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Long-term project observations for project P1101 semester 2025APRS_02
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... -
Bushfire fuel classification fuel types map
This map describes Australian fuel type classes and their estimated extents using the Bushfire Fuel Classification (BFC) framework of Hollis et al. (2015) and Cruz et al.... -
Parkes observations for project P1356 semester 2025APRS_06
Magnetars are neutron stars with exceptionally high magnetic fields. From the 30 known magnetars, only six have had radio emission detected so far. The remaining 24 magnetars... -
Parkes observations for project P1345 semester 2025APRS_06
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 pulsar observations with undefined project IDs for 2025APRS_02
Parkes pulsar observations with undefined project IDs for 2025APRS. This collection contains observations from project ID PX135. -
Parkes observations for project P595 semester 2025APRS_05
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 PX600 semester 2020APRS_118
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... -
Long-term project observations for project P574 semester 2025APRS_02
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 PX500 semester 2025APRS_12
This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been... -
Parkes observations for project P1345 semester 2025APRS_05
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... -
My Climate Copilot User Study Annotations
A collection of 357 annotations from 13 climate experts for Climate Adaptation NLP. It contains evaluations of Large Language Model (LLM) capability on climate questions as well... -
Parkes observations for project P1345 semester 2025APRS_07
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... -
Infragravity waves 1D linear numerical model (Matlab)
Written as part of Stephanie Contardo's PhD thesis -
Long-term project observations for project P456 semester 2025APRS_02
The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale,... -
Parkes observations for project PX500 semester 2025APRS_13
This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been... -
Long-term project observations for project P1321 semester 2025APRS_02
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 P1338 semester 2025APRS_20
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 P1338 semester 2025APRS_21
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... -
Long-term project observations for project P574 semester 2025APRS_03
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... -
Long-term project observations for project P1041 semester 2025APRS_02
Omega Cen is the largest globular cluster in the Milky Way. I contains at least 18 known MPSs, and there are solid hints for the presence of an even larger pulsar population. We...