31, 2024 (AEST), departing from Hobart and returning to Sydney, collecting imagery of benthic habitats together with oceanographic data.\n\nInstrument(s) used to collect this data:\nMNF Deep Towed camera (DTC)\n\nDatasets include: \nVideo (oblique forward view)\nStereo stills (oblique forward view)\nNavigational 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":"CSIRO; Marine National Facility; Little, Rich; Webb, David; Pietraroia, Ella; Sheehan, Kieran; Tyndall, Aaron; Forcey, Karl; Jackett, Chris; Untiedt, Candice; Althaus, Franzis; & Scoulding, Ben (2026): Image Collection - RV Investigator Voyage IN2024_V03 - SEA-MES: Untangling the causes of change over 25 years in the southeast marine ecosystem - Voyage 2. v1. CSIRO. Data Collection. https://doi.org/10.25919/dtde-p783","rights":"All Rights (including copyright) CSIRO 2025.","published":"2026-06-14T05:21:55.567+10:00","leadResearcher":"CSIRO","serviceCount":0,"spatialParameters":{"projection":"WGS84","northLatitude":"-33.8248","southLatitude":"-43.2989","westLongitude":"147.3914","eastLongitude":"151.3967"},"contributors":["Marine National Facility","Rich Little","David Webb","Ella Pietraroia","Kieran Sheehan","Aaron Tyndall","Karl Forcey","Chris Jackett","Candice Untiedt","Franzis Althaus","Ben Scoulding"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/735561","doi":"10.25919/dtde-p783","project":{"irpHierarchy":true,"wbs":"R-18194","projectDescription":"SP-COR-The Southeast Marine Ecosystem Survey (SEA-MES)"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:69167"},"dataCollectionId":69167,"self":"https://data.csiro.au/dap/ws/v2/collections/69167","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:69167","fileUpload":false,"fileId":0},"title":"Image Collection - RV Investigator Voyage IN2025_V04 - SEA-MES: Untangling the causes of change over 25 years in the southeast marine ecosystem - Voyage 4","description":"This data set contains the imagery collected on 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 between May 27, 2025 and June 28, 2025 (AEST), departing from Hobart and returning to Hobart, collecting imagery of benthic habitats together with oceanographic data.\n\nInstrument(s) used to collect this data:\nMNF Deep Towed camera (DTC)\n\nDatasets include: \nVideo (oblique forward view)\nStereo stills (oblique forward view)\nNavigational 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":"CSIRO; Marine National Facility; Little, Rich; Webb, David; Pietraroia, Ella; Sheehan, Kieran; Jamson, Ryder; Thomas, Stephen; Tyndall, Aaron; Jackett, Chris; Untiedt, Candice; Althaus, Franzis; & Scoulding, Ben (2026): Image Collection - RV Investigator Voyage IN2025_V04 - SEA-MES: Untangling the causes of change over 25 years in the southeast marine ecosystem - Voyage 4. v1. CSIRO. Data Collection. https://doi.org/10.25919/rx9f-cy26","rights":"All Rights (including copyright) CSIRO 2025.","published":"2026-06-14T05:00:14.699+10:00","leadResearcher":"CSIRO","serviceCount":0,"spatialParameters":{"projection":"WGS84","northLatitude":"-36.5277","southLatitude":"-43.3202","westLongitude":"147.339","eastLongitude":"150.3939"},"contributors":["Marine National Facility","Rich Little","David Webb","Ella Pietraroia","Kieran Sheehan","Ryder Jamson","Stephen Thomas","Aaron Tyndall","Chris Jackett","Candice Untiedt","Franzis Althaus","Ben Scoulding"],"activity":{},"collectionType":"Data","domainType":"Everything Else","andsPid":"102.100.100/735560","doi":"10.25919/rx9f-cy26","project":{"irpHierarchy":true,"wbs":"R-18194","projectDescription":"SP-COR-The Southeast Marine Ecosystem Survey (SEA-MES)"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75042"},"dataCollectionId":75042,"self":"https://data.csiro.au/dap/ws/v2/collections/75042","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75042","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1054 semester 2026APRS_22","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_22. v1. CSIRO. Data Collection. https://doi.org/10.25919/6s0k-5m43","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T21:14:08.822+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":"102.100.100/735581","doi":"10.25919/6s0k-5m43","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75043"},"dataCollectionId":75043,"self":"https://data.csiro.au/dap/ws/v2/collections/75043","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75043","fileUpload":false,"fileId":0},"title":"Long-term project observations for project L124 semester 2026APRS_05","description":"We 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 (RM) and dispersion measure (DM) evolution, along with distinctive behavior at 3GHz frequency. This makes the UWL receiver uniquely suited for detailed studies and long-term monitoring of this repeating FRB. Through this program, we anticipate detecting a large sample of bursts from this FRB. In collaboration with FAST, we aim to investigate the time evolution of various properties of FRB 20190520B, enhance our understanding of polarisation across an extremely wide bandwidth with high sensitivity, and gain deeper insights into