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Parkes observations for project P1211 semester 2024APRS_13
Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary... -
Long-term project observations for project P1321 semester 2025APRS_05
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 P1325 semester 2025APRS_02
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 P1328 semester 2025APRS_13
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... -
Tropical Cyclone Potential Intensity (TCPI)
This data collection consists of Tropical Cyclone (TC) Potential Intensity (PI) calculated from the ERA5 reanalysis dataset (1979 to 2023) and a selection of global climate... -
Parkes observations for project P1344 semester 2025APRS_06
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_31
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 P1348 semester 2024OCTS_04
We have discovered 6 candidate eclipsing binary millisecond pulsar (BMSPs) systems via image-plane searches for steep-spectrum radio sources with periodic variability. The radio... -
Long-term project observations for project P1361 semester 2025APRS_04
PSR J1227-6208 is a recycled pulsar in a bianry with a massive white dwarf companion. A recent timing measurement from combined MeerKAT and Parkes observations shows the... -
Parkes observations for project P1356 semester 2025APRS_09
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_08
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_05
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 PX600 semester 2020APRS_119
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 P595 semester 2025APRS_07
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... -
Long-term project observations for project P885 semester 2025APRS_06
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 P960 semester 2025APRS_06
We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time... -
Parkes observations for project P1362 semester 2025APRS_02
PSR J1757-1854 is the most relativistic galactic double neutron star system. Its eccentricity makes it an ideal playground for gravity experiments with pulsar timing. Via... -
Long-term project observations for project P456 semester 2025APRS_04
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 P737 semester 2025APRS_02
Instrumental Commissioning -
Parkes observations for project P1364 semester 2025APRS_03
The propagation effects of the ionized interstellar medium (IISM) on pulsars are not well understood, and increase uncertainty on pulsar timing measurements. As high-precision...