-
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... -
Long-term project observations for project P885 semester 2025APRS_04
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 pulsar observations with undefined project IDs for 2025APRS_03
Parkes pulsar observations with undefined project IDs for 2025APRS. This collection contains observations from project ID PX135. -
Parkes observations for project P1363 semester 2025APRS_05
We propose to monitor the bursts from the hyperactive repeating fast radio burst FRB 20240619D over six months using the Murriyang UWL receiver. The primary aim is to study the... -
Stable carbon isotope values of plant bulk tissue from 540 species surveyed...
This data set contains the stable isotope carbon values for plants surveyed by Australia’s Terrestrial Ecosystem Research Network (TERN) between 2011 and May 2022 (inclusive).... -
Data supporting "Satellite-tracked movements of juvenile Great Egrets (Ardea...
The data and files in these directories underpin analyses of telemetry data for two Australian waterbird species. The goal is to understand the movement strategies of these... -
Long-term project observations for project P1101 semester 2025APRS_03
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... -
Long-term project observations for project P1321 semester 2025APRS_03
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... -
Long-term project observations for project P1361 semester 2025APRS_02
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 P1338 semester 2025APRS_22
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 P1363 semester 2025APRS_06
We propose to monitor the bursts from the hyperactive repeating fast radio burst FRB 20240619D over six months using the Murriyang UWL receiver. The primary aim is to study the... -
Parkes observations for project P960 semester 2025APRS_04
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 P1338 semester 2025APRS_23
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 P1344 semester 2025APRS_03
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 pulsar observations with undefined project IDs for 2025APRS_04
Parkes pulsar observations with undefined project IDs for 2025APRS. This collection contains observations from project ID PX135. -
Parkes observations for project P1338 semester 2025APRS_24
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... -
Canola establishment data 2024. Geraldton core research site CSP2212-005RTX
Data is the result of field experiment(s) conducted in 2024 to examine factors affecting canola establishment. -
Canola establishment data 2024. Condoblin and Canowindra core research sites...
Data is the result of field experiment(s) conducted in 2024 to examine factors affecting canola establishment. Data is for Condoblin (-33.0427,147.2308 ) and Canowindra... -
Canola establishment data 2024. Ungarra core research site CSP2212-005RTX
Data is the result of field experiment(s) conducted in 2024 to examine factors affecting canola establishment.