the local environment and emission mechanisms of FRBs.","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":"Dai, Shi; Hobbs, George; Li, Di; Wang, Pei; Zhang, Lei; Zhu, Weiwei; Feng, Yi; Xue, Mengyao; Yang, Yuanpei; Zhang, YongKun; Niu, Chenhui; Xu, Jiaying; Zhu, Yuhao; & Zhang, Jiaheng (2026): Long-term project observations for project L124 semester 2026APRS_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/d973-ev33","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T21:14:06.021+10:00","leadResearcher":"Shi Dai","serviceCount":0,"contributors":["George Hobbs","Di Li","Pei Wang","Lei Zhang","Weiwei Zhu","Yi Feng","Mengyao Xue","Yuanpei Yang","YongKun Zhang","Chenhui Niu","Jiaying Xu","Yuhao Zhu","Jiaheng Zhang"],"activity":{"activityTitle":"L124 - Long-term monitoring of FRB 20190520B with the Ultra-Wideband Low receiver"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735580","doi":"10.25919/d973-ev33","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75044"},"dataCollectionId":75044,"self":"https://data.csiro.au/dap/ws/v2/collections/75044","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75044","fileUpload":false,"fileId":0},"title":"Long-term project observations for project L132 semester 2026APRS_02","description":"PSR 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 potentially profound physical implications. However, the timing precision is limited by the DM timing noise. We propose regular monitoring of this pulsar with the Parkes UWL receiver in conjunction with MeerKAT observations during the following four years. The joint monitoring will significantly improve the constraints on the Post-Keplerian parameters, with Parkes observations contributing to constrain the DM noise due to its large frequency bandwidth. These observations will be added to the already existing 11-year-long timing baseline, of which the later 5 years already include high-precision MeerKAT data and Parkes UWL data. After four years of further timing with the inclusion of UWL observations, we predict an uncertainty on the masses smaller than 0.01 solar masses based on simulations. If UWL is not included, the mass uncertainties may not improve beyond their current values.","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; & Venkatraman Krishnan, Vivek (2026): Long-term project observations for project L132 semester 2026APRS_02. v1. CSIRO. Data Collection. https://doi.org/10.25919/726p-hq13","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T21:14:05.903+10:00","leadResearcher":"Miquel Colom I Bernadich","serviceCount":0,"contributors":["Andrea Possenti","Michael Kramer","Marta Burgay","Matthew Bailes","Vivek Venkatraman Krishnan"],"activity":{"activityTitle":"L132 - TRACKING THE DM VARIATIONS IN PSR J1227-6208"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735579","doi":"10.25919/726p-hq13","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75040"},"dataCollectionId":75040,"self":"https://data.csiro.au/dap/ws/v2/collections/75040","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75040","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1413 semester 2026APRS_12","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_12. v1. CSIRO. Data Collection. https://doi.org/10.25919/bmsa-s335","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T19:06:40.932+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":"102.100.100/735578","doi":"10.25919/bmsa-s335","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75041"},"dataCollectionId":75041,"self":"https://data.csiro.au/dap/ws/v2/collections/75041","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75041","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1422 semester 2026APRS_05","description":"Interplanetery Scintillation (IPS) is a powerful observing technique for measuring the size and structure of radio sources, as well as characterising solar wind turbulence. Murriyang was used for IPS in the 1960 and 1980s for IPS observations. However, with the the UWL's ultra-wide bandwidth, we believe that Murriyang IPS observations can once again provide a unique science opportunity. Recent observations with the Five-hundred-metre Aperture Spherical Telescope revealed an unexpected trend of scintillation timescale with frequency. Murriyang is the perfect instrument to corroborate this finding. Furthermore, we believe this effect is due to the inner scale of the turbulence, which can be uniquely probed with the high sensitivity and bandwidth of Murriyang in unprecedented detail, with a modest amount of observing time. As well as providing the most detailed study of the Heliosphere's inner scale yet, we can also determine if it can act as a new and direct probe of heliospheric density: an important complement to IPS and extremely useful for understanding the impact of the solar wind to pulsar DM variations. Finally, these observations will also provide useful insights for instrumental systematics on timescales rather longer than pulsar periods (1-10s) but similar to the timescales of the new class of Ultra-long period magnetars. Thus we can better