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Parkes observations for project P455 semester 2024OCTS_05
This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Important results published in our... -
AS201 EMU: EMUCAT supermosaic images
EMUCAT generates “supermosaics” by linearly mosaicing together the adjacent EMU tiles within each of EMUCAT’s “source extraction regions”. These supermosaics ensure close to... -
Parkes observations for project P737 semester 2024OCTS_02
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. In particular for commissioning... -
Parkes observations for project P885 semester 2024OCTS_16
We propose a reduced even more modest program to continue monitoring 4 of the 6 known radio magnetars, tracking their rotational, flux density, and polarisation properties. The... -
Parkes observations for project P960 semester 2024OCTS_14
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... -
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... -
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...