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Morphological data for 838 Australian Asteraceae text-mined from taxonomic...
Morphological data for 838 Australian Asteraceae text-mined from taxonomic descriptions -
Parkes observations for project P595 semester 2025APRS_10
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... -
Parkes observations for project P630 semester 2011APRS_06
We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank... -
Parkes observations for project P1338 semester 2025APRS_34
Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a... -
Parkes observations for project P1345 semester 2025APRS_10
This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade... -
Parkes observations for project PX133 semester 2025APRS_01
Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations -
Parkes observations for project PX133 semester 2025APRS_02
Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations -
Parkes observations for project P1343 semester 2025APRS_03
Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a... -
Parkes observations for project PX133 semester 2025APRS_03
Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations -
Parkes observations for project P1345 semester 2025APRS_11
This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade... -
Parkes observations for project P1032 semester 2025APRS_02
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... -
Parkes observations for project P1165 semester 2025APRS_03
We recently discovered two new pulsars J1849+1001 (35.1 ms) and J1839+0542 (57.9 ms) in a FAST pulsar survey at intermediate Galactic latitudes (PT2020_0141). Follow-up timing... -
Parkes observations for project P1338 semester 2025APRS_35
Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a... -
Parkes observations for project P1219 semester 2025APRS_05
Magnetic fields are fundamental in regulating star formation and the evolution of molecular clouds. Zeeman splitting offers a unique method to directly measure line-of-sight... -
Parkes observations for project P1054 semester 2025APRS_10
With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourtytwo sources have been discovered in targeted... -
Parkes observations for project P1345 semester 2025APRS_12
This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade... -
Long-term project observations for project P574 semester 2025APRS_06
We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what... -
Parkes observations for project P595 semester 2025APRS_11
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... -
Parkes observations for project PX135 semester 2025APRS_01
Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations -
Long-term project observations for project P1321 semester 2025APRS_06
The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this...