understand whether Murriyang has a role to play in this important discovery space.","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":"Morgan, John; Bignall, Hayley; Hobbs, George; Reynolds, Cormac; Zic, Andrew; Waszewski, Angelica; & Forte, Biagio (2026): Parkes observations for project P1422 semester 2026APRS_05. v1. CSIRO. Data Collection. https://doi.org/10.25919/714x-pq55","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T19:03:00.937+10:00","leadResearcher":"John Morgan","serviceCount":0,"contributors":["Hayley Bignall","George Hobbs","Cormac Reynolds","Andrew Zic","Angelica Waszewski","Biagio Forte"],"activity":{"activityTitle":"P1422 - Measuring the inner scale of solar wind turbulence with ultra-wideband Interplanetary Scintillation Observations."},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735577","doi":"10.25919/714x-pq55","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75037"},"dataCollectionId":75037,"self":"https://data.csiro.au/dap/ws/v2/collections/75037","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75037","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1379 semester 2026APRS_06","description":"We propose a simultaneous joint observation campaign using the Parkes radio telescope and the EP satellite to observation three magnetars with known radio emission. Under simultaneous observations, we aim to investigate the correlation between their radio and X-ray emissions, including pulse profiles, flux intensity, polarization evolution, correlated multi-wavelength behavior and timing behavior.","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":"zhang, zhen; Yan, Wenming; Zhu, Weiwei; Bai, Juntao; & lin, lin (2026): Parkes observations for project P1379 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/01m5-2061","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T17:58:28.588+10:00","leadResearcher":"zhen zhang","serviceCount":0,"contributors":["Wenming Yan","Weiwei Zhu","Juntao Bai","lin lin"],"activity":{"activityTitle":"P1379 - Simultaneous joint observations of the active magnetar by the Einstein Probe and the Parkes Telescope"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735575","doi":"10.25919/01m5-2061","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75039"},"dataCollectionId":75039,"self":"https://data.csiro.au/dap/ws/v2/collections/75039","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75039","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1410 semester 2026APRS_06","description":"Neutron stars are compact remnants formed in core-collapse supernovae of massive stars. A subset of these objects, known as pulsars, emit highly regular pulses of radiation that make them powerful tools for studying fundamental physics, stellar evolution, and the structure of our Galaxy. Despite decades of surveys, the known pulsar population remains incomplete: while about 4,800 pulsars are currently catalogued, population studies predict that roughly 10,000 or more radio-detectable pulsars should be observable with our current instrumentation.\n  A significant fraction of the missing population is expected to consist of slowly rotating pulsars, which are difficult to detect with standard search pipelines. These pulsars often have very narrow pulse duty cycles and long spin periods, making them susceptible to reduced signal-to-noise ratios and contamination by low-frequency (\"red\") noise in Fourier-based searches. As a result, many such objects may remain hidden in archival survey data.\n  Motivated by this, we reprocessed archival data from the Parkes Multibeam Pulsar Survey targeting narrow-duty-cycle signals and allowing to investigate lower signal to noise ratios for these candidates. This approach led to the identification of 12 highly credible new slow pulsar candidates that were missed in previous analyses. Several of these candidates show strong folded signal-to-noise ratios and physically plausible dispersion measures, indicating they are likely genuine pulsars.\n  The primary goal of this proposal is to obtain targeted follow-up observations to confirm and time these newly identified pulsar candidates. Confirming them will help close the gap between predicted and observed pulsar populations and demonstrate the continued scientific value of archival radio survey 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":"Botnariuc, Alexandra; Clark, Colin James; & Sengar, Rahul (2026): Parkes observations for project P1410 semester 2026APRS_06. v1. CSIRO. Data Collection. https://doi.org/10.25919/ffg0-w810","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T17:55:51.906+10:00","leadResearcher":"Alexandra Botnariuc","serviceCount":0,"contributors":["Colin James Clark","Rahul Sengar"],"activity":{"activityTitle":"P1410 - Confirmation of pulsar candidates found in a reprocessing of the PMPS archival data"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735576","doi":"10.25919/ffg0-w810","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75038"},"dataCollectionId":75038,"self":"https://data.csiro.au/dap/ws/v2/collections/75038","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75038","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1402 