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Long-term project observations for project P574 semester 2024OCTS_14
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 2024OCTS_18
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... -
SCHISM-WWMIII hydrological and wave model hindcast for Vanuatu
This collection contains netCDF formatted data produced by the SCHSIM-WWMIII hydrological and wave coupled model v5.9 around Vanuatu as part of the VanKIRAP project, described... -
Ecological Knowledge System: State and Transition Models
Collection: This collection contains models and datasets describing the State and Transition Models (STMs) developed as part of the Ecological Knowledge System (EKS). The EKS is... -
Parkes observations for project P1176 semester 2024OCTS_03
Pulsars and their winds are among nature's most powerful particle accelerators, producing particles with energies up to a few PeVatrons. In addition to high-energy radiation... -
Parkes observations for project P1165 semester 2024OCTS_10
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 P1183 semester 2024OCTS_16
After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we... -
Parkes observations for project P1054 semester 2024OCTS_14
With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Thirtysix sources have been discovered in targeted... -
Parkes observations for project P1101 semester 2024OCTS_09
We propose to continue our fortnightly monitoring of a very active repeater, FRB 20190520B, with the Parkes UWL system. Our current observations show that FRB 20190520B is not... -
Parkes observations for project P1189 semester 2024OCTS_09
The solar wind and space weather events have a significant impact on the solar system and can pose hazards to both space and Earth-based technologies. Understanding the origins... -
Parkes observations for project P1185 semester 2023APRS_42
Ultra-long period neutron stars (ULPNSs) are an emerging class of objects that have sparked interest and curiosity in the fast transient community. Along with standard... -
Parkes observations for project P1219 semester 2023OCTS_29
The magnetic field potentially regulates the process of star formation and the evolution of molecular clouds. It is inherently difficult to measure interstellar magnetic field... -
OzWheat V1.0 SNP data assets
Single nucleotide polymorphism genotypes for ~300 varieties from the OzWheat diversity panel generated with alternative platforms combined in a single matrix. Original platform... -
OzWheat v1.0 GWAS platform datasets
Genomic/pedigree and marker-trait association data associated with the following publication; Hyles, J., Eagles, H., et al. (2024). OzWheat; a genome-to-phenome platform to... -
Parkes observations for project P1281 semester 2024OCTS_19
The physical origin of fast radio bursts (FRBs) has been hotly debated over the past decade until the discovery of bright radio bursts from the Galactic magnetar in 2020. The... -
Parkes observations for project P1238 semester 2024OCTS_09
Young and energetic pulsars can power strong pulsar wind nebula (PWN), which can be observed from radio to X-ray and beyond. Leveraging the sensitivity and high-resolution of... -
Parkes observations for project P1321 semester 2024OCTS_07
We propose to search for temporal variations in HI absorption spectra seen against background pulsars to characterise Tiny Scale Atomic Structure (TSAS) in the Milky Way... -
Parkes observations for project P1328 semester 2024OCTS_19
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 P1317 semester 2024OCTS_06
The existence of a population of millisecond pulsars (MSPs) in the Galactic bulge is supported, among others, by the Fermi GeV excess, a signal of gamma rays coming from the... -
Parkes observations for project P1334 semester 2024OCTS_06
The Galactic Centre is the most complex and dynamic region of our Galaxy. Radio images have revealed a plethora of filamentary structures that trace out magnetic fields running...