-
Parkes observations for project P1338 semester 2025APRS_37
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_14
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 P1338 semester 2025APRS_36
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 P1327 semester 2025APRS_11
The radio radiation neutron star includes objects with spin periods ranging from milliseconds to tens of seconds. In the past years, however, the discovery of ultra-long period... -
Parkes observations for project PX138 semester 2025APRS_04
Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations -
Parkes observations for project PX139 semester 2025APRS_03
Pulsar data from Parkes (Murriyang) Target of Opportunity (ToO) observations -
Long-term project observations for project P885 semester 2025APRS_08
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... -
Parkes observations for project PX600 semester 2020APRS_122
The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the... -
Parkes observations for project P1345 semester 2025APRS_15
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 P1357 semester 2025APRS_06
MeerKAT has already discovered a number of Galactic transients, which are most likely to be Rotating Radio Transients (RRATs). Previous observations of a few of these sources... -
Australia-wide Machine Learning Evapotranspiration for Trees (AMLETT) model...
This dataset contains the monthly evapotranspiration (ET, mm/month) data at 30 meters spatial resolution from Feb 2000 to Dec 2022 for Murray-Darling Basin wetlands, Australia.... -
Time-tronics: from temporal printed circuit board to quantum computer;...
Scripts used to calculate the fidelity of quantum simulation and quantum computing in the Time-tronics: from temporal printed circuit board to quantum computer paper; pre-print... -
Coupled Coastal Hazard Prediction System (CCHaPS) Hindcast for Australia
CCHaPS, the Coupled Coastal Hazard Prediction System, is a 2D hydrodynamic and wave model (Semi-implicit Cross-scale Hydroscience Integrated System Model and Wind Wave Model... -
Solar and Kinetic Energy Harvesting Dataset for Human Activity Recognition (SKEH)
This data was collected from wearable accelerometer, solar and kinetic energy harvesters for human activity recognition. The data was collected to explore the performance of... -
Long-term project observations for project P1321 semester 2025APRS_08
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... -
Parkes observations for project P595 semester 2025APRS_16
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 P1328 semester 2025APRS_15
Fast radio bursts are peculiar micro-millisecond duration transients, which have been seen to be extragalactic in origin. Since their discovery, a dichotomy has emerged in their... -
Parkes observations for project P1219 semester 2025APRS_07
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 P1325 semester 2025APRS_05
We request 15 hours of observing time with the Parkes UWL receiver (700-4000 MHz) to investigate frequency-dependent eclipsing in three spider millisecond pulsars (MSPs): one... -
Parkes observations for project P1325 semester 2025APRS_06
We request 15 hours of observing time with the Parkes UWL receiver (700-4000 MHz) to investigate frequency-dependent eclipsing in three spider millisecond pulsars (MSPs): one...