semester 2026APRS_15","description":"We propose a dedicated Parkes/Murriyang timing campaign of the newly confirmed narrow-duty cycle (~6 %) millisecond pulsar (MSP) PSR J2147-3604. This source was identified in a reprocessing of the Green Bank North Celestial Cap (GBNCC) survey as a high-confidence candidate with a spin period of 3.2 ms, and a dispersion measure, DM of 17 pc/cc. The pulsar was subsequently confirmed by the Fermi--TRAPUM collaboration via MeerKAT beamforming localisation and Parkes follow-up. Parkes/UWL observations allocated using green time detected this pulsar between 700--1500~MHz, and confirmed that it's in a binary system. Due to its low DM, we also detected strong interstellar scintillation. We request 35~hr of Murriyang time using the UWL receiver and APOLLO backend to obtain a phase-coherent timing solution and to characterise its spin, orbital, and propagation properties. Since the pulsar is also associated with a FERMI source, a precise radio ephemeris will also enable sensitive searches for gamma-ray pulsations in Fermi-LAT data and assess PSR J2147-3604's suitability for pulsar timing arrays (PTAs) and future gamma-ray timing applications.","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":"Vleeschower, Laila; Ransom, Scott; Van Leeuwen, Joeri; DeCesar, Megan; Cromartie, Thankful; Kaplan, David; Lynch, Ryan; Sengar, Rahul; & Dolch, Timothy (2026): Parkes observations for project P1402 semester 2026APRS_15. v1. CSIRO. Data Collection. https://doi.org/10.25919/ctp3-b997","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T17:55:00.804+10:00","leadResearcher":"Laila Vleeschower","serviceCount":0,"contributors":["Scott Ransom","Joeri Van Leeuwen","Megan DeCesar","Thankful Cromartie","David Kaplan","Ryan Lynch","Rahul Sengar","Timothy Dolch"],"activity":{"activityTitle":"P1402 - Timing of a narrow duty-cycle millisecond pulsar"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735574","doi":"10.25919/ctp3-b997","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75036"},"dataCollectionId":75036,"self":"https://data.csiro.au/dap/ws/v2/collections/75036","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75036","fileUpload":false,"fileId":0},"title":"Parkes observations for project P1365 semester 2026APRS_03","description":"Following the successful demonstration of a pilot first-pass (shallow) search of a small fraction of the sky, the second-pass processing has commenced for the SMART pulsar survey, which involves deep searches of 80-minute observations. Over the past year, this second-pass processing has led to the discovery of 16 new pulsars (including two millisecond pulsars), bringing the total number of SMART discoveries to 20 when combined with the first-pass results. These outcomes hint at the exciting promise of this first southern-sky pulsar survey in the frequency band of SKA-Low. All new pulsars require timing observations to determine their spin and astrometric parameters. Another important aspect of timing newly discovered pulsars is to identify specialised targets for further detailed follow-ups. Since the MWA no longer supports routine pulsar observations from 2025, timing follow-ups rely on other telescopes. The Parkes Murriyang telescope, with an identical sky coverage, sensitivity and the wide frequency coverage, offers the best option to time SMART discoveries. We have demonstrated Murriyang's suitability for this through previous semesters and are now extending the project to a sample of 11 pulsars, including six from the last semester. The data will also allow us to study pulse profiles, polarisation, and flux densities from ~100 MHz to 4 GHz. The analysis/results will be included in a publication in preparation that will detail the deep-search pipeline and report on initial pulsar 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":"Xue, Mengyao; Bhat, Ramesh; Zhu, Weiwei; Meyers, Bradley; Zhou, Yukai; Fu, Qiuyang; Tan, Chia Min; & Lee, Christopher (2026): Parkes observations for project P1365 semester 2026APRS_03. v1. CSIRO. Data Collection. https://doi.org/10.25919/x5a2-7w30","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T16:17:52.834+10:00","leadResearcher":"Mengyao Xue","serviceCount":0,"contributors":["Ramesh Bhat","Weiwei Zhu","Bradley Meyers","Yukai Zhou","Qiuyang Fu","Chia Min Tan","Christopher Lee"],"activity":{"activityTitle":"P1365 - Timing new pulsars discovered in the SMART survey"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735573","doi":"10.25919/x5a2-7w30","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75030"},"dataCollectionId":75030,"self":"https://data.csiro.au/dap/ws/v2/collections/75030","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75030","fileUpload":false,"fileId":0},"title":"Parkes observations for project P737 semester 2026APRS_04","description":"Instrumental Commissioning","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":"Johnston, Simon; Sarkissian, John; Hobbs, George; Mader, Stacy; Toomey, Lawrence; & Dai, Shi (2026): Parkes observations for project P737 semester 2026APRS_04. v1. CSIRO. Data Collection. https://doi.org/10.25919/ft00-es47","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T15:54:59.615+10:00","leadResearcher":"Simon Johnston","serviceCount":0,"contributors":["John Sarkissian","George Hobbs","Stacy Mader","Lawrence Toomey","Shi Dai"],"activity":{"activityTitle":"P737 - Instrumental Commissioning at Parkes"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735572","doi":"10.25919/ft00-es47","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:75031"},"dataCollectionId":75031,"self":"https://data.csiro.au/dap/ws/v2/collections/75031","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:75031","fileUpload":false,"fileId":0},"title":"Parkes observations for project P595 semester 2026APRS_18","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_18. v1. CSIRO. Data Collection. https://doi.org/10.25919/ytjc-sy34","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T15:29:59.860+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":"102.100.100/735571","doi":"10.25919/ytjc-sy34","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ATNF"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74183"},"dataCollectionId":75033,"self":"https://data.csiro.au/dap/ws/v2/collections/75033","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. v3. CSIRO. Data Collection. https://doi.org/10.25919/xzbr-te90","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T04:50:43.124+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/xzbr-te90","project":{"irpHierarchy":true,"wbs":"R-22956","projectDescription":"GRDC: New Tools and knowledge for Optimising Heterotic Pools in Canola - CSP2512-009RTX"},"dataRestricted":"TRUE","dataVersionNumber":"3"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:74963"},"dataCollectionId":74963,"self":"https://data.csiro.au/dap/ws/v2/collections/74963","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:74963","fileUpload":false,"fileId":0},"title":"ASKAP Project AS110 - The Rapid ASKAP Continuum Survey (RACS): The RACS-low2 887.5 MHz images and catalogues","description":"Data products associated with the release of the Stokes I and V catalogues from the second epoch of the Rapid ASKAP Continuum Survey (RACS) at 887.5 MHz (RACS-low2, Duchesne+2026). This work took the images of the tiles associated with the RACS-low2 survey at 887.5 MHz, convolved them to a common resolution, and mosaicked them with neighbouring images to obtain near-uniform sensitivity images covering the sky up to declination +49 degrees. Released are the 947 Stokes I images constructed in this manner, and the resulting source and component catalogue covering the region. Catalogues were made by running PyBDSF (see Mohan and Rafferty: 2015ascl.soft02007M) over each mosaicked tile image. These tile catalogues were combined together and duplicates removed.  The Stokes V sources are obtained from the single-observation images prior to mosaicking with neighbouring images to ensure each detection corresponds to only one ~15 min observation. This also means some sources are detected in multiple images so appear multiple times in the Stokes V catalogue.\n","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":"Duchesne, Stefan; Rose, Kovi; Murphy, Tara; Driessen, Laura; Pritchard, Josh; Moss, Vanessa; Galvin, Tim; Lenc, Emil; Hotan, Aidan; Ross, Kathryn; Thomson, Alec; & Whiting, Matthew (2026): ASKAP Project AS110 - The Rapid ASKAP Continuum Survey (RACS): The RACS-low2 887.5 MHz images and catalogues. v1. CSIRO. Data Collection. https://doi.org/10.25919/m8t2-b486","rights":"All Rights (including copyright) CSIRO 2026.","published":"2026-06-13T04:30:14.172+10:00","leadResearcher":"Stefan Duchesne","serviceCount":0,"contributors":["Kovi Rose","Tara Murphy","Laura Driessen","Josh Pritchard","Vanessa Moss","Tim Galvin","Emil Lenc","Aidan Hotan","Kathryn Ross","Alec Thomson","Matthew Whiting"],"activity":{"activityTitle":"AS110 - The Rapid ASKAP Continuum Survey"},"collectionType":"Data","domainType":"Astronomy Data","andsPid":"102.100.100/735559","doi":"10.25919/m8t2-b486","project":{"irpHierarchy":true,"wbs":"","projectDescription":"ASKAP"},"dataRestricted":"FALSE","dataVersionNumber":"1"},{"id":{"identifierType":"Fedora PID","identifier":"csiro:63896"},"dataCollectionId":75035,"self":"https://data.csiro.au/dap/ws/v2/collections/75035","landingPage":{"relationship":"alternate","mediaType":"text/html","href":"https://data.csiro.au/collection/csiro:63896","fileUpload":false,"fileId":0},"title":"Compound climate events threaten tropical semi-enclosed marine ecosystems","description":"Compound climate events threaten tropical semi-enclosed marine ecosystems ","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":"Plaganyi-Lloyd, Eva; Crous, Laura Blamey; Kenyon, Rob; Brodie, Steph; Deng, Roy; Parker, Denham; Pillans, Richard; Murphy, Nicole; Miller, Margaret; Pascoe, Sean; & Punt, Andre (2026): Compound climate events threaten tropical semi-enclosed marine ecosystems. v3. CSIRO